Electron-Phonon interaction and superconducting properties of Al

<html><head><title>Tutorial “eph”</title></head> <body bgcolor=“#ffffff”> <hr> <p>This lesson demonstrates how to obtain the following physical properties, for a metal : </p><ul> <li>the phonon linewidths (lifetimes) due to the electron-phonon interaction</li> <li>the Eliashberg spectral function</li> <li>the coupling strength</li> <li>the McMillan critical temperature</li> </ul> Here you will learn to use the electron-phonon coupling part of the anaddb utility. This implies a preliminary calculation of the electron-phonon matrix elements and phonon frequencies and eigenvectors, from a standard ABINIT phonon calculation, which will be reviewed succinctly.

<p>This lesson should take about 1 hour.

</p><h5>Copyright (C) 2005-2013 ABINIT group (MVer) <br> This file is distributed under the terms of the GNU General Public License, see ~abinit/COPYING or <a href=“http://www.gnu.org/copyleft/gpl.txt”> http://www.gnu.org/copyleft/gpl.txt </a>. <br> For the initials of contributors, see ~abinit/doc/developers/contributors.txt . </h5>

<br>  <h3><b>Content of lesson Elphon</b></h3>

<ul>

<li><a href="lesson_eph.html#E1">1</a> Calculation of the ground state and phonon structure of fcc Al.</li>
<li><a href="lesson_eph.html#E2">2</a> Merging of the 2DTE _DDB files using MRGDDB.</li>
<li><a href="lesson_eph.html#E3">3</a> Extraction and merging of the electron-phonon matrix elements using MRGGKK.</li>
<li><a href="lesson_eph.html#E4">4</a> Basic ANADDB calculation of electron-phonon quantities.</li>
<li><a href="lesson_eph.html#E5">5</a> Convergence tests of the integration techniques.</li>
<li><a href="lesson_eph.html#E6">6</a> Transport quantities within Boltzmann theory.</li>

</ul>

<hr>

<h3><b>1. Calculation of the ground state and phonon structure of fcc Al.</b> </h3> <h3> </h3>

<p> <i>Before beginning, you might consider making a different subdirectory to

work in.

Why not create “Work_eph” in ~abinit/tests/tutorespfn/Input ? </i> <br> </p>

<p> It is presumed that the user has already followed the Tutorials

    <a href="lesson_rf1.html" target="kwimg">RF1</a>

and <a href=“lesson_rf2.html” target=“kwimg”>RF2</a>, and understands the calculation of ground state and response function (phonon) properties with ABINIT.</p>

<p> The file ~abinit/tests/tutorespfn/Input/teph_1.files lists the file names and root names for the first run (GS+perturbations). You can copy it to the working directory. You can also copy the file ~abinit/tests/tutorespfn/Input/teph_1.in to your working directory. This is your input file.</p>

<li><i>cp ../teph_1.files . </i></li> <li><i>cp ../teph_1.in . </i></li>

<p>In order to save time, you should immediately start this run ; the input files will be examined later … </p>

<pre> ../../abinit < teph_1.files > tmp-log & </pre>

<p>The calculation is done using minimal values of a number of parameters, in order to make it tractable in a time appropriate for a tutorial. The results will be completely unconverged, but by the end of the lesson you should know how to improve the convergence.</p> <p>Edit the file teph_1.in. We now examine several variables. The kinetic energy cutoff <a

href="../input_variables/varbas.html#ecut"
target="kwimg">ecut</a> is a bit low, and the number of k-points

(determined by <a href=“../input_variables/varbas.html#ngkpt”

target="kwimg">ngkpt</a>) is much too low. Electron-phonon calculations

require a very precise determination of the Fermi surface of the metal. This implies a very dense k-point mesh, and the convergence of the grid must be checked. In our case, for Al, we will use a 4x4x4 k-point grid, but a converged calculation needs more than 16x16x16 points. This will be re-considered in section <a href=“lesson_eph.html#E5”>5</a>. The q-point grid will be 2x2x2, must be a sub-grid of the full k-point grid, and must contain Γ.</p>

<p> The value of <a

href="../input_variables/varbas.html#acell"
target="kwimg">acell</a> is fixed to a rounded value from experiment.

It too should be converged to get physical results (see <a

href="lesson_base3.html"
target="kwimg"> Tutorial 3</a>).</p>

<p> Note that the value of 1.0E-14 for <a

href="../input_variables/varbas.html#tolwfr"
target="kwimg">tolwfr</a> is tight, and could be even lower (down to

1.0E-20). This is because the wavefunctions determined will be included later explicitly in the matrix elements used in ANADDB (as opposed to only energy values or densities, which are averages of the wavefunctions over k-points and bands). </p>

<p> Two important variables for electron-phonon coupling calculations are <a

href="../input_variables/varfil.html#prtgkk"
target="kwimg">prtgkk</a> and <a
href="../input_variables/varrf.html#prepgkk"
target="kwimg">prepgkk</a>. The former

prints out files suffixed with GKK, which contain only the electron-phonon matrix elements. This means you can set <a

href="../input_variables/varfil.html#prtwf"
target="kwimg">prtwf</a> to 0 in the phonon calculations,

and avoid saving huge perturbed wavefunction files to disk (you need to keep the ground state with prtwf1 1). Prepgkk enforces the calculation of all the perturbations at a given q-point. For the moment this is always necessary, because of random phase factors in the matrix elements. </p>

<p> Run the first input (a few minutes on a PC), and you should obtain a value of <pre> etotal -2.0828579336121 Ha </pre> for the energy at the end of DATASET 1. The following datasets calculate the second order energy variations under atomic displacement in the three reduced directions of the fcc unit cell. This is done for three different phonons, Gamma, (1/2,0,0), and X, which generate the 2x2x2 q-point grid. The whole calculation follows the same lines as <a

href="lesson_rf1.html"

target=“kwimg”> Tutorial RF1</a>. As an example, DATASET 3 calculates the wavefunctions at k+q for k in the ground state k-point mesh, and q=(1/2,0,0). Then, DATASET 3 calculates <pre> 2DTE 0.80951882353353 </pre> for the second-order energy variation for movement of the (unique) atom along the first reduced direction for q=(1/2,0,0). The main differences with <a

href="lesson_rf1.html"
target="kwimg"> Tutorial RF1</a> are that

<ol> <li> given we are dealing with a metal, no perturbation wrt electric fields is considered ; However, if you want to do transport calculations, you need the ddk calculation anyway, to get the electron band velocities. This is added in dataset 5.</li> <li> all of the perturbations in the three directions (for each atom) must be done explicitly. This is enforced with the <a

href="../input_variables/varrf.html#prepgkk" target="kwimg">prepgkk</a>

input variable, as mentioned above.</li> </ol> In the standard case, ABINIT uses symmetry operations and non-stationary expressions to calculate a minimal number of 2DTE for different mixed second derivatives of the total energy. In our case we use the first derivatives, and they must all be calculated explicitly. </p>

<p> You are now the proud owner of 9 first-order matrix element files (suffixed _GKKx), corresponding to the three directional perturbations of the atom at each of the three q-points. The _GKK files contain the matrix elements of the electron-phonon interaction, which we will extract and use in the following. Besides the _GKK files there are the _DDB files for each perturbation which contain the 2DTE for the different phonons wavevectors q.</p>

<p></p>

<h3><b>2. Merging of the 2DTE _DDB files using MRGDDB.</b> </h3> <h3> </h3>

<p> You can copy the following content to a file teph_2.in within your working directory:</p> <pre> teph_2.ddb.out Total ddb for Al FCC system 3 teph_1o_DS2_DDB teph_1o_DS3_DDB teph_1o_DS4_DDB </pre> <p> This is your input file for the <a href=“../users/mrgddb_help.html”

target="kwimg">MRGDDB</a> utility, which will take the different _DDB

files and merge them into a single one which ANADDB will use to determine the phonon frequencies and eigenvectors. teph_2.in contains the name of the final file, a comment line, then the number of _DDB files to be merged and their names.</p>

</p><a href=“../users/mrgddb_help.html” target=“kwimg”>MRGDDB</a> is run with the command <pre> mrgddb < teph_2.in </pre> It runs in a few seconds.<p>

</p><h3><b>3. Extraction and merging of the electron-phonon matrix elements using MRGGKK.</b> </h3> <h3> </h3>

<p> A merge similar to that in the last section must be carried out for the electron-phonon matrix elements. This is done using the MRGGKK utility, and its input file is ~abinit/tests/tutorespfn/Input/teph_3.in, shown below <pre> teph_3o_GKK.bin # Name of output file 0 # binary (0) or ascii (1) output teph_1o_DS1_WFK # GS wavefunction file 0 9 9 # number of 1WF files, of GKK files, and of perturbations in the GKK files teph_1o_DS2_GKK1 # names of the 1WF then the (eventual) GKK files teph_1o_DS2_GKK2 …</pre> The matrix element sections of all the _GKK files will be extracted and concatenated into one (binary) file, here named teph_3o_GKK.bin. The following lines in teph_3.in give the output format (0 for binary), then the name of the ground state wavefunction file. The fourth line contains 3 integers, which give the number of _1WF files (which can also be used to salvage the GKK), the number of _GKK files, and the number of perturbations in the _GKK files. Thus, MRGGKK functions like <a

href="../users/mrgddb_help.html"
target="kwimg">MRGDDB</a>, and can merge _GKK files

which already contain several perturbations (q-points or atomic displacements). Finally, the names of the different _1WF and _GKK files are listed.</p>

<p> MRGGKK will run on this example in a few seconds. In more general cases, the runtime will depend on the size of the system, and for a large number of bands or k-points can extend up to 20 minutes or more. </p>

</p><p> </p><hr>

</p><h3><b>4. Basic ANADDB calculation of electron-phonon quantities.</b> </h3> <h3> </h3>

<p>The general theory of electron-phonon coupling and Eliashberg superconductivity is reviewed in <i>Theory of Superconducting Tc, P.B. Allen

and B. Mitrovic in Sol. State Phys. <b>37</b> (1982) ed. Ehrenreich,
Seitz, and Turnbull</i>. The first implementations similar to that in

ABINIT are those in <i>S.Y. Savrasov and D.Y. Savrasov, Phys. Rev. B

<b>54</b> 16487 (1996)</i> and <i>A.Y. Liu and A.A. Quong, Phys.
Rev. B <b>53</b> R7575-R7579 (1996)</i>.</p>

<p> File ~abinit/tests/tutorespfn/Input/teph_4.in contains the input needed by ANADDB to carry out the calculation of the electron-phonon quantities. ANADDB takes a files file, just like ABINIT, which tells it where to find the input, ddb, and gkk files, and what to name the output, thermodynamical output, and electron phonon output files. ~abinit/tests/tutorespfn/Input/teph_4.files is your files file for ANADDB. You can edit it now.</p>

<p> The new variables are at the head of the file: <pre> # turn on calculation of the electron-phonon quantities elphflag 1

# Path in reciprocal space along which the phonon linewidths # and band structure will be calculated nqpath 7 qpath 0.0 0.0 0.0 1/2 1/2 0.0 1 1 1 1/2 1/2 1/2 1/2 1/2 0.0 1/2 3/4 1/4 1/2 1/2 1/2

# Coulomb pseudopotential parameter mustar 0.136</pre> <a href=“../users/anaddb_help.html#elphflag” target=“kwimg”> elphflag</a> is a flag to turn on the calculation of the electron-phonon quantities. The first quantities which will be calculated are the phonon linewidths along a path in reciprocal space (exactly like the band structure in <a

href="lesson_base3.html#35"
target="kwimg">Lesson 3.5</a>). The path is specified by the variable

<a href=“../users/anaddb_help.html#qpath”

target="kwimg">qpath</a> giving the apexes of the path in reciprocal

space, which are usually special points of high symmetry. The number of points is given by <a href=“../users/anaddb_help.html#nqpath”

target="kwimg">nqpath</a>. The phonon linewidths are printed to a file

suffixed _LWD.</p>

<p>The phonon linewidths are proportional to the electron phonon coupling, and still depend on the phonon wavevector q. The other electron-phonon calculations which are presently implemented in ANADDB, in particular for superconductivity, determine isotropic quantities, which are averaged over the Fermi surface and summed over q-points. Integrating the coupling over reciprocal space, but keeping the resolution in the phonon mode's energy, one calculates the Eliashberg spectral function α²F. The α²F function is similar to the density of states of the phonons, but is weighted according to the coupling of the phonons to the electrons. It is output to a file with suffix _A2F, which is ready to be represented using any graphical software (Xmgr, matlab, OpenDX…). The first inverse moment of α²F gives the global coupling strength, or mass renormalization factor, λ. From λ, using the McMillan formula (<i>Phys. Rev. <b>167</b> 331-344 (1968)</i>) as modified by Allen and Dynes (<i>Phys. Rev. B <b>12</b> 905 (1975)</i>), ANADDB calculates the critical temperature for superconductivity. The formula contains an adjustable parameter μ which approximates the effect of Coulomb interactions, and is given by the input variable <a

href="../users/anaddb_help.html#mustar"
target="kwimg">mustar</a>. For Al with the k-point grid given and a

value of μ=0.136 the ANADDB output file shows the following values <pre> mka2f: lambda <omega^2> = 8.890935E-07 mka2f: lambda <omega^3> = 7.653347E-10 mka2f: lambda <omega^4> = 8.752205E-13 mka2f: lambda <omega^5> = 1.124640E-15 mka2f: isotropic lambda = 1.005830E+01 mka2f: omegalog = 1.706719E-04 (Ha) 5.389384E+01 (Kelvin) mka2f: input mustar = 1.360000E-01 mka2f: MacMillan Tc = 4.004565E-05 (Ha) 1.264540E+01 (Kelvin) </pre> As expected, this is a fairly bad estimation of the experimental value of 1.2 K. The coupling strength is severely overestimated (experiment gives 0.44), and the logarithmic average frequency is too low, but not nearly enough to compensate λ. Aluminum is a good case in which things can be improved, because its Fermi surface is isotropic (adapted to the approximations in the present version of ABINIT) and the coupling is weak.</p>

</p><p> </p><hr>

</p><h3><b>5. Convergence tests of the integration techniques.</b> </h3> <h3> </h3>

<p> In section <a href=“lesson_eph.html#E4”>4</a>, we used the default method for integration on the Fermi surface, which employs a smearing of the DOS and attributes Gaussian weights to each k-point as a function of its distance from the Fermi surface. Another efficient method of integration in k-space is the tetrahedron method, which is also implemented in ANADDB, and can be used by setting <a

href="../users/anaddb_help.html#telphint"
target="kwimg">telphint</a> = 0. In this case the k-point grid must be

specified explicitly in the input, repeating the variable <a

href="../users/anaddb_help.html#kptrlatt"
target="kwimg">kptrlatt</a> from the ABINIT output, so that ANADDB can

re-construct the different tetrahedra which fill the reciprocal unit cell. In the Gaussian case, the width of the smearing can be controlled using the input variable <a href=“../users/anaddb_help.html#elphsmear”

target="kwimg">elphsmear</a>. </p>

<p> To test our calculations, they should be re-done with a denser k-point grid and a denser q-point grid, until the results (α²F or λ) are converged. The value of <a

href="../users/anaddb_help.html#elphsmear"
target="kwimg">elphsmear</a> should also be checked, to make sure that

it does not affect results. Normally, the limit for a very small <a

href="../users/anaddb_help.html#elphsmear"
target="kwimg">elphsmear</a> and a very dense k-point grid is

the same as the value obtained with the tetrahedron method (which usually converges with a sparser k-point grid). </p>

<p>Edit input file ~abinit/tests/tutorespfn/Input/teph_5.in and you will see the main difference with teph_4.in is the choice of the tetrahedron integration method. If you are patient, save the output _LWD and _A2F files and run the full lesson again with a denser k-point grid (say, 6x6x6) and you will be able to observe the differences in convergence.</p>

<hr> <p><a name=“E6”></a><br> <h3><b>6. Transport quantities within Boltzmann theory.</b> </h3> <h3> </h3>

<p> The electron-phonon interaction is also responsible for the resistivity of normal metals and related phenomena. Even in a perfect crystal, interaction with phonons will limit electron life times (and vice versa). This can be calculated fairly simply using Boltzmann theory of transport with first order scattering by phonons (see, e.g., “Electrons and Phonons” by Ziman). </p> <p> The additional ingredient needed to calculate transport quantities (electrical resistivity, heat conductivity limited by electron-phonon coupling) is the Fermi velocity, ie the group velocity of a wavepacket of electrons placed at the Fermi surface. This is the “true” velocity the charge will move at, once you have displaced the Fermi sphere a little bit in k space (see, e.g. Ashcroft and Mermin as well). The velocity can be related simply to a commutator of the position, which is also used for dielectric response, using a DDK calculation (see <a href=“./lesson_rf1.html#5”>the Gamma point phonon tutorial</a>). The phonon calculation at Gamma need not include the electric field (this is a metal after all, so the effect on the phonons should be negligible), but we need an additional dataset to calculate the 3 DDK files along the 3 primitive directions of the unit cell. To be more precise, just as for the el-ph matrix elements, we do not need the perturbed wavefunctions, only the perturbed eigenvalues. Calculating the DDK derivatives with <a

href="../input_variables/varfil.html#prtgkk" target="kwimg">prtgkk</a>

set to 1 will output files named _GKKxx (xx=3*natom+1 to 3*natom+3) containing the matrix elements of the ddk perturbation (these are basically the first part of the normal DDK files for E field perturbation, without the wave function coefficients). </p> <p> The anaddb “files” file must specify where the ddk files are, so anaddb can calculate the Fermi velocities. It actually reads: <pre> teph_6.in teph_6.out teph_2.ddb.out moldyn teph_3o_GKK.bin teph.ep teph_6.ddk </pre> where the last line is the name of a small file listing the 3 DDK files to be used: <pre> teph_1_DS5_GKK4 teph_1_DS5_GKK5 teph_1_DS5_GKK6 </pre> The abinit input file teph_1.in already obtained the DDK files from the additional dataset, DS5, with the following lines of teph_1.in: <pre> tolwfr5 1.0d-14 qpt5 0 0 0 rfphon5 0 rfelfd5 2 </pre> Copy the additional .ddk file from the tutorespfn/Inputs directory, and run anaddb with the new “files” file. The input for teph_6 has added to teph_5.in the following 2 lines: <pre> ifltransport 1 ep_keepbands 1 </pre> and has produced a number of additional files: <ul> <li> *_A2F_TR* contain the equivalent Eliashberg spectral functions with Fermi speed factors. Integrating with appropriate functions of the phonon energy, one gets:</li> <li>the resistivity as a function of temperature (teph_6.out_ep_RHO and figure) and</li> <li>the thermal conductivity as a function of temperature (teph_6.out_ep_WTH) but ONLY the electronic contribution. You are still missing the phonon-phonon interactions, which limit the thermal conductivity beyond a few 100 K</li> </ul> </p> <img style=“width: 640px; height: 480px;” alt=“Resistivity of Al as a function of T” src=“images/teph_6_RHO.png” /> <p> The high T behavior is necessarily linear if you include only first order e-p coupling, and the inset shows the low T behavior, which is not a simple polynomial (with simple models it should be T^3 or T^5 - see Ashcroft and Mermin). See the Savrasov paper above for reference values in simple metals using well converged k- and q- point grids. </p> <p> Finally, note that the _RHO and _WTH files contain a series of tensor components, for the resistivity tensor (2 1 = y x or the current response along y when you apply an electric field along x). This is still in beta phase (as of August 2012) and only the diagonal terms should be taken seriously. </p>

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