The DFPT (respfn) code¶
This page complements the main abinit help file, for matters related to responses to perturbations computed with DFPT. It will be easier to discover the present file with the help of the DFPT1 tutorial.
0 Introducing the computation of responses¶
ABINIT can compute the response to different perturbations, and provide access to quantities that are second derivatives of total energy (2DTE) with respect to these perturbations. Presently, they can be of four types:
 phonons
 static homogeneous electric field
 strain
 magnetic field (coupling to the spin, not the orbital motion)
The physical properties connected to 2DTE with respect to perturbations (1) and (2) are the phonon dynamical matrices, the dielectric tensor, and the Born effective charges, while the additional strain perturbation (3), mixed with phonon and electric field leads to elastic constant, internal strain, and piezoelectricity. The magnetic field perturbation is a recent addition to ABINIT, and will not be detailed at present.
More functionalities of the computation of responses should be implemented sooner or later. Some third derivatives of the total energy (3DTE) are also implemented. The 3DTE might give phononphonon coupling, nonlinear electric response, anharmonic elastic constants, Gruneisen parameters,…
The basic quantities that ABINIT will compute are the firstorder derivatives of the wavefunctions (1WF) with respect to these perturbations. The later calculation of the 2DTE and 3DTE from these 1WF is an easy computational task: the construction of the 2DTE with respect to perturbations j1 and j2 involves mainly evaluating matrix elements between the 1WF of j1 and/or the 1WF of j2. More details on this technique can be found in [Gonze1997] and [Gonze1997a].
The calculation of the 1WF for a particular perturbation is done using a variational principle and an algorithm rather similar to the one used to find the unperturbed groundstate wavefunctions. Thus, a lot of technical details and parameters are the same for both groundstate and responsefunction calculations. This justifies the development of one unique code for these two classes of properties: many of the routines of abinit are common in these calculations, or had to be duplicated, but with relatively small modifications.
The ABINIT code performs a rather primitive analysis of the calculated 2DTEs. For example, it gives the phonon frequencies, electronic dielectric tensor and effective charges. But the main output of the code is the Derivative DataBase (DDB): a file that contains the set of all 2DTEs and 3DTEs calculated by the code. This DDB can be manipulated by the MRGDDB code, and fully analyzed by the Anaddb code. See the corresponding mrgddb help file and anaddb help file.
1 Description of perturbations¶
The perturbation of the phonon type is the displacement of one atom along one of the axis of the unit cell, by a unit of length (in reduced coordinates). It is characterized by two integer numbers and one wavevector. The two integer numbers are the number of the moved atom, which will be noted ipert, and the number of the axis of the unit cell, which will be noted idir.
Important
ipert for phonon perturbation can have values between 1 and natom, idir can have values between 1 and 3.
The set of all possible phonon perturbations for one wavevector has thus 3 * natom elements. From this basis set, all phonons can be constructed by linear combination. The set of atoms to be moved in one dataset of ABINIT is determined by the input variable rfatpol. The set of directions to be considered in one dataset of ABINIT is determined by the input variable rfdir. The wavevector to be considered in one dataset of ABINIT is determined by the input variables nqpt, qpt, and qptnrm.
The perturbations of the electric field type are
 the application of the homogeneous electric field along the axes of the reciprocal lattice
 the derivative of the Hamiltonian with respect to the electronic wavevector along the axes of the reciprocal lattice (which allows to compute derivatives of wavefunctions with respect to their wavevector), an auxiliary quantity needed before the application of the homogeneous electric field. The perturbation is the change of wavevector by dk in the Hamiltonian, hence the perturbation is referred to as the derivative dk perturbation (“ddk” perturbation).
 Note 1
 the ddk perturbation is defined as the derivative with respect to k in reduced coordinates; this is equivalent to applying a linear perturbation of strength 2\pi along the conjugate direction in real space. This statement comes from the derivation of the phase factor \exp(i2\pi kr) with respect to k in reduced coordinates.
 Note 2
 in case the electric field type perturbation is computed inside a finite electric field, the derivative of the Hamiltonian with respect to the electronic wavevector is not computed: everything is done by a finite difference technique. Also, the definition of the homogeneous electric field perturbation is not along the axes of the reciprocal lattice, but in cartesian coordinates. Sorry for the possible confusion …
These electrictype perturbations are also characterized by two numbers: ipert being natom + 1 for the ddk perturbation and natom + 2 for the electric field, and idir being 1, 2 or 3, as for phonon perturbations. Although the possibility of electric field characterized by a nonzero wavevector is envisioned for a future version of the code, at present only homogeneous fields are considered. So the wavevector of the electric field type perturbations is \Gamma (q=0).
The perturbations of the strain type are either an uniaxial strain or a shear strain. The strain perturbations are considered in cartesian coordinates (x,y,z). They are characterized by two numbers, with ipert being natom + 3 for the uniaxial strains, and natom + 4 for the shear strains, and idir describes the particular component.
Explicitly, for uniaxial strains:
 idir = 1 gives the xx strain perturbation,
 idir = 2 gives the yy strain perturbation,
 idir = 3 gives the zz strain perturbation,
while for shear strains:
 idir=1 gives the yz strain perturbation,
 idir=2 gives the xz perturbation,
 idir=3 gives the xy perturbation.
Note that the “rigidatom” elastic constants, as output of ABINIT, are those
obtained with frozen internal coordinates. The internal coordinate
relaxation, needed to give “physical” elastic constants can be handled through
the knowledge of the internal strain and dynamical matrix at \Gamma, in ANADDB.
Of course, if all the internal coordinate are fixed by symmetry, all the
internal strains vanish, and the “rigidatom” and “physical” elastic constants are equal.
Limitations of the present implementation (as of v5.7):
 Symmetry is presently used to skip redundant k points in the BZ sum, but not to skip redundant strain perturbations.
We also define the index of the perturbation, called pertcase, equal to idir + 3 * (ipert  1). Accordingly, pertcase runs from 1 to 3 * (natom + 4), and will be needed to identify output and input files, see section 6.
Summary
To summarize, the perturbations are characterized by two numbers, ipert from 1 to natom + 4, and idir, from 1 to 3, as well as one wavevector (that is gamma when a nonphonon perturbation is considered). A number called pertcase combines ipert and idir, and runs from 1 to 3 * (natom + 4).
The 2DTE, being derivative of the total energy with respect to two perturbations, will be characterized by two sets of (idir,ipert), or by two pertcase numbers, while 3DTE will need three such sets or pertcase numbers. In addition they will depend on one wavevector (for 2DTE) or two wavevectors (for 3DTE).
In the nonstationary implementation of the 2DTE, used for offdiagonal elements in ABINIT, the first pertcase corresponds to the perturbation that gives the derivative of the potential, and the second pertcase corresponds to the perturbation that gives the derivative of the wavefunctions.
2 Filenames and input of groundstate wavefunctions¶
The same ‘files’ file as for GS calculations is used for RF calculations. Actually, in the multidataset mode, one will be able to make in one ABINIT run, groundstate computations as well as responsefunction computations, so that the ‘files’ file must be the same.... The ‘input’ file will have many common input variables for these different cases, but also some separate ones.
Two groundstate wavefunction files might be needed:
 the file of groundstate wavefunctions at a set of wavevectors, named kpoints
 the file of groundstate wavefunctions at the corresponding k+q, where q is the wavevector of the perturbation
These files also contain the corresponding eigenvalues.
Note that the second file (k+q) will be identical to the first one (k), in the case of zerowavevector perturbation. Also, if the qwavevector maps the kpoint grid onto itself (q being the difference between points that belong to the grid), all the information on the k+q grid is contained in the k grid, a fact that ABINIT is able to exploit.
One should have a look at the input variables irdwfk, and irdwfq, for a description of the groundstate wavefunction file names generated from the root names provided in the ‘files’ file. In the multidataset mode, the following input variables will be relevant: getwfk, and getwfq. The file names of the groundstate wavefunction file follow the same convention as for the groundstate case. Thus, read the corresponding section of the abinit help file, if needed.
In the case of an electric field perturbation, the output 1WF of the corresponding ddk perturbation is needed as input. If the option rfelfd=1 is used, then the code will take care of doing first the derivative dk perturbation calculation, then write the 1WF at the correct place, as an output file, then begin the homogeneous field perturbation calculation. Usually, the use of rfelfd=1 is not recommended, as the ddk computation is the most often done with different parameters as the electric field perturbation, a dataset with rfelfd=2 being followed with a dataset with rfelfd=3.
The nomenclature for firstorder wavefunction files is also given in the abinit help file, but it is worth to specify it in more detail here. The root name is formed from the string of character in the third line of the ‘files’ file (for an input file) or the fourth line of the ‘files’ file (for an output file), that is complemented, in the multidataset mode, by ‘ _DS ‘ and the dataset number, and then, the string ‘ _1WF ‘ is added, followed by pertcase (the index of the perturbation). This gives, e.g., for a ‘files’ file whose fourth line is ‘/tmp/o’, for the dataset number 3, and a perturbation corresponding to the displacement of the second atom in the x direction (pertcase=4), the following name of the corresponding 1^{st}order wavefunction output file:
/tmp/o_DS3_1WF4
Such a file might be used as input of another computation, or of another dataset.
The relevant input variables are: ird1wf, and irdddk, as well as get1wf, and getddk, in the multidataset mode.
3 The use of symmetries¶
In order to understand correctly the behaviour of responsefunction runs, some information on the use of symmetries must be given.
Some perturbations (including their wavevector) may be invariant for some symmetries. The code is able to use symmetries to skip perturbations of which a symmetric has already been calculated (except in the case of strain perturbations). ABINIT is also able to use the symmetries that keeps the perturbations invariant, to reduce the number of k points needed for the sampling of electronic wavefunctions in the Brillouin zone (although this feature is not optimal yet). There is one exception to this, the ddk perturbation, for which the spatial symmetries cannot be used yet.
In any case, unlike for the groundstate, the input kpoint set for response function should NOT have been decreased by using spatial symmetries, prior to the loop over perturbations (see section 4). Only the timereversal symmetry, retained by calculations at q=0, ought to be used to decrease this input kpoint set. Considering each perturbation in turn, ABINIT will be able to select from this nonreduced set of kpoints, the proper kpoint set, automatically, by using the symmetries that leave each perturbation invariant.
Accordingly, the preferred way to generate the kpoint grid is of course to use the ngkpt or kptrlatt input variables, with different values of kptopt:
 kptopt = 1 for the ground state
 kptopt = 2 for response functions at q=0
 kptopt = 3 for response functions at nonzero q
4 Organisation of responsefunction computations¶
In agreement with the information provided in the previous sections, different cases can be distinguished.
When one considers the response to an atomic displacement with q=0, the following procedure is suggested:

first, a selfconsistent groundstate computation with the restricted set of kpoints in the Irreducible Brillouin Zone (with kptopt=1)

second, a selfconsistent responsefunction computation with the atomic displacement perturbation, with the half set of kpoints (with kptopt=2)
When one considers the response to an electric field (with q=0), the following procedure is suggested:

first, a selfconsistent groundstate computation with the restricted set of kpoints in the Irreducible Brillouin Zone (with kptopt=1)

second, a nonselfconsistent responsefunction computation of the d/dk perturbation, with the half set of kpoints (with kptopt=2, and iscf=3)

third, a selfconsistent responsefunction computation of the electric field perturbation, with the half set of kpoints (with kptopt=2)
When one considers the response to an atomic displacement in the special case where q connects kpoints that both belong to the special kpoint grid, the following procedure is suggested:

first, a selfconsistent groundstate computation with the restricted set of kpoints in the Irreducible Brillouin Zone (with kptopt=1)

second, a selfconsistent responsefunction computation of the atomic displacement perturbation, with the full set of kpoints (with kptopt=3)
When one considers the response to an atomic displacement for a general q point, the following procedure is suggested:

first, a selfconsistent groundstate computation with the restricted set of kpoints in the Irreducible Brillouin Zone (with kptopt=1)

second, a nonselfconsistent groundstate run with the set of k+q points, that might be reduced thanks to symmetries (with kptopt=1)

third, a selfconsistent responsefunction computation of the atomic displacement perturbation, with the full set of kpoints (with kptopt=3)
Of course, these different steps can be combined when a set of responses is looked for. In particular, the computations of responses at gamma, in the case where the full dynamical matrix as well as the dielectric tensor and the Born effective charges are needed, can be combined as follows:

first, a selfconsistent groundstate computation with the restricted set of kpoints in the Irreducible Brillouin Zone (with kptopt=1)

second, the three nonselfconsistent responsefunction computations (one for each direction) of the d/dk perturbation, with the half set of kpoints (with kptopt=2, and iscf=3)

third, all the selfconsistent responsefunction computations of the electric field perturbations and of the atomic displacements, with the half set of kpoints (with kptopt=2)
Still, computations of perturbations at different q wavevectors cannot be mixed. But they can follow the other computations. Supposing that perturbations at q=0 and a general q point are to be performed, they will be combined as follows:

first, a selfconsistent groundstate computation with the restricted set of kpoints in the Irreducible Brillouin Zone (with kptopt=1)

second, the three nonselfconsistent responsefunction computations (one for each direction) of the d/dk perturbation, with the half set of kpoints (with kptopt=2, and iscf=3)

third, all q=0 selfconsistent responsefunction computations of the electric field perturbations and of the atomic displacements, with the half set of kpoints (with kptopt=2)

fourth, a nonselfconsistent groundstate computation with the set of k+q points, that might be reduced thanks to symmetries (with kptopt=1)

fifth, the selfconsistent responsefunction computations of the atomic displacement perturbations with a q wavevector, with the full set of kpoints (with kptopt=3)
Note that the error in the 2DTE is linear in the groundstate wavefunction error (unlike the error due to the 1WFs). Moreover, a large prefactor is associated with this source of error (it can even cause cause the instability of the SCF procedure). As a consequence, the convergence of the groundstate wavefunction should be very good. The same is true at the level of the ddk wavefunctions.
As mentioned in the introduction, inside the responsefunction part of the code, the calculation proceeds in two steps: first the calculation of the firstorder derivative of the wavefunctions (1WF), then the combinations of these 1WF to build the 2DTE and 3DTE.
In an initialisation part, the input file and all the groundstate files are read, and a few basic quantities are constructed.
In the first part, every perturbation is examined, one at a time, separately:

A file containing previous RF wavefunctions is eventually read.

The minimisation of the variational expression is performed, and this procedure generates the 1WF as well as the firstorder density and potential.

It is possible, knowing these quantities for the perturbation ipert1, to construct all the 2DTE with respect to this perturbation and any ipert2, except for ipert2 being an homogeneous electric field, in which case the derivative of the groundstate wavefunctions with respect to their wavevector (ddk) is also needed. This feature has been implemented for ipert2 being any phonon (of the same wavevector than ipert1), or an homogeneous electric field.

The firstorder wavefunctions (1WF) are written as well as the firstorder density or potential (if requested).
5 List of relevant input variables¶
A subset of the ABINIT input variables have a modified meaning or a modified behaviour in case of RF calculations. Here is the list of these input variables, together with the variables that applies only to RF computations. Note that the code will do a RF calculation (optdriver=1) when one of rfphon or rfelfd is nonzero.
 amu
 getwfk, getwfq, get1wf, getddk
 irdwfk, irdwfq, ird1wf, irdddk
 iscf
 nkpt
 nqpt, qpt, qptnrm
 nsym
 rfasr
 rfatpol
 rfdir
 rfelfd
 rfphon
 dfpt_sciss
 tolwfr, toldfe, tolvrs
6 The different output files¶
Output from the code goes to several places listed below.
6.1. The log file
This file is the same as the log file of the abinit code when computing ground state (GS) results. Possibly, the output of datasets related to response functions will be intertwined with those concerned with groundstate case. The purpose of this file is the same as in the GS case, and the use of error messages is unchanged.
This file is the same as the main output file of the abinit code when computing ground state (GS) results. Possibly, the output of datasets related to response functions will be intertwined with those concerned with groundstate case. We explain here the parts related to the RF computation.
The initialisation part is the same as for the GS. So, the reader is advised to read the section 6.2 of the abinit help file, as well as the first paragraph of the section 6.3 of this file. Afterwards, the content of the main output file differs a bit…
The main output file reports on the initialisation of the groundstate wavefunctions at k+q, then the loop on the perturbations begins. For each perturbation, there is:
 a short description of the perturbation
 the timing information
 the report on the initialisation of the 1WF
 then the iterations for the minimisation begin, and the output file describes the number of the iteration, the second derivative of the total energy obtained (2DTEnergy in Ha), the change in 2DTEnergy since last iteration, the maximum residual over all bands and k points, and the square of the potential residual.
 after the iterations are completed, the residuals are reported
 in case of the derivative dk perturbation, ek2 (to be explained) and the fsum rule ratio value are printed. The fsum rule ratio should be close to 1 (not when ecutsm/=0, however).
 then the components of the 2DTEnergy, broken in at most 14 pieces, depending on the perturbation
 then the 2DTEnergy in Hartree and in eV
 then the relaxation contribution (caused by changes in wavefunctions), and the nonrelaxation contribution (Ewald and frozenwavefunction contribution)
 then the 2DTEnergy evaluated using a nonvariational expression.
After the computation of each perturbation, the output file reports on the 2DTE matrix elements. This part is not executed if the only perturbation is the derivative dk perturbation. It will give the following information:
 if prtvol=1 or bigger, the full detail of every contribution to the 2DTE in reduced coordinates.
 the 2DTE in reduced coordinates.
 then it will use the 2DTE to perform already some analysis of the data without use the Mrgddb and Anaddb codes, namely: the full dynamical matrix (cartesian coordinates, masses included) the effective charges, and the dielectric tensor, the phonon frequencies (including the analysis of the non analyticity if we are at \Gamma). Note that phonon frequencies lower than 1.0d8Ha (absolute value) are automatically set to zero, while imaginary phonon frequencies (square roots of negative eigenvalues  indicating an instability) are printed as negative (this facilitates the postprocessing).
For this last analysis, the code assumes that the whole set of perturbations in a class has been calculated, either all the phonon perturbations or the homogeneous electric field perturbation, or both. If this is not true, the code will give results that may be wrong in the case that the reduced system of coordinates is not cartesian (for the dynamical matrix, the effective charge tensor of the dielectric matrix), or in all case wrong (the phonon frequencies); also the code will put zero in the matrix elements that have not been calculated. A Warning message is issued if the above information cannot be trusted.
Finally, the code provides the timing information.
6.3. The firstorder wavefunction (1WF) files
These are unformatted data files containing the planewaves coefficients of all the wavefunctions, written in the following format. First, the header (see section 6.4 of the abinit help file), followed by
bantot=0 < counts over all bands
index=0 < index for the wavefunctions
do isppol=1,nsppol
do ikpt=1,nkpt
write(unit) npw1,nspinor,nband < for each k point
write(unit) kg(1:3,1:npw1) < plane wave reduced coordinates
do iband=1,nband1
write(unit) (eigen1(jband+(iband1)*nband+bantot),jband=1,2*nband) < column of eigenvalue matrix
write(unit) (cg(ii+index),ii=1,2*npw1*nspinor) < wavefunction coefficients
enddo for a single band and k point
bantot=bantot+nband
index=index+2*npw1*nspinor*nband1
enddo
enddo
In this code section, npw1(ikpt) is the number of planewaves in the basis at
the k+q point, nband1(ikpt) is likewise the number of bands at the k point
(which may vary among k points depending on occopt), and the factor of 2 in
writing the wavefunction results from the fact that it is complex.
eigen1 is the array that contains the matrix element of the firstorder
Hamiltonian between the different groundstate wavefunctions. It could be used
to build the electronphonon coupling and deformation potentials.
Note that the format for firstorder WF file differs from the format used for
the groundstate WF file by the fact that eigen1 is now an array, and no more
a vector, and is written with the corresponding wf, and no more before the
writing of all wf for one k point.
6.4. The firstorder density files
They consist of the header lines, followed by
write(unit) (rhor1(ir),ir=1,cplex*ngfft(1)*ngfft(2)*ngfft(3))
Here, rhor1 is the change of electron density in electrons/Bohr^3. The parameter cplex is 1 when q=0 and 2 when q/=0 . Indeed, for q=0, the density change is a real quantity, while it is complex in general when q/=0 .
6.5. The derivative database (DDB)
It is made of two parts. The first should allow one to unambiguously identify the run that has generated the DDB, while the second part contains the 2DTE, grouped by blocks of data.
Note that the DDB output of the ABINIT code can be merged with other DDBs as described in the Mrgddb help file.
The first part contains:
 the DDB version number (that defines the structure of the DDB)
 seven parameters needed for the dimensionning of the DDB file (natom, nkpt, nsppol, nsym, ntypat, occopt, and nband  or the array nband (nkpt* nsppol) if occopt=2)
 different information on the run that generated the 2DTE (acell,amu,ecut,iscf,ixc,kpt,kptnrm, ngfft,occ,rprim,dfpt_sciss,symrel,xred,tnons,typat,tolwfr,wtk,%ziontypat, as well as information on the pseudopotentials by means of their KleinmanBylander energies). These values are simply a transcription of the input data, or other simple internal parameters.
Note: the format and content of this first part of the DDBs have to be updated in the future …
The second part contains:
 the number of data blocks
 for each data block, the type of the block, its number of elements, and the list of elements.
The elements of a 2DTE block are described by 4 integers and 2 real numbers. The 2 first integers define a first perturbation in the form (idir1,ipert1), the two next define a second perturbation in the form (idir2,ipert2). The matrix element corresponds to the derivative of the total energy with respect to the parameters corresponding to these perturbations. The real numbers are the real and imaginary parts of the 2DTE. Sometimes, the code uses spatial symmetries, the timereversal symmetry, or even the permutation of first and second perturbations to deduce the value of noncomputed matrix elements. This behaviour might be improved, as it is sometimes confusing …
7 Numerical quality of the calculations¶
It is possible to get from the RF calculations essentially EXACT derivatives of the total energy with respect to perturbations. There is a published account of this fact in [Gonze1995]. An agreement of 8 digits or more was obtained in the comparison with finitedifference derivatives of GS data.
The accuracy of these calculations are thus entirely determined by the input parameters the user choose for the RF run, and the preparatory GS runs.
We will now review the convergence parameters, usually the same as for the GS calculations, indicating only the specific features related to RF calculations.
Input parameters that could influence the accuracy of the calculation are:
 ecut (the energy cutoff, that depends strongly on the pseudopotential)
 ixc (describing the exchangecorrelation functional)
 nkpt(or, more accurately, the Brillouin zone sampling, that can be determined alternatively by the inputs variables ngkpt or kptrlatt)
 one of the selfconsistent convergence tolerance parameters, toldfe, tolvrs, or tolwfr.
The input parameters ecut, ecutsm, ixc, intxc, the set of kwavevectors, as well as the related variables have to be the SAME in the groundstate calculations that go before a RF run and this RF run.
Namely: do not try to use groundstate wavefunction files produced with ecut=10Ha for a RF run with ecut=20Ha. In some cases, the code will complain and stop, but in other cases, it might simply produce garbage !
If the value of ngfft is input by hand, its value must also be equal in the GS and RF cases. ALWAYS use ngfft large enough to have boxcut=2 or larger, in order to avoid any FFT filter error. In the GS case, boxcut as small as 1.5 could be allowed in some cases. It is not allowed with RF calculations, because they are more sensitive to that error.
The convergence tests with respect to ecut, and the kpoint grid should be done carefully. This was already emphasized in the abinit help file and is re emphasized here. The user should test the convergence DIRECTLY on the property he or she is interested in. For example, if the user wants a phonon frequency accurate to 10 cm^1, he/she could be lead to do a full calculation (GS+RF) of phonons at 30Ha, then another full calculation at 35Ha, then another at 40Ha… It is an error to rely on tolerance on the total energy (for example 1mHa/atom) or geometry (accuracy of one part per thousand on the bond lengths) to draw ‘a priori’ conclusions on the convergence of other quantities, and not monitor the convergence of these directly. To be clear: if phonon frequencies are needed, check the convergence of phonon frequencies !
The user should note that for bands with very small occupancy in the metallic case as well as unoccupied bands for insulators, the ground state run preceeding response function runs will not necessarily converge these wavefunctions using usual groundstate tests such as toldfe or (better) tolvrs. To be sure that inaccuracies are not introduced into the response function calculation by poorly converged unoccupied bands, a separate run starting from a saved charge density (prtden=1 in the selfconsistent run) and using iscf=2 and tolwfr may be needed.