AMSification of ADF¶
Restructuring of the input¶
The input for the following features belongs (mostly) to the AMS driver part of the input:
-
Geometry
Total charge
Masses of atoms (isotopes)
Electric field, point charges
Regions
Structure and Reactivity, Molecular Dynamics
Geometry Optimizations
Linear Transit (LT), Transition States (TS), Nudged Elastic Band (NEB), TSRC
Intrinsic Reaction Coordinate (IRC)
Constraints, restraints
Excited state optimizations
Molecular Dynamics
Gradients, Hessian, Thermodynamics
Nuclear gradients, Hessian, PES point character
Thermodynamics, gas phase Gibbs free energy
-
IR frequencies and intensities
Mobile Block Hessian (MBH), Mode Scanning, Mode Refinement, Mode Tracking
(Resonance) Raman, vibrational Raman optical activity (VROA)
Vibrational Circular Dichroism (VCD)
Vibrational resolved electronic spectra
Vibrational resolved absorption, emission, phosphorescence, ionization
Adiabatic Hessian Franck-Condon
Vertical Gradient Franck-Condon
The input for QM/MM, QM/QM, Quild calculations uses the Hybrid engine
Model Hamiltonians
The input for most other features belongs to the ADF engine part of the input.
Restructuring of input keys¶
ADF2019 key / feature |
ADF2020 key / AMS2020 key / comments |
---|---|
$ADFBIN |
$AMSBIN |
$ADFHOME |
$AMSHOME |
$ADFRESOURCES |
$AMSRESOURCES=$AMSHOME/atomicdata |
$ADFHOME/atomicdata |
$AMSHOME/atomicdata/ADF. Directory with ADF basis sets. |
$ADFHOME/atomicdata/ZORA |
$AMSHOME/atomicdata/ADF/ZORA. Directory with ADF ZORA basis sets. |
‘ANALYTICALFREQ’ |
subkey ‘NormalModes’ of key ‘Properties’ in AMS driver. |
‘AORESPONSE’ |
subkey ‘FreqRange’ and ‘Frequency’ removed. Use new subkey ‘Frequencies’. |
‘ATOMPROPS’ |
key removed. See alternative elements. |
‘ATOMS’ |
subkey ‘Atoms’ of key ‘System’ in AMS driver. |
… f=fragtype/n |
… adf.f=fragtype|n. |
… R=CosmoRadius |
… adf.R=CosmoRadius. |
‘CHARGE’ |
subkey ‘Charge’ of key ‘System’ in AMS driver. key ‘SpinPolarization’ in ADF. |
‘CONSTRAINTS’ |
key ‘Constraints’ in AMS driver. |
‘COLLINEAR’ |
subkey ‘SpinOrbitMagnetization Collinear’ in key ‘Relativity’ in ADF. |
‘CRDFILEXYZ’ |
key removed. |
‘CRDFILEMOL’ |
key removed. |
EField |
subkey ‘ElectroStaticEmbedding%ElectricField’ of key ‘System’ in AMS driver. |
fcf |
program ‘fcf’ documented in AMS driver |
‘GEOMETRY’ |
key ‘Task’ and key ‘Properties’ in AMS driver. |
Geometry optimization |
key ‘Task GeometryOptimization’ in AMS driver. |
‘GEOVAR’ |
key removed. |
‘GRADIENT’ |
subkey ‘Gradients’ of key ‘Properties’ in AMS driver. |
‘HESSDIAG’ |
key removed. |
‘HESSTEST’ |
key removed. |
Initial Hessian |
subkey ‘InitialHessian’ of key ‘GeometryOptimization’ in AMS driver. |
Intrinsic Reaction Coordinate |
key ‘Task IRC’ in AMS driver. |
IR frequencies |
subkey ‘NormalModes’ of key ‘Properties’ in AMS driver. |
… Mobile Block Hessian |
subkey ‘Displacements Block’ of key ‘NormalModes’ in AMS driver. |
… symmetric displacements |
subkey ‘Displacements Symmetric’ of key ‘NormalModes’ in AMS driver. |
‘IRCSTART’ |
key removed. |
‘ISOTOPICSHIFT’ |
key removed. |
Linear Transit |
key ‘Task PESScan’ in AMS driver. |
‘LINEARCONSTRAINTS’ |
key removed. |
MBH |
subkey ‘Displacements Block’ of key ‘NormalModes’ in AMS driver. |
‘MP2’ |
key ‘MBPT’. |
‘NONCOLLINEAR’ |
subkey ‘SpinOrbitMagnetization NonCollinear’ in key ‘Relativity’ in ADF. |
Nudged Elastic Band |
key ‘Task NEB’ in AMS driver. |
Partial Hessian |
subkey ‘SelectedRegionForHessian’ and ‘NormalModes’ of key ‘Properties’ in AMS driver. |
‘POINTCHARGES’ |
subkey ‘ElectroStaticEmbedding%MultipolePotential’ of key ‘System’ in AMS driver. |
‘POLTDDFT’ |
subkey ‘NFreq’ and ‘NGrid’ added. |
‘QMMM’ |
|
QM/MM; QM/QM; Quild |
|
Raman |
subkey ‘Raman’ of key ‘Properties’ in AMS driver. |
‘RELATIVISTIC’ |
block key ‘Relativity’ in ADF. |
‘RESPONSE’ |
subkey ‘FrqBeg’, ‘FrqEnd, and ‘NFreq’ removed. Use new subkey ‘Frequencies’. |
‘RESTRAINT’ |
key ‘Restraints’ in AMS driver. |
‘Restart’ |
The file should be specified in ‘EngineRestart’ in AMS driver |
‘SYMMETRY’ |
both in ADF and AMS driver. |
symmetrization |
ADF does not symmetrize anymore. Subkey ‘Symmetrize’ of key ‘System’ in AMS driver. |
‘THERMO’ |
key ‘Thermo’ in AMS driver. |
Transit State search |
key ‘Task TransitionStateSearch’ in AMS driver. |
‘UNITS’ |
key removed. Possibility added to add units for many keys. |
VCD |
subkey ‘VCD’ of key ‘Properties’ in AMS driver. |
vcdtools |
program ‘vcdtools’ documented in AMS driver |
VIBRON module |
VIBRON module removed. For resonance Raman application see AMS driver. |
VROA |
subkey ‘VROA’ of key ‘Properties’ in AMS driver. |
Example shell script changes¶
The example below shows how a shell script for ADF2019 is converted to ADF2020 (see also Automatic tool for conversion of ADF2019 shell scripts).
ADF2019 shell script (obsolete):
#!/bin/sh
# This is a shell script for ADF2019 which will not work for ADF2020
$ADFBIN/adf <<eor
Title WATER Geometry Optimization
Atoms
O 0.000000 0.000000 0.000000
H 0.000000 -0.689440 -0.578509
H 0.000000 0.689440 -0.578509
End
Geometry
Converge grad=1e-4
End
Basis
Type TZP
End
XC
GGA PBE
End
eor
ADF2020 shell script:
#!/bin/sh
# This is a shell script for ADF2020
# You should use '$ADFBIN/ams' instead of '$ADFBIN/adf'
$ADFBIN/ams <<eor
# Input options for the AMS driver:
System
Atoms
O 0.000000 0.000000 0.000000
H 0.000000 -0.689440 -0.578509
H 0.000000 0.689440 -0.578509
End
End
Task GeometryOptimization
GeometryOptimization
Convergence gradients=1e-4
End
# The input options for ADF, which are described in this manual,
# should be specified in the 'Engine ADF' block:
Engine ADF
Basis
Type TZP
End
XC
GGA PBE
End
EndEngine
eor
Automatic tool for conversion of ADF2019 shell scripts¶
The executable $AMSBIN/adf
no longer performs ADF calculations. Instead, it will call an input-conversion tool [1] which will automatically convert an ADF2019 input into an ADF2020 input.
For example, if you save and execute the following script (note that the $AMSBIN/adf
executable is used):
#!/bin/sh
# This is a shell scripts of an ADF2019 calculation, which will not work for ADF2020
# If you execute this script, the ADF2019 input will be converted into an ADF2020 input.
$AMSBIN/adf <<eor
Atoms
O 0.000000 0.000000 0.000000
H 0.000000 -0.689440 -0.578509
H 0.000000 0.689440 -0.578509
End
Basis
Type TZP
End
eor
no ADF calculation will actually be performed. Instead, the input conversion tool will be called, and you will obtain the new shell script for ADF2020 (note the $AMSBIN/ams
executable):
# =========
# IMPORTANT
# =========
# Starting from AMS2020, ADF can only be used through the AMS driver program.
# Many input options for ADF have changed since the 2019 version.
# Below you will find an automatically-converted input script for AMS2020.
# The automatic conversion is not 100% accurate, so double check your input!
# ==================================================
# Automatic conversion of ADF-2019 input to AMS-2020
# ==================================================
# === NOTES ===
# - "TAPE21" is now called "adf.rkf" and is located in AMS results folder (by default "ams.results")
# - Unlike ADF2019, AMS does not symmetrize the structure by default. See "System -> Symmetrize" in the AMS driver manual.
# - The AMS default symmetrization tolerance is larger than the ADF2019 one. See "Symmetry -> SymmetrizeTolerance" in the AMS driver manual.
# - Scalar relativistic effects (ZORA) are included by default in the 2020 version of ADF.
$AMSBIN/ams << eor
System
Atoms
O 0.0000000000 0.0000000000 0.0000000000
H 0.0000000000 -0.6894400000 -0.5785090000
H 0.0000000000 0.6894400000 -0.5785090000
End
Symmetrize True
End
Symmetry
SymmetrizeTolerance 0.001
End
Engine ADF
Relativity
Level None
End
Basis
Type TZP
End
EndEngine
eor
The conversion tool might raise WARNINGS
. Make sure to address them before using the converted the script!
Input, execution and output¶
See the AMS driver documentation:
ADF specific files¶
The ADF engine may generate several output / result files, along that ADF writes part of the standard output file. The most important one is adf.rkf (previously ADF<=2019 known as TAPE21 or as a .t21 file), the general result file. The adf.rkf contains relevant information about the outcome of the calculation. It is a binary file that contains a lot of information about the calculation, such as the one-electron orbitals expressed in the basis functions. It can be used as a fragment file for subsequent calculations, or can be used as input to a property program, like NMR, CPL, or LFDFT.
Files attached to the job, such as fragment files, are by default also assumed to exist in the directory where you start AMS. You must take care to move or copy required files to that directory before starting the calculation, or to provide via input adequate information to the program where to find the files. In many cases you can specify a complete path to the file.
Most files that are generated by the program, in particular the standard result file that can be used as a fragment file in other calculations, are binary files. A binary file should usually not be moved from one machine to another, i.e. it may not be readable by another machine than the one that generated the file, unless the two machines are of the same type. The ADF package provides utilities to convert the ADF binary result files from binary to ASCII, and vice versa, so that you don’t have to regenerate your fragment libraries when going to another machine. See the Scripting Section for further details regarding such aspects.
ADF is an engine that lends itself particularly well for chemical analysis. This is a direct result of the fragment-based approach, where properties of the molecule are related to the properties of the constituent fragments, which is precisely how the chemist thinks. Molecular Orbitals are (optionally) analyzed extensively as how they are composed from occupied and virtual fragment orbitals. This inherently implies a large amount of output. Even computations on small molecules may produce startlingly many pages of output. This is not necessarily so because you can regulate the production of output in detail. Obviously, some kind of default production of output had to be implemented. The field of ADF users is so wide and diverse that it is hard to satisfy everybody as regards this default level of output. Depending on your purposes the automatic settings, which determine how much output is generated without instructions to the contrary, may yield boringly many numbers that you just skip through in search for the one value you’re interested in, or it may be widely insufficient. Therefore, take notice of the possibilities to regulate output.
Above all, however get familiar with the analysis tools that ADF provides to see in what ways these may help to interpret your results. In a later chapter a global description of output is given as it is normally produced. The chapter below gives an introduction in some of the essential features of ADF, which may be sufficiently different from what you are used to in other Quantum Chemistry codes to deserve your attention.