pert (c49b1)
Free Energy Perturbation Calculations
The PERTurb command allows the scaling of energy between PSFs for use in
energy analysis, comparisons, slow growth free energy simulations,
widowing free energy simulation, and for slow growth homology modelling.
This is a rather flexible implementation of free energy perturbation
that allows connectivity to change. Also, three energy restraint
terms (harmonic, dihedral and NOE) and the SKIP command flags are subject
to change which allows a flexible way in which to compute free energy
differences between different conformations. This code in implemented
in a non-intrusive manner and works with all minimizers and
integrators. SHAKE can now be applied to bonds which are mutated as
well; an appropriate constraint corrections is calculated
automatically in these cases.
LOOKup tables can be used with PERT, provided that it is only used for
the non-perturbed part of the system:
define pertatm sele ... end
energy ....
lookup sele resn tip3 .and. .not. pertatm end NOUU NOVU ENERGY
pert sele pertatm end
* Syntax | Syntax of PERT Commands
* Description | Description of PERT Commands
* Restrictions | Restrictions in PERT Command usage
* References | References regarding Free Energy Perturbations
* Examples | A Sample Input Files
* Constraints | Special considerations regarding SHAKE
* WHAM::
* PERT/PSSP | Background on the use of soft core potentials (PSSP)
* PATCH::
* PERT/MMFP | MMFP in PERT
* CHEMical PERT | Easier setup of alchemical simulations of "chemical paths"
* LRCorrection | Preliminary support of LJ long-range corrections
The PERTurb command allows the scaling of energy between PSFs for use in
energy analysis, comparisons, slow growth free energy simulations,
widowing free energy simulation, and for slow growth homology modelling.
This is a rather flexible implementation of free energy perturbation
that allows connectivity to change. Also, three energy restraint
terms (harmonic, dihedral and NOE) and the SKIP command flags are subject
to change which allows a flexible way in which to compute free energy
differences between different conformations. This code in implemented
in a non-intrusive manner and works with all minimizers and
integrators. SHAKE can now be applied to bonds which are mutated as
well; an appropriate constraint corrections is calculated
automatically in these cases.
LOOKup tables can be used with PERT, provided that it is only used for
the non-perturbed part of the system:
define pertatm sele ... end
energy ....
lookup sele resn tip3 .and. .not. pertatm end NOUU NOVU ENERGY
pert sele pertatm end
* Syntax | Syntax of PERT Commands
* Description | Description of PERT Commands
* Restrictions | Restrictions in PERT Command usage
* References | References regarding Free Energy Perturbations
* Examples | A Sample Input Files
* Constraints | Special considerations regarding SHAKE
* WHAM::
* PERT/PSSP | Background on the use of soft core potentials (PSSP)
* PATCH::
* PERT/MMFP | MMFP in PERT
* CHEMical PERT | Easier setup of alchemical simulations of "chemical paths"
* LRCorrection | Preliminary support of LJ long-range corrections
Top
Syntax of Free Energy Perturbation Commands
[Syntax PERT]
PERTurb [OFF] [INBFrq int nonbond-specs] [RESEt] [MMFP] soft-core-spec
atom-selection [INBFrq 0] [CHEM]
[QMMM]
soft-core-spec::= [SCL0 SCR0 real] [SCL1 SCR1 real]
The PERT OFF command disables the free energy routines and the current
(lambda=1) PSF is used for subsequent commands.
When OFF is not specified, this command saves the current PSF as the lambda=0
state. The atom-selection indicated which atoms have changed. This is to
make the calculation run more efficiently. If only a small percent of the
atoms have changed, this doubles the performance. The nonbond specs are
included to make sure the nonbond exclusion lists are properly setup. This
then allows the connectivity to change during the simulation. INBFrq should
not be set to zero here unless the exclusion lists have already been setup
in a previous command.
Adding the MMFP keyword signals that the user intends to
change MMFP restraints as part of an alchemical
transformation. If it is omitted, the MMF-potentials are used as constant
energy terms as was the case in CHARMM versions up to c30a2(x).
The soft-core-spec specifies whether the shift-based soft-core potential
applies to the the simulations. The soft-core only applies on the
repulsive part (as defined by the WCA separation) of the Lennard-Jones
potential. To get meaningful free energy, the soft-core potential
only is to be used when the electrostatic and WCA attractive
interaction between the selected atoms and the rest of the system are
turned off by using the scalar CHARGE and WCAD. There are two sets
of parameters that correspond to the energy evaluation
in the initial and final state. SCL0 specifies that soft-core
potential is used for the initial state. SCR0 is the
corresponding parameter that controls the strength of the soft-core
potential for the initial state. SCL1 and SCR0 are the corresponding
values for the final state. When SCR? equals to zero, all WCA repulsive
interaction of the selected atoms is off. When SCR? equals to one,
full WCA repulsive interaction of the selected atoms is on.
A typical usage of the soft-core potential is to compute the free energy
from non-interaction state to repulsively interaction state for
a given selection of atoms. The simulation can be conducted with
a serious of Widom insertion/deletion stages. The following values
of the SCR? are typical to perform the simulation in stages.
SCR0 SCR1
1. 0 0.2
2. 0.2 0.3
3. 0.3 0.4
4. 0.4 0.5
5. 0.5 0.6
6. 0.6 0.7
7. 0.7 0.8
8. 0.8 0.9
9. 0.9 1.0
Because of the number of stages, the repulsive potential change in
each stage is so small that a single Widom insertion or deletion
(the sampling is done at the two end points, no intermediate windows
required) is sufficient for the free energy in each stages.
Notice this implementation of soft-core potential only works
with FEP or WHAM (exponential average). Once the selected atoms
interact with the rest of the system with full repulsion, it is
straightforward to compute free energy contributions from
WCA attraction and electrostatics. For details,
see Deng Y. and Roux B., J. Phys. Chem. B, 108 (42) 16567-16576
The WCA separation is implemented for
group based slow (fast off) vdW routine,
atom based slow routine with distance switch cutoff (fast off),
group based fast (fast gene) vdW routine and
atom based fast (fast gene) vdW energy with distance switch cutoff.
The QMMM keyword indicates that the QM atoms will be perturbed into MM atoms.
This works for SCCDFTB only at this point.
Also, when part of the QM region is perturbed into MM atoms, a different setup
is used (scc sccdftb.info). See examples below.
----------------------------------------------------------------------------
ENERgy ... [ RESET ] [ free-energy-step-spec ]
DYNAmics ... [ PUNIt integer ] [WHAM integer]
MINImize ...
[ RESET ] ! Resets all all accumulation data and counters.
(automatic for the first PERT or after a PERT OFF command)
free-energy-step-spec::=
[PWINdow [LAMBda real] ] [PSTArt int] [PSTOp int] [LSTArt real] [LSTOp real] -
[PSLOwgrowth ]
[PINCrement int] [PEQUilibrate int] [LAVErage] [LINCrement real]
[PWINdow ] ! specifies the windowing algorithm (default)
[PSLOwgrowth] ! specifies the slow growth algorithm
[LAMBda real] ! specifies the lambda value for windowing methods or for
energy or minimization calculations.
[PSTArt int] ! starting dynamics step number for accumulation (default 1)
[PSTOp int] ! ending dynamics step number for accumulation (default 0)
[LSTArt real] ! specifies the starting lambda value (default 0.0)
[LSTOp real] ! specifies the final lambda value (default 1.0)
[PINCrement int] ! specifies number of steps to next window (auto mode).
[PEQUil int] ! specifies number of steps for equilibration (auto mode).
[LAVErage] ! specifies that lambda = (LSTART+LSTOP)/2 (auto mode).
[LINCrement] ! Specifies the lambda increment between windows (auto mode).
[LEXP] ! Specifies the lambda exponential increment constant (auto mode).
[PSSP] ! use soft core potentials for interactions in reac.
! and product list. This option is remembered. With
! the PSSP keyword, two parameters, ALAM and DLAM can
! be set.
[ALAM real] ! Separation parameter for elec. interaction (defaults to 5A^2)
[DLAM real] ! Separation parameter for LJ interaction (defaults to 5A^2)
[NOPSsp] ! Turn off use of soft core interactions.
[ END ] ! Turns off the free energy code
The PSTArt and PSTOp values are relative to the number of dynamics steps
since PERT command was first enabled, or if a PERT RESET command is used
(regardless of whether the DYNAmics commands is run more than once or
whether the dynamic run involved the use of restart files).
By specifying the auto mode parameters (PINCrement, PEQUilibrate, LINCrement, LEXP),
a new window will start at the conclusion of the current window with modified
parameters. Also, in auto mode, the run will terminate at the end of a window
where LAMBDA reaches the LSTOP value.
The auto mode can be specified in DYNAmic input line by LINC and/or LEXP.
The range of LAMBDA is defined by LSTA (default 0) and LSTOP (default 1).
When LEXP is set to 0, linear windows of LAMBDA will be defined between LSTA
and LSTOP. When LEXP>0 (suggested value:3.5 for transiting to dummy atoms),
the windows will exponentially approch LSTOP. When LEXP<0 (suggested
value: -3.5 for transiting from dummy atoms), the windows will
exponentially approach LSTA. Number of windows is defined by (LSTOP-LSTA)/LINC+1.
LSTA can be smaller or larger than LSTOP. LINC must be positive when LSTA<LSTOP,
or negative when LSTA>LSTOP. Dynamic simulation steps, NSTEP, should be equal to
or larger than PINC*((LSTOP-LSTA)/LINC+1). The auto mode will be turned off or
redefined when PUNIT is set.
The exponential distribution of LAMBDA windows are designed for the double
exponential (DE) VDW potential. DE potential has no signularity and is
convenient for free energy calculation. To properly sample the repulsive core
region, it is recommanded to use the expoential LAMBDA windows specified
by LEXP. Alternatively, a soft core implementation is implmented in PSSP.
With PSSP, DE potential free energy can be calculated with linear distribution
of LAMBDA windows with LEXP=0. Detailed description of DE softcore can be
found in the PSSP section.
The new commands PSSP/NOPSsp and the optional parameters ALAM and DLAM
control the interactions between soft core potentials and PERT. After
you specify PSSP in an energy, minimization or Dynamics command, soft
core LJ and elec. interactions are used in all reactant and product
nonbonded list terms. The separation parameters for elec. and LJ
interactions can be set with the ALAM and DLAM options, the default of
5A^2 should be reasonable. The option is remembered, i.e., after the
first invocation of PSSP all further calls to EPERT use soft core
interactions. To turn this off, use the NOPSsp keyword. Use of
softcore interactions is also turned off after a PERT RESEt or a PERT
OFF command. For example (assuming that PERT has been already set
up):
ENER LAMB 0.5 ! calc. system energy for L=0.5
ENER LAMB 0.5 PSSP ! calc. system energy for L=0.5 using soft core potentials
ENER LAMB 0.6 ! calc. system energy for L=0.6 using soft core potentials
! since the PSSP option is remembered
ENER LAMB 0.6 NOPS ! calc. system energy for L=0.6, use of soft
! core pots. turned off.
The PERT/PSSP code supports only thermodynamic integration and slow-growth.
Please ignore all results starting with TP> when using PSSP.
The PUNIt option allows the free-energy-step-spec to be specified
more than once and acts as a scheduler for a particular simulation.
The format of the PUNIt file is;
* title
repeat-lines-of(free-energy-step-specs)
END
The end is optional and terminates the free energy run.
Lack of an END (i.e. and end-of-file or blank lines) will put PERT into
auto mode which will continue until LSTOP becomes 1.0 or 0.0 (based on
the LINCrement value).
The WHAM option allows to write a formatted file to post-process with
the Weighted Histogram Analysis Method (see below).
Syntax of Free Energy Perturbation Commands
[Syntax PERT]
PERTurb [OFF] [INBFrq int nonbond-specs] [RESEt] [MMFP] soft-core-spec
atom-selection [INBFrq 0] [CHEM]
[QMMM]
soft-core-spec::= [SCL0 SCR0 real] [SCL1 SCR1 real]
The PERT OFF command disables the free energy routines and the current
(lambda=1) PSF is used for subsequent commands.
When OFF is not specified, this command saves the current PSF as the lambda=0
state. The atom-selection indicated which atoms have changed. This is to
make the calculation run more efficiently. If only a small percent of the
atoms have changed, this doubles the performance. The nonbond specs are
included to make sure the nonbond exclusion lists are properly setup. This
then allows the connectivity to change during the simulation. INBFrq should
not be set to zero here unless the exclusion lists have already been setup
in a previous command.
Adding the MMFP keyword signals that the user intends to
change MMFP restraints as part of an alchemical
transformation. If it is omitted, the MMF-potentials are used as constant
energy terms as was the case in CHARMM versions up to c30a2(x).
The soft-core-spec specifies whether the shift-based soft-core potential
applies to the the simulations. The soft-core only applies on the
repulsive part (as defined by the WCA separation) of the Lennard-Jones
potential. To get meaningful free energy, the soft-core potential
only is to be used when the electrostatic and WCA attractive
interaction between the selected atoms and the rest of the system are
turned off by using the scalar CHARGE and WCAD. There are two sets
of parameters that correspond to the energy evaluation
in the initial and final state. SCL0 specifies that soft-core
potential is used for the initial state. SCR0 is the
corresponding parameter that controls the strength of the soft-core
potential for the initial state. SCL1 and SCR0 are the corresponding
values for the final state. When SCR? equals to zero, all WCA repulsive
interaction of the selected atoms is off. When SCR? equals to one,
full WCA repulsive interaction of the selected atoms is on.
A typical usage of the soft-core potential is to compute the free energy
from non-interaction state to repulsively interaction state for
a given selection of atoms. The simulation can be conducted with
a serious of Widom insertion/deletion stages. The following values
of the SCR? are typical to perform the simulation in stages.
SCR0 SCR1
1. 0 0.2
2. 0.2 0.3
3. 0.3 0.4
4. 0.4 0.5
5. 0.5 0.6
6. 0.6 0.7
7. 0.7 0.8
8. 0.8 0.9
9. 0.9 1.0
Because of the number of stages, the repulsive potential change in
each stage is so small that a single Widom insertion or deletion
(the sampling is done at the two end points, no intermediate windows
required) is sufficient for the free energy in each stages.
Notice this implementation of soft-core potential only works
with FEP or WHAM (exponential average). Once the selected atoms
interact with the rest of the system with full repulsion, it is
straightforward to compute free energy contributions from
WCA attraction and electrostatics. For details,
see Deng Y. and Roux B., J. Phys. Chem. B, 108 (42) 16567-16576
The WCA separation is implemented for
group based slow (fast off) vdW routine,
atom based slow routine with distance switch cutoff (fast off),
group based fast (fast gene) vdW routine and
atom based fast (fast gene) vdW energy with distance switch cutoff.
The QMMM keyword indicates that the QM atoms will be perturbed into MM atoms.
This works for SCCDFTB only at this point.
Also, when part of the QM region is perturbed into MM atoms, a different setup
is used (scc sccdftb.info). See examples below.
----------------------------------------------------------------------------
ENERgy ... [ RESET ] [ free-energy-step-spec ]
DYNAmics ... [ PUNIt integer ] [WHAM integer]
MINImize ...
[ RESET ] ! Resets all all accumulation data and counters.
(automatic for the first PERT or after a PERT OFF command)
free-energy-step-spec::=
[PWINdow [LAMBda real] ] [PSTArt int] [PSTOp int] [LSTArt real] [LSTOp real] -
[PSLOwgrowth ]
[PINCrement int] [PEQUilibrate int] [LAVErage] [LINCrement real]
[PWINdow ] ! specifies the windowing algorithm (default)
[PSLOwgrowth] ! specifies the slow growth algorithm
[LAMBda real] ! specifies the lambda value for windowing methods or for
energy or minimization calculations.
[PSTArt int] ! starting dynamics step number for accumulation (default 1)
[PSTOp int] ! ending dynamics step number for accumulation (default 0)
[LSTArt real] ! specifies the starting lambda value (default 0.0)
[LSTOp real] ! specifies the final lambda value (default 1.0)
[PINCrement int] ! specifies number of steps to next window (auto mode).
[PEQUil int] ! specifies number of steps for equilibration (auto mode).
[LAVErage] ! specifies that lambda = (LSTART+LSTOP)/2 (auto mode).
[LINCrement] ! Specifies the lambda increment between windows (auto mode).
[LEXP] ! Specifies the lambda exponential increment constant (auto mode).
[PSSP] ! use soft core potentials for interactions in reac.
! and product list. This option is remembered. With
! the PSSP keyword, two parameters, ALAM and DLAM can
! be set.
[ALAM real] ! Separation parameter for elec. interaction (defaults to 5A^2)
[DLAM real] ! Separation parameter for LJ interaction (defaults to 5A^2)
[NOPSsp] ! Turn off use of soft core interactions.
[ END ] ! Turns off the free energy code
The PSTArt and PSTOp values are relative to the number of dynamics steps
since PERT command was first enabled, or if a PERT RESET command is used
(regardless of whether the DYNAmics commands is run more than once or
whether the dynamic run involved the use of restart files).
By specifying the auto mode parameters (PINCrement, PEQUilibrate, LINCrement, LEXP),
a new window will start at the conclusion of the current window with modified
parameters. Also, in auto mode, the run will terminate at the end of a window
where LAMBDA reaches the LSTOP value.
The auto mode can be specified in DYNAmic input line by LINC and/or LEXP.
The range of LAMBDA is defined by LSTA (default 0) and LSTOP (default 1).
When LEXP is set to 0, linear windows of LAMBDA will be defined between LSTA
and LSTOP. When LEXP>0 (suggested value:3.5 for transiting to dummy atoms),
the windows will exponentially approch LSTOP. When LEXP<0 (suggested
value: -3.5 for transiting from dummy atoms), the windows will
exponentially approach LSTA. Number of windows is defined by (LSTOP-LSTA)/LINC+1.
LSTA can be smaller or larger than LSTOP. LINC must be positive when LSTA<LSTOP,
or negative when LSTA>LSTOP. Dynamic simulation steps, NSTEP, should be equal to
or larger than PINC*((LSTOP-LSTA)/LINC+1). The auto mode will be turned off or
redefined when PUNIT is set.
The exponential distribution of LAMBDA windows are designed for the double
exponential (DE) VDW potential. DE potential has no signularity and is
convenient for free energy calculation. To properly sample the repulsive core
region, it is recommanded to use the expoential LAMBDA windows specified
by LEXP. Alternatively, a soft core implementation is implmented in PSSP.
With PSSP, DE potential free energy can be calculated with linear distribution
of LAMBDA windows with LEXP=0. Detailed description of DE softcore can be
found in the PSSP section.
The new commands PSSP/NOPSsp and the optional parameters ALAM and DLAM
control the interactions between soft core potentials and PERT. After
you specify PSSP in an energy, minimization or Dynamics command, soft
core LJ and elec. interactions are used in all reactant and product
nonbonded list terms. The separation parameters for elec. and LJ
interactions can be set with the ALAM and DLAM options, the default of
5A^2 should be reasonable. The option is remembered, i.e., after the
first invocation of PSSP all further calls to EPERT use soft core
interactions. To turn this off, use the NOPSsp keyword. Use of
softcore interactions is also turned off after a PERT RESEt or a PERT
OFF command. For example (assuming that PERT has been already set
up):
ENER LAMB 0.5 ! calc. system energy for L=0.5
ENER LAMB 0.5 PSSP ! calc. system energy for L=0.5 using soft core potentials
ENER LAMB 0.6 ! calc. system energy for L=0.6 using soft core potentials
! since the PSSP option is remembered
ENER LAMB 0.6 NOPS ! calc. system energy for L=0.6, use of soft
! core pots. turned off.
The PERT/PSSP code supports only thermodynamic integration and slow-growth.
Please ignore all results starting with TP> when using PSSP.
The PUNIt option allows the free-energy-step-spec to be specified
more than once and acts as a scheduler for a particular simulation.
The format of the PUNIt file is;
* title
repeat-lines-of(free-energy-step-specs)
END
The end is optional and terminates the free energy run.
Lack of an END (i.e. and end-of-file or blank lines) will put PERT into
auto mode which will continue until LSTOP becomes 1.0 or 0.0 (based on
the LINCrement value).
The WHAM option allows to write a formatted file to post-process with
the Weighted Histogram Analysis Method (see below).
Top
Description of PERT Commands
The PERTurb command copies and saves the current PSF and restraint
data for harmonic, NOE and dihedral restraints to the initial (lambda=0)
saved state. The SKIP command flags are also saved to allow linear scaling
of entire energy terms.
The structure may then be modified or perturbed with patches,
SCALar commands, with the DELEte command, or by generating or reading
a new PSF.
The Basic mode of operation is;
....
PERTurb ! Define the lambda=0 state.
PATCH .... ! Define the lambda=1 state.
DYNAmics .... ! Run MD on intermediate surface...
....
The PSF in use when dynamics or energy minimization is invoked
becomes the final (lambda=1) state. The actual energy computed
is a linear combination of these two endpoints.
The PATCH command may be replaced with any other command that
modifies the PSF. Some examples which modify the PSF;
SCALAR CHARGE SET -0.55 SELE ATOM A 1 O* SHOW END ! change a charge
DELETE ATOM SELE ALL END
READ SEQUENCE ....
GENERATE ... ! generate a new different PSF.
DELETE CONNECTIVITY .... ! modify the PSF by changing the connectivity.
! see a word of warning below!
SCALAR TYPE SET 14 SELE ATOM A 1 O SHOW END ! change the vdw atom type
OPEN .... ! Read a new PSF
READ PSF ...
It is not required that the PSF be modified. If one wants to
carry out coordinate perturbation only, it is sufficient to modify
the harmonic restraints, the NOE restraints, or the dihedral restraints.
In this way, it is possible to calculate the free energy differences
between different conformers. (However, this option should not be
used with simultaneous change of SHAKE constraints)
Note that with this implementation, because two PSFs are used,
that the connectivity may change. The use of 1-4 interactions and
nonbond exclusions is fully supported. This allows this method to be
used for examining changes that involve bond changes, such as cystine
bridge formation. [Note added by Stefan Boresch (stefan@mdy.univie.ac.at)
Changes in connectivity that involve bond breaking or forming are
highly problematic and may not converge. This is explained in
detail in Boresch & Karplus, J. Phys. Chem. B 1999, 103, 103-136.
The flexibility made possible by the implementation of PERT puts
the responsibility of what can be done and what not on the user!]
The advanced mode of operation is;
....
PERTurb
PATCH ....
DYNAmics ....
....
PERTurb
PATCH ....
DYNAmics ....
....
PERTurb
PATCH ....
DYNAmics ....
....
In this way, several changes can be affected in a single CHARMM run.
For example, the first patch might be the removal of charges, and the
second patch could correspond to a change in atom size, and the third
patch could simply consist of modifying dihedral restraints so as to
affect a conformational change. The free energy differences and
fluctuations will be calculated for each window as well as the total
for all previous windows.
Description of PERT Commands
The PERTurb command copies and saves the current PSF and restraint
data for harmonic, NOE and dihedral restraints to the initial (lambda=0)
saved state. The SKIP command flags are also saved to allow linear scaling
of entire energy terms.
The structure may then be modified or perturbed with patches,
SCALar commands, with the DELEte command, or by generating or reading
a new PSF.
The Basic mode of operation is;
....
PERTurb ! Define the lambda=0 state.
PATCH .... ! Define the lambda=1 state.
DYNAmics .... ! Run MD on intermediate surface...
....
The PSF in use when dynamics or energy minimization is invoked
becomes the final (lambda=1) state. The actual energy computed
is a linear combination of these two endpoints.
The PATCH command may be replaced with any other command that
modifies the PSF. Some examples which modify the PSF;
SCALAR CHARGE SET -0.55 SELE ATOM A 1 O* SHOW END ! change a charge
DELETE ATOM SELE ALL END
READ SEQUENCE ....
GENERATE ... ! generate a new different PSF.
DELETE CONNECTIVITY .... ! modify the PSF by changing the connectivity.
! see a word of warning below!
SCALAR TYPE SET 14 SELE ATOM A 1 O SHOW END ! change the vdw atom type
OPEN .... ! Read a new PSF
READ PSF ...
It is not required that the PSF be modified. If one wants to
carry out coordinate perturbation only, it is sufficient to modify
the harmonic restraints, the NOE restraints, or the dihedral restraints.
In this way, it is possible to calculate the free energy differences
between different conformers. (However, this option should not be
used with simultaneous change of SHAKE constraints)
Note that with this implementation, because two PSFs are used,
that the connectivity may change. The use of 1-4 interactions and
nonbond exclusions is fully supported. This allows this method to be
used for examining changes that involve bond changes, such as cystine
bridge formation. [Note added by Stefan Boresch (stefan@mdy.univie.ac.at)
Changes in connectivity that involve bond breaking or forming are
highly problematic and may not converge. This is explained in
detail in Boresch & Karplus, J. Phys. Chem. B 1999, 103, 103-136.
The flexibility made possible by the implementation of PERT puts
the responsibility of what can be done and what not on the user!]
The advanced mode of operation is;
....
PERTurb
PATCH ....
DYNAmics ....
....
PERTurb
PATCH ....
DYNAmics ....
....
PERTurb
PATCH ....
DYNAmics ....
....
In this way, several changes can be affected in a single CHARMM run.
For example, the first patch might be the removal of charges, and the
second patch could correspond to a change in atom size, and the third
patch could simply consist of modifying dihedral restraints so as to
affect a conformational change. The free energy differences and
fluctuations will be calculated for each window as well as the total
for all previous windows.
Top
RESTRICTIONS:
The number of atoms in both sets must match! If the system of
interest has different numbers of atoms, then dummy atoms must be
used. The mapping of atoms between the first and last structure is
one to one.
The following CHARMM features are not currently supported for use
with free energy perturbation;
INTEraction_energy
These commands will continue to work, but will only use the final
(lambda=1) structure. Most other energy related CHARMM features
are supported.
The IMAGE/CRYSTAL facility has been supported now for some time;
however, IMAGE/CRYSTAL needs to be set up *after* the PERT command!!!
The following CHARMM energy related features cannot be modified with
the PERT command (e.g. cannot be part of what is changing, and are
only determined by the final state).
HBON - hydrogen bond energy
ST2 - ST2 energy
CIC - internal coordinate constraint energy
CDRO - quartic droplet potential energy
USER - user supplied energy (USERLINK)
RXNF - Reaction field energy
IMNB - image van der Waal energy
IMEL - image electrostatic energy
IMHB - image hydrogen bond energy
IMST - image ST2 energy
SBOU - solvent boundary energy
UREY - Urey Bradley energy terms
XTLV - Crystal vdw terms
XTLE - Crystal electrostatics
Extended electrostatics is implemented within PERT and can be used with
the following CHARMM commands:
NBONDS GROUP SWITCH CDIE VDW VSWITCH EXTEND GRAD QUAD -
CTONNB 12.0 CTOFNB 12.0 CUTNB 12.0 WMIN 1.2 WRNMXD 1.2 EPS 1.0
NOTE: The ctonnb, ctofnb and cutnb values should be the same when
implementing extended electrostatics in PERT to prevent problems with
mixing of usage of switching functions and extended electrostatics
RESTRICTIONS:
The number of atoms in both sets must match! If the system of
interest has different numbers of atoms, then dummy atoms must be
used. The mapping of atoms between the first and last structure is
one to one.
The following CHARMM features are not currently supported for use
with free energy perturbation;
INTEraction_energy
These commands will continue to work, but will only use the final
(lambda=1) structure. Most other energy related CHARMM features
are supported.
The IMAGE/CRYSTAL facility has been supported now for some time;
however, IMAGE/CRYSTAL needs to be set up *after* the PERT command!!!
The following CHARMM energy related features cannot be modified with
the PERT command (e.g. cannot be part of what is changing, and are
only determined by the final state).
HBON - hydrogen bond energy
ST2 - ST2 energy
CIC - internal coordinate constraint energy
CDRO - quartic droplet potential energy
USER - user supplied energy (USERLINK)
RXNF - Reaction field energy
IMNB - image van der Waal energy
IMEL - image electrostatic energy
IMHB - image hydrogen bond energy
IMST - image ST2 energy
SBOU - solvent boundary energy
UREY - Urey Bradley energy terms
XTLV - Crystal vdw terms
XTLE - Crystal electrostatics
Extended electrostatics is implemented within PERT and can be used with
the following CHARMM commands:
NBONDS GROUP SWITCH CDIE VDW VSWITCH EXTEND GRAD QUAD -
CTONNB 12.0 CTOFNB 12.0 CUTNB 12.0 WMIN 1.2 WRNMXD 1.2 EPS 1.0
NOTE: The ctonnb, ctofnb and cutnb values should be the same when
implementing extended electrostatics in PERT to prevent problems with
mixing of usage of switching functions and extended electrostatics
Top
Some References:
M Mezei and D.L. Beveridge, in Annals of the NYAS, "Free Energy
Simulations" 482 (1986)
T. P. Straatsma Ph.D. Thesis "Free Energy Evaluation by
Molecular Dynamics Simulations"
Kollman, P. A.; et al. J. Am. Chem. Soc. 1987, 109, 1607.
Kollman, P. A.; et al. J. Am. Chem. Soc. 1987, 109, 6283.
Kollman, P. A.; et al. J. Chem. Phys. 1989, 91, 7831.
Bell, C. D.; Harvey, S. C., J. Phys. Chem. 1986, 90, 6595.
van Gunsteren, W.F. et al. in: Computer Simulation of Biomolecular
Systems: Theoretical and Experimental Applications, vol. 2, eds. van
Gunsteren W.F. and Weiner P.K. (Escom, Leiden, 1994), p. 349
Some References:
M Mezei and D.L. Beveridge, in Annals of the NYAS, "Free Energy
Simulations" 482 (1986)
T. P. Straatsma Ph.D. Thesis "Free Energy Evaluation by
Molecular Dynamics Simulations"
Kollman, P. A.; et al. J. Am. Chem. Soc. 1987, 109, 1607.
Kollman, P. A.; et al. J. Am. Chem. Soc. 1987, 109, 6283.
Kollman, P. A.; et al. J. Chem. Phys. 1989, 91, 7831.
Bell, C. D.; Harvey, S. C., J. Phys. Chem. 1986, 90, 6595.
van Gunsteren, W.F. et al. in: Computer Simulation of Biomolecular
Systems: Theoretical and Experimental Applications, vol. 2, eds. van
Gunsteren W.F. and Weiner P.K. (Escom, Leiden, 1994), p. 349
Top
Examples:
The input file:
* A SIMPLE TEST RUN FOR PERT
bomlev -1
OPEN READ FILE UNIT 1 NAME ~/c22pt/toph19.mod
READ RTF UNIT 1
OPEN READ FILE UNIT 2 NAME ~/c22pt/param19.mod
READ PARAMETER UNIT 2
READ SEQUENCE CARD
* FIRST SEQUENCE FOR SECOND DERIVATIVE TEST
2
AMN CBX
GENERATE A
GENERATE B DUPLICATE A
OPEN UNIT 3 READ CARD NAME perttest.crd
READ COOR CARD UNIT 3
! modify the charge for the lambda=0 state
SCALAR CHARGE SET -0.55 SELE ATOM A 1 O* SHOW END
! minimize initial state so initial forces will be small.
MINI ABNR NSTEP 100 CTOFNB 12.0 CUTNB 14.0
PERT ! save all PSF data for the lambda=0 state
! modify the charge again for the lambda=1 state
SCALAR CHARGE SET -0.15 SELE ATOM A 1 O* SHOW END
! carry out free energy run from first to final state
OPEN READ CARD UNIT 88 NAME perttest.punit
DYNA VERLET STRT NSTEP 12000 TIMESTEP 0.001 -
IPRFRQ 100 IHTFRQ 0 IEQFRQ 100 NTRFRQ 2000 -
IUNCRD 50 ISEED 314159 -
NPRINT 100 NSAVC 0 NSAVV 0 INBFRQ 25 IHBFRQ 0 -
CTOFNB 12.0 CUTNB 14.0 -
FIRSTT 300.0 FINALT 300.0 TEMINC 100.0 -
IASORS 0 IASVEL 1 ISCVEL 0 ICHECW 1 TWINDH 20.0 TWINDL -20.0 -
PUNIT 88
PERT OFF
energy ! just a check at lamda=1
STOP
The punit file:
* PUNIT FILE FOR SIMPLE TEST CASE
* use window method with 2000 steps of equilibration
* and 8000 steps of analysis for each of 10 evenly spaces
* windows.
LSTART 0.0 LAMBDA 0.0 LSTOP 0.05 PSTART 12000 PSTOP 20000 PWIND
LSTART 0.05 LAMBDA 0.1 LSTOP 0.15 PSTART 22000 PSTOP 30000 PWIND
LSTART 0.15 LAMBDA 0.2 LSTOP 0.25 PSTART 32000 PSTOP 40000 PWIND
LSTART 0.25 LAMBDA 0.3 LSTOP 0.35 PSTART 42000 PSTOP 50000 PWIND
LSTART 0.35 LAMBDA 0.4 LSTOP 0.45 PSTART 52000 PSTOP 60000 PWIND
LSTART 0.45 LAMBDA 0.5 LSTOP 0.55 PSTART 62000 PSTOP 70000 PWIND
LSTART 0.55 LAMBDA 0.6 LSTOP 0.65 PSTART 72000 PSTOP 80000 PWIND
LSTART 0.65 LAMBDA 0.7 LSTOP 0.75 PSTART 82000 PSTOP 90000 PWIND
LSTART 0.75 LAMBDA 0.8 LSTOP 0.85 PSTART 92000 PSTOP 100000 PWIND
LSTART 0.85 LAMBDA 0.9 LSTOP 0.95 PSTART 102000 PSTOP 110000 PWIND
LSTART 0.95 LAMBDA 1.0 LSTOP 1.0 PSTART 112000 PSTOP 120000 PWIND
END
Or equivalently using auto mode:
* PUNIT FILE FOR SIMPLE TEST CASE
* use window method with 2000 steps of equilibration
* and 8000 steps of analysis for each of 10 evenly spaces
* windows.
LSTART 0.0 LAMBDA 0.0 LSTOP 0.05 PSTART 12000 PSTOP 20000 PWIND PEQUIL 2000 PINCR 10000 LINCR 0.1
Or also equivalently as:
* PUNIT FILE FOR SIMPLE TEST CASE
* use window method with 2000 steps of equilibration
* and 8000 steps of analysis for each of 10 evenly spaces
* windows.
LSTART 0.0 LAMBDA 0.0 LSTOP 0.05 PSTART 12000 PSTOP 20000 PWIND
LSTART 0.05 LAMBDA 0.1 LSTOP 0.15 PEQUIL 2000 PINCR 10000 PWIND
LSTART 0.15 LAMBDA 0.2 LSTOP 0.25 PEQUIL 2000 PINCR 10000 PWIND
LSTART 0.25 LAMBDA 0.3 LSTOP 0.35 PEQUIL 2000 PINCR 10000 PWIND
LSTART 0.35 LAMBDA 0.4 LSTOP 0.45 PEQUIL 2000 PINCR 10000 PWIND
LSTART 0.45 LAMBDA 0.5 LSTOP 0.55 PEQUIL 2000 PINCR 10000 PWIND
LSTART 0.55 LAMBDA 0.6 LSTOP 0.65 PEQUIL 2000 PINCR 10000 PWIND
LSTART 0.65 LAMBDA 0.7 LSTOP 0.75 PEQUIL 2000 PINCR 10000 PWIND
LSTART 0.75 LAMBDA 0.8 LSTOP 0.85 PEQUIL 2000 PINCR 10000 PWIND
LSTART 0.85 LAMBDA 0.9 LSTOP 0.95 PEQUIL 2000 PINCR 10000 PWIND
LSTART 0.95 LAMBDA 1.0 LSTOP 1.0 PEQUIL 2000 PINCR 10000 PWIND
END
------------------------------------------------------------------------------
An annotated output example:
This output is a short excerpt from perttest.out where the input
lines start with "|" and output lines start with ".....|".
The CHARMM command is:
| CHARMM> DYNA VERLET STRT NSTEP 12000 TIMESTEP 0.001 -
| CHARMM> IPRFRQ 100 IHTFRQ 0 IEQFRQ 100 NTRFRQ 2000 -
| CHARMM> IUNCRD 50 ISEED 314159 -
| CHARMM> NPRINT 100 NSAVC 0 NSAVV 0 INBFRQ 25 IHBFRQ 0 -
| CHARMM> CTOFNB 12.0 CUTNB 14.0 -
| CHARMM> FIRSTT 300.0 FINALT 300.0 TEMINC 100.0 -
| CHARMM> IASORS 0 IASVEL 1 ISCVEL 0 ICHECW 1 TWINDH 20.0 TWINDL -20.0 -
| CHARMM> PUNIT 88
and the relevent punit data is in perttest.punit:
|* PUNIT FILE FOR SIMPLE TEST CASE
|* use window method with 2000 steps of equilibration
|* and 8000 steps of analysis for each of 10 evenly spaces
|* windows.
|*
| LSTART 0.0 LAMBDA 0.0 LSTOP 0.05 PSTART 1200 -
| PSTOP 2000 PWIND PEQUIL 200 PINCR 1000 LINCR 0.1
The output starting at line 1618 (in the middle of the dynamics command) is:
.....| PERTURBATION> Free energy perturbation results:
This indicates that a "window" was just completed.
**
.....| PERTURBATION> results, LSTART= 0.050000 LSTOP= 0.150000 LLAST= 0.100000 Number of steps used= 800
This says that the window started at lambda=0.05 and ended at 0.15.
The window "center" was at lambda=0.1
A total of 800 steps was used for collecting averages and fluctuations.
.....| PERTURBATION> result: EXPAVE=0.155456E+01 EXPFLC=0.225213E+00 DIFAVE= -0.256530 DIFFLC= 0.088960
The values:
EXPAVE is the time average of exp((ef(t)-ei(t)-ef(0)+ei(0))/kT)
EXPFLC is the fluctuation of this value about its average
DIFAVE is the time average of (ef(t)-ei(t)-ef(0)+ei(0))
DIFFLC is the fluctuation of this value about its average
Note: this value should not be much larger than kT for a
good window schedule. If this value is too large,
then smaller window lambda steps should be used.
The value here (0.09) indicates that a much larger
window would have been OK. ef(t) is the energy at
lambda=LSTOP, ei(t) is the energy at lambda=LSTART
ef(0) is the initial energy at LSTOP, ei(0) is the
initial energy at LSTART
.....| PERTURBATION> TP Windowing result, EPRTOT= 1.392400 EFORWARD= 0.914282 EPREF= 1.177303
This is the old format. In the new format the values EPRTOT,EFORWARD,
EBACKWARD,EPREFF,EPREFB are reported where the forward energy is from LLAST
to LSTOP and the backward from LLAST to LSTART. Separating the window into
two halves (double wide sampling) improves the accuracy of the the TP method.
.....| PERTURBATION> TI Windowing result, EPRTOT= 1.400218 EFORWARD= 0.920773 EPREF= 1.177303
EPRTOT is the total energy for this window and all previous (since a PERT
RESET).
EFORWARD is the energy for this current window.
EPREF is the initial energy difference (ef(0)-ei(0))
.....| PERTRES> LSTART= 0.05000 LSTOP= 0.15000 EPRTOT= 1.40022 EFORWARD= 0.92077 EPREF= 1.17730 DIFAVE= -0.25653 DIFFLC= 0.08896
This is the same data on a one line format. To use this, grep (search)
for "PERTRES".
.....| PERTURBATION> Averages for the last 800 steps:
.....|PAVE DYN: Step Time TOTEner TOTKe ENERgy TEMPerature
.....|PAVE PROP: GRMS VEREner VERKe EHFCor VIRKe
.....|PAVE EXTERN: VDWaals ELEC HBONds USER
.....|PAVE PRESS: VIRE VIRI PRESSE PRESSI VOLUme
.....| ---------- --------- --------- --------- --------- ---------
.....|PAVE> 800 0.00000 0.92077 -0.00039 0.92077 0.00000
<delF*v> <delE>
.....|PAVE PROP> 0.00000 0.00000 0.00000 0.00000 0.00000
.....|PAVE EXTERN> 0.00000 0.92077 0.00000 0.00000
.....|PAVE PRESS> 0.00000 0.00000 0.00000 0.00000 0.00000
This is the average values for this window (TI results).
Note: the <delF*v> is a "correction" term that shows how well the window is
equilibrated. This value should be close to zero and much smaller than
its fluctuation. If it is not, then the assumptions required for a
free energy calculation using windowing are not met.
This can occur if there is a "snapping" event with releases energy in
an irreversible manner, or if the system is not at equilibrium.
For a slow growth "window", this is a correction term which should be
multiplied by the estimated delay of the equilibration at the current
step and then added to the total.
For example, if the configuration distribution lags behind the energy
potential by 100 steps, this value should be scaled by 100.
When forcing a "continuous" change through slow growth, there tends to
be a delay since the structure does not respond instantly to the
potential.
.....| ---------- --------- --------- --------- --------- ---------
.....| PERTURBATION> Fluctuations for the last 800 steps:
.....|PFLC> 800 0.00000 0.08911 0.00985 0.08896 0.00000
.....|PFLC PROP> 0.00000 0.00000 0.00000 0.00000 0.00000
.....|PFLC EXTERN> 0.00000 0.08896 0.00000 0.00000
.....|PFLC PRESS> 0.00000 0.00000 0.00000 0.00000 0.00000
This is the fluctuation data for the current window (TI results).
.....| ---------- --------- --------- --------- --------- ---------
.....| PERTURBATION> TOTALS since last reset:
.....|PTOT> 800 0.00000 1.40022 -0.00038 1.40022 0.00000
.....|PTOT PROP> 0.00000 0.00000 0.00000 0.00000 0.00000
.....|PTOT EXTERN> 0.00000 1.40022 0.00000 0.00000
.....|PTOT PRESS> 0.00000 0.00000 0.00000 0.00000 0.00000
This is the total for this window and all previous (since the last PERT RESET).
.....| ---------- --------- --------- --------- --------- ---------
.....|
.....| PERTURBATION> EOF on punit file: PERT in auto mode.
This indicates that no more data was found on the PUNIT file.
.....| PERTURBATION> Free energy perturbation calculation continues.
Now we start a new window.
.....| PERTURBATION> PSTART= 3200 PSTOP= 4000
We will run equilibration until step 3200, then we will collect data until step 4000.
.....| PERTURBATION> LSTART= 0.150000 LSTOP= 0.250000 LAMBDA= 0.200000
This indicates the boundaries of the new window.
.....| PERTURBATION> Windowing will be used.
We are using windowing (fixed lambda values), instead of slow growth.
.....|
PERT also works with SCC-DFTB. In one case, the entire QM region is perturbed into MM.
In the secon case, part of the QM region is perturbed into MM. These calculations can
be combined with properly designed thermodynamic cycles to compute solvation free energy
or ligand binding energy with SCC-DFTB/MM. For more discussions, see the review by
X. Lu et al., Mol. Simul. 42, 1056-1078 (2016).
Example 1: Perturb the entire QM region (an acetate) into MM in the background of MM water.
define qm sele segid ACET show end
...SCC-DFTB setup...
pert qmmm sele qm end !the qmmm keyword has been added to pert
scalar WMAIN set 1.0 sele (qm) .and. type C* SHOW end
scalar WMAIN set 2.0 sele (qm) .and. type H* SHOW end
scalar WMAIN set 3.0 sele (qm) .and. type O* SHOW end
SCCDFTB remove CHRG -1 SELE QM END TEMP 0.0 SCFT 0.00000001 D3RD HBOND
...standard MD setup...
set lam 0.5
calc lstart = (@lam - 0.05)
calc lstop = (@lam + 0.05)
scalar FBETA set 80.0 sele (type OH2) end
shake bonh para
open unit 26 write form name @9/acet2_droplet_3ob_qmmm_@lam_equi.res
open unit 27 write file name @9/acet2_droplet_3ob_qmmm_@lam_equi.dcd
open unit 54 write card name @9/acet2_droplet_3ob_qmmm_@lam_equi.dat
dynamics start lang timestep 0.001 nstep 500 nprint 10 iprfrq 10 -
firstt 300.0 finalt 300 TEMINC 0.0 twindl -10.0 twindh 10.0 -
IHTFRQ 0 IEQFRQ 0 NTRFRQ 0 ISEED 2069904569 -
IASORS 1 IASVEL 1 ISCVEL 0 ICHECW 0 isvfrq 100 -
iunrea -1 iunwri 26 iuncrd 27 iunvel -1 kunit -1 nsavc 100 nsavv 0 -
inbfrq -1 imgfrq 0 ilbfrq -1 ihbfrq 0 tbath 300 rbuffer 16.0 -
LSTART @lstart LAMBDA @lam LSTOP @lstop PSTART 100 PSTOP 500 PWIND -
wham 54
Example 2: Perturb part (acetate) of the QM region (acetate plus first solvation shell) into MM.
define inwat sele (segid BULK .and. -
(resid 152 .or. resid 385 .or. resid 404 .or. resid 463 .or. -
resid 534 .or. resid 617 .or. resid 705 .or. -
resid 782 .or. resid 825 .or. resid 912 .or. resid 926 .or. -
resid 1015 .or. resid 1101 .or. resid 1170 .or. resid 1239 .or. -
resid 1253 .or. resid 1279 .or. resid 1355 .or. resid 1494 .or. -
resid 1547 .or. resid 1599 .or. resid 1905 .or. resid 1992 .or. -
resid 2037)) .or. (segid BUL5 .and. resid 517) show end
define outwat sele (.not. (inwat .or. segid ACET)) end
! QC: in realistic simulations, should include FIRES (RMAX in MMFP)
define qm sele segid ACET .or. inwat show end
scalar WMAIN set 1.0 sele (qm) .and. type C* SHOW end
scalar WMAIN set 2.0 sele (qm) .and. type H* SHOW end
scalar WMAIN set 3.0 sele (qm) .and. type O* SHOW end
SCCDFTB remove pert D3RD HBOND TEMP 0.0 SCFT 0.00000001 CHRG -1 -
TEMP 0.0 SCFT 0.00000001 CHRG 0 -
sele qm end -
sele (qm .and. .not. segid ACET) end
pert sele qm end !Note no qmmm keyword is needed with pert
...standard MD setup...
set lam 0.5
calc lstart = (@lam - 0.05)
calc lstop = (@lam + 0.05)
scalar FBETA set 80.0 sele (type OH2) end
shake bonh sele .not. qm end
open unit 26 write form name @9/acet2_droplet_3ob_sccpert_@lam_equi.res
open unit 27 write file name @9/acet2_droplet_3ob_sccpert_@lam_equi.dcd
open unit 54 write card name @9/acet2_droplet_3ob_sccpert_@lam_equi.dat
dynamics start lang timestep 0.001 nstep 500 nprint 10 iprfrq 10 -
firstt 300.0 finalt 300 TEMINC 0.0 twindl -10.0 twindh 10.0 -
IHTFRQ 0 IEQFRQ 0 NTRFRQ 0 ISEED 914194955 -
IASORS 1 IASVEL 1 ISCVEL 0 ICHECW 0 isvfrq 100 -
iunrea -1 iunwri 26 iuncrd 27 iunvel -1 kunit -1 nsavc 100 nsavv 0 -
inbfrq -1 imgfrq 0 ilbfrq -1 ihbfrq 0 tbath 300 rbuffer 16.0 -
LSTART @lstart LAMBDA @lam LSTOP @lstop PSTART 100 PSTOP 500 PWIND -
wham 54
PERT now works with the double exponential potential(DE). DE potential has no
signularity and its free energy can be calculated with or without PSSP. Here
are examples for systems with DE potential.
Example 1: Pert on DE potential with automatic exponential LAMBDA windows.
DYNA VERLET STRT NSTEP 12000 TIMESTEP 0.001 -
IPRFRQ 100 IHTFRQ 0 IEQFRQ 100 NTRFRQ 2000 -
IUNCRD 50 ISEED 314159 -
NPRINT 100 NSAVC 0 NSAVV 0 INBFRQ 25 IHBFRQ 0 -
CTOFNB 12.0 CUTNB 14.0 EIPS VIPS PXYZ DBEXP -
FIRSTT 300.0 FINALT 300.0 TEMINC 100.0 -
IASORS 0 IASVEL 1 ISCVEL 0 ICHECW 1 TWINDH 20.0 TWINDL -20.0 -
EIPS VIPS PXYZ DBEXP -
PEQUIL 200 PINCR 1000 LSTA 0 LSTOP 1 LINCR 0.1 LEXP 3.5
Example 2: PSSP Pert on DE potential with automatic linear LAMBDA windows.
DYNA VERLET STRT NSTEP 12000 TIMESTEP 0.001 -
IPRFRQ 100 IHTFRQ 0 IEQFRQ 100 NTRFRQ 2000 -
IUNCRD 50 ISEED 314159 -
NPRINT 100 NSAVC 0 NSAVV 0 INBFRQ 25 IHBFRQ 0 -
CTOFNB 12.0 CUTNB 14.0 EIPS VIPS PXYZ DBEXP -
FIRSTT 300.0 FINALT 300.0 TEMINC 100.0 -
IASORS 0 IASVEL 1 ISCVEL 0 ICHECW 1 TWINDH 20.0 TWINDL -20.0 -
EIPS VIPS PXYZ DBEXP -
PEQUIL 200 PINCR 1000 LSTA 0 LSTOP 1 LINCR 0.1 LEXP 0 PSSP
Examples:
The input file:
* A SIMPLE TEST RUN FOR PERT
bomlev -1
OPEN READ FILE UNIT 1 NAME ~/c22pt/toph19.mod
READ RTF UNIT 1
OPEN READ FILE UNIT 2 NAME ~/c22pt/param19.mod
READ PARAMETER UNIT 2
READ SEQUENCE CARD
* FIRST SEQUENCE FOR SECOND DERIVATIVE TEST
2
AMN CBX
GENERATE A
GENERATE B DUPLICATE A
OPEN UNIT 3 READ CARD NAME perttest.crd
READ COOR CARD UNIT 3
! modify the charge for the lambda=0 state
SCALAR CHARGE SET -0.55 SELE ATOM A 1 O* SHOW END
! minimize initial state so initial forces will be small.
MINI ABNR NSTEP 100 CTOFNB 12.0 CUTNB 14.0
PERT ! save all PSF data for the lambda=0 state
! modify the charge again for the lambda=1 state
SCALAR CHARGE SET -0.15 SELE ATOM A 1 O* SHOW END
! carry out free energy run from first to final state
OPEN READ CARD UNIT 88 NAME perttest.punit
DYNA VERLET STRT NSTEP 12000 TIMESTEP 0.001 -
IPRFRQ 100 IHTFRQ 0 IEQFRQ 100 NTRFRQ 2000 -
IUNCRD 50 ISEED 314159 -
NPRINT 100 NSAVC 0 NSAVV 0 INBFRQ 25 IHBFRQ 0 -
CTOFNB 12.0 CUTNB 14.0 -
FIRSTT 300.0 FINALT 300.0 TEMINC 100.0 -
IASORS 0 IASVEL 1 ISCVEL 0 ICHECW 1 TWINDH 20.0 TWINDL -20.0 -
PUNIT 88
PERT OFF
energy ! just a check at lamda=1
STOP
The punit file:
* PUNIT FILE FOR SIMPLE TEST CASE
* use window method with 2000 steps of equilibration
* and 8000 steps of analysis for each of 10 evenly spaces
* windows.
LSTART 0.0 LAMBDA 0.0 LSTOP 0.05 PSTART 12000 PSTOP 20000 PWIND
LSTART 0.05 LAMBDA 0.1 LSTOP 0.15 PSTART 22000 PSTOP 30000 PWIND
LSTART 0.15 LAMBDA 0.2 LSTOP 0.25 PSTART 32000 PSTOP 40000 PWIND
LSTART 0.25 LAMBDA 0.3 LSTOP 0.35 PSTART 42000 PSTOP 50000 PWIND
LSTART 0.35 LAMBDA 0.4 LSTOP 0.45 PSTART 52000 PSTOP 60000 PWIND
LSTART 0.45 LAMBDA 0.5 LSTOP 0.55 PSTART 62000 PSTOP 70000 PWIND
LSTART 0.55 LAMBDA 0.6 LSTOP 0.65 PSTART 72000 PSTOP 80000 PWIND
LSTART 0.65 LAMBDA 0.7 LSTOP 0.75 PSTART 82000 PSTOP 90000 PWIND
LSTART 0.75 LAMBDA 0.8 LSTOP 0.85 PSTART 92000 PSTOP 100000 PWIND
LSTART 0.85 LAMBDA 0.9 LSTOP 0.95 PSTART 102000 PSTOP 110000 PWIND
LSTART 0.95 LAMBDA 1.0 LSTOP 1.0 PSTART 112000 PSTOP 120000 PWIND
END
Or equivalently using auto mode:
* PUNIT FILE FOR SIMPLE TEST CASE
* use window method with 2000 steps of equilibration
* and 8000 steps of analysis for each of 10 evenly spaces
* windows.
LSTART 0.0 LAMBDA 0.0 LSTOP 0.05 PSTART 12000 PSTOP 20000 PWIND PEQUIL 2000 PINCR 10000 LINCR 0.1
Or also equivalently as:
* PUNIT FILE FOR SIMPLE TEST CASE
* use window method with 2000 steps of equilibration
* and 8000 steps of analysis for each of 10 evenly spaces
* windows.
LSTART 0.0 LAMBDA 0.0 LSTOP 0.05 PSTART 12000 PSTOP 20000 PWIND
LSTART 0.05 LAMBDA 0.1 LSTOP 0.15 PEQUIL 2000 PINCR 10000 PWIND
LSTART 0.15 LAMBDA 0.2 LSTOP 0.25 PEQUIL 2000 PINCR 10000 PWIND
LSTART 0.25 LAMBDA 0.3 LSTOP 0.35 PEQUIL 2000 PINCR 10000 PWIND
LSTART 0.35 LAMBDA 0.4 LSTOP 0.45 PEQUIL 2000 PINCR 10000 PWIND
LSTART 0.45 LAMBDA 0.5 LSTOP 0.55 PEQUIL 2000 PINCR 10000 PWIND
LSTART 0.55 LAMBDA 0.6 LSTOP 0.65 PEQUIL 2000 PINCR 10000 PWIND
LSTART 0.65 LAMBDA 0.7 LSTOP 0.75 PEQUIL 2000 PINCR 10000 PWIND
LSTART 0.75 LAMBDA 0.8 LSTOP 0.85 PEQUIL 2000 PINCR 10000 PWIND
LSTART 0.85 LAMBDA 0.9 LSTOP 0.95 PEQUIL 2000 PINCR 10000 PWIND
LSTART 0.95 LAMBDA 1.0 LSTOP 1.0 PEQUIL 2000 PINCR 10000 PWIND
END
------------------------------------------------------------------------------
An annotated output example:
This output is a short excerpt from perttest.out where the input
lines start with "|" and output lines start with ".....|".
The CHARMM command is:
| CHARMM> DYNA VERLET STRT NSTEP 12000 TIMESTEP 0.001 -
| CHARMM> IPRFRQ 100 IHTFRQ 0 IEQFRQ 100 NTRFRQ 2000 -
| CHARMM> IUNCRD 50 ISEED 314159 -
| CHARMM> NPRINT 100 NSAVC 0 NSAVV 0 INBFRQ 25 IHBFRQ 0 -
| CHARMM> CTOFNB 12.0 CUTNB 14.0 -
| CHARMM> FIRSTT 300.0 FINALT 300.0 TEMINC 100.0 -
| CHARMM> IASORS 0 IASVEL 1 ISCVEL 0 ICHECW 1 TWINDH 20.0 TWINDL -20.0 -
| CHARMM> PUNIT 88
and the relevent punit data is in perttest.punit:
|* PUNIT FILE FOR SIMPLE TEST CASE
|* use window method with 2000 steps of equilibration
|* and 8000 steps of analysis for each of 10 evenly spaces
|* windows.
|*
| LSTART 0.0 LAMBDA 0.0 LSTOP 0.05 PSTART 1200 -
| PSTOP 2000 PWIND PEQUIL 200 PINCR 1000 LINCR 0.1
The output starting at line 1618 (in the middle of the dynamics command) is:
.....| PERTURBATION> Free energy perturbation results:
This indicates that a "window" was just completed.
**
.....| PERTURBATION> results, LSTART= 0.050000 LSTOP= 0.150000 LLAST= 0.100000 Number of steps used= 800
This says that the window started at lambda=0.05 and ended at 0.15.
The window "center" was at lambda=0.1
A total of 800 steps was used for collecting averages and fluctuations.
.....| PERTURBATION> result: EXPAVE=0.155456E+01 EXPFLC=0.225213E+00 DIFAVE= -0.256530 DIFFLC= 0.088960
The values:
EXPAVE is the time average of exp((ef(t)-ei(t)-ef(0)+ei(0))/kT)
EXPFLC is the fluctuation of this value about its average
DIFAVE is the time average of (ef(t)-ei(t)-ef(0)+ei(0))
DIFFLC is the fluctuation of this value about its average
Note: this value should not be much larger than kT for a
good window schedule. If this value is too large,
then smaller window lambda steps should be used.
The value here (0.09) indicates that a much larger
window would have been OK. ef(t) is the energy at
lambda=LSTOP, ei(t) is the energy at lambda=LSTART
ef(0) is the initial energy at LSTOP, ei(0) is the
initial energy at LSTART
.....| PERTURBATION> TP Windowing result, EPRTOT= 1.392400 EFORWARD= 0.914282 EPREF= 1.177303
This is the old format. In the new format the values EPRTOT,EFORWARD,
EBACKWARD,EPREFF,EPREFB are reported where the forward energy is from LLAST
to LSTOP and the backward from LLAST to LSTART. Separating the window into
two halves (double wide sampling) improves the accuracy of the the TP method.
.....| PERTURBATION> TI Windowing result, EPRTOT= 1.400218 EFORWARD= 0.920773 EPREF= 1.177303
EPRTOT is the total energy for this window and all previous (since a PERT
RESET).
EFORWARD is the energy for this current window.
EPREF is the initial energy difference (ef(0)-ei(0))
.....| PERTRES> LSTART= 0.05000 LSTOP= 0.15000 EPRTOT= 1.40022 EFORWARD= 0.92077 EPREF= 1.17730 DIFAVE= -0.25653 DIFFLC= 0.08896
This is the same data on a one line format. To use this, grep (search)
for "PERTRES".
.....| PERTURBATION> Averages for the last 800 steps:
.....|PAVE DYN: Step Time TOTEner TOTKe ENERgy TEMPerature
.....|PAVE PROP: GRMS VEREner VERKe EHFCor VIRKe
.....|PAVE EXTERN: VDWaals ELEC HBONds USER
.....|PAVE PRESS: VIRE VIRI PRESSE PRESSI VOLUme
.....| ---------- --------- --------- --------- --------- ---------
.....|PAVE> 800 0.00000 0.92077 -0.00039 0.92077 0.00000
<delF*v> <delE>
.....|PAVE PROP> 0.00000 0.00000 0.00000 0.00000 0.00000
.....|PAVE EXTERN> 0.00000 0.92077 0.00000 0.00000
.....|PAVE PRESS> 0.00000 0.00000 0.00000 0.00000 0.00000
This is the average values for this window (TI results).
Note: the <delF*v> is a "correction" term that shows how well the window is
equilibrated. This value should be close to zero and much smaller than
its fluctuation. If it is not, then the assumptions required for a
free energy calculation using windowing are not met.
This can occur if there is a "snapping" event with releases energy in
an irreversible manner, or if the system is not at equilibrium.
For a slow growth "window", this is a correction term which should be
multiplied by the estimated delay of the equilibration at the current
step and then added to the total.
For example, if the configuration distribution lags behind the energy
potential by 100 steps, this value should be scaled by 100.
When forcing a "continuous" change through slow growth, there tends to
be a delay since the structure does not respond instantly to the
potential.
.....| ---------- --------- --------- --------- --------- ---------
.....| PERTURBATION> Fluctuations for the last 800 steps:
.....|PFLC> 800 0.00000 0.08911 0.00985 0.08896 0.00000
.....|PFLC PROP> 0.00000 0.00000 0.00000 0.00000 0.00000
.....|PFLC EXTERN> 0.00000 0.08896 0.00000 0.00000
.....|PFLC PRESS> 0.00000 0.00000 0.00000 0.00000 0.00000
This is the fluctuation data for the current window (TI results).
.....| ---------- --------- --------- --------- --------- ---------
.....| PERTURBATION> TOTALS since last reset:
.....|PTOT> 800 0.00000 1.40022 -0.00038 1.40022 0.00000
.....|PTOT PROP> 0.00000 0.00000 0.00000 0.00000 0.00000
.....|PTOT EXTERN> 0.00000 1.40022 0.00000 0.00000
.....|PTOT PRESS> 0.00000 0.00000 0.00000 0.00000 0.00000
This is the total for this window and all previous (since the last PERT RESET).
.....| ---------- --------- --------- --------- --------- ---------
.....|
.....| PERTURBATION> EOF on punit file: PERT in auto mode.
This indicates that no more data was found on the PUNIT file.
.....| PERTURBATION> Free energy perturbation calculation continues.
Now we start a new window.
.....| PERTURBATION> PSTART= 3200 PSTOP= 4000
We will run equilibration until step 3200, then we will collect data until step 4000.
.....| PERTURBATION> LSTART= 0.150000 LSTOP= 0.250000 LAMBDA= 0.200000
This indicates the boundaries of the new window.
.....| PERTURBATION> Windowing will be used.
We are using windowing (fixed lambda values), instead of slow growth.
.....|
PERT also works with SCC-DFTB. In one case, the entire QM region is perturbed into MM.
In the secon case, part of the QM region is perturbed into MM. These calculations can
be combined with properly designed thermodynamic cycles to compute solvation free energy
or ligand binding energy with SCC-DFTB/MM. For more discussions, see the review by
X. Lu et al., Mol. Simul. 42, 1056-1078 (2016).
Example 1: Perturb the entire QM region (an acetate) into MM in the background of MM water.
define qm sele segid ACET show end
...SCC-DFTB setup...
pert qmmm sele qm end !the qmmm keyword has been added to pert
scalar WMAIN set 1.0 sele (qm) .and. type C* SHOW end
scalar WMAIN set 2.0 sele (qm) .and. type H* SHOW end
scalar WMAIN set 3.0 sele (qm) .and. type O* SHOW end
SCCDFTB remove CHRG -1 SELE QM END TEMP 0.0 SCFT 0.00000001 D3RD HBOND
...standard MD setup...
set lam 0.5
calc lstart = (@lam - 0.05)
calc lstop = (@lam + 0.05)
scalar FBETA set 80.0 sele (type OH2) end
shake bonh para
open unit 26 write form name @9/acet2_droplet_3ob_qmmm_@lam_equi.res
open unit 27 write file name @9/acet2_droplet_3ob_qmmm_@lam_equi.dcd
open unit 54 write card name @9/acet2_droplet_3ob_qmmm_@lam_equi.dat
dynamics start lang timestep 0.001 nstep 500 nprint 10 iprfrq 10 -
firstt 300.0 finalt 300 TEMINC 0.0 twindl -10.0 twindh 10.0 -
IHTFRQ 0 IEQFRQ 0 NTRFRQ 0 ISEED 2069904569 -
IASORS 1 IASVEL 1 ISCVEL 0 ICHECW 0 isvfrq 100 -
iunrea -1 iunwri 26 iuncrd 27 iunvel -1 kunit -1 nsavc 100 nsavv 0 -
inbfrq -1 imgfrq 0 ilbfrq -1 ihbfrq 0 tbath 300 rbuffer 16.0 -
LSTART @lstart LAMBDA @lam LSTOP @lstop PSTART 100 PSTOP 500 PWIND -
wham 54
Example 2: Perturb part (acetate) of the QM region (acetate plus first solvation shell) into MM.
define inwat sele (segid BULK .and. -
(resid 152 .or. resid 385 .or. resid 404 .or. resid 463 .or. -
resid 534 .or. resid 617 .or. resid 705 .or. -
resid 782 .or. resid 825 .or. resid 912 .or. resid 926 .or. -
resid 1015 .or. resid 1101 .or. resid 1170 .or. resid 1239 .or. -
resid 1253 .or. resid 1279 .or. resid 1355 .or. resid 1494 .or. -
resid 1547 .or. resid 1599 .or. resid 1905 .or. resid 1992 .or. -
resid 2037)) .or. (segid BUL5 .and. resid 517) show end
define outwat sele (.not. (inwat .or. segid ACET)) end
! QC: in realistic simulations, should include FIRES (RMAX in MMFP)
define qm sele segid ACET .or. inwat show end
scalar WMAIN set 1.0 sele (qm) .and. type C* SHOW end
scalar WMAIN set 2.0 sele (qm) .and. type H* SHOW end
scalar WMAIN set 3.0 sele (qm) .and. type O* SHOW end
SCCDFTB remove pert D3RD HBOND TEMP 0.0 SCFT 0.00000001 CHRG -1 -
TEMP 0.0 SCFT 0.00000001 CHRG 0 -
sele qm end -
sele (qm .and. .not. segid ACET) end
pert sele qm end !Note no qmmm keyword is needed with pert
...standard MD setup...
set lam 0.5
calc lstart = (@lam - 0.05)
calc lstop = (@lam + 0.05)
scalar FBETA set 80.0 sele (type OH2) end
shake bonh sele .not. qm end
open unit 26 write form name @9/acet2_droplet_3ob_sccpert_@lam_equi.res
open unit 27 write file name @9/acet2_droplet_3ob_sccpert_@lam_equi.dcd
open unit 54 write card name @9/acet2_droplet_3ob_sccpert_@lam_equi.dat
dynamics start lang timestep 0.001 nstep 500 nprint 10 iprfrq 10 -
firstt 300.0 finalt 300 TEMINC 0.0 twindl -10.0 twindh 10.0 -
IHTFRQ 0 IEQFRQ 0 NTRFRQ 0 ISEED 914194955 -
IASORS 1 IASVEL 1 ISCVEL 0 ICHECW 0 isvfrq 100 -
iunrea -1 iunwri 26 iuncrd 27 iunvel -1 kunit -1 nsavc 100 nsavv 0 -
inbfrq -1 imgfrq 0 ilbfrq -1 ihbfrq 0 tbath 300 rbuffer 16.0 -
LSTART @lstart LAMBDA @lam LSTOP @lstop PSTART 100 PSTOP 500 PWIND -
wham 54
PERT now works with the double exponential potential(DE). DE potential has no
signularity and its free energy can be calculated with or without PSSP. Here
are examples for systems with DE potential.
Example 1: Pert on DE potential with automatic exponential LAMBDA windows.
DYNA VERLET STRT NSTEP 12000 TIMESTEP 0.001 -
IPRFRQ 100 IHTFRQ 0 IEQFRQ 100 NTRFRQ 2000 -
IUNCRD 50 ISEED 314159 -
NPRINT 100 NSAVC 0 NSAVV 0 INBFRQ 25 IHBFRQ 0 -
CTOFNB 12.0 CUTNB 14.0 EIPS VIPS PXYZ DBEXP -
FIRSTT 300.0 FINALT 300.0 TEMINC 100.0 -
IASORS 0 IASVEL 1 ISCVEL 0 ICHECW 1 TWINDH 20.0 TWINDL -20.0 -
EIPS VIPS PXYZ DBEXP -
PEQUIL 200 PINCR 1000 LSTA 0 LSTOP 1 LINCR 0.1 LEXP 3.5
Example 2: PSSP Pert on DE potential with automatic linear LAMBDA windows.
DYNA VERLET STRT NSTEP 12000 TIMESTEP 0.001 -
IPRFRQ 100 IHTFRQ 0 IEQFRQ 100 NTRFRQ 2000 -
IUNCRD 50 ISEED 314159 -
NPRINT 100 NSAVC 0 NSAVV 0 INBFRQ 25 IHBFRQ 0 -
CTOFNB 12.0 CUTNB 14.0 EIPS VIPS PXYZ DBEXP -
FIRSTT 300.0 FINALT 300.0 TEMINC 100.0 -
IASORS 0 IASVEL 1 ISCVEL 0 ICHECW 1 TWINDH 20.0 TWINDL -20.0 -
EIPS VIPS PXYZ DBEXP -
PEQUIL 200 PINCR 1000 LSTA 0 LSTOP 1 LINCR 0.1 LEXP 0 PSSP
Top
If SHAKE is applied to bond terms which are changed as the
result of an alchemical mutation a constraint correction is calculated
where required in slow-growth mode and TI in windowing mode. The
exponential formula in windowing mode is not supported. The user has
to beware of subtle problems regarding a possible "moment of inertia"
term that may be or may be not included in this correction (S. Boresch
& M. Karplus, to be published) In order for the constraint correction
to work properly, attention has to be given to the following points:
(1) SHAKE must not be applied to angle terms
(2) the PARA option has to be used (it's not clear, how to support
reference coordinates in the context of an alchemical mutation)
(3) the SHAKE command has to issued after the PERT command. (This
is similar to setting up IMAGEs in connection with PERT). A
typical input will look something like
PERT SELE ... END
!change psf; after ALL changes have been made
SHAKe BOND PARA
DYNA ... ! carry out MD simulations etc.
PERT OFF
(4) One should not mix situations where a constraint correction for
SHAKE is necessary with the use of harmonic, NOE and dihedral
restraints to calculate conformational free energy differences.
Items (2) and (3) can lead to error messages in situations where there
is actually no problem, e.g. you just want to apply SHAKe to your
solvent which is not affected by the mutation, so you specify SHAKe
before PERT and "bomb". Nevertheless, I thought better safe than
sorry and if wanted one can override the warnings with a BOMLEV -3.
Item (4) is simply untested.
If SHAKE is applied to bond terms which are changed as the
result of an alchemical mutation a constraint correction is calculated
where required in slow-growth mode and TI in windowing mode. The
exponential formula in windowing mode is not supported. The user has
to beware of subtle problems regarding a possible "moment of inertia"
term that may be or may be not included in this correction (S. Boresch
& M. Karplus, to be published) In order for the constraint correction
to work properly, attention has to be given to the following points:
(1) SHAKE must not be applied to angle terms
(2) the PARA option has to be used (it's not clear, how to support
reference coordinates in the context of an alchemical mutation)
(3) the SHAKE command has to issued after the PERT command. (This
is similar to setting up IMAGEs in connection with PERT). A
typical input will look something like
PERT SELE ... END
!change psf; after ALL changes have been made
SHAKe BOND PARA
DYNA ... ! carry out MD simulations etc.
PERT OFF
(4) One should not mix situations where a constraint correction for
SHAKE is necessary with the use of harmonic, NOE and dihedral
restraints to calculate conformational free energy differences.
Items (2) and (3) can lead to error messages in situations where there
is actually no problem, e.g. you just want to apply SHAKe to your
solvent which is not affected by the mutation, so you specify SHAKe
before PERT and "bomb". Nevertheless, I thought better safe than
sorry and if wanted one can override the warnings with a BOMLEV -3.
Item (4) is simply untested.
Top
The post-processing Wheigthed Histogram Analysis Method (WHAM) can
be used to help reaching better statistical convergence on free energy
perturbations calculations. The approach represents a generalization
of the histogram method developed by Ferrenberg and Swendsen (1989).
The central idea, which goes back to the maximum overlap method
developed by Bennet (1976) to estimate free energy differences,
consists in constructing an optimal estimate of the unbiased distribution
function as a weighted sum over the data extracted from all the
simulations and determining the functional form of the weight factors that
minimizes the statistical error. The WHAM approach can be used to calculate
the PMF along coordinates (Kollman, 1992; Boczko, 1993; Brooks, 1993;
Roux, 1995) and can also be used to post-process free energy perturbation
calculations in which no PMF is desired.
Assuming that the simulations are performed (as in PERT) with a potential
function given by a linear switching from E_0 to E_1, that is,
E_k = (Lambda_k-1)*E_1 + (Lambda_k)*E_0
The free energy constants F_k corresponding to any Lambda_k window are
given by,
exp(-F_k/kBT) = Sum_i { Sum_t ( Top_i(t) / Bot_i(t) ) },
where
Top_i(t) = Exp(-E_k[X_i(t)]/kBT)
and
Bot_i(t) = Sum_j { Ntime(j) * Exp(+F_j/kBT-E_j[x_i(t)]/kBT) }
where E_j[x_i(t)] = (lambda_j-1)*E_1[x_i(t)] + (lambda_j)*E_0[x_i(t)]
is the potential energy function of the j-th window evaluated with
the configuration taken from the i-th simulation. The WHAM equations
for the F_k must be solved interatively.
The syntax of the command is:
WHAM MAXWindow <integer> MAXTime <integer> unit <integer> -
tolerance <real> nstep <integer> [guess] -
ioffset <integer> nskip <integer> {lambda <real> lambda <real> ...}
where
MAXWindow is the total number of windows
MAXTime is the total number of time-step configuration for each window
unit is the unit of the formatted file containing all the information
tolerance is the tolerance on the F_k to reach convergence
nstep is the maximum number of iterations on the WHAM equations
guess to flag that an initial guess is provided for the F_k. Those
are read directly from the input stream with one line per
window in the format [ window <integer> F() <real> ]
nskip use only every nskip data point to reach convergence (faster)
lambda give any value of lambda for which you want the free energy (a list)
ioffset reference energy level at window number "ioffset".
The file containing the information can be written by PERT during dynamics
if the keyword WHAM is used in the dynamics command (see above). In
principle, the WHAM could also be used with non-linear perturbations,
but then the code in PERT would have to evaluate several energies since
those could not be obtained by lambda interpolations.
The total free energy of is stored in 'WHAMFE' substitution viriable.
Some references on WHAM:
S. Kumar, D. Bouzida, R.H. Swendsen, P.A. Kollman, and J.M. Rosenberg.
J. Comp. Chem. 13, 1011--1021 (1992).
E.M. Boczko and C.L. Brooks III. J. Phys. Chem. 97, 4509--4513 (1993).
A.M. Ferrenberg and R.H. Swendsen. Phys. Rev. Lett. 63, 1195--1198 (1989).
C.M. Bennet. J. Comp. Phys. 22, 245--268 (1976).
C.L. Brooks III and L. Nilsson. J. Am. Chem. Soc. 115, 11034--11035 (1993).
B. Roux, Comp. Phys. Comm. 91, 275-282 (1995).
The post-processing Wheigthed Histogram Analysis Method (WHAM) can
be used to help reaching better statistical convergence on free energy
perturbations calculations. The approach represents a generalization
of the histogram method developed by Ferrenberg and Swendsen (1989).
The central idea, which goes back to the maximum overlap method
developed by Bennet (1976) to estimate free energy differences,
consists in constructing an optimal estimate of the unbiased distribution
function as a weighted sum over the data extracted from all the
simulations and determining the functional form of the weight factors that
minimizes the statistical error. The WHAM approach can be used to calculate
the PMF along coordinates (Kollman, 1992; Boczko, 1993; Brooks, 1993;
Roux, 1995) and can also be used to post-process free energy perturbation
calculations in which no PMF is desired.
Assuming that the simulations are performed (as in PERT) with a potential
function given by a linear switching from E_0 to E_1, that is,
E_k = (Lambda_k-1)*E_1 + (Lambda_k)*E_0
The free energy constants F_k corresponding to any Lambda_k window are
given by,
exp(-F_k/kBT) = Sum_i { Sum_t ( Top_i(t) / Bot_i(t) ) },
where
Top_i(t) = Exp(-E_k[X_i(t)]/kBT)
and
Bot_i(t) = Sum_j { Ntime(j) * Exp(+F_j/kBT-E_j[x_i(t)]/kBT) }
where E_j[x_i(t)] = (lambda_j-1)*E_1[x_i(t)] + (lambda_j)*E_0[x_i(t)]
is the potential energy function of the j-th window evaluated with
the configuration taken from the i-th simulation. The WHAM equations
for the F_k must be solved interatively.
The syntax of the command is:
WHAM MAXWindow <integer> MAXTime <integer> unit <integer> -
tolerance <real> nstep <integer> [guess] -
ioffset <integer> nskip <integer> {lambda <real> lambda <real> ...}
where
MAXWindow is the total number of windows
MAXTime is the total number of time-step configuration for each window
unit is the unit of the formatted file containing all the information
tolerance is the tolerance on the F_k to reach convergence
nstep is the maximum number of iterations on the WHAM equations
guess to flag that an initial guess is provided for the F_k. Those
are read directly from the input stream with one line per
window in the format [ window <integer> F() <real> ]
nskip use only every nskip data point to reach convergence (faster)
lambda give any value of lambda for which you want the free energy (a list)
ioffset reference energy level at window number "ioffset".
The file containing the information can be written by PERT during dynamics
if the keyword WHAM is used in the dynamics command (see above). In
principle, the WHAM could also be used with non-linear perturbations,
but then the code in PERT would have to evaluate several energies since
those could not be obtained by lambda interpolations.
The total free energy of is stored in 'WHAMFE' substitution viriable.
Some references on WHAM:
S. Kumar, D. Bouzida, R.H. Swendsen, P.A. Kollman, and J.M. Rosenberg.
J. Comp. Chem. 13, 1011--1021 (1992).
E.M. Boczko and C.L. Brooks III. J. Phys. Chem. 97, 4509--4513 (1993).
A.M. Ferrenberg and R.H. Swendsen. Phys. Rev. Lett. 63, 1195--1198 (1989).
C.M. Bennet. J. Comp. Phys. 22, 245--268 (1976).
C.L. Brooks III and L. Nilsson. J. Am. Chem. Soc. 115, 11034--11035 (1993).
B. Roux, Comp. Phys. Comm. 91, 275-282 (1995).
Top
Some details concerning the implementation of the PERT/PSSP code,
including present limitations:
1. Introduction
---------------
The PERT free energy module of CHARMM is based on a linear dependence
on the coupling parameter. While simplifying implementation, this
approach is prone to van der Waals endpoint problems. One widely used
method to overcome the van der Waals endpoint problem is the use of
soft core Lennard Jones and electrostatic interactions for those
energy terms that cause problems. Even for double expoenetial potential (DE)
that does not have endpoint singularity, a softcore treatment can help
the sampling without use expoential distribution of LAMBDA windows.
This capability has been added, following Zacharias, Straatsma and
McCammon, J. Chem. Phys. 1994, 100, 9025.
2. Outline of the implementation
--------------------------------
In the following L denotes the coupling parameter lambda. Subscripts
_i and _f denote initial and final state respectively. The variables
de (ALAM) and dv (DLAM) can be set by the user; reasonable defaults (5
A^2) are used.
The functional form of the soft core routines in combination with PERT
is as follows:
U_LJ(L) = U_LJ,0 +
A_f B_f
L * (------------------- - --------------------) +
(r^2 + dv*(1-L))^6 (r^2 + dv*(1-L))^3
A_i B_i
(1-L) * (------------------- - --------------------) +
(r^2 + dv*L)^6 (r^2 + dv*L)^3
U_ELEC(L) = U_ELEC,0 +
qi_f*qj_f
L * (----------------------) +
sqrt(r^2 + de*(1-L))
qi_i*qj_i
(1-L) * (----------------------)
sqrt(r^2 + de*L)
U_DE(L) = U_DE,0 +
L * (A_f * exp(-a*(r/rm+(1-L)^6))-B_f*exp(-c*(r/rm+(1-L)^6)) +
(1-L) * (A_f * exp(-a*(r/rm+L^6))-B_f*exp(-c*(r/rm+L^6))
Of course, the effects of tapering functions (SHIF, SWIT etc.) have
to be taken into account properly; this is particularly important for
the calculation of the forces and of the derivative dU/dL
In principle, soft core potentials are only required for atoms that
'vanish' at one of the endpoints (i.e., dummy atoms). In this
implementation, a simpler approach was used: When PERT is activated,
the "environment" part (the part of the system that remains
unchanged), (2) one for the "reactant" part (interactions between
initial state atoms themselves and initial state atoms and the
environment), and (3) one for the "product" part (interactions between
final state atoms themselves and final state atoms and the
environment). All reactant and product list interactions are calculated
using soft core potentials. Since (see equations above) at the
endpoints the soft core expressions reduce to normal interactions, use
of the soft core potentials is equivalent to a modified
path, but the overall result of the free energy simulation is unchanged.
(Note: the effect on free energy components has not been explored
systematically!)
Obviously, using soft core potentials breaks the standard scheme how
PERT calculates dU(L)/dL since instead of
U(L) = U_0 + (1-L)*U_i + L*U_f ! standard PERT
we now have
U(L) = U_0 + (1-L)*U_i(L) + L*U_f(L) ! PERT/PSSP
with corresponding differences for dU/dL. One sees that the
standard PERT scheme gives approximately "half" of the required
derivative, but we still need the terms (1-L)*[dU_i(L)/dL] and
L*[dU_f(L)/dL]. The modified energy routines I use do these
additional calculations.
Summing up, modifications of the code were necessary in the
following three areas:
(a) Additions to the parser: PSSP/NOPSsp keywords, ALAM, DLAM
parameters; initializations and resets
(b) Modifications to subroutine EPERT itself, making (i) sure that the
correct energy subroutines are called if PSSP is active, and (ii) that
the additional contributions to dU/dL are temporarily stored and
added to the LJ and elec free energy contributions calculated in the
standard PERT way. To achieve (i), subroutines FASTST,
EVDW (enbonda.src) and EGROUP (enbondg.src) were modified slightly
as well.
(c) Special purpose nonbonded energy routines (based on the
standard slow energy routines) have been added to the file epert.src.
Currently only a subset of nonbonded options is supported (see below)
All new nonlocal variables (no arrays are needed!) have been added
in pert.fcm (epert.fcm is unchanged)
The outline given here together with the comments in the code
should make the inner workings of the PERT/PSSP code clear.
To quickly 'grep' for all changes, seach for lines(comments) starting
with Cpssp
For a description of how to use the new functionality, see the modified
PERT documentation and the new test cases.
3. Comments and present limitations
-----------------------------------
To the best of my knowledge, all reported uses of soft core potentials
in free energy simulations have been based on thermodynamic
integration (TI), not the "exponential formula" ("thermodynamic
perturbation", "free energy perturbation (FEP)"). The present
implementation also supports only TI. While the output claims to give
values obtained with the exponential formula (TP> lines in output
file), the reported values ARE W R O N G if soft core potentials are
used. This is similar to all cases when the constraint correction is
needed, which also only works with TI !!! At present, it is not clear
whether the exponential formula can be supported easily.
Only a limited subset of nonbonded options is supported at presented.
Nonsupported options are hopefully caught and should make CHARMM die.
Nevertheless, check against the following list:
At present, the following limitations apply:
* Only constant dielectric (CDIE)
* For group based cutoffs (GROU / VGROU), the following nonbonded options
are supported at present:
VDW (LJ) ELEC
-----------------------------
VSWI SWIT
VIPS EIPS
* For atom based cutoffs (ATOM / VATO), the following nonbonded options
are supported at present:
VDW (LJ) ELEC
-----------------------------
VIPS EIPS
VSWI SHIF
FSWI
EWAL (tradional or PME)
* When using Double Exponential (DE) potential for VDW interactions, VIPS or direct cutoff options are supported.
Finally, note that there is no support for parallel architectures.
4. Outlook / TODO
-----------------
* Support parallel architectures (someone else needs to do this, since
I have no hardware) -- this should probably postponed until a merge
with the standard slow energy routines
? All PERT/PSSP specific modifications could easily be put behind a
separate compilation flag (e.g., #if KEY_PSSP==1) if this were
desired.
* Support additional tapering functions: While it doesn't seem
necessary to support all combinations of nonbonded options in
CHARMM, support for FSHIft and RDIE is planned.
* Use the slow energy routines instead of special purpose routines in
epert.src. Further, maybe a merge with the existing soft core
routines in CHARMM (intended primarily for docking) is possible.
This would lead to a unified, general and flexible soft core
facility. Also, this would cure (maybe?) (most of) the parallel code
incompatibilities...
? Consider support of the exponential formula; if this cannot be
done easily, remove the output lines to avoid confusion.
Some details concerning the implementation of the PERT/PSSP code,
including present limitations:
1. Introduction
---------------
The PERT free energy module of CHARMM is based on a linear dependence
on the coupling parameter. While simplifying implementation, this
approach is prone to van der Waals endpoint problems. One widely used
method to overcome the van der Waals endpoint problem is the use of
soft core Lennard Jones and electrostatic interactions for those
energy terms that cause problems. Even for double expoenetial potential (DE)
that does not have endpoint singularity, a softcore treatment can help
the sampling without use expoential distribution of LAMBDA windows.
This capability has been added, following Zacharias, Straatsma and
McCammon, J. Chem. Phys. 1994, 100, 9025.
2. Outline of the implementation
--------------------------------
In the following L denotes the coupling parameter lambda. Subscripts
_i and _f denote initial and final state respectively. The variables
de (ALAM) and dv (DLAM) can be set by the user; reasonable defaults (5
A^2) are used.
The functional form of the soft core routines in combination with PERT
is as follows:
U_LJ(L) = U_LJ,0 +
A_f B_f
L * (------------------- - --------------------) +
(r^2 + dv*(1-L))^6 (r^2 + dv*(1-L))^3
A_i B_i
(1-L) * (------------------- - --------------------) +
(r^2 + dv*L)^6 (r^2 + dv*L)^3
U_ELEC(L) = U_ELEC,0 +
qi_f*qj_f
L * (----------------------) +
sqrt(r^2 + de*(1-L))
qi_i*qj_i
(1-L) * (----------------------)
sqrt(r^2 + de*L)
U_DE(L) = U_DE,0 +
L * (A_f * exp(-a*(r/rm+(1-L)^6))-B_f*exp(-c*(r/rm+(1-L)^6)) +
(1-L) * (A_f * exp(-a*(r/rm+L^6))-B_f*exp(-c*(r/rm+L^6))
Of course, the effects of tapering functions (SHIF, SWIT etc.) have
to be taken into account properly; this is particularly important for
the calculation of the forces and of the derivative dU/dL
In principle, soft core potentials are only required for atoms that
'vanish' at one of the endpoints (i.e., dummy atoms). In this
implementation, a simpler approach was used: When PERT is activated,
the "environment" part (the part of the system that remains
unchanged), (2) one for the "reactant" part (interactions between
initial state atoms themselves and initial state atoms and the
environment), and (3) one for the "product" part (interactions between
final state atoms themselves and final state atoms and the
environment). All reactant and product list interactions are calculated
using soft core potentials. Since (see equations above) at the
endpoints the soft core expressions reduce to normal interactions, use
of the soft core potentials is equivalent to a modified
path, but the overall result of the free energy simulation is unchanged.
(Note: the effect on free energy components has not been explored
systematically!)
Obviously, using soft core potentials breaks the standard scheme how
PERT calculates dU(L)/dL since instead of
U(L) = U_0 + (1-L)*U_i + L*U_f ! standard PERT
we now have
U(L) = U_0 + (1-L)*U_i(L) + L*U_f(L) ! PERT/PSSP
with corresponding differences for dU/dL. One sees that the
standard PERT scheme gives approximately "half" of the required
derivative, but we still need the terms (1-L)*[dU_i(L)/dL] and
L*[dU_f(L)/dL]. The modified energy routines I use do these
additional calculations.
Summing up, modifications of the code were necessary in the
following three areas:
(a) Additions to the parser: PSSP/NOPSsp keywords, ALAM, DLAM
parameters; initializations and resets
(b) Modifications to subroutine EPERT itself, making (i) sure that the
correct energy subroutines are called if PSSP is active, and (ii) that
the additional contributions to dU/dL are temporarily stored and
added to the LJ and elec free energy contributions calculated in the
standard PERT way. To achieve (i), subroutines FASTST,
EVDW (enbonda.src) and EGROUP (enbondg.src) were modified slightly
as well.
(c) Special purpose nonbonded energy routines (based on the
standard slow energy routines) have been added to the file epert.src.
Currently only a subset of nonbonded options is supported (see below)
All new nonlocal variables (no arrays are needed!) have been added
in pert.fcm (epert.fcm is unchanged)
The outline given here together with the comments in the code
should make the inner workings of the PERT/PSSP code clear.
To quickly 'grep' for all changes, seach for lines(comments) starting
with Cpssp
For a description of how to use the new functionality, see the modified
PERT documentation and the new test cases.
3. Comments and present limitations
-----------------------------------
To the best of my knowledge, all reported uses of soft core potentials
in free energy simulations have been based on thermodynamic
integration (TI), not the "exponential formula" ("thermodynamic
perturbation", "free energy perturbation (FEP)"). The present
implementation also supports only TI. While the output claims to give
values obtained with the exponential formula (TP> lines in output
file), the reported values ARE W R O N G if soft core potentials are
used. This is similar to all cases when the constraint correction is
needed, which also only works with TI !!! At present, it is not clear
whether the exponential formula can be supported easily.
Only a limited subset of nonbonded options is supported at presented.
Nonsupported options are hopefully caught and should make CHARMM die.
Nevertheless, check against the following list:
At present, the following limitations apply:
* Only constant dielectric (CDIE)
* For group based cutoffs (GROU / VGROU), the following nonbonded options
are supported at present:
VDW (LJ) ELEC
-----------------------------
VSWI SWIT
VIPS EIPS
* For atom based cutoffs (ATOM / VATO), the following nonbonded options
are supported at present:
VDW (LJ) ELEC
-----------------------------
VIPS EIPS
VSWI SHIF
FSWI
EWAL (tradional or PME)
* When using Double Exponential (DE) potential for VDW interactions, VIPS or direct cutoff options are supported.
Finally, note that there is no support for parallel architectures.
4. Outlook / TODO
-----------------
* Support parallel architectures (someone else needs to do this, since
I have no hardware) -- this should probably postponed until a merge
with the standard slow energy routines
? All PERT/PSSP specific modifications could easily be put behind a
separate compilation flag (e.g., #if KEY_PSSP==1) if this were
desired.
* Support additional tapering functions: While it doesn't seem
necessary to support all combinations of nonbonded options in
CHARMM, support for FSHIft and RDIE is planned.
* Use the slow energy routines instead of special purpose routines in
epert.src. Further, maybe a merge with the existing soft core
routines in CHARMM (intended primarily for docking) is possible.
This would lead to a unified, general and flexible soft core
facility. Also, this would cure (maybe?) (most of) the parallel code
incompatibilities...
? Consider support of the exponential formula; if this cannot be
done easily, remove the output lines to avoid confusion.
Top
PATCHING DUMMY SIDECHAINS FOR FREE ENERGY PERTURBATIONS
The command MKPRES has been introduced to write a PATCH for adding a dummy
sidechain onto a backbone with the goal of performing free energy calculations.
The command generates the list of needed dihedral angles and non-bonded
exclusions. Only the cross internal energy terms between the dummy sidechain
and the bakbone are introduced, the rest is generated from the normal generate
command. Basically, it is ok to use such a mixed topology (single vs dual)
by branching at the carbon CB. With this treatment, all the bonds and angles
are kept, some dihedrals may need to be turned off for statistical consistency
of the reference state (this requires some thinking by the user, sorry...).
It can be shown that free energy differences calculated with these end-points
are correct (even though the individual free energies are themselves different
than those with ideal gas of free particle in which all internal energy terms
are turned off). Proline is not supported by this method. Glycine might
be ok, but remain vigilant.
One can introduce dummy atoms, which retain all the covalent interactions,
in a "hybrid residue", in such a way that the influence of the bonded
interactions with dummy atoms do not influence the final free energy change.
The simulations thus can be done using a transformation protocol in which
all covalent bond contributions are maintained invariant throughout the
calculations; only the nonbonded interactions are varied.
The hybrid method is a scheme which retains some features of both the single
and dual topology techniques. The dummy atoms, which are covalently linked
to the protein in question, have no nonbonded interactions at one or the
other of the two end point reference states. The potential energy function
describing the transformation is constructed such that all internal energy
terms are invariant with respect to the thermodynamic coupling parameter
lambda. This simulation procedure therefore has similarities with both
the "single topology" and "dual topology" methods.
The coupling of the dummy atoms to the real atoms cancels out exactly from
the calculated free energy differences. The equivalence holds as long as
the coupling between the dummy atoms and the rest of the system satisfies
certain conditions. First, there can be only one bond between the dummy atoms
of a mutated residue and the real atoms in the rest of the system, because
multiple bonds would add spurious coupling between the real atoms. Second,
to avoid spurious coupling between the dummy atoms and the rest of the system,
there cannot be multiple bond angles and dihedral torsion angles between
the dummy atoms of a transformed residue and more than two real atoms in
the rest of the system.
The theoretical arguments explaining the approach have been elaborated in
the following references:
Boresch, S.; Karplus, M. J. Phys. Chem. A 1999, 103, 103-118.
Boresch, S.; Karplus, M. J. Phys. Chem. A 1999, 103, 119-136.
Shobana S.,B. Roux, and Olaf S. Andersen, J. Phys. Chem. B 2000, 104, 5179-5190
Syntax:
MKPRES {PatchName} unit <integer> atom_selection atom_selection atom_selection atom_selection
The four atom_selections correspond to the following pieces of the psf:
first: is the invariant backbone of state 0
second: is the mutated sidechain for state 0
third: is the invariant backbone of state 1
(normally this should correspond identically to the first selection)
fourth: is the mutated sidechain for state 1
Here is an example for liking a dummy valine to an alanine:
set Residue1 = ALA
set Residue2 = VAL
!first state
read sequence card
* residue1
3
ALA @Residue1 ALA
generate SEG1 setup
! second state (must have complete second segment to generate internal
! energy terms of second state)
read sequence card
* residue2
3
ALA @Residue2 ALA
generate SEG2 setup
define BACK select type CA .or. type HA* .or. type N .or. type HN .or. -
type C .or. type O .or. type HT* .or. type OT* .or. type CB show end
open write card unit 10 name mkpres.rtf
write title unit 10
** Patch for alchemical mutation of ALA to VAL
**
MKPRES @PatchName unit 10 -
select segid SEG1 .and. back end -
select segid SEG1 .and. resid 2 .and. (.not. back ) end -
select segid SEG2 .and. back end -
select segid SEG2 .and. resid 2 .and. (.not. back ) end
Two patches are written in unit 10. The first one is for real alanin/dummy
valine while the second patch turns the system into dummy alanine/real valine.
Please check your patch before lengthy calculations!
PATCHING DUMMY SIDECHAINS FOR FREE ENERGY PERTURBATIONS
The command MKPRES has been introduced to write a PATCH for adding a dummy
sidechain onto a backbone with the goal of performing free energy calculations.
The command generates the list of needed dihedral angles and non-bonded
exclusions. Only the cross internal energy terms between the dummy sidechain
and the bakbone are introduced, the rest is generated from the normal generate
command. Basically, it is ok to use such a mixed topology (single vs dual)
by branching at the carbon CB. With this treatment, all the bonds and angles
are kept, some dihedrals may need to be turned off for statistical consistency
of the reference state (this requires some thinking by the user, sorry...).
It can be shown that free energy differences calculated with these end-points
are correct (even though the individual free energies are themselves different
than those with ideal gas of free particle in which all internal energy terms
are turned off). Proline is not supported by this method. Glycine might
be ok, but remain vigilant.
One can introduce dummy atoms, which retain all the covalent interactions,
in a "hybrid residue", in such a way that the influence of the bonded
interactions with dummy atoms do not influence the final free energy change.
The simulations thus can be done using a transformation protocol in which
all covalent bond contributions are maintained invariant throughout the
calculations; only the nonbonded interactions are varied.
The hybrid method is a scheme which retains some features of both the single
and dual topology techniques. The dummy atoms, which are covalently linked
to the protein in question, have no nonbonded interactions at one or the
other of the two end point reference states. The potential energy function
describing the transformation is constructed such that all internal energy
terms are invariant with respect to the thermodynamic coupling parameter
lambda. This simulation procedure therefore has similarities with both
the "single topology" and "dual topology" methods.
The coupling of the dummy atoms to the real atoms cancels out exactly from
the calculated free energy differences. The equivalence holds as long as
the coupling between the dummy atoms and the rest of the system satisfies
certain conditions. First, there can be only one bond between the dummy atoms
of a mutated residue and the real atoms in the rest of the system, because
multiple bonds would add spurious coupling between the real atoms. Second,
to avoid spurious coupling between the dummy atoms and the rest of the system,
there cannot be multiple bond angles and dihedral torsion angles between
the dummy atoms of a transformed residue and more than two real atoms in
the rest of the system.
The theoretical arguments explaining the approach have been elaborated in
the following references:
Boresch, S.; Karplus, M. J. Phys. Chem. A 1999, 103, 103-118.
Boresch, S.; Karplus, M. J. Phys. Chem. A 1999, 103, 119-136.
Shobana S.,B. Roux, and Olaf S. Andersen, J. Phys. Chem. B 2000, 104, 5179-5190
Syntax:
MKPRES {PatchName} unit <integer> atom_selection atom_selection atom_selection atom_selection
The four atom_selections correspond to the following pieces of the psf:
first: is the invariant backbone of state 0
second: is the mutated sidechain for state 0
third: is the invariant backbone of state 1
(normally this should correspond identically to the first selection)
fourth: is the mutated sidechain for state 1
Here is an example for liking a dummy valine to an alanine:
set Residue1 = ALA
set Residue2 = VAL
!first state
read sequence card
* residue1
3
ALA @Residue1 ALA
generate SEG1 setup
! second state (must have complete second segment to generate internal
! energy terms of second state)
read sequence card
* residue2
3
ALA @Residue2 ALA
generate SEG2 setup
define BACK select type CA .or. type HA* .or. type N .or. type HN .or. -
type C .or. type O .or. type HT* .or. type OT* .or. type CB show end
open write card unit 10 name mkpres.rtf
write title unit 10
** Patch for alchemical mutation of ALA to VAL
**
MKPRES @PatchName unit 10 -
select segid SEG1 .and. back end -
select segid SEG1 .and. resid 2 .and. (.not. back ) end -
select segid SEG2 .and. back end -
select segid SEG2 .and. resid 2 .and. (.not. back ) end
Two patches are written in unit 10. The first one is for real alanin/dummy
valine while the second patch turns the system into dummy alanine/real valine.
Please check your patch before lengthy calculations!
Top
Details about the use of MFF-potentials in PERT:
The MMFP keyword makes it possible to modify (add/remove)
MMF-potentials during an alchemical PERT mutation. If the keyword was
specified when activating PERT, the original call to the MMFP routines
in the constant-energy section of EPERT (epert.src) is omitted.
Instead, two new calls to the MMFP routines, one in the lambda=0
section and one in the lambda=1 section, are used. It is an optional
command, so the original use of the MMFP potentials in PERT (as
constant energy terms, independent from lambda) is still available
(and the default behaviour). The possibility of lambda-dependent
MMF-potentials should facilitate free energy simulations where
auxiliary restraints are needed, such as calculations of absolute
binding free energies.
Note: It is *important* to choose a MAXGEO value
(see » mmfp ) appropriate for
the sum of all GEO restraints that will be set up *before* and *after*
the call to PERT.
The testcase 'pert-mmfp.inp' demonstrates the new functionality.
Details about the use of MFF-potentials in PERT:
The MMFP keyword makes it possible to modify (add/remove)
MMF-potentials during an alchemical PERT mutation. If the keyword was
specified when activating PERT, the original call to the MMFP routines
in the constant-energy section of EPERT (epert.src) is omitted.
Instead, two new calls to the MMFP routines, one in the lambda=0
section and one in the lambda=1 section, are used. It is an optional
command, so the original use of the MMFP potentials in PERT (as
constant energy terms, independent from lambda) is still available
(and the default behaviour). The possibility of lambda-dependent
MMF-potentials should facilitate free energy simulations where
auxiliary restraints are needed, such as calculations of absolute
binding free energies.
Note: It is *important* to choose a MAXGEO value
(see » mmfp ) appropriate for
the sum of all GEO restraints that will be set up *before* and *after*
the call to PERT.
The testcase 'pert-mmfp.inp' demonstrates the new functionality.
Top
Experimental support of "chemical paths" in PERT free energy simulations
(i.e., simulations in which a solute is decoupled from solvent or in
which a ligand is decoupled from the protein). CHARMM has to
be compiled with the CHEMPERT keyword in pref.dat for this functionality
to be available.
The CHEM keyword on the PERT commandline changes how energies and
forces are computed when PERT is active. (Note that there are no
provisions to turn this mode off other than specifying PERT OFF!)
Its intended use is as follows: Suppose you have a solute in SEGI SOLU
and water in SEGI WAT. Now specify
fast off ! important, otherwise SCALAR RSCA has no effect!!
! as of version 42 fast can be ON; it will autmatically
! be turned off for interactions with perturbed atoms if
! scalar RSCA is being used.
PERT sele segi SOLU end CHEM
scalar char set 0. sele segi SOLU end ! turn off solute charges
scalar rsca set 0. sele segi SOLU end ! turn off solute LJ interactions
Then lambda=0 corresponds to a fully interacting system and lambda=1
corresponds to water plus the "solute" in the gas phase. However, within
the SOLU segment (the solute) *all* interactions, in particular the
intramolecular nonbonded terms, are computed normally.
If the CHEM keyword were missing, then at lambda=1 no solute
intramolecular nonbonded interactions would be needed, requiring a
separate calculation correcting for this.
The code (should) work(s) with most nonbonded options, including EWALD
and PSSP soft-cores (note that these impose there own limitations
which nonbonded options can be used). The EWALD support is admittedly
a wild hack. Quite generally I do recommend to test correct
functionality by applying tests similarly to the new testcases
chempert1.inp and chempert2.inp adapted to one's particular system one
wishes to study.
Experimental support of "chemical paths" in PERT free energy simulations
(i.e., simulations in which a solute is decoupled from solvent or in
which a ligand is decoupled from the protein). CHARMM has to
be compiled with the CHEMPERT keyword in pref.dat for this functionality
to be available.
The CHEM keyword on the PERT commandline changes how energies and
forces are computed when PERT is active. (Note that there are no
provisions to turn this mode off other than specifying PERT OFF!)
Its intended use is as follows: Suppose you have a solute in SEGI SOLU
and water in SEGI WAT. Now specify
fast off ! important, otherwise SCALAR RSCA has no effect!!
! as of version 42 fast can be ON; it will autmatically
! be turned off for interactions with perturbed atoms if
! scalar RSCA is being used.
PERT sele segi SOLU end CHEM
scalar char set 0. sele segi SOLU end ! turn off solute charges
scalar rsca set 0. sele segi SOLU end ! turn off solute LJ interactions
Then lambda=0 corresponds to a fully interacting system and lambda=1
corresponds to water plus the "solute" in the gas phase. However, within
the SOLU segment (the solute) *all* interactions, in particular the
intramolecular nonbonded terms, are computed normally.
If the CHEM keyword were missing, then at lambda=1 no solute
intramolecular nonbonded interactions would be needed, requiring a
separate calculation correcting for this.
The code (should) work(s) with most nonbonded options, including EWALD
and PSSP soft-cores (note that these impose there own limitations
which nonbonded options can be used). The EWALD support is admittedly
a wild hack. Quite generally I do recommend to test correct
functionality by applying tests similarly to the new testcases
chempert1.inp and chempert2.inp adapted to one's particular system one
wishes to study.
Top
Since c29 CHARMM supports an isotropic Lennard-Jones long range
correction (lrc nonbonded option, #if KEY_LRVDW==1keyword in pref.dat). So far,
there is no support for this correction in connection with PERT.
In principle, this support has now been added; both the energy, as
well as the virial correction are supported. HOWEVER, because
of the way the LRC interfaces with the energy routines, the correction
is NOT computed correctly if LJ interactions are turned off by
scalar RSCA set 0. Thus, in the presumably most interesting
case, simulations where a solute or a ligand is decoupled from
the rest of the system (cf. CHEMical PERT above), the LRCorrection
cannot be computed in the most obvious manner. It is hoped that
full support can be added, but this will entail a rewrite of how
the LRC is computed in general.
"PERT-BLOCK Lambda Dynamics"
New code is added in current version so that PERT and BLOCK
lambda-dynamcs can be used together. Keyword QLDM of lambda-dynamcs
will trigger the mixture of PERT/BLOCK. No additional setup is required
as long as the traditional PERT and BLOCK setup is kept. FAST OFF is
recommended for this setup. The acdemic usage of this method will be
published shortly. -- H. Li and W. Yang
Since c29 CHARMM supports an isotropic Lennard-Jones long range
correction (lrc nonbonded option, #if KEY_LRVDW==1keyword in pref.dat). So far,
there is no support for this correction in connection with PERT.
In principle, this support has now been added; both the energy, as
well as the virial correction are supported. HOWEVER, because
of the way the LRC interfaces with the energy routines, the correction
is NOT computed correctly if LJ interactions are turned off by
scalar RSCA set 0. Thus, in the presumably most interesting
case, simulations where a solute or a ligand is decoupled from
the rest of the system (cf. CHEMical PERT above), the LRCorrection
cannot be computed in the most obvious manner. It is hoped that
full support can be added, but this will entail a rewrite of how
the LRC is computed in general.
"PERT-BLOCK Lambda Dynamics"
New code is added in current version so that PERT and BLOCK
lambda-dynamcs can be used together. Keyword QLDM of lambda-dynamcs
will trigger the mixture of PERT/BLOCK. No additional setup is required
as long as the traditional PERT and BLOCK setup is kept. FAST OFF is
recommended for this setup. The acdemic usage of this method will be
published shortly. -- H. Li and W. Yang