Welcome to MRChem’s documentation!¶

MRChem is a numerical real-space code for molecular electronic structure calculations within the self-consistent field (SCF) approximations of quantum chemistry (Hartree-Fock and Density Functional Theory). The code is divided in two main parts: the MultiResolution Computation Program Package (MRCPP), which is a general purpose numerical mathematics library based on multiresolution analysis and the multiwavelet basis which provide low-scaling algorithms as well as rigorous error control in numerical computations, and the MultiResolution Chemistry (MRChem) program that uses the functionalities of MRCPP for computational chemistry applications.

The code is being developed at the Hylleraas Centre for Quantum Molecular Sciences at UiT - The Arctic University of Norway.

The code is under active development, and the latest stable releases as well as development versions can be found on GitHub.

Features in MRChem-1.1:¶

Wave functions:
- Kohn-Sham DFT
  
  Spin-polarized
  
  Spin-unpolarized
  
  LDA, GGA and hybrid functionals
- Hartree-Fock
  
  Restricted closed-shell
  
  Unrestricted
- Explicit external fields
  
  Electric field
- Solvent effects
  
  Cavity-free PCM
Properties:
- Ground state energy
- Dipole moment
- Quadrupole moment
- Polarizability
- Magnetizability
- NMR shielding constant
- Geometric derivative
Parallel implementation:
- Shared memory (OpenMP): ~20 cores
- Distributed memory (MPI): ~1000 procs
- Hybrid scheme (MPI + OpenMP): ~10 000 cores
Current size limitations:
- ~2000 orbitals on ~100 high-end compute nodes (128 core/256GiB mem)
- ~100 orbitals on a single high-memory (1TB) compute node

Upcoming features:¶

Wave functions:
- Meta-GGAs
- ZORA Hamiltonian
- Periodic Boundary Conditions
- External magnetic field
Properties:
- Optical rotation
- Spin-spin coupling constant
- Hyperfine coupling constant
- Magnetically induced currents
- Hyperpolarizability
- Geometry optimization
Performance:
- Reduced memory footprint
- Improved DFT scaling and performance

Installation¶

Build prerequisites¶

Python-3.7 (or later)
CMake-3.14 (or later)
GNU-5.4 or Intel-17 (or later) compilers (C++14 standard)

Hint

We have collected the recommended modules for the different Norwegian HPC systems under tools/<machine>.env. These files can be sourced in order to get a working environment on the respective machines, and may also serve as a guide for other HPC systems.

C++ dependencies¶

The MRChem program depends on the following C++ libraries:

Input handling: nlohmann/json-3.6
Multiwavelets: MRCPP-1.4
Linear algebra: Eigen-3.4
DFT functionals: XCFun-2.0

All these dependencies will be downloaded automatically at configure time by CMake, but can also be linked manually by setting the variables:

MRCPP_DIR=<path_to_mrcpp>/share/cmake/MRCPP
XCFun_DIR=<path_to_xcfun>/share/cmake/XCFun
Eigen3_DIR=<path_to_eigen3>/share/eigen3/cmake
nlohmann_json_DIR=<path_to_nlohmann_json>

Python dependencies¶

Users only need a Python3 interpreter, which is used for configuration (setup script) as well as launching the program (mrchem script).

Developers will need some extra Python packages to update the input parser and build the documentation locally with Sphinx.

We strongly suggest not to install these Python dependencies globally, but rather to use a local virtual environment. We provide a Pipfile for specifying the Python dependencies. We recommend using Pipenv, since it manages virtual environment and package installation seamlessly. After installing it with your package manager, run:

$ pipenv install --dev

to create a virtual environment with all developer packages installed.

The environment can be activated with:

$ pipenv shell

Alternatively, any Python command can be run within the virtual environment by doing:

$ pipenv run python -c "print('Hello, world')"

Obtaining and building the code¶

The latest development version of MRChem can be found on the master branch on GitHub:

$ git clone https://github.com/MRChemSoft/mrchem.git

The released versions can be found from Git tags vX.Y.Z under the release/X.Y branches in the same repository, or a zip file can be downloaded from Zenodo.

By default, all dependencies will be fetched at configure time if they are not already available.

Configure¶

The setup script will create a directory called <build-dir> and run CMake. There are several options available for the setup, the most important being:

--cxx=<CXX>: C++ compiler [default: g++]
--omp: Enable OpenMP parallelization [default: False]
--mpi: Enable MPI parallelization [default: False]
--type=<TYPE>: Set the CMake build type (debug, release, relwithdebinfo, minsizerel) [default: release]
--prefix=<PATH>: Set the install path for make install [default: ‘/usr/local’]
--cmake-options=<STRING>: Define options to CMake [default: ‘’]
-h --help: List all options

The code can be built with four levels of parallelization:

no parallelization

only shared memory (OpenMP)

only distributed memory (MPI)

hybrid OpenMP + MPI

Note

In practice we recommend the shared memory version for running on your personal laptop/workstation, and the hybrid version for running on a HPC cluster. The serial and pure MPI versions are only useful for debugging.

The default build is without parallelization and using GNU compilers:

$ ./setup --prefix=<install-dir> <build-dir>

To use Intel compilers you need to specify the --cxx option:

$ ./setup --prefix=<install-dir> --cxx=icpc <build-dir>

To build the code with shared memory (OpenMP) parallelization, add the --omp option:

$ ./setup --prefix=<install-dir> --omp <build-dir>

To build the code with distributed memory (MPI) parallelization, add the --mpi option and change to the respective MPI compilers (--cxx=mpicxx for GNU and --cxx=mpiicpc for Intel):

$ ./setup --prefix=<install-dir> --omp --mpi --cxx=mpicxx <build-dir>

When dependencies are fetched at configuration time, they will be downloaded into <build-dir>/_deps. For the example of MRCPP, sources are saved into the folders <build-dir>/_deps/mrcpp_sources-src and built into <build-dir>/_deps/mrcpp_sources-build.

Note

If you compile the MRCPP library manually as a separate project, the level of parallelization must be the same for MRCPP and MRChem. Similar options apply for the MRCPP setup, see mrcpp.readthedocs.io.

Build¶

If the CMake configuration is successful, the code is compiled with:

$ cd <build-dir>
$ make

Test¶

A test suite is provided to make sure that everything compiled properly. To run a collection of small unit tests:

$ cd <build-dir>
$ ctest -L unit

To run a couple of more involved integration tests:

$ cd <build-dir>
$ ctest -L integration

Install¶

After the build has been verified with the test suite, it can be installed with the following command:

$ cd <build-dir>
$ make install

This will install two executables under the <install-path>:

<install-path>/bin/mrchem       # Python input parser and launcher
<install-path>/bin/mrchem.x     # MRChem executable

Please refer to the User’s Manual for instructions for how to run the program.

Hint

We have collected scripts for configure and build of the hybrid OpenMP + MPI version on the different Norwegian HPC systems under tools/<machine>.sh. These scripts will build the current version under build-${version}, run the unit tests and install under install-${version}, e.g. to build version v1.0.0 on Fram:

$ cd mrchem
$ git checkout v1.0.0
$ tools/fram.sh

The configure step requires internet access, so the scripts must be run on the login nodes, and it will run on a single core, so it might take some minutes to complete. The scripts will not install the Python dependencies, so this must be done manually in order to run the code.

User’s Manual¶

The MRChem program comes as two executables:

<install-path>/bin/mrchem                   # Python input parser and launcher
<install-path>/bin/mrchem.x                 # MRChem main executable

where the former is a Python script that reads and validates the user input file and produces a new program input file which is then passed as argument to the latter, which is the actual C++ executable.

The input and output of the program is thus organized as three separate files:

File extension	Description	Format
`.inp`	User input file	GETKW/JSON
`.json`	Program input/output	JSON
`.out`	User output file	Text

The name of the user input file can be anything, as long as it has the .inp extension, and the corresponding .json and .out files will get the same name prefix. The JSON program file will get both an "input" and an "output" section. This "input" section is rather detailed and contains very implementation specific keywords, but it is automatically generated by the mrchem script, based on the more generic keywords of the user input file. The mrchem script will further launch the mrchem.x main executable, which will produce the text output file as well as the "output" section of the JSON in/out file. The contents of all these files will be discussed in more detail in the sections below.

Running the program¶

In the following we will assume to have a valid user input file for the water molecule called h2o.inp, e.g. like this

world_prec = 1.0e-4

WaveFunction {
  method = B3LYP
}

Molecule {
$coords
O  0.0000  0.000 -0.125
H -1.4375  0.000  1.025
H  1.4375  0.000  1.025
$end
}

To run the calculation, pass the file name (without extension) as argument to the mrchem script (make sure you understand the difference between the .inp, .json and .out file, as described in the previous section):

$ mrchem h2o

This will under the hood actually do the following two steps:

$ mrchem h2o.inp > h2o.json
$ mrchem.x h2o.json > h2o.out

The first step includes input validation, which means that everything that passes this step is a well-formed computation.

Dry-running the input parser¶

The execution of the two steps above can be done separately by dry-running the parser script:

$ mrchem --dryrun h2o

This will run only the input validation part and generate the h2o.json program input, but it will not launch the main executable mrchem.x. This can then be done manually in a subsequent step by calling:

$ mrchem.x h2o.json

This separation can be useful for instance for developers or advanced users who want to change some automatically generated input values before launching the actual program, see Input schema.

Printing to standard output¶

By default the program will write to the text output file (.out extension), but if you rather would like it printed in the terminal you can add the --stdout option (then no text output file is created):

$ mrchem --stdout h2o

Reproducing old calculations¶

The JSON in/out file acts as a full record of the calculation, and can be used to reproduce old results. Simply pass the JSON file once more to mrchem.x, and the "output" section will be overwritten:

$ mrchem.x h2o.json

User input in JSON format¶

The user input file can be written in JSON format instead of the standard syntax which is described in detail below. This is very convenient if you have for instance a Python script to generate input files. The water example above in JSON format reads (the coords string is not very elegant, but unfortunately that’s just how JSON works…):

{
  "world_prec": 1.0e-4,
  "WaveFunction": {
    "method": "B3LYP"
  },
  "Molecule": {
    "coords": "O  0.0000  0.000 -0.125\nH -1.4375  0.000  1.025\nH  1.4375  0.000  1.025\n"
  }
}

which can be passed to the input parser with the --json option:

$ mrchem --json h2o

Note

A user input file in JSON format must NOT be confused with the JSON in/out file for the mrchem.x program. The file should still have a .inp extension, and contain all the same keywords which have to be validated and translated by the mrchem script into the .json program input file.

Parallel execution¶

The MRChem program comes with support for both shared memory and distributed memory parallelization, as well as a hybrid combination of the two. In order to activate these capabilities, the code needs to be compiled with OpenMP and/or MPI support (--omp and/or --mpi options to the CMake setup script, see Installation instructions).

Shared memory OpenMP¶

For the shared memory part, the program will automatically pick up the number of threads from the environment variable OMP_NUM_THREADS. If this variable is not set it will usually default to the maximum available. So, to run the code on 16 threads (all sharing the same physical memory space):

$ OMP_NUM_THREADS=16 mrchem h2o

Distributed memory MPI¶

In order to run a program in an MPI parallel fashion, it must be executed with an MPI launcher like mpirun, mpiexec, srun, etc. Note that it is only the main executable mrchem.x that should be launched in parallel, not the mrchem input parser script. This can be achieved either by running these separately in a dry-run (here two MPI processes):

$ mrchem --dryrun h2o
$ mpirun -np 2 mrchem.x h2o.json

or in a single command by passing the launcher string as argument to the parser:

$ mrchem --launcher="mpirun -np 2" h2o

This string can contain any argument you would normally pass to mpirun as it will be literally prepended to the mrchem.x command when the mrchem script executes the main program.

Hint

For best performance, it is recommended to use shared memory within each NUMA domain (usually one per socket) of your CPU, and MPI across NUMA domains and ultimately machines. Ideally, the number of OpenMP threads should be between 8-20. E.g. on hardware with two sockets of 16 cores each, use OMP_NUM_THREADS=16 and scale the number of MPI processes by the size of the molecule, typically one process per ~5 orbitals or so (and definitely not more than one process per orbital).

Job example (Betzy)¶

This job will use 4 compute nodes, with 12 MPI processes on each, and the MPI process will use up to 15 OpenMP threads. 4 MPI process per node are used for the “Bank”. The Bank processes are using only one thread, therefore there is in practice no overallocation. It is however important that bank_size is set to be at least 4*4 = 16 (it is by default set, correctly, to one third of total MPI size, i.e. 4*12/3=16). It would also be possible to set 16 tasks per node, and set the bank size parameter accordingly to 8*4=32. The flags are optimized for the OpenMPI (foss) library on Betzy (note that H2O is a very small molecule for such setup!).

#!/bin/bash -l
#SBATCH --nodes=4
#SBATCH --tasks-per-node=12

export UCX_LOG_LEVEL=ERROR
export OMP_NUM_THREADS=15

~/my_path/to/mrchem --launcher='mpirun --rank-by node --map-by socket --bind-to numa --oversubscribe' h2o

--rank-by node: Tells the system to place the first MPI rank on the first node, the second MPI rank on the second node, until the last node, then start at the first node again.
--map-by socket: Tells the system to map (group) MPI ranks according to socket before distribution between nodes. This will ensure that for example two bank cores will access different parts of memory and be placed as the 16th thread of a numa group.
--bind-to numa: Tells the system to bind cores to one NUMA (Non Uniform Memory Access) group. On Betzy memory configuration groups cores by groups of 16, with cores in the same group having the same access to memory (other cores will have access to that part of the memory too, but slower). That means that a process will only be allowed to use one of the 16 cores of the group. (The operating system may change the core assigned to a thread/process and, without precautions, it may be assigned to any other core, which would result in much reduced performance). The 16 cores of the group may then be used by the threads initiated by that MPI process.
--oversubscribe: To tell MPI that it is should accept that the number of MPI processes times the number of threads is larger than the number of available cores.

Advanced option: Alternatively one can get full control of task placement using the Slurm workload manager by replacing mpirun with srun and setting explicit CPU masks as:

~/my_path/to/mrchem --launcher='srun --cpu-bind=mask_cpu:0xFFFE00000000, \\
0xFFFE000000000000000000000000,0xFFFE000000000000,0xFFFE0000000000000000000000000000, \\
0xFFFE,0xFFFE0000000000000000,0xFFFE0000,0xFFFE00000000000000000000,0x10000, \\
0x100000000000000000000,0x100000000,0x1000000000000000000000000 \\
--distribution=cyclic:cyclic' h2o

--cpu-bind=mask_cpu:0xFFFE00000000,0xFFFE000000000000000000000000,... give the core (or cpu) masks the process have access to. 0x means that the number is in hexadecimal. For example 0xFFFE00000000 is 111111111111111000000000000000000000000000000000 in binary, meaning that the first process can not use the first 33 cores, then it can use the cores from position 34 up to position 48, and nothing else.

--distribution=cyclic:cyclic The first cyclic will put the first rank on the first node, the second rank on the second node etc. The second cyclic distribute the ranks withing the nodes.

More examples can be found in the mrchem-examples repository on GitHub.

Parallel pitfalls¶

Warning

Parallel program execution is not a black box procedure, and the behavior and efficiency of the run depends on several factors, like hardware configuration, operating system, compiler type and flags, libraries for OpenMP and MPI, type of queing system on a shared cluster, etc. Please make sure that the program runs correctly on your system and is able to utilize the computational resources before commencing production calculations.

Typical pitfalls for OpenMP¶

Not compiling with correct OpenMP support.
Not setting number of threads correctly.
Hyper-threads: the round-robin thread distribution might fill all hyper-threads on each core before moving on to the next physical core. In general we discourage the use of hyper-threads, and recommend a single thread per physical core.
Thread binding: all threads may be bound to the same core, which means you can have e.g. 16 threads competing for the limited resources available on this single core (typically two hyper-threads) while all other cores are left idle.

Typical pitfalls for MPI¶

Not compiling with the correct MPI support.
Default launcher options might not give correct behavior.
Process binding: if a process is bound to a core, then all its spawned threads will also be bound to the same core. In general we recommend binding to socket/NUMA.
Process distribution: in a multinode setup, all MPI processes might land on the same machine, or the round-robin procedure might count each core as a separate machine.

How to verify a parallel MRChem run¶

In the printed output, verify that MRCPP has actually been compiled with correct support for MPI and/or OpenMP:

----------------------------------------------------------------------

MRCPP version         : 1.2.0
Git branch            : master
Git commit hash       : 686037cb78be601ac58b
Git commit author     : Stig Rune Jensen
Git commit date       : Wed Apr 8 11:35:00 2020 +0200

Linear algebra        : EIGEN v3.3.7
Parallelization       : MPI/OpenMP

----------------------------------------------------------------------

In the printed output, verify that the correct number of processes and threads has been detected:

----------------------------------------------------------------------

 MPI processes         :      (no bank)                             2
 OpenMP threads        :                                           16
 Total cores           :                                           32

----------------------------------------------------------------------

Monitor your run with top to see that you got the expected number of mrchem.x processes (MPI), and that they actually run at the expected CPU percentage (OpenMP):

PID   USER      PR  NI    VIRT    RES    SHR S   %CPU  %MEM     TIME+ COMMAND
9502  stig      25   5  489456 162064   6628 R 1595,3   2,0   0:14.50 mrchem.x
9503  stig      25   5  489596 162456   6796 R 1591,7   2,0   0:14.33 mrchem.x

Monitor your run with htop to see which core/hyper-thread is being used by each process. This is very useful to get the correct binding/pinning of processes and threads. In general you want one threads per core, which means that every other hyper-thread should remain idle. In a hybrid MPI/OpenMP setup it is rather common that each MPI process becomes bound to a single core, which means that all threads spawned by this process will occupy the same core (possibly two hyper-threads). This is then easily detected with htop.
Perform dummy executions of your parallel launcher (mpirun, srun, etc) to check whether it picks up the correct parameters from the resource manager on your cluster (SLURM, Torque, etc). You can then for instance report bindings and host name for each process:
```
$ mpirun --print-rank-map hostname
```
Play with the launcher options until you get it right. Note that Intel and OpenMPI have slightly different options for their mpirun and usually different behavior. Beware that the behavior can also change when you move from single- to multinode execution, so it is in general not sufficient to verify you runs on a single machine.
Perform a small scaling test on e.g. 1, 2, 4 processes and/or 1, 2, 4 threads and verify that the total computation time is reduced as expected (don’t expect 100% efficiency at any step).

User input file¶

The input file is organized in sections and keywords that can be of different type. Input keywords and sections are case-sensitive, while values are case-insensitive.

Section {
  keyword_1 = 1                         # int
  keyword_2 = 3.14                      # float
  keyword_3 = [1, 2, 3]                 # int array
  keyword_4 = foo                       # string
  keyword_5 = true                      # boolean
}

Valid options for booleans are true/false, on/off or yes/no. Single word strings can be given without quotes (be careful of special characters, like slashes in file paths). A complete list of available input keywords can be found in the User input reference.

Top section¶

The main input section contain four keywords: the relative precision $\epsilon_{rel}$ that will be guaranteed in the calculation and the size, origin and unit of the computational domain. The top section is not specified by name, just write the keywords directly, e.g

world_prec = 1.0e-5                     # Overall relative precision
world_size = 5                          # Size of domain 2^{world_size}
world_unit = bohr                       # Global length unit
world_origin = [0.0, 0.0, 0.0]          # Global gauge origin

The relative precision sets an upper limit for the number of correct digits you are expected to get out of the computation (note that $\epsilon_{rel}=10^{-6}$ yields $\mu$ Ha accuracy for the hydrogen molecule, but only mHa accuracy for benzene).

The computational domain is always symmetric around the origin, with total size given by the world_size parameter as $[2^n]^3$, e.i. world_size = 5 gives a domain of $[-16,16]^3$. Make sure that the world is large enough to allow the molecular density to reach zero on the boundary. The world_size parameter can be left out, in which case the size will be estimated based on the molecular geometry. The world_unit relates to all coordinates given in the input file and can be one of two options: angstrom or bohr.

Note

The world_size will be only approximately scaled by the angstrom unit, by adding an extra factor of 2 rather than the appropriate factor of ~1.89. This means that e.g. world_size = 5 ($[-16,16]^3$) with world_unit = angstrom will be translated into $[-32,32]^3$ bohrs.

Precisions¶

MRChem uses a smoothed nuclear potential to avoid numerical problems in connection with the $Z/|r-R|$ singularity. The smoothing is controlled by a single parameter nuc_prec that is related to the expected error in the energy due to the smoothing. There are also different precision parameters for the construction of the Poisson and Helmholtz integral operators.

Precisions {
  nuclear_prec = 1.0e-6                 # For construction of nuclear potential
  poisson_prec = 1.0e-6                 # For construction of Poisson operators
  helmholtz_prec = 1.0e-6               # For construction of Helmholtz operatos
}

By default, all precision parameters follow world_prec and usually don’t need to be changed.

Printer¶

This section controls the format of the printed output file (.out extension). The most important option is the print_level, but it also gives options for number of digits in the printed output, as well as the line width (defaults are shown):

Printer {
  print_level = 0                       # Level of detail in the printed output
  print_width = 75                      # Line width (in characters) of printed output
  print_prec = 6                        # Number of digits in floating point output
}

Note that energies will be printed with twice as many digits. Available print levels are:

print_level=-1 no output is printed
print_level=0 prints mainly properties
print_level=1 adds timings for individual steps
print_level=2 adds memory and timing information on OrbitalVector level
print_level=3 adds details for individual terms of the Fock operator
print_level=4 adds memory and timing information on Orbital level
print_level>=5 adds debug information at MRChem level
print_level>=10 adds debug information at MRCPP level

MPI¶

This section defines some parameters that are used in MPI runs (defaults shown):

MPI {
  bank_size = -1                        # Number of processes used as memory bank
  numerically_exact = false             # Guarantee MPI invariant results
  share_nuclear_potential = false       # Use MPI shared memory window
  share_coulomb_potential = false       # Use MPI shared memory window
  share_xc_potential = false            # Use MPI shared memory window
}

The memory bank will allow larger molecules to get though if memory is the limiting factor, but it will be slower, as the bank processes will not take part in any computation. For calculations involving exact exchange (Hartree-Fock or hybrid DFT functionals) a memory bank is required whenever there’s more than one MPI process. A negative bank size will set it automatically based on the number of available processes. For pure DFT functionals on smaller molecules it is likely more efficient to set bank_size = 0, otherwise it’s recommended to use the default. If a particular calculation runs out of memory, it might help to increase the number of bank processes from the default value.

The numerically_exact keyword will trigger algorithms that guarantee that the computed results are invariant (within double precision) with respect to the number or MPI processes. These exact algorithms require more memory and are thus not default. Even when the numbers are not MPI invariant they should be correct and identical within the chosen world_prec.

The share_potential keywords are used to share the memory space for the particular functions between all processes located on the same physical machine. This will save memory but it might slow the calculation down, since the shared memory cannot be “fast” memory (NUMA) for all processes at once.

Basis¶

This section defines the polynomial MultiWavelet basis

Basis {
  type = Interpolating                  # Legendre or Interpolating
  order = 7                             # Polynomial order of MW basis
}

The MW basis is defined by the polynomial order $k$, and the type of scaling functions: Legendre or Interpolating polynomials (in the current implementation it doesn’t really matter which type you choose). Note that increased precision requires higher polynomial order (use e.g $k = 5$ for $\epsilon_{rel} = 10^{-3}$, and $k = 13$ for $\epsilon_{rel} = 10^{-9}$, and interpolate in between). If the order keyword is left out it will be set automatically according to

\[k=-1.5*log_{10}(\epsilon_{rel})\]

The Basis section can usually safely be omitted in the input.

Molecule¶

This input section specifies the geometry (given in world_unit units), charge and spin multiplicity of the molecule, e.g. for water (coords must be specified, otherwise defaults are shown):

Molecule {
  charge = 0                            # Total charge of molecule
  multiplicity = 1                      # Spin multiplicity
  translate = false                     # Translate CoM to world_origin
$coords
O   0.0000     0.0000     0.0000        # Atomic symbol and coordinate
H   0.0000     1.4375     1.1500        # Atomic symbol and coordinate
H   0.0000    -1.4375     1.1500        # Atomic symbol and coordinate
$end
}

Since the computational domain is always cubic and symmetric around the origin it is usually a good idea to translate the molecule to the origin (as long as the world_origin is the true origin).

WaveFunction¶

Here we give the wavefunction method and whether we run spin restricted (alpha and beta spins are forced to occupy the same spatial orbitals) or not (method must be specified, otherwise defaults are shown):

WaveFunction {
  method = <wavefunction_method>        # Core, Hartree, HF or DFT
  restricted = true                     # Spin restricted/unrestricted
}

There are currently four methods available: Core Hamiltonian, Hartree, Hartree-Fock (HF) and Density Functional Theory (DFT). When running DFT you can either set one of the default functionals in this section (e.g. method = B3LYP), or you can set method = DFT and specify a “non-standard” functional in the separate DFT section (see below). See User input reference for a list of available default functionals.

Note

Restricted open-shell wavefunctions are not supported.

DFT¶

This section can be omitted if you are using a default functional, see above. Here we specify the exchange-correlation functional used in DFT (functional names must be specified, otherwise defaults are shown)

DFT {
  spin = false                          # Use spin-polarized functionals
  density_cutoff = 0.0                  # Cutoff to set XC potential to zero
$functionals
<func1>     1.0                         # Functional name and coefficient
<func2>     1.0                         # Functional name and coefficient
$end
}

You can specify as many functionals as you want, and they will be added on top of each other with the given coefficient. Both exchange and correlation functionals must be set explicitly, e.g. SLATERX and VWN5C for the standard LDA functional. For hybrid functionals you must specify the amount of exact Hartree-Fock exchange as a separate functional EXX (EXX 0.2 for B3LYP and EXX 0.25 for PBE0 etc.). Option to use spin-polarized functionals or not. Unrestricted calculations will use spin-polarized functionals by default. The XC functionals are provided by the XCFun library.

Properties¶

Specify which properties to compute. By default, only the ground state SCF energy as well as orbital energies will be computed. Currently the following properties are available (all but the dipole moment are false by default)

Properties {
  dipole_moment = true                  # Compute dipole moment
  quadrupole_moment = false             # Compute quadrupole moment
  polarizabiltity = false               # Compute polarizability
  magnetizability = false               # Compute magnetizability
  nmr_shielding = false                 # Compute NMR shieldings
  geometric_derivative = false          # Compute geometric derivative
  plot_density = false                  # Plot converged density
  plot_orbitals = []                    # Plot converged orbitals
}

Some properties can be further specified in dedicated sections.

Warning

The computation of the molecular gradient suffers greatly from numerical noise. The code replaces the nucleus-electron attraction with a smoothed potential. This can only partially recover the nuclear cusps, even with tight precision. The molecular gradient is only suited for use in geometry optimization of small molecules and with tight precision thresholds.

Polarizability¶

The polarizability can be computed with several frequencies (by default only static polarizability is computed):

Polarizability {
  frequency = [0.0, 0.0656]             # List of frequencies to compute
}

NMRShielding¶

For the NMR shielding we can specify a list of nuclei to compute (by default all nuclei are computed):

NMRShielding {
  nuclear_specific = false              # Use nuclear specific perturbation operator
  nucleus_k = [0,1,2]                   # List of nuclei to compute (-1 computes all)
}

The nuclear_specific keyword triggers response calculations using the nuclear magnetic moment operator instead of the external magnetic field. For small molecules this is not recommended since it requires a separate response calculation for each nucleus, but it might be beneficial for larger systems if you are interested only in a single shielding constant. Note that the components of the perturbing operator defines the row index in the output tensor, so nuclear_specific = true will result in a shielding tensor which is the transpose of the one obtained with nuclear_specific = false.

Plotter¶

The plot_density and plot_orbitals properties will use the Plotter section to specify the parameters of the plots (by default you will get a cube plot on the unit cube):

Plotter {
  path = plots                          # File path to store plots
  type = cube                           # Plot type (line, surf, cube)
  points = [20, 20, 20]                 # Number of grid points
  O = [-4.0,-4.0,-4.0]                  # Plot origin
  A = [8.0, 0.0, 0.0]                   # Boundary vector
  B = [0.0, 8.0, 0.0]                   # Boundary vector
  C = [0.0, 0.0, 8.0]                   # Boundary vector
}

The plotting grid is computed from the vectors O, A, B and C in the following way:

line plot: along the vector A starting from O, using points[0] number of points.

surf plot: on the area spanned by the vectors A and B starting from O, using points[0] and points[1] points in each direction.

cube plot: on the volume spanned by the vectors A, B and C starting from O, using points[0], points[1] and points[2] points in each direction.

The above example will plot on a 20x20x20 grid in the volume [-4,4]^3, and the generated files (e.g. plots/phi_1_re.cube) can be viewed directly in a web browser by blob , like this benzene orbital:

SCF¶

This section specifies the parameters for the SCF optimization of the ground state wavefunction.

SCF solver¶

The optimization is controlled by the following keywords (defaults shown):

SCF {
  run = true                            # Run SCF solver
  kain = 5                              # Length of KAIN iterative subspace
  max_iter = 100                        # Maximum number of SCF iterations
  rotation = 0                          # Iterations between diagonalize/localize
  localize = false                      # Use canonical or localized  orbitals
  start_prec = -1.0                     # Dynamic precision, start value
  final_prec = -1.0                     # Dynamic precision, final value
  orbital_thrs = 10 * world_prec        # Convergence threshold orbitals
  energy_thrs = -1.0                    # Convergence threshold energy
}

If run = false no SCF is performed, and the properties are computed directly on the initial guess wavefunction.

The kain (Krylov Accelerated Inexact Newton) keyword gives the length of the iterative subspace accelerator (similar to DIIS). The rotation keyword gives the number of iterations between every orbital rotation, which can be either localization or diagonalization, depending on the localize keyword. The first two iterations in the SCF are always rotated, otherwise it is controlled by the rotation keyword (usually this is not very important, but sometimes it fails to converge if the orbitals drift too far away from the localized/canonical forms).

The dynamic precision keywords control how the numerical precision is changed throughout the optimization. One can choose to use a lower start_prec in the first iterations which is gradually increased to final_prec (both are equal to world_prec by default). Note that lower initial precision might affect the convergence rate.

In general, the important convergence threshold is that of the orbitals, and by default this is set one order of magnitude higher than the overall world_prec. For simple energy calculations, however, it is not necessary to converge the orbitals this much due to the quadratic convergence of the energy. This means that the number of correct digits in the total energy will be saturated well before this point, and one should rather use the energy_thrs keyword in this case in order to save a few iterations.

Note

It is usually not feasible to converge the orbitals beyond the overall precision world_prec due to numerical noise.

Initial guess¶

Several types of initial guess are available:

core and sad requires no further input and computes guesses from scratch.

chk and mw require input files from previous MW calculations.

cube requires input files computed from other sources.

The core and sad guesses are computed by diagonalizing the Hamiltonian matrix using a Core or Superposition of Atomic Densities (SAD) Hamiltonian, respectively. The matrix is constructed in a small AO basis with a given “zeta quality”, which should be added as a suffix in the keyword. Available AO bases are hydrogenic orbitals of single sz, double dz, triple tz and quadruple qz zeta size.

The SAD guess can also be computed in a small GTO basis (3-21G), using the guess type sad_gto. In this case another input keyword guess_screen becomes active for screening in the MW projection of the Gaussians. The screening value is given in standard deviations. Such screening will greatly improve the efficiency of the guess for large systems. It is, however, not recommended to reduce the value much below 10 StdDevs, as this will have the opposite effect on efficiency due to introduction of discontinuities at the cutoff point, which leads to higher grid refinement. sad_gto is usually the preferred guess both for accuracy and efficiency, and is thus the default choice.

The core and sad guesses are fully specified with the following keywords (defaults shown):

SCF {
  guess_prec = 1.0e-3                   # Numerical precision used in guess
  guess_type = sad_gto                  # Type of inital guess (chk, mw, cube, core_XX, sad_XX)
  guess_screen = 12.0                   # Number of StdDev before a GTO is set to zero (sad_gto)
}

Checkpointing¶

The program can dump checkpoint files at every iteration using the write_checkpoint keyword (defaults shown):

SCF {
  path_checkpoint = checkpoint          # Path to checkpoint files
  write_checkpoint = false              # Save checkpoint files every iteration
}

This allows the calculation to be restarted in case it crashes e.g. due to time limit or hardware failure on a cluster. This is done by setting guess_type = chk in the subsequent calculation:

SCF {
  guess_type = chk                      # Type of inital guess (chk, mw, cube, core_XX, sad_XX)
}

In this case the path_checkpoint must be the same as the previous calculation, as well as all other parameters in the calculation (Molecule and Basis in particular).

Write orbitals¶

The converged orbitals can be saved to file with the write_orbitals keyword (defaults shown):

SCF {
  path_orbitals = orbitals              # Path to orbital files
  write_orbitals = false                # Save converged orbitals to file
}

This will make individual files for each orbital under the path_orbitals directory. These orbitals can be used as starting point for subsequent calculations using the guess_type = mw initial guess:

SCF {
  guess_prec = 1.0e-3                   # Numerical precision used in guess
  guess_type = mw                       # Type of inital guess (chk, mw, cube, core_XX, sad_XX)
}

Here the orbitals will be re-projected onto the current MW basis with precision guess_prec. We also need to specify the paths to the input files:

Files {
  guess_phi_p = initial_guess/phi_p     # Path to paired MW orbitals
  guess_phi_a = initial_guess/phi_a     # Path to alpha MW orbitals
  guess_phi_b = initial_guess/phi_b     # Path to beta MW orbitals
}

Note that by default orbitals are written to the directory called orbitals but the mw guess reads from the directory initial_guess (this is to avoid overwriting the files by default). So, in order to use MW orbitals from a previous calculation, you must either change one of the paths (SCF.path_orbitals or Files.guess_phi_p etc), or manually copy the files between the default locations.

Note

The mw guess must not be confused with the chk guess, although they are similar. The chk guess will blindly read in the orbitals that are present, regardless of the current molecular structure and computational setup (if you run with a different computational domain or MW basis type/order the calculation will crash). The mw guess will re-project the old orbitals onto the new computational setup and populate the orbitals based on the new molecule (here the computation domain and MW basis do not have to match).

Response¶

This section specifies the parameters for the SCF optimization of the linear response functions. There might be several independent response calculations depending on the requested properties, e.g.

Polarizability {
  frequency = [0.0, 0.0656]             # List of frequencies to compute
}

will run one response for each frequency (each with three Cartesian components), while

Properties {
  magnetizability = true                # Compute magnetizability
  nmr_shielding = true                  # Compute NMR shieldings
}

will combine both properties into a single response calculation, since the perturbation operator is the same in both cases (unless you choose NMRShielding.nuclear_specific = true, in which case there will be a different response for each nucleus).

Response solver¶

The optimization is controlled by the following keywords (defaults shown):

Response {
  run = [true,true,true]                # Run response solver [x,y,z] direction
  kain = 5                              # Length of KAIN iterative subspace
  max_iter = 100                        # Maximum number of SCF iterations
  localize = false                      # Use canonical or localized  orbitals
  start_prec = -1.0                     # Dynamic precision, start value
  final_prec = -1.0                     # Dynamic precision, final value
  orbital_thrs = 10 * world_prec        # Convergence threshold orbitals
}

Each linear response calculation involves the three Cartesian components of the appropriate perturbation operator. If any of the components of run is false, no response is performed in that particular direction, and the properties are computed directly on the initial guess response functions (usually zero guess).

The kain (Krylov Accelerated Inexact Newton) keyword gives the length of the iterative subspace accelerator (similar to DIIS). The localize keyword relates to the unperturbed orbitals, and can be set independently of the SCF.localize keyword.

The dynamic precision keywords control how the numerical precision is changed throughout the optimization. One can choose to use a lower start_prec in the first iterations which is gradually increased to final_prec (both are equal to world_prec by default). Note that lower initial precision might affect the convergence rate.

For response calculations, the important convergence threshold is that of the orbitals, and by default this is set one order of magnitude higher than the overall world_prec.

Note

The quality of the response property depends on both the perturbed as well as the unperturbed orbitals, so they should be equally well converged.

Initial guess¶

The following initial guesses are available:

none start from a zero guess for the response functions.

chk and mw require input files from previous MW calculations.

By default, no initial guess is generated for the response functions, but the chk and mw guesses work similarly as for the SCF.

Checkpointing¶

The program can dump checkpoint files at every iteration using the write_checkpoint keyword (defaults shown):

Response {
  path_checkpoint = checkpoint          # Path to checkpoint files
  write_checkpoint = false              # Save checkpoint files every iteration
}

This allows the calculation to be restarted in case it crashes e.g. due to time limit or hardware failure on a cluster. This is done by setting guess_type = chk in the subsequent calculation:

Response {
  guess_type = chk                      # Type of inital guess (none, chk, mw)
}

In this case the path_checkpoint must be the same as the previous calculation, as well as all other parameters in the calculation (Molecule and Basis in particular).

Write orbitals¶

The converged response orbitals can be saved to file with the write_orbitals keyword (defaults shown):

Response {
  path_orbitals = orbitals              # Path to orbital files
  write_orbitals = false                # Save converged orbitals to file
}

This will make individual files for each orbital under the path_orbitals directory. These orbitals can be used as starting point for subsequent calculations using the guess_type = mw initial guess:

Response {
  guess_prec = 1.0e-3                   # Numerical precision used in guess
  guess_type = mw                       # Type of inital guess (chk, mw, cube, core_XX, sad_XX)
}

Here the orbitals will be re-projected onto the current MW basis with precision guess_prec. We also need to specify the paths to the input files (only X for static perturbations, X and Y for dynamic perturbations):

Files {
  guess_X_p = initial_guess/X_p         # Path to paired MW orbitals
  guess_X_a = initial_guess/X_a         # Path to alpha MW orbitals
  guess_X_b = initial_guess/X_b         # Path to beta MW orbitals
  guess_Y_p = initial_guess/Y_p         # Path to paired MW orbitals
  guess_Y_a = initial_guess/Y_a         # Path to alpha MW orbitals
  guess_Y_b = initial_guess/Y_b         # Path to beta MW orbitals
}

Note that by default orbitals are written to the directory called orbitals but the mw guess reads from the directory initial_guess (this is to avoid overwriting the files by default). So, in order to use MW orbitals from a previous calculation, you must either change one of the paths (Response.path_orbitals or Files.guess_X_p etc), or manually copy the files between the default locations.

User input reference¶

Keywords without a default value are required.
Default values are either explicit or computed from the value of other keywords in the input.
Sections where all keywords have a default value can be omitted.
Predicates, if present, are the functions run to validate user input.

Keywords

world_prec

Overall relative precision in the calculation.

Type float

Predicates

1.0e-10 < value < 1.0

world_size

Total size of computational domain given as 2**(world_size). Always cubic and symmetric around the origin. Negative value means it will be computed from the molecular geometry.

Type int

Default -1

Predicates

value <= 10

world_unit

Length unit for all coordinates given in user input. Everything will be converted to atomic units (bohr) before the main executable is launched, so the JSON input is always given in bohrs.

Type str

Default bohr

Predicates

value.lower() in ["bohr", "angstrom"]

world_origin

Global gauge origin of the calculation.

Type List[float]

Default [0.0, 0.0, 0.0]

Predicates

len(value) == 3

Sections

Precisions

Define specific precision parameters.

Keywords

exchange_prec

Precision parameter used in construction of Exchange operators. Negative value means it will follow the dynamic precision in SCF.

Type float

Default -1.0

helmholtz_prec

Precision parameter used in construction of Helmholtz operators. Negative value means it will follow the dynamic precision in SCF.

Type float

Default -1.0

poisson_prec

Precision parameter used in construction of Poisson operators.

Type float

Default user['world_prec']

Predicates

1.0e-10 < value < 1.0

nuclear_prec

Precision parameter used in smoothing and projection of nuclear potential.

Type float

Default user['world_prec']

Predicates

1.0e-10 < value < 1.0

Printer

Define variables for printed output.

Keywords

print_level

Level of detail in the written output. Level 0 for production calculations, negative level for complete silence.

Type int

Default 0

print_mpi

Write separate output from each MPI to file called <file_name>-<mpi-rank>.out.

Type bool

Default False

print_prec

Number of digits in property output (energies will get twice this number of digits).

Type int

Default 6

Predicates

0 < value < 10

print_width

Line width of printed output (in number of characters).

Type int

Default 75

Predicates

50 < value < 100

print_constants

Print table of physical constants used by MRChem.

Type bool

Default False

Plotter

Give details regarding the density and orbital plots. Three types of plots are available, line, surface and cube, and the plotting ranges are defined by three vectors (A, B and C) and an origin (O): line: plots on line spanned by A, starting from O. surf: plots on surface spanned by A and B, starting from O. cube: plots on volume spanned by A, B and C, starting from O.

Keywords

path

File path to plot directory.

Type str

Default plots

Predicates

value[-1] != '/'

type

Type of plot: line (1D), surface (2D) or cube (3D).

Type str

Default cube

Predicates

value.lower() in ['line', 'surf', 'cube']

points

Number of points in each direction on the cube grid.

Type List[int]

Default [20, 20, 20]

Predicates

all(p > 0 for p in value)
not (user['Plotter']['type'] == 'line' and len(value) < 1)
not (user['Plotter']['type'] == 'surf' and len(value) < 2)
not (user['Plotter']['type'] == 'cube' and len(value) < 3)

O

Origin of plotting ranges.

Type List[float]

Default [0.0, 0.0, 0.0]

Predicates

len(value) == 3

A

First boundary vector for plot.

Type List[float]

Default [1.0, 0.0, 0.0]

Predicates

len(value) == 3

B

Second boundary vector for plot.

Type List[float]

Default [0.0, 1.0, 0.0]

Predicates

len(value) == 3

C

Third boundary vector for plot.

Type List[float]

Default [0.0, 0.0, 1.0]

Predicates

len(value) == 3

MPI

Define MPI related parameters.

Keywords

numerically_exact

This will use MPI algorithms that guarantees that the output is invariant wrt the number of MPI processes.

Type bool

Default False

shared_memory_size

Size (MB) of the MPI shared memory blocks of each shared function.

Type int

Default 10000

share_nuclear_potential

This will use MPI shared memory for the nuclear potential.

Type bool

Default False

share_coulomb_potential

This will use MPI shared memory for the Coulomb potential.

Type bool

Default False

share_xc_potential

This will use MPI shared memory for the exchange-correlation potential.

Type bool

Default False

bank_size

Number of MPI processes exclusively dedicated to manage orbital bank.

Type int

Default -1

Basis

Define polynomial basis.

Keywords

order

Polynomial order of multiwavelet basis. Negative value means it will be set automatically based on the world precision.

Type int

Default -1

type

Polynomial type of multiwavelet basis.

Type str

Default interpolating

Predicates

value.lower() in ['interpolating', 'legendre']

Derivatives

Define various derivative operators used in the code.

Keywords

kinetic

Derivative used in kinetic operator.

Type str

Default abgv_55

h_b_dip

Derivative used in magnetic dipole operator.

Type str

Default abgv_00

h_m_pso

Derivative used in paramagnetic spin-orbit operator.

Type str

Default abgv_00

Molecule

Define molecule.

Keywords

charge

Total charge of molecule.

Type int

Default 0

multiplicity

Spin multiplicity of molecule.

Type int

Default 1

Predicates

value > 0

translate

Translate coordinates such that center of mass coincides with the global gauge origin.

Type bool

Default False

coords

Coordinates in xyz format. Atoms can be given either using atom symbol or atom number

Type str

WaveFunction

Define the wavefunction method.

Keywords

method

Wavefunction method. See predicates for valid methods. hf, hartreefock and hartree-fock all mean the same thing, while lda is an alias for svwn5. You can set a non-standard DFT functional (e.g. varying the amount of exact exchange) by choosing dft and specifing the functional(s) in the DFT section below.

Type str

Predicates

value.lower() in ['core', 'hartree', 'hf', 'hartreefock', 'hartree-fock', 'dft', 'lda', 'svwn3', 'svwn5', 'pbe', 'pbe0', 'bpw91', 'bp86', 'b3p86', 'b3p86-g', 'blyp', 'b3lyp', 'b3lyp-g', 'olyp', 'kt1', 'kt2', 'kt3']

restricted

Use spin restricted wavefunction.

Type bool

Default True

environment

Set method for treatment of environment. none for vacuum calculation. PCM for Polarizable Continuum Model, which will activate the PCM input section for further parametrization options.

Type str

Default none

Predicates

value.lower() in ['none', 'pcm']

DFT

Define the exchange-correlation functional in case of DFT.

Keywords

density_cutoff

Hard cutoff for passing density values to XCFun.

Type float

Default 0.0

functionals

List of density functionals with numerical coefficient. E.g. for PBE0 EXX 0.25, PBEX 0.75, PBEC 1.0, see XCFun documentation <https://xcfun.readthedocs.io/>_.

Type str

Default `` ``

spin

Use spin separated density functionals.

Type bool

Default not(user['WaveFunction']['restricted'])

Properties

Provide a list of properties to compute (total SCF energy and orbital energies are always computed).

Keywords

dipole_moment

Compute dipole moment.

Type bool

Default True

quadrupole_moment

Compute quadrupole moment. Note: Gauge origin dependent, should be used with translate = true in Molecule.

Type bool

Default False

polarizability

Compute polarizability tensor.

Type bool

Default False

magnetizability

Compute magnetizability tensor.

Type bool

Default False

nmr_shielding

Compute NMR shielding tensor.

Type bool

Default False

geometric_derivative

Compute geometric derivative.

Type bool

Default False

plot_density

Plot converged electron density.

Type bool

Default False

plot_orbitals

Plot converged molecular orbitals from list of indices, negative index plots all orbitals.

Type List[int]

Default []

ExternalFields

Define external electromagnetic fields.

Keywords

electric_field

Strength of external electric field.

Type List[float]

Default []

Predicates

len(value) == 0 or len(value) == 3

Polarizability

Give details regarding the polarizability calculation.

Keywords

frequency

List of external field frequencies.

Type List[float]

Default [0.0]

NMRShielding

Give details regarding the NMR shileding calculation.

Keywords

nuclear_specific

Use nuclear specific perturbation operator (h_m_pso).

Type bool

Default False

nucleus_k

List of nuclei to compute. Negative value computes all nuclei.

Type List[int]

Default [-1]

Files

Defines file paths used for program input/output. Note: all paths must be given in quotes if they contain slashes “path/to/file”.

Keywords

guess_basis

File name for GTO basis set, used with gto guess.

Type str

Default initial_guess/mrchem.bas

guess_gto_p

File name for paired orbitals, used with gto guess.

Type str

Default initial_guess/mrchem.mop

guess_gto_a

File name for alpha orbitals, used with gto guess.

Type str

Default initial_guess/mrchem.moa

guess_gto_b

File name for beta orbitals, used with gto guess.

Type str

Default initial_guess/mrchem.mob

guess_phi_p

File name for paired orbitals, used with mw guess. Expected path is ``<path_orbitals>/phi_p_scf_idx_<0…Np>_<re/im>.mw

Type str

Default initial_guess/phi_p

guess_phi_a

File name for alpha orbitals, used with mw guess. Expected path is ``<path_orbitals>/phi_a_scf_idx_<0…Na>_<re/im>.mw

Type str

Default initial_guess/phi_a

guess_phi_b

File name for beta orbitals, used with mw guess. Expected path is ``<path_orbitals>/phi_b_scf_idx_<0…Nb>_<re/im>.mw

Type str

Default initial_guess/phi_b

guess_x_p

File name for paired response orbitals, used with mw guess. Expected path is ``<path_orbitals>/x_p_rsp_idx_<0…Np>_<re/im>.mw

Type str

Default initial_guess/X_p

guess_x_a

File name for alpha response orbitals, used with mw guess. Expected path is ``<path_orbitals>/x_a_rsp_idx_<0…Na>_<re/im>.mw

Type str

Default initial_guess/X_a

guess_x_b

File name for beta response orbitals, used with mw guess. Expected path is ``<path_orbitals>/x_b_rsp_idx_<0…Nb>_<re/im>.mw

Type str

Default initial_guess/X_b

guess_y_p

File name for paired response orbitals, used with mw guess. Expected path is ``<path_orbitals>/y_p_rsp_idx_<0…Np>_<re/im>.mw

Type str

Default initial_guess/Y_p

guess_y_a

File name for alpha response orbitals, used with mw guess. Expected path is ``<path_orbitals>/y_a_rsp_idx_<0…Na>_<re/im>.mw

Type str

Default initial_guess/Y_a

guess_y_b

File name for beta response orbitals, used with mw guess. Expected path is ``<path_orbitals>/y_b_rsp_idx_<0…Nb>_<re/im>.mw

Type str

Default initial_guess/Y_b

guess_cube_p

File name for paired orbitals, used with cube guess. Expected path is ``<path_orbitals>/phi_p_scf_idx_<0…Np>_<re/im>.cube

Type str

Default initial_guess/phi_p

guess_cube_a

File name for alpha orbitals, used with cube guess. Expected path is ``<path_orbitals>/phi_a>_scf_idx_<0…Na>_<re/im>.cube

Type str

Default initial_guess/phi_a

guess_cube_b

File name for beta orbitals, used with cube guess. Expected path is ``<path_orbitals>/phi_b_scf_idx_<0…Nb>_<re/im>.cube

Type str

Default initial_guess/phi_b

cube_vectors

Directory where cube vectors are stored for mrchem calculation.

Type str

Default cube_vectors/

SCF

Includes parameters related to the ground state SCF orbital optimization.

Keywords

run

Run SCF solver. Otherwise properties are computed on the initial orbitals.

Type bool

Default True

max_iter

Maximum number of SCF iterations.

Type int

Default 100

kain

Length of KAIN iterative history.

Type int

Default 5

rotation

Number of iterations between each diagonalization/localization.

Type int

Default 0

localize

Use canonical or localized orbitals.

Type bool

Default False

energy_thrs

Convergence threshold for SCF energy.

Type float

Default -1.0

guess_prec

Precision parameter used in construction of initial guess.

Type float

Default 0.001

Predicates

1.0e-10 < value < 1.0

guess_screen

Screening parameter used in GTO evaluations, in number of standard deviations. Every coordinate beyond N StdDev from the Gaussian center is evaluated to zero. Note that too aggressive screening is counter productive, because it leads to a sharp cutoff in the resulting function which requires higher grid refinement. Negative value means no screening.

Type float

Default 12.0

start_prec

Incremental precision in SCF iterations, initial value.

Type float

Default -1.0

final_prec

Incremental precision in SCF iterations, final value.

Type float

Default -1.0

guess_type

Type of initial guess for ground state orbitals. chk restarts a previous calculation which was dumped using the write_checkpoint keyword. This will load MRA and electron spin configuration directly from the checkpoint files, which are thus required to be identical in the two calculations. mw will start from final orbitals in a previous calculation written using the write_orbitals keyword. The orbitals will be re-projected into the new computational setup, which means that the electron spin configuration and MRA can be different in the two calculations. gto reads precomputed GTO orbitals (requires extra non-standard input files for basis set and MO coefficients). core and sad will diagonalize the Fock matrix in the given AO basis (SZ, DZ, TZ or QZ) using a Core or Superposition of Atomic Densities Hamiltonian, respectively.

Type str

Default sad_dz

Predicates

value.lower() in ['mw', 'chk', 'gto', 'core_sz', 'core_dz', 'core_tz', 'core_qz', 'sad_sz', 'sad_dz', 'sad_tz', 'sad_qz', 'sad_gto', 'cube']

write_checkpoint

Write orbitals to disk in each iteration, file name <path_checkpoint>/phi_scf_idx_<0..N>. Can be used as chk initial guess in subsequent calculations. Note: must be given in quotes if there are slashes in the path “path/to/checkpoint”.

Type bool

Default False

path_checkpoint

Path to checkpoint files during SCF, used with write_checkpoint and chk guess.

Type str

Default checkpoint

Predicates

value[-1] != '/'

write_orbitals

Write final orbitals to disk, file name <path_orbitals>/phi_<p/a/b>_scf_idx_<0..Np/Na/Nb>. Can be used as mw initial guess in subsequent calculations.

Type bool

Default False

path_orbitals

Path to where converged orbitals will be written in connection with the write_orbitals keyword. Note: must be given in quotes if there are slashes in the path “path/to/orbitals”.

Type str

Default orbitals

Predicates

value[-1] != '/'

orbital_thrs

Convergence threshold for orbital residuals.

Type float

Default 10 * user['world_prec']

Response

Includes parameters related to the response SCF optimization.

Keywords

run

In which Cartesian directions to run response solver.

Type List[bool]

Default [True, True, True]

max_iter

Maximum number of response iterations.

Type int

Default 100

kain

Length of KAIN iterative history.

Type int

Default 5

property_thrs

Convergence threshold for symmetric property. Symmetric meaning the property computed from the same operator as the response purturbation, e.g. for external magnetic field the symmetric property corresponds to the magnetizability (NMR shielding in non-symmetric, since one of the operators is external magnetic field, while the other is nuclear magnetic moment).

Type float

Default -1.0

start_prec

Incremental precision in SCF iterations, initial value.

Type float

Default -1.0

final_prec

Incremental precision in SCF iterations, final value.

Type float

Default -1.0

guess_prec

Precision parameter used in construction of initial guess.

Type float

Default 0.001

Predicates

1.0e-10 < value < 1.0

guess_type

Type of initial guess for response. none will start from a zero guess for the response functions. chk restarts a previous calculation which was dumped using the write_checkpoint keyword. mw will start from final orbitals in a previous calculation written using the write_orbitals keyword. The orbitals will be re-projected into the new computational setup.

Type str

Default none

Predicates

value.lower() in ['none', 'chk', 'mw']

write_checkpoint

Write perturbed orbitals to disk in each iteration, file name <path_checkpoint>/<X/Y>_rsp_<direction>_idx_<0..N>. Can be used as chk initial guess in subsequent calculations.

Type bool

Default False

path_checkpoint

Path to checkpoint files during SCF, used with write_checkpoint and chk guess.

Type str

Default checkpoint

Predicates

value[-1] != '/'

write_orbitals

Write final perturbed orbitals to disk, file name <path_orbitals>/<X/Y>_<p/a/b>_rsp_<direction>_idx_<0..Np/Na/Nb>. Can be used as mw initial guess in subsequent calculations.

Type bool

Default False

path_orbitals

Path to where converged orbitals will be written in connection with the write_orbitals keyword.

Type str

Default orbitals

Predicates

value[-1] != '/'

orbital_thrs

Convergence threshold for orbital residuals.

Type float

Default 10 * user['world_prec']

localize

Use canonical or localized unperturbed orbitals.

Type bool

Default user['SCF']['localize']

PCM

Includes parameters related to the computation of the reaction field energy of a system in an environment within the Polarizable Continuum Model.

Sections

SCRF

Parameters for the Self-Consistent Reaction Field optimization.

Keywords

max_iter

Max number of iterations allowed in the nested procedure.

Type int

Default 100

dynamic_thrs

Set the convergence threshold for the nested procedure. true will dynamically tighten the convergence threshold based on the absolute value of the latest orbital update as. When the orbitals are close to convergence (mo_residual < world_prec*10) the convergence threshold will be set equal to world_prec. false uses world_prec as convergence threshold throughout.

Type bool

Default True

optimizer

Choose which function to use in the KAIN solver, the surface charge density (gamma) or the reaction potential (V_R).

Type str

Default potential

Predicates

value.lower() in ['density', 'potential']

density_type

What part of the total molecular charge density to use in the algorithm. total uses the total charge density. nuclear uses only the nuclear part of the total charge density. electronic uses only the electronic part of the total charge density.

Type str

Default total

Predicates

value.lower() in ['total', 'nuclear', 'electronic']

kain

Number of previous reaction field iterates kept for convergence acceleration during the nested precedure.

Type int

Default user['SCF']['kain']

Cavity

Define the interlocking spheres cavity.

Keywords

mode

Determines how to set up the interlocking spheres cavity. atoms: centers are taken from the molecular geometry, radii taken from tabulated data (van der Waals radius), and rescaled using the parameters alpha, beta and sigma (R_i <- alpha*R_i + beta*sigma). Default spheres can be modified and/or extra spheres added, using the $spheres section, see documentation. explicit: centers and radii given explicitly in the spheres block.

Type str

Default atoms

Predicates

value.lower() in ['atoms', 'explicit']

spheres

This input parameter affects the list of spheres used to generate the cavity. In all cases, values for the radius, the radius scaling factor (alpha), the width (sigma), and the width scaling factor (beta) can be modified. If they are not specified their global default values are used. In atoms mode, we modify the default list of spheres, built with centers from the molecular geometry and radii from internal tabulated van der Waals values. To substitute a sphere, include a line like: $spheres i R [alpha] [beta] [sigma] $end to specify that the i atom in the molecule (0-based indexing) should use radius R instead of the pre-tabulated vdW radius. To add a sphere, include a line like: $spheres x y z R [alpha] [beta] [sigma] $end to specify that a sphere of radius R should be added at position (x, y, z). Spheres added in this way are not aware of their parent atom, if any. They will not contribute to the molecular gradient. In explicit mode, we build the complete sphere list from scratch. You can add a line like: $spheres x y z R [alpha] [beta] [sigma] $end to specify that a sphere of radius R should be added at position (x, y, z). Spheres added in this way are not aware of their parent atom, if any. They will not contribute to the molecular gradient. Alternatively, you can specify a line like: $spheres i R [alpha] [beta] [sigma] $end to specify that the i atom in the molecule (0-based indexing) should use radius R. Spheres added in this way are aware of their parent atom. They will contribute to the molecular gradient.

Type str

Default ````

alpha

Scaling factor on the radius term for the cavity rescaling (R_i <- alpha*R_i + beta*sigma). Only used for the default vdW radii in atoms mode, not if explicit $spheres are given.

Type float

Default 1.1

beta

Scaling factor on the boundary width term for the cavity rescaling (R_i <- alpha*R_i + beta*sigma). Only used for the default vdW radii in atoms mode, not if explicit $spheres are given.

Type float

Default 0.5

sigma

Width of cavity boundary, smaller value means sharper transition.

Type float

Default 0.2

Permittivity

Parameters for the permittivity function.

Keywords

epsilon_in

Permittivity inside the cavity. 1.0 is the permittivity of free space, anything other than this is undefined behaviour.

Type float

Default 1.0

epsilon_out

Permittivity outside the cavity. This is characteristic of the solvent used.

Type float

Default 1.0

formulation

Formulation of the Permittivity function. Currently only the exponential is used.

Type str

Default exponential

Predicates

value.lower() in ['exponential']

Constants

Physical and mathematical constants used by MRChem

Keywords

hartree2simagnetizability

Conversion factor for magnetizability from atomic units to SI units (unit: J T^-2). Affected code: Printed value of the magnetizability property.

Type float

Default 78.9451185

light_speed

Speed of light in atomic units (unit: au). Affected code: Relativistic Hamiltonians (ZORA, etc.)

Type float

Default 137.035999084

angstrom2bohrs

Conversion factor for Cartesian coordinates from Angstrom to Bohr (unit: Å^-1). Affected code: Parsing of input coordinates, printed coordinates

Type float

Default 1.8897261246257702

hartree2kjmol

Conversion factor from Hartree to kJ/mol (unit: kJ mol^-1). Affected code: Printed value of energies.

Type float

Default 2625.4996394798254

hartree2kcalmol

Conversion factor from Hartree to kcal/mol (unit: kcal mol^-1). Affected code: Printed value of energies.

Type float

Default 627.5094740630558

hartree2ev

Conversion factor from Hartree to eV (unit: ev). Affected code: Printed value of energies.

Type float

Default 27.211386245988

hartree2wavenumbers

Conversion factor from Hartree to wavenumbers (unit: cm^-1). Affected code: Printed value of frequencies.

Type float

Default 219474.6313632

fine_structure_constant

Fine-structure constant in atomic units (unit: au). Affected code: Certain magnetic interaction operators.

Type float

Default 0.0072973525693

electron_g_factor

Electron g factor in atomic units (unit: au). Affected code: Certain magnetic interaction operators.

Type float

Default -2.00231930436256

dipmom_au2debye

Conversion factor for dipoles from atomic units to Debye (unit: ?). Affected code: Printed value of dipole moments.

Type float

Default 2.5417464739297717

Running MRChem with QCEngine¶

MRChem >=1.0 can be used as a computational engine with the QCEngine program executor. QCEngine can be useful for running calculations on large sets of molecules and input parameters. The results are collected in standardised QCScheme format, which makes it easy to build post-processing pipelines and store data according to Findability, Accessibility, Interoperability, and Reuse (FAIR) of digital assets principles. Furthermore, QCEngine provides different geometry optimization drivers that can use the molecular gradient computed by MRChem for structural optimization.

Installation¶

The easiest way is to install both QCEngine and MRChem in a Conda environment using the precompiled version:

conda create -n mrchem-qcng mrchem qcengine qcelemental geometric optking pip -c conda-forge
conda activate mrchem-qcng
python -m pip install -U pyberny

It is also possible to use your own installation of MRChem: just make sure that the installation folder is in your PATH.

Note

If you want to use the precompiled, MPI-parallel version of MRChem with OpenMPI, install mrchem=*=*openmpi* insted of just mrchem. A binary package compiled against MPICH is also available: mrchem=*=*mpich*.

Single compute¶

Calculations in QCEngine are defined in Python scripts. For example, the following runs MRChem to obtain the energy of water:

import qcelemental as qcel
import qcengine as qcng


mol = qcel.models.Molecule(geometry=[[0, 0, 0], [0, 1.5, 0], [0, 0, 1.5]],
                           symbols=["O", "H", "H"],
                           connectivity=[[0, 1, 1], [0, 2, 1]])
print(mol)

computation = {
    "molecule": mol,
    "driver": "energy",
    "model": {"method": "HF"},
    "keywords": {"world_prec": 1.0e-3},
}
ret = qcng.compute(computation, "mrchem")

print(f"E_HF = {ret.return_result} Hartree")

You can save this sample as mrchem-run-hf.py and execute it with:

python mrchem-run-hf.py

Which will print to screen:

Molecule(name='H2O', formula='H2O', hash='b41d0c5')
E_HF = -75.9789291596064 Hartree

Note that:

The molecule is specified, in Angstrom, using a QCElemental object.
The computation is described using a Python dictionary.
The driver selects the kind of calculation you want to run with MRChem. Available drivers are:
- energy, for single-point energy calculations.
- gradient, for evaluation of the molecular gradient at a given geometry.
- properties, for the calculation of molecular properties.
The model selects the wavefunction: HF for Hartree-Fock and any of the DFT functionals known to MRChem for a corresponding DFT calculation.
The keywords key in the dictionary accepts a dictionary of MRChem options. Any of the options in the usual input file are recognized.

Once you have a dictionary defining your computation, you can run it with:

ret = qcng.compute(computation, "mrchem")

You can reuse the same dictionary with multiple computational engine, e.g. other quantum chemistry programs that are recognized as executors by QCEngine. The return value from the compute function contains all data produced during the calculation in QCSchema format including, for example, the execution time elapsed. The full JSON output produced by MRChem is also available and can be inspected in Python as:

mrchem_json_out = ret.extras["raw_output"]["output"]

The full, human-readable input is saved as the stdout property of the object returned by compute.

Parallelism¶

QCEngine allows you to exploit available parallel hardware. For example, to use 20 OpenMP threads in your MRChem calculation you would provide an additional task configuration dictionary as a task_config argument to compute:

ret = qcng.compute(
        computation,
        "mrchem",
        task_config={"ncores": 20})

You can inspect how the job was launched by printing out the provenance dictionary:

print(ret.extras["raw_output"]["output"]["provenance"])

{
 "creator": "MRChem",
 "mpi_processes": 1,
 "routine": "/home/roberto/miniconda3/envs/mrchem-qcng/bin/mrchem.x",
 "total_cores": 1,
 "version": "1.1.0",
 "ncores": 12,
 "nnodes": 1,
 "ranks_per_node": 1,
 "cores_per_rank": 12,
 "total_ranks": 1
}

It is also possible to run MPI-parallel and hybrid MPI+OpenMP jobs. Assuming that you installed the MPICH version of the MRChem MPI-parallel Conda package, the basic task_config argument to compute would look like:

task = {
  "nnodes": 1,  # number of nodes
  "ncores": 12,  # number of cores per task on each node
  "cores_per_rank": 6,  # number of cores per MPI rank
  "use_mpiexec": True,  # launch with MPI
  "mpiexec_command": "mpiexec -n {total_ranks}",  # the invocation of MPI
}

This task configuration will launch a MPI job with 2 ranks on a single node. Each rank has access to 6 cores for OpenMP parallelization. The provenance dictionary now shows:

{
 "creator": "MRChem",
 "mpi_processes": 2,
 "routine": "mpiexec -n 2 /home/roberto/miniconda3/envs/mrchem-qcng/bin/mrchem.x",
 "total_cores": 12,
 "version": "1.1.0",
 "ncores": 12,
 "nnodes": 1,
 "ranks_per_node": 2,
 "cores_per_rank": 6,
 "total_ranks": 2
}

The mpiexec_command is a string that will be interpolated to provide the exact invocation. In the above example, MRChem will be run with:

mpiexec -n 2 /home/roberto/miniconda3/envs/mrchem-qcng/bin/mrchem.x

The following interpolation parameters are understood by QCEngine when creating the MPI invocation:

{nnodes}: number of nodes.
{cores_per_rank}: number of cores to use for each MPI rank.
{ranks_per_node}: number of MPI ranks per node. Computed as ncores // cores_per_rank.
{total_ranks}: total number of MPI ranks. Computed as nnodes * ranks_per_node.

More complex MPI invocations are possible by setting the appropriate mpiexec_command in the task configuration. For usage with a scheduler, such as SLURM, you should refer to the documentation of your computing cluster and the documentation of QCEngine.

Geometry optimizations¶

Running geometry optimizations is just as easy as single compute. The following example optimizes the structure of water using the SVWN5 functional with MW4. The geomeTRIC package is used as optimization driver, but pyberny or optking would also work.

Warning

The computation of the molecular gradient can be affected by significant numerical noise for MW3 and MW4, to the point that it can be impossible to converge a geometry optimization. Using a tighter precision might help, but the cost of the calculation might be prohibitively large.

import qcelemental as qcel
import qcengine as qcng

mol =  qcel.models.Molecule(
    geometry=[
        [ 0.29127930, 3.00875625, 0.20308515],
        [-1.21253048, 1.95820900, 0.10303324],
        [ 0.10002049, 4.24958115,-1.10222079]
    ],
    symbols=["O", "H", "H"],
    fix_com=True,
    fix_orientation=True,
    fix_symmetry="c1")

opt_input =  {
    "keywords": {
        "program": "mrchem",
        "maxiter": 70
    },
    "input_specification": {
        "driver": "gradient",
        "model": {
            "method": "SVWN5",
        },
        "keywords": {
            "world_prec": 1.0e-4,
            "SCF": {
                "guess_type": "core_dz",
            }
        }
    },
    "initial_molecule": mol,
}

opt = qcng.compute_procedure(
        opt_input,
        "geometric",
        task_config={"ncores": 20})

print(opt.stdout)

print("==> Optimized geometry <==")
print(opt.final_molecule.pretty_print())

print("==> Optimized geometric parameters <==")
for m in [[0, 1], [0, 2], [1, 0, 2]]:
    opt_val = opt.final_molecule.measure(m)
    print(f"Internal degree of freedom {m} = {opt_val:.3f}")

Running this script will print all the steps taken during the structural optimization. The final printout contains the optimized geometry:

Geometry (in Angstrom), charge = 0.0, multiplicity = 1:

   Center              X                  Y                   Z
------------   -----------------  -----------------  -----------------
O                -4.146209038013     2.134923126314    -3.559202294678
H                -4.906566693905     1.536801624016    -3.587431156799
H                -4.270830051398     2.773072094238    -4.275607223691

and the optimized values of bond distances and bond angle:

Internal degree of freedom [0, 1] = 1.829
Internal degree of freedom [0, 2] = 1.828
Internal degree of freedom [1, 0, 2] = 106.549

Program input/output file¶

Input schema¶

"input": {
  "schema_name": string,                     # Name of the input schema
  "schema_version": int,                     # Version of the input schema
  "molecule": {                              # Section for Molecule specification
    "charge": int,                           # Total molecular charge
    "multiplicity": int,                     # Total spin multiplicity
    "coords": array[                         # Array of atoms
      {                                      # (one entry per atom)
        "atom": string,                      # Atomic symbol
        "xyz": array[float]                  # Nuclear Cartesian coordinate
      }
    ],
    "cavity": {
      "spheres": array[                      # Array of cavity spheres
        {                                    # (one entry per sphere)
          "center": array[float],            # Cartesian coordinate of sphere center
          "radius": float                    # Radius of cavity sphere
          "alpha": float                     # Scaling factor of radius
          "beta": float                      # Scaling factor of width
          "sigma": float                     # Width of cavity boundary
        }
      ],
    }
  },
  "mpi": {                                   # Section for MPI specification
    "bank_size": int,                        # Number of MPI ranks in memory bank
    "numerically_exact": bool,               # Guarantee MPI invariant results
    "shared_memory_size": int                # Size (MB) of MPI shared memory blocks
  },
  "mra": {                                   # Section for MultiResolution Analysis
    "basis_type": string,                    # Basis type (interpolating/legendre)
    "basis_order": int,                      # Polynomial order of basis
    "max_scale": int,                        # Maximum level of refinement
    "min_scale": int,                        # Minimum level of refinement (root scale)
    "boxes": array[int],                     # Number of root boxes
    "corner": array[int]                     # Translation of first root box
  },
  "printer": {                               # Section for printed output
    "file_name": string,                     # Name of output file
    "print_level": int,                      # Amount of printed output
    "print_mpi": bool,                       # Use separate output file for each MPI
    "print_prec": int,                       # Number of digits for printed output
    "print_width": int                       # Line width of printed output
  },
  "scf_calculation": {                       # Section for SCF specification
    "fock_operator": {                       # Contributions to Fock operator
      "kinetic_operator": {                  # Add Kinetic operator to Fock
        "derivative": string                 # Type of derivative operator
      },
      "nuclear_operator": {                  # Add Nuclear operator to Fock
        "proj_prec": float,                  # Projection prec for potential
        "smooth_prec": float,                # Smoothing parameter for potential
        "shared_memory": bool                # Use shared memory for potential
      },
      "coulomb_operator": {                  # Add Coulomb operator to Fock
        "poisson_prec": float,               # Build prec for Poisson operator
        "shared_memory": bool                # Use shared memory for potential
      },
      "exchange_operator": {                 # Add Exchange operator to Fock
        "poisson_prec": float,               # Build prec for Poisson operator
        "screen": bool                       # Use screening in Exchange operator
      },
      "reaction_operator": {                 # Add Reaction operator to Fock
        "poisson_prec": float,               # Precision for Poisson operator
        "kain": int,                         # Length of KAIN history in nested SCRF procedure
        "max_iter": int,                     # Maximum number of iterations in nested SCRF procedure
        "optimizer": string,                 # Use density or potential in KAIN solver
        "dynamic_thrs": bool,                # Use static or dynamic convergence threshold
        "density_type": string,              # Type of charge density [total, nuclear, electronic]
        "epsilon_in": float,                 # Permittivity inside the cavity
        "epsilon_out": float,                # Permittivity outside the cavity
        "formulation": string                # Formulation of the permittivity function
      },
      "xc_operator": {                       # Add XC operator to Fock
        "shared_memory": bool,               # Use shared memory for potential
        "xc_functional": {                   # XC functional specification
          "spin": bool,                      # Use spin separated functional
          "cutoff": float,                   # Cutoff value for small densities
          "functionals": array[              # Array of density functionals
            {
              "coef": float,                 # Numerical coefficient
              "name": string                 # Functional name
            }
          ]
        }
      },
      "external_operator": {                 # Add external field operator to Fock
        "electric_field": array[float],      # Electric field vector
        "r_O": array[float]                  # Gauge orgigin for electric field
      }
    },
    "initial_guess": {                       # Initial guess specification
      "type": string,                        # Type of initial guess
      "prec": float,                         # Precision for initial guess
      "zeta": int,                           # Zeta quality for AO basis
      "method": string,                      # Name of method for initial energy
      "localize": bool,                      # Use localized orbitals
      "restricted": bool,                    # Use spin restricted orbitals
      "relativity": string,                  # Name of relativistic method
      "screen": float,                       # Screening used in GTO evaluations
      "file_chk": string,                    # Path to checkpoint file
      "file_basis": string,                  # Path to GTO basis file
      "file_gto_a": string,                  # Path to GTO MO file (alpha)
      "file_gto_b": string,                  # Path to GTO MO file (beta)
      "file_gto_p": string,                  # Path to GTO MO file (paired)
      "file_phi_a": string,                  # Path to MW orbital file (alpha)
      "file_phi_b": string,                  # Path to MW orbital file (beta)
      "file_phi_p": string,                  # Path to MW orbital file (paired)
      "file_CUBE_a": str,                    # Path to CUBE orbital file (alpha)
      "file_CUBE_b": str,                    # Path to CUBE orbital file (beta)
      "file_CUBE_p": str                     # Path to CUBE orbital file (paired)
    },
    "scf_solver": {                          # SCF solver specification
      "kain": int,                           # Length of KAIN history
      "max_iter": int,                       # Maximum number of iterations
      "method": string,                      # Name of electronic structure method
      "relativity": string,                  # Name of relativistic method
      "rotation": int,                       # Iterations between localize/diagonalize
      "localize": bool,                      # Use localized orbitals
      "checkpoint": bool,                    # Save checkpoint file
      "file_chk": string,                    # Name of checkpoint file
      "start_prec": float,                   # Start precision for solver
      "final_prec": float,                   # Final precision for solver
      "helmholtz_prec": float,               # Precision for Helmholtz operators
      "orbital_thrs": float,                 # Convergence threshold orbitals
      "energy_thrs":float                    # Convergence threshold energy
    },
    "properties": {                          # Collection of properties to compute
      "dipole_moment": {                     # Collection of dipole moments
        id (string): {                       # Unique id: 'dip-${number}'
          "precision": float,                # Operator precision
          "operator": string,                # Operator used for property
          "r_O": array[float]                # Operator gauge origin
        }
      },
      "quadrupole_moment": {                 # Collection of quadrupole moments
        id (string): {                       # Unique id: 'quad-${number}'
          "precision": float,                # Operator precision
          "operator": string,                # Operator used for property
          "r_O": array[float]                # Operator gauge origin
        }
      },
      "geometric_derivative": {              # Collection of geometric derivatives
        id (string): {                       # Unique id: 'geom-${number}'
          "precision": float,                # Operator precision
          "operator": string,                # Operator used for property
          "smooth_prec": float               # Smoothing parameter for potential
        }
      }
    },
    "plots": {                               # Collection of plots to perform
      "density": bool,                       # Plot converged densities
      "orbitals": array[int],                # List of orbitals to plot
      "plotter": {                           # Section specifying plotting parameters
        "path": string,                      # Path to output files
        "type": string,                      # Type of plot (line, surf or cube)
        "points": array[int],                # Number of points in each direction
        "O": array[float],                   # Plotting range origin
        "A": array[float],                   # Plotting range A vector
        "B": array[float],                   # Plotting range B vector
        "C": array[float]                    # Plotting range C vector
    }
  },
  "rsp_calculations": {                      # Collection of response calculations
    id (string): {                           # Response id: e.g. 'ext_el-${frequency}'
      "dynamic": bool,                       # Use dynamic response solver
      "frequency": float,                    # Perturbation frequency
      "perturbation": {                      # Perturbation operator
        "operator": string                   # Operator used in response calculation
      },
      "components": array[                   # Array of perturbation components
        {                                    # (one per Cartesian direction)
          "initial_guess": {                 # Initial guess specification
            "type": string,                  # Type of initial guess
            "prec": float,                   # Precision for initial guess
            "file_chk_x": string,            # Path to checkpoint file for X
            "file_chk_y": string,            # Path to checkpoint file for Y
            "file_x_a": string,              # Path to MW file for X (alpha)
            "file_x_b": string,              # Path to MW file for X (beta)
            "file_x_p": string,              # Path to MW file for X (paired)
            "file_y_a": string,              # Path to MW file for Y (alpha)
            "file_y_b": string,              # Path to MW file for Y (beta)
            "file_y_p": string               # Path to MW file for Y (paired)
          },
          "rsp_solver": {                    # Response solver specification
            "kain": int,                     # Length of KAIN history
            "max_iter": int,                 # Maximum number of iterations
            "method": string,                # Name of electronic structure method
            "checkpoint": bool,              # Save checkpoint file
            "file_chk_x": string,            # Name of X checkpoint file
            "file_chk_y": string,            # Name of Y checkpoint file
            "orth_prec": float,              # Precision for orthogonalization
            "start_prec": float,             # Start precision for solver
            "final_prec": float,             # Final precision for solver
            "helmholtz_prec": float,         # Precision for Helmholtz operators
            "orbital_thrs": float,           # Convergence threshold orbitals
            "property_thrs": float           # Convergence threshold property
          }
        }
      ],
      "properties": {                        # Collection of properties to compute
        "polarizability": {                  # Collection of polarizabilities
           id (string): {                    # Unique id: 'pol-${frequency}'
            "precision": float,              # Operator precision
            "operator": string,              # Operator used for property
            "r_O": array[float]              # Operator gauge origin
          }
        },
        "magnetizability": {                 # Collection of magnetizabilities
          id (string): {                     # Unique id: 'mag-${frequency}'
            "frequency": float,              # Perturbation frequency
            "precision": float,              # Operator precision
            "dia_operator": string,          # Operator used for diamagnetic property
            "para_operator": string,         # Operator used for paramagnetic property
            "derivative": string,            # Operator derivative type
            "r_O": array[float]              # Operator gauge origin
          }
        },
        "nmr_shielding": {                   # Collection of NMR shieldings
          id (string): {                     # Unique id: 'nmr-${nuc_idx}${atom_symbol}'
            "precision": float,              # Operator precision
            "dia_operator": string,          # Operator used for diamagnetic property
            "para_operator": string,         # Operator used for paramagnetic property
            "derivative": string,            # Operator derivative type
            "smoothing": float,              # Operator smoothing parameter
            "r_O": array[float],             # Operator gauge origin
            "r_K": array[float]              # Nuclear coordinate
          }
        }
      },
      "fock_operator": {                     # Contributions to perturbed Fock operator
        "coulomb_operator": {                # Add Coulomb operator to Fock
          "poisson_prec": float,             # Build prec for Poisson operator
          "shared_memory": bool              # Use shared memory for potential
        },
        "exchange_operator": {               # Add Exchange operator to Fock
          "poisson_prec": float,             # Build prec for Poisson operator
          "screen": bool                     # Use screening in Exchange operator
        },
        "xc_operator": {                     # Add XC operator to Fock
          "shared_memory": bool,             # Use shared memory for potential
          "xc_functional": {                 # XC functional specification
            "spin": bool,                    # Use spin separated functional
            "cutoff": float,                 # Cutoff value for small densities
            "functionals": array[            # Array of density functionals
              {
                "coef": float,               # Numerical coefficient
                "name": string               # Functional name
              }
            ]
          }
        }
      },
      "unperturbed": {                       # Section for unperturbed part of response
        "prec": float,                       # Precision used for unperturbed system
        "localize": bool,                    # Use localized unperturbed orbitals
        "fock_operator": {                   # Contributions to unperturbed Fock operator
          "kinetic_operator": {              # Add Kinetic operator to Fock
            "derivative": string             # Type of derivative operator
          },
          "nuclear_operator": {              # Add Nuclear operator to Fock
            "proj_prec": float,              # Projection prec for potential
            "smooth_prec": float,            # Smoothing parameter for potential
            "shared_memory": bool            # Use shared memory for potential
          },
          "coulomb_operator": {              # Add Coulomb operator to Fock
            "poisson_prec": float,           # Build prec for Poisson operator
            "shared_memory": bool            # Use shared memory for potential
          },
          "exchange_operator": {             # Add Exchange operator to Fock
            "poisson_prec": float,           # Build prec for Poisson operator
            "screen": bool                   # Use screening in Exchange operator
          },
          "xc_operator": {                   # Add XC operator to Fock
            "shared_memory": bool,           # Use shared memory for potential
            "xc_functional": {               # XC functional specification
              "spin": bool,                  # Use spin separated functional
              "cutoff": float,               # Cutoff value for small densities
              "functionals": array[          # Array of density functionals
                {
                  "coef": float,             # Numerical coefficient
                  "name": string             # Functional name
                }
              ]
            }
          },
          "external_operator": {             # Add external field operator to Fock
            "electric_field": array[float],  # Electric field vector
            "r_O": array[float]              # Gauge orgigin for electric field
          }
        }
      }
    }
  },
  "constants": {                             # Physical constants used throughout MRChem
    "angstrom2bohrs": float,                 # Conversion factor from Angstrom to Bohr
    "dipmom_au2debye": float,                # Conversion factor from atomic units to Debye
    "electron_g_factor": float,              # Electron g factor in atomic units
    "fine_structure_constant": float,        # Fine-structure constant in atomic units
    "hartree2ev": float,                     # Conversion factor from Hartree to eV
    "hartree2kcalmol": float,                # Conversion factor from Hartree to kcal/mol
    "hartree2kjmol": float,                  # Conversion factor from Hartree to kJ/mol
    "hartree2simagnetizability": float,      # Conversion factor from Hartree to J T^-2
    "hartree2wavenumbers": float,            # Conversion factor from Hartree to cm^-1
    "light_speed": float                     # Speed of light in vacuo in atomic units
  }
}

Output schema¶

"output": {
  "success": bool,                           # Whether all requested calculations succeeded
  "schema_name": string,                     # Name of the output schema
  "schema_version": int,                     # Version of the output schema
  "provenance": {                            # Information on how the results were obtained
    "creator": string,                       # Program name
    "version": string,                       # Program version
    "nthreads": int,                         # Number of OpenMP threads used
    "mpi_processes": int,                    # Number of MPI processes used
    "total_cores": int,                      # Total number of cores used
    "routine": string                        # The function that generated the output
  },
  "properties": {                            # Collection of final properties
    "charge": int,                           # Total molecular charge
    "multiplicity": int,                     # Total spin multiplicity
    "center_of_mass": array[float],          # Center of mass coordinate
    "geometry": array[                       # Array of atoms
      {                                      # (one entry per atom)
        "symbol": string,                    # Atomic symbol
        "xyz": array[float]                  # Cartesian coordinate
      }
    ],
    "orbital_energies": {                    # Collection of orbital energies
      "spin": array[string],                 # Array of spins ('p', 'a' or 'b')
      "energy": array[float],                # Array of energies
      "occupation": array[int],              # Array of orbital occupations
      "sum_occupied": float                  # \sum_i occupation[i]*energy[i]
    },
    "scf_energy": {                          # Collection of energy contributions
      "E_kin": float,                        # Kinetic energy
      "E_nn": float,                         # Classical nuclear-nuclear interaction
      "E_en": float,                         # Classical electron-nuclear interaction
      "E_ee": float,                         # Classical electron-electron interaction
      "E_next": float,                       # Classical nuclear-external field interaction
      "E_eext": float,                       # Classical electron-external field interaction
      "E_x": float,                          # Hartree-Fock exact exchange energy
      "E_xc": float,                         # DFT exchange-correlation energy
      "E_el": float,                         # Sum of electronic contributions
      "E_nuc": float,                        # Sum of nuclear contributions
      "E_tot": float,                        # Sum of all contributions
      "Er_el": float,                        # Electronic reaction energy
      "Er_nuc": float,                       # Nuclear reaction energy
      "Er_tot": float                        # Sum of all reaction energy contributions
    },
    "dipole_moment": {                       # Collection of electric dipole moments
      id (string): {                         # Unique id: 'dip-${number}'
        "r_O": array[float],                 # Gauge origin vector
        "vector": array[float],              # Total dipole vector
        "vector_el": array[float],           # Electronic dipole vector
        "vector_nuc": array[float],          # Nuclear dipole vector
        "magnitude": float                   # Magnitude of total vector
      }
    },
    "quadrupole_moment": {                   # Collection of electric quadrupole moments
      id (string): {                         # Unique id: 'quad-${number}'
        "r_O": array[float],                 # Gauge origin vector
        "tensor": array[float],              # Total quadrupole tensor
        "tensor_el": array[float],           # Electronic quadrupole tensor
        "tensor_nuc": array[float]           # Nuclear quadrupole tensor
      }
    },
    "polarizability": {                      # Collection of polarizabilities
      id (string): {                         # Unique id: 'pol-${frequency}'
        "frequency": float,                  # Perturbation frequency
        "r_O": array[float],                 # Gauge origin vector
        "tensor": array[float],              # Full polarizability tensor
        "isotropic_average": float           # Diagonal average
      }
    },
    "magnetizability": {                     # Collection of magnetizability
      id (string): {                         # Unique id: 'mag-${frequency}'
        "frequency": float,                  # Perturbation frequency
        "r_O": array[float],                 # Gauge origin vector
        "tensor": array[float],              # Full magnetizability tensor
        "tensor_dia": array[float],          # Diamagnetic tensor
        "tensor_para": array[float],         # Paramagnetic tensor
        "isotropic_average": float           # Diagonal average
      }
    },
    "nmr_shielding": {                       # Collection of NMR shielding tensors
      id (string): {                         # Unique id: 'nmr-${nuc_idx}+${atom_symbol}'
        "r_O": array[float],                 # Gauge origin vector
        "r_K": array[float],                 # Nuclear coordinate vector
        "tensor": array[float],              # Full NMR shielding tensor
        "tensor_dia": array[float],          # Diamagnetic tensor
        "tensor_para": array[float],         # Paramagnetic tensor
        "diagonalized_tensor": array[float], # Diagonalized tensor used for (an)isotropy
        "isotropic_average": float,          # Diagonal average
        "anisotropy": float                  # Anisotropy of tensor
      }
    },
    "geometric_derivative": {                # Collection of geometric derivatives
      id (string): {                         # Unique id: 'geom-${number}'
        "electronic": array[float],          # Electronic component of the geometric derivative
        "electronic_norm": float,            # Norm of the electronic component of the geoemtric derivative
        "nuclear": array[float],             # Nuclear component of the geometric derivative
        "nuclear_norm": float,               # Norm of the nuclear component of the geometric derivative
        "total": array[float],               # Geometric derivative
        "total_norm": float                  # Norm of the geometric derivative
      }
    }
  },
  "scf_calculation": {                       # Ground state SCF calculation
    "success": bool,                         # SCF finished successfully
    "initial_energy": {                      # Energy computed from initial orbitals
      "E_kin": float,                        # Kinetic energy
      "E_nn": float,                         # Classical nuclear-nuclear interaction
      "E_en": float,                         # Classical electron-nuclear interaction
      "E_ee": float,                         # Classical electron-electron interaction
      "E_next": float,                       # Classical nuclear-external field interaction
      "E_eext": float,                       # Classical electron-external field interaction
      "E_x": float,                          # Hartree-Fock exact exchange energy
      "E_xc": float,                         # DFT exchange-correlation energy
      "E_el": float,                         # Sum of electronic contributions
      "E_nuc": float,                        # Sum of nuclear contributions
      "E_tot": float,                        # Sum of all contributions
      "Er_el": float,                        # Electronic reaction energy
      "Er_nuc": float,                       # Nuclear reaction energy
      "Er_tot": float                        # Sum of all reaction energy contributions
    },
    "scf_solver": {                          # Details from SCF optimization
      "converged": bool,                     # Optimization converged
      "wall_time": float,                    # Wall time (sec) for SCF optimization 
      "cycles": array[                       # Array of SCF cycles
        {                                    # (one entry per cycle)
          "energy_total": float,             # Current total energy
          "energy_update": float,            # Current energy update
          "mo_residual": float,              # Current orbital residual
          "wall_time": float,                # Wall time (sec) for SCF cycle
          "energy_terms": {                  # Energy contributions
            "E_kin": float,                  # Kinetic energy
            "E_nn": float,                   # Classical nuclear-nuclear interaction
            "E_en": float,                   # Classical electron-nuclear interaction
            "E_ee": float,                   # Classical electron-electron interaction
            "E_next": float,                 # Classical nuclear-external field interaction
            "E_eext": float,                 # Classical electron-external field interaction
            "E_x": float,                    # Hartree-Fock exact exchange energy
            "E_xc": float,                   # DFT exchange-correlation energy
            "E_el": float,                   # Sum of electronic contributions
            "E_nuc": float,                  # Sum of nuclear contributions
            "E_tot": float,                  # Sum of all contributions
            "Er_el": float,                  # Electronic reaction energy
            "Er_nuc": float,                 # Nuclear reaction energy
            "Er_tot": float                  # Sum of all reaction energy contributions
          }
        }
      ]
    }
  },
  "rsp_calculations": {                      # Collection of response calculations
    id (string): {                           # Response id: e.g. 'ext_el-${frequency}'
      "success": bool,                       # Response finished successfully
      "frequency": float,                    # Frequency of perturbation
      "perturbation": string,                # Name of perturbation operator
      "components": array[                   # Array of operator components
        {                                    # (one entry per Cartesian direction)
          "rsp_solver": {                    # Details from response optimization
            "wall_time": float,              # Wall time (sec) for response calculation
            "converged": bool,               # Optimization converged
            "cycles": array[                 # Array of response cycles
              {                              # (one entry per cycle)
                "symmetric_property": float, # Property computed from perturbation operator
                "property_update": float,    # Current symmetric property update
                "mo_residual": float,        # Current orbital residual
                "wall_time": float           # Wall time (sec) for response cycle
              }
            ]
          }
        }
      ]
    }
  }
}

Programmer’s Manual¶

Classes and functions reference¶

Chemistry¶

Classes for the chemistry overlay

Environment¶

Classes for the solvent environment overlay

Cavity¶

class Cavity : public mrcpp::RepresentableFunction<3>¶

Interlocking spheres cavity centered on the nuclei of the molecule. The Cavity class represents the following function Fosso-Tande2013.

\[\begin{split} C(\mathbf{r}) = 1 - \prod^N_{i=1} (1-C_i(\mathbf{r})) \\ C_i(\mathbf{r}) = 1 - \frac{1}{2}\left( 1 + \textrm{erf}\left(\frac{|\mathbf{r} - \mathbf{r}_i| - R_i}{\sigma_i}\right) \right) \end{split}\]

where $\mathbf{r}$ is the coordinate of a point in 3D space, $\mathbf{r}_i$ is the coordinate of the i-th nucleus, $R_i$ is the radius of the i-th sphere, and $\sigma_i$ is the width of the transition between the inside and outside of the cavity. The transition has a sigmoidal shape, such that the boundary is a smooth function instead of sharp boundaries often seen in other continuum models. This function is $1$ inside and $0$ outside the cavity.

The radii are computed as:

\[ R_{i} = \alpha_{i} R_{0,i} + \beta_{i}\sigma_{i} \]

where:

$R_{0,i}$ is the atomic radius. By default, the van der Waals radius.
$\alpha_{i}$ is a scaling factor. By default, 1.1
$\beta_{i}$ is a width scaling factor. By default, 0.5
$\sigma_{i}$ is the width. By default, 0.2

Public Functions

Cavity(const std::vector<mrcpp::Coord<3>> &coords, const std::vector<double> &R, const std::vector<double> &alphas, const std::vector<double> &betas, const std::vector<double> &sigmas)¶: Initializes the members of the class and constructs the analytical gradient vector of the Cavity.

Cavity(const std::vector<mrcpp::Coord<3>> &coords, const std::vector<double> &R, double sigma)¶

Initializes the members of the class and constructs the analytical gradient vector of the Cavity.

This CTOR applies a single width factor to the cavity and does not modify the radii. That is, in the formula:

\[ R_{i} = \alpha_{i} R_{0,i} + \beta_{i}\sigma_{i} \]

for every atom $i$, $\alpha_{i} = 1.0$ and $\beta_{i} = 0.0$.

double evalf(const mrcpp::Coord<3> &r) const override¶

Evaluates the value of the cavity at a 3D point $\mathbf{r}$.

Parameters: r – coordinate of 3D point at which the Cavity is to be evaluated at.
Returns: double value of the Cavity at point $\mathbf{r}$

inline std::vector<mrcpp::Coord<3>> getCoordinates() const¶: Returns centers.

inline std::vector<double> getOriginalRadii() const¶: Returns radii_0.

inline std::vector<double> getRadii() const¶: Returns radii.

inline std::vector<double> getRadiiScalings() const¶: Returns alphas.

inline std::vector<double> getWidths() const¶: Returns sigmas.

inline std::vector<double> getWidthScalings() const¶: Returns betas.

Protected Attributes

std::vector<double> radii_0¶: Contains the unscaled radius of each sphere in #Center.

std::vector<double> alphas¶: The radius scaling factor for each sphere.

std::vector<double> betas¶: The width scaling factor for each sphere.

std::vector<double> sigmas¶: The width for each sphere.

std::vector<double> radii¶: Contains the radius of each sphere in #Center. $R_i = \alpha_{i} R_{0,i} + \beta_{i}\sigma_{i}$.

std::vector<mrcpp::Coord<3>> centers¶: Contains each of the spheres centered on the nuclei of the Molecule.

auto gradCavity(const mrcpp::Coord<3> &r, int index, const std::vector<mrcpp::Coord<3>> &centers, const std::vector<double> &radii, const std::vector<double> &widths) -> double¶

Constructs a single element of the gradient of the Cavity.

This constructs the analytical partial derivative of the Cavity $C$ with respect to $x$, $y$ or $z$ coordinates and evaluates it at a point $\mathbf{r}$. This is given for $x$ by

\[ \frac{\partial C\left(\mathbf{r}\right)}{\partial x} = \left(1 - C{\left(\mathbf{r} \right)}\right) \sum_{i=1}^{N} - \frac{\left(x-{x}_{i}\right)e^{- \frac{\operatorname{s_{i}}^{2}{\left(\mathbf{r} \right)}}{\sigma^{2}}}} {\sqrt{\pi}\sigma\left(0.5 \operatorname{erf}{\left(\frac{\operatorname{s_{i}}{\left(\mathbf{r} \right)}}{\sigma} \right)} + 0.5\right) \left| \mathbf{r} - \mathbf{r}_{i} \right|} \]

where the subscript $i$ is the index related to each sphere in the cavity, and $\operatorname{s}$ is the signed normal distance from the surface of each sphere.

Parameters

r – The coordinates of a test point in 3D space.
index – An integer that defines the variable of differentiation (0->x, 1->z and 2->z).
centers – A vector containing the coordinates of the centers of the spheres in the cavity.
radii – A vector containing the radii of the spheres.
width – A double value describing the width of the transition at the boundary of the spheres.

Returns

A double number which represents the value of the differential (w.r.t. x, y or z) at point r.

Permittivity¶

class Permittivity : public mrcpp::RepresentableFunction<3>¶

Permittivity function related to a substrate molecule and a solvent continuum. The Permittivity class represents the following function Fosso-Tande2013

\[ \epsilon(\mathbf{r}) = \epsilon_{in}\exp\left(\left(\log\frac{\epsilon_{out}}{\epsilon_{in}} \right) \left(1 - C(\mathbf{r})\right)\right) \]

where $\mathbf{r}$ is the coordinate of a point in 3D space, $ C $ is the cavity function of the substrate, and $\epsilon_{in}$ and $ \epsilon_{out} $ are the dielectric constants describing, respectively, the permittivity inside and outside the cavity of the substrate.

Public Functions

Permittivity(const Cavity cavity, double epsilon_in, double epsilon_out, std::string formulation)¶

Standard constructor. Initializes the cavity, epsilon_in and epsilon_out with the input parameters.

Parameters

cavity – interlocking spheres of Cavity class.
epsilon_in – permittivity inside the cavity.
epsilon_out – permittivity outside the cavity.
formulation – Decides which formulation of the Permittivity function to implement, only exponential available as of now.

double evalf(const mrcpp::Coord<3> &r) const override¶

Evaluates Permittivity at a point in 3D space with respect to the state of inverse.

Parameters: r – coordinates of a 3D point in space.
Returns: $\frac{1}{\epsilon(\mathbf{r})}$ if inverse is true, and $ \epsilon(\mathbf{r})$ if inverse is false.

inline void flipFunction(bool is_inverse)¶: Changes the value of inverse.

inline auto isInverse() const¶: Returns the current state of inverse.

inline auto getCoordinates() const¶: Calls the Cavity::getCoordinates() method of the cavity instance.

inline auto getRadii() const¶: Calls the Cavity::getRadii() method of the cavity instance.

inline auto getGradVector() const¶: Calls the Cavity::getGradVector() method of the cavity instance.

inline auto getEpsIn() const¶: Returns the value of epsilon_in.

inline auto getEpsOut() const¶: Returns the value of epsilon_out.

inline Cavity getCavity() const¶: Returns the cavity.

inline std::string getFormulation() const¶: Returns the formulation.

void printParameters() const¶: Print parameters.

Private Members

bool inverse = false¶: State of evalf.

double epsilon_in¶: Dielectric constant describing the permittivity of free space.

double epsilon_out¶: Dielectric constant describing the permittivity of the solvent.

std::string formulation¶: Formulation of the permittivity function, only exponential is used as of now.

Cavity cavity¶: A Cavity class instance.

SCRF¶

class SCRF¶

class that performs the computation of the ReactionPotential, named Self Consistent Reaction Field.

Private Members

mrcpp::FunctionTreeVector<3> d_cavity¶: Vector containing the 3 partial derivatives of the cavity function.

Initial Guess¶

Classes providing the initial guess of the orbitals

Properties¶

Classes for the calculation of molecular properties

Quantum Mechanical Functions¶

Classes to handle quantum mechanical functions such as electronic density, molecular orbitals.

QMOperators¶

The classes that implement quantum mechanical operators

QMPotential¶

class QMPotential¶

Operator defining a multiplicative potential.

Inherits the general features of a complex function from QMFunction and implements the multiplication of this function with an Orbital. The actual function representing the operator needs to be implemented in the derived classes, where the *re and *im FunctionTree pointers should be assigned in the setup() function and deallocated in the clear() function.

XCOperator¶

class XCOperator¶

DFT Exchange-Correlation operator containing a single XCPotential.

This class is a simple TensorOperator realization of

XCPotential¶

class XCPotential¶

Exchange-Correlation potential defined by a particular (spin) density.

The XC potential is computed by mapping of the density through a XC functional, provided by the XCFun library. There are two ways of defining the density:

1) Use getDensity() prior to setup() and build the density as you like. 2) Provide a default set of orbitals in the constructor that is used to compute the density on-the-fly in setup().

If a set of orbitals has NOT been given in the constructor, the density MUST be explicitly computed prior to setup(). The density will be computed on-the-fly in setup() ONLY if it is not already available. After setup() the operator will be fixed until clear(), which deletes both the density and the potential.

LDA and GGA functionals are supported as well as two different ways to compute the XC potentials: either with explicit derivatives or gamma-type derivatives.

ReactionPotential¶

class ReactionPotential : public mrchem::QMPotential¶

class containing the solvent-substrate interaction reaction potential obtained by solving

\[ \Delta V_{R} = -4\pi\left( \rho\frac{1-\epsilon}{\epsilon} + \gamma_s \right) \]

where $\rho$ is the total molecular density of a solute molecule, $\epsilon$ is the Permittivity function of the continuum and $\gamma_s$ is the surface charge distribution.

Public Functions

ReactionPotential(std::unique_ptr<SCRF> scrf_p, std::shared_ptr<mrchem::OrbitalVector> Phi_p)¶

Initializes the ReactionPotential class.

Parameters

scrf_p – A SCRF instance which contains the parameters needed to compute the ReactionPotential.
Phi_p – A pointer to a vector which contains the orbitals optimized in the SCF procedure.

inline void updateMOResidual(double const err_t)¶: Updates the helper.mo_residual member variable. This variable is used to set the convergence criterion in the dynamic convergence method.

Private Members

std::unique_ptr<SCRF> helper¶: A SCRF instance used to compute the ReactionPotential.

std::shared_ptr<mrchem::OrbitalVector> Phi¶: holds the Orbitals needed to compute the electronic density for the SCRF procedure.

SCF Solver¶

Classes for the resolution of the SCF equations of HF and DFT