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analysis.rst half done and some other minor changes
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Tools for analysis
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==================
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.. warning::
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TO BE UPDATED!
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This section explains how to use some tools of the package in order to analyse the data.
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There are two practical tools for which a self energy on the real axis is not needed, namely:
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* :meth:`dos_wannier_basis` for the density of states of the Wannier orbitals and
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* :meth:`partial_charges` for the partial charges according to the Wien2k definition.
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However, a real frequency self energy has to be provided by the user to use the methods:
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* :meth:`dos_parproj_basis` for the momentum-integrated spectral function including self energy effects and
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* :meth:`spaghettis` for the momentum-resolved spectral function (i.e. ARPES)
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.. warning::
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The package does NOT provide an explicit method to do an **analytic continuation** of the
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self energies and Green functions from Matsubara frequencies to the real frequancy axis!
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There are methods included e.g. in the :program:`ALPS` package, which can be used for these purposes. But
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be careful: All these methods have to be used very carefully!
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This package does NOT provide an explicit method to do an **analytic continuation** of the
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self energies and Green functions from Matsubara frequencies to the real frequency axis!
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There are methods included e.g. in the :program:`ALPS` package, which can be used for these purposes.
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Keep in mind that all these methods have to be used very carefully!
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The tools for analysis can be found in an extension of the :class:`SumkDFT` class and are
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loaded by importing the module :class:`SumkDFTTools`::
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Most conveniently, you have your self energy already stored as a real frequency :class:`BlockGf` object
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in a hdf5 file, which can be easily loaded::
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from pytriqs.applications.dft.sumk_dft_tools import *
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There are two practical tools for which you do not need a self energy on the real axis, namely the:
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* density of states of the Wannier orbitals,
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* partial charges according to the Wien2k definition.
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The self energy on the real frequency axis is necessary in computing the:
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* momentum-integrated spectral function including self-energy effects,
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* momentum-resolved spectral function (i.e. ARPES).
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The initialisation of the class is equivalent to that of the :class:`SumkDFT`
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class::
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SK = SumkDFTTools(hdf_file = filename)
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Note that all routines available in :class:`SumkDFT` are also available here.
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Routines without real-frequency self energy
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-------------------------------------------
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For plotting the
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density of states of the Wannier orbitals, you simply type::
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SK.check_input_dos(om_min, om_max, n_om)
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which produces plots between the real frequencies `om_min` and `om_max`, using a mesh of `n_om` points. There
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is an optional parameter `broadening` which defines an additional Lorentzian broadening, and has the default value of
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`0.01` by default.
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Since we can calculate the partial charges directly from the Matsubara Green's functions, we also do not need a
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real-frequency self energy for this purpose. The calculation is done by::
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ar = HDFArchive(SK.hdf_file)
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SK.put_Sigma([ ar['SigmaImFreq'] ])
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ar = HDFArchive(filename+'.h5','r')
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SigmaReFreq = ar['SigmaReFreq']
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del ar
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dm = SK.partial_charges()
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which calculates the partial charges using the data stored in the hdf5 file, namely the self energy, double counting, and
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chemical potential. Here we assumed that the final self energy is stored as `SigmaImFreq` in the archive.
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On return, `dm` is a list, where the list items correspond to the density matrices of all shells
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defined in the list `SK.shells`. This list is constructed by the Wien2k converter routines and stored automatically
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in the hdf5 archive. For the detailed structure of `dm`, see the reference manual.
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Routines with real-frequency self energy
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----------------------------------------
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In order to plot data including correlation effects on the real axis, one has to provide the real frequency self energy.
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Most conveniently, it is stored as a real frequency :class:`BlockGf` object in the hdf5 file::
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ar = HDFArchive(filename+'.h5','a')
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ar['SigmaReFreq'] = SigmaReFreq
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del ar
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.. note::
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What happens if one has a self energy only in text files...?
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You may also store it in text files. If all blocks of your self energy are of dimension 1x1, you store them in `fname_(block)0.dat` files. Here `(block)` is a block name (`up`, `down`, or combined `ud`). In the case when you have matrix blocks, you store them in `(i)_(j).dat` files, where `(i)` and `(j)` are the orbital indices, in the `fname_(block)` directory.
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@ -88,6 +46,57 @@ where:
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The chemical potential as well as the double counting correction were already read in the initialisation process.
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Initialisation
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--------------
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All tools described below are collected in an extension of the :class:`SumkDFT` class and are
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loaded by importing the module :class:`SumkDFTTools`::
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from pytriqs.applications.dft.sumk_dft_tools import *
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The initialisation of the class is equivalent to that of the :class:`SumkDFT`
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class::
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SK = SumkDFTTools(hdf_file = filename + '.h5')
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Note that all routines available in :class:`SumkDFT` are also available here.
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If required, the real frequency self energy is set with::
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SK.put_Sigma(Sigma_imp = [ SigmaReFreq ])
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Density of states of the Wannier orbitals
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-----------------------------------------
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For plotting the
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density of states of the Wannier orbitals, you simply type::
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SK.check_input_dos(om_min, om_max, n_om)
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which produces plots between the real frequencies `om_min` and `om_max`, using a mesh of `n_om` points. There
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is an optional parameter `broadening` which defines an additional Lorentzian broadening, and has the default value of
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`0.01` by default.
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Partial charges
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---------------
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Since we can calculate the partial charges directly from the Matsubara Green's functions, we also do not need a
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real-frequency self energy for this purpose. The calculation is done by::
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ar = HDFArchive(SK.hdf_file)
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SK.put_Sigma([ ar['SigmaImFreq'] ])
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del ar
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dm = SK.partial_charges()
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which calculates the partial charges using the data stored in the hdf5 file, namely the self energy, double counting, and
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chemical potential. Here we assumed that the final self energy is stored as `SigmaImFreq` in the archive.
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On return, `dm` is a list, where the list items correspond to the density matrices of all shells
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defined in the list `SK.shells`. This list is constructed by the Wien2k converter routines and stored automatically
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in the hdf5 archive. For the detailed structure of `dm`, see the reference manual.
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Correlated spectral function (with self energy)
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-----------------------------------------------
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With this self energy, we can now execute::
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SK.dos_partial(broadening=broadening)
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@ -103,6 +112,9 @@ The output is printed into the files
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* `DOScorr(sp)_proj(i)_(m)_(n).dat`: As above, but printed as orbitally-resolved matrix in indices
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`(m)` and `(n)`. For `d` orbitals, it gives the DOS seperately for, e.g., :math:`d_{xy}`, :math:`d_{x^2-y^2}`, and so on.
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Momentum resolved spectral function (with self energy)
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------------------------------------------------------
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Another quantity of interest is the momentum-resolved spectral function, which can directly be compared to ARPES
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experiments. We assume here that we already converted the output of the :program:`dmftproj` program with the
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converter routines (see :ref:`interfacetowien`). The spectral function is calculated by::
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@ -133,6 +133,10 @@ After this step, all the necessary information for the DMFT loop is
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stored in the hdf5 archive, where the string variable
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`Converter.hdf_filename` gives the file name of the archive.
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At this point you should use the method :meth:`dos_wannier_basis`
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contained in the module :class:`SumkDFTTools` to check the density of
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states of the Wannier orbitals (see :ref:`analysis`).
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You have now everything for performing a DMFT calculation, and you can
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proceed with :ref:`singleshot`.
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@ -18,7 +18,7 @@ Before doing the calculation, we have to intialize all the objects that we will
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to get the local quantities used in DMFT. It is initialized by::
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from pytriqs.applications.dft.sumk_dft import *
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SK = SumkDFT(hdf_file = filename)
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SK = SumkDFT(hdf_file = filename + '.h5')
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Setting up the impurity solver
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@ -36,9 +36,13 @@ Prerequisites
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First perform a standard :ref:`DFT+DMFT calculation <dftdmft_selfcons>` for your desired material and obtain the real-frequency self energy by doing an
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analytic continuation.
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.. note::
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It is crucial to perform the analytic continuation in such a way that the obtained real-frequency self energy is accurate around the Fermi energy as only its
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low energy structure influences the final results!
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.. warning::
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This package does NOT provide an explicit method to do an **analytic continuation** of
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self energies and Green functions from Matsubara frequencies to the real frequency axis!
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There are methods included e.g. in the :program:`ALPS` package, which can be used for these purposes.
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Keep in mind that all these methods have to be used very carefully. Especially for optics calculations
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it is crucial to perform the analytic continuation in such a way that the obtained real frequency self energy
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is accurate around the Fermi energy as low energy features strongly influence the final results!
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Besides the self energy the Wien2k files read by the transport converter (:meth:`convert_transport_input <pytriqs.applications.dft.converters.wien2k_converter.Wien2kConverter.convert_transport_input>`) are:
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* :file:`.struct`: The lattice constants specified in the struct file are used to calculate the unit cell volume.
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