##########################################################################
#
# TRIQS: a Toolbox for Research in Interacting Quantum Systems
#
# Copyright (C) 2011 by M. Aichhorn, L. Pourovskii, V. Vildosola
#
# TRIQS is free software: you can redistribute it and/or modify it under the
# terms of the GNU General Public License as published by the Free Software
# Foundation, either version 3 of the License, or (at your option) any later
# version.
#
# TRIQS is distributed in the hope that it will be useful, but WITHOUT ANY
# WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS
# FOR A PARTICULAR PURPOSE. See the GNU General Public License for more
# details.
#
# You should have received a copy of the GNU General Public License along with
# TRIQS. If not, see <http://www.gnu.org/licenses/>.
#
##########################################################################
"""
Extension to the SumkDFT class with some analyiss tools
"""

import sys
from types import *
import numpy
from triqs.gf import *
import triqs.utility.mpi as mpi
from .symmetry import *
from .sumk_dft import SumkDFT
from scipy.integrate import *
from scipy.interpolate import *

if not hasattr(numpy, 'full'):
    # polyfill full for older numpy:
    numpy.full = lambda a, f: numpy.zeros(a) + f

class SumkDFTTools(SumkDFT):
    """
    Extends the SumkDFT class with some tools for analysing the data.
    """

    def __init__(self, hdf_file, h_field=0.0, mesh=None, beta=40, n_iw=1025, use_dft_blocks=False, dft_data='dft_input', symmcorr_data='dft_symmcorr_input',
                 parproj_data='dft_parproj_input', symmpar_data='dft_symmpar_input', bands_data='dft_bands_input',
                 transp_data='dft_transp_input', misc_data='dft_misc_input', cont_data='dft_contours_input'):
        """
        Initialisation of the class. Parameters are exactly as for SumKDFT.
        """

        SumkDFT.__init__(self, hdf_file=hdf_file, h_field=h_field, mesh=mesh, beta=beta, n_iw=n_iw,
                        use_dft_blocks=use_dft_blocks, dft_data=dft_data, symmcorr_data=symmcorr_data,
                        parproj_data=parproj_data, symmpar_data=symmpar_data, bands_data=bands_data,
                        transp_data=transp_data, misc_data=misc_data, cont_data=cont_data)

    # Uses .data of only GfReFreq objects.
    # Uses .data of only GfReFreq objects.
    def density_of_states(self, mu=None, broadening=None, mesh=None, with_Sigma=True, with_dc=True, proj_type=None, dosocc=False, save_to_file=True):
        """
        Calculates the density of states. The basis of the projected density of states is 
        specified by proj_type.
        Parameters
        ----------
        mu           : double, optional
                       Chemical potential, overrides the one stored in the hdf5 archive.
        broadening   : double, optional
                       Lorentzian broadening of the spectra. 
                       If not given, standard value of lattice_gf is used.
        mesh         : real frequency MeshType, optional
                       Omega mesh for the real-frequency Green's function. 
                       Given as parameter to lattice_gf.
        with_Sigma   : boolean, optional
                       If True, the self energy is used for the calculation. 
                       If false, the DOS is calculated without self energy.
        with_dc      : boolean, optional
                       If True the double counting correction is used.
        proj_type     : string, optional
                       Output the orbital-projected DOS type from the following options:
                       'wann'   - Wannier DOS calculated from the Wannier projectors
                       'vasp'   - Vasp orbital-projected DOS only from Vasp inputs
                       'wien2k' - Wien2k orbital-projected DOS from the wien2k theta projectors
                       'elk'    - Elk orbital-projected DOS only from Elk inputs
        dosocc       : boolean, optional
                       If True, the occupied DOS, DOSproj and DOSproj_orb will be returned.
                       The prerequisite of this option is to have calculated the band-resolved
                       density matrices generated by occupations().
        save_to_file : boolean, optional
                       If True, text files with the calculated data will be created.
        Returns
        -------
        DOS          : Dict of numpy arrays
                       Contains the full density of states.
        DOSproj      : Dict of numpy arrays
                       DOS projected to atoms. Empty if proj_type = None
        DOSproj_orb  : Dict of numpy arrays
                       DOS projected to atoms and resolved into orbital contributions.
                       Empty if proj_type = None
        """
        if(proj_type!=None):
            #assert proj_type in ('wann', 'vasp','wien2k','elk'), "'proj_type' must be either 'wann', 'vasp', 'wien2k', or 'elk'"
            assert proj_type in ('wann', 'vasp','wien2k',), "'proj_type' must be either 'wann', 'vasp', 'wien2k'"
            if(proj_type!='wann'):
                assert proj_type==self.dft_code, "proj_type must be from the corresponding dft inputs."

        if (with_Sigma):
            assert isinstance(self.Sigma_imp[0].mesh, MeshReFreq), "SumkDFT.mesh must be real if with_Sigma is True"
            mesh=self.Sigma_imp[0].mesh
        elif mesh is not None:
            assert isinstance(mesh, MeshReFreq), "mesh must be of form MeshReFreq"
            if broadening is None:
                broadening=0.001
        elif self.mesh is not None:
            assert isinstance(self.mesh, MeshReFreq), "self.mesh must be of form MeshReFreq"
            mesh=self.mesh
            if broadening is None:
                broadening=0.001
        else:
            assert 0, "ReFreqMesh input required for calculations without real frequency self-energy"
        mesh_val = numpy.linspace(mesh.w_min,mesh.w_max,len(mesh))
        n_om = len(mesh)
        om_minplot = mesh_val[0] - 0.001
        om_maxplot = mesh_val[-1] + 0.001

        #Read in occupations from HDF5 file if required
        if(dosocc):
            mpi.report('Reading occupations generated by self.occupations().')
            thingstoread = ['occik']
            subgroup_present, values_not_read = self.read_input_from_hdf(
                subgrp=self.misc_data, things_to_read=thingstoread)
            if len(values_not_read) > 0 and mpi.is_master_node:
            	raise ValueError(
                'ERROR: One or more necessary SumK input properties have not been found in the given h5 archive:', self.values_not_read)    

        #initialise projected DOS type if required
        spn = self.spin_block_names[self.SO]
        n_shells=1
        if (proj_type == 'wann'):
            n_shells = self.n_corr_shells
            gf_struct = self.gf_struct_sumk.copy()
            dims = [self.corr_shells[ish]['dim'] for ish in range(n_shells)]
            shells_type = 'corr'
        elif (proj_type == 'vasp'):
            n_shells=1
            gf_struct = [[(sp, list(range(self.proj_mat_csc.shape[2]))) for sp in spn]]
            dims = [self.proj_mat_csc.shape[2]]
            shells_type = 'csc'
        elif (proj_type == 'wien2k'):
            self.load_parproj()
            n_shells = self.n_shells
            gf_struct = [[(sp, self.shells[ish]['dim']) for sp in spn]
                             for ish in range(n_shells)]
            dims = [self.shells[ish]['dim'] for ish in range(n_shells)]
            shells_type = 'all'
#	#commented out for now - unsure this produces DFT+DMFT PDOS
#        elif (proj_type == 'elk'):
#            n_shells = self.n_shells
#            dims = [self.shells[ish]['dim'] for ish in range(n_shells)]
#            gf_struct = [[(sp, self.shells[ish]['dim']) for sp in spn]
#                             for ish in range(n_shells)]
#            things_to_read = ['band_dens_muffin']
#            subgroup_present, values_not_read =  self.read_input_from_hdf(
#                           subgrp=self.bc_data, things_to_read=things_to_read)
#            if len(values_not_read) > 0 and mpi.is_master_node:
#            	raise ValueError(
#                'ERROR: One or more necessary SumK input properties have not been found in the given h5 archive:', self.values_not_read)

        #set-up output arrays
        DOS = {sp: numpy.zeros([n_om],float) for sp in spn}
        DOSproj = [{} for ish in range(n_shells)]
        DOSproj_orb = [{} for ish in range(n_shells)]
        #set-up Green's function object
        if (proj_type != None):
          G_loc = []
          for ish in range(n_shells):
              glist = [GfReFreq(target_shape=(block_dim, block_dim), mesh=mesh)
                     for block, block_dim in gf_struct[ish]]
              G_loc.append(
                  BlockGf(name_list=spn, block_list=glist, make_copies=False))
              G_loc[ish].zero()
              dim = dims[ish]
              for sp in spn:
                  DOSproj[ish][sp] = numpy.zeros([n_om], float)
                  DOSproj_orb[ish][sp] = numpy.zeros(
                      [n_om, dim, dim], complex)

        #calculate the DOS
        ikarray = numpy.array(list(range(self.n_k)))
        for ik in mpi.slice_array(ikarray):
            G_latt_w = self.lattice_gf(
                ik=ik, mu=mu, broadening=broadening, mesh=mesh, with_Sigma=with_Sigma, with_dc=with_dc)
            G_latt_w *= self.bz_weights[ik]
            #output occupied DOS if nk inputted
            if(dosocc):
              for bname, gf in G_latt_w:
                G_latt_w[bname].data[:,:,:] *= self.occik[bname][ik]
            # DOS 
            for bname, gf in G_latt_w:
                DOS[bname] -= gf.data.imag.trace(axis1=1, axis2=2)/numpy.pi
            # Projected DOS:
            if (proj_type != None):
                for ish in range(n_shells):
                    tmp = G_loc[ish].copy()
                    tmp.zero()
                    tmp << self.proj_type_G_loc(G_latt_w, tmp, ik, ish, proj_type)
                    G_loc[ish] += tmp
        mpi.barrier()

        # Collect data from mpi:
        for bname in DOS:
            DOS[bname] = mpi.all_reduce(DOS[bname])
        # Collect data from mpi and put in projected arrays
        if(proj_type != None):
          for ish in range(n_shells):
              G_loc[ish] << mpi.all_reduce(G_loc[ish])
        # Symmetrize and rotate to local coord. system if needed:
          if((proj_type!='vasp') and (proj_type!='elk')):
            if self.symm_op != 0:
                if proj_type=='wann':
                    G_loc = self.symmcorr.symmetrize(G_loc)
                else:
                    G_loc = self.symmpar.symmetrize(G_loc)
            if self.use_rotations:
                for ish in range(n_shells):
                    for bname, gf in G_loc[ish]:
                        G_loc[ish][bname] << self.rotloc(
                            ish, gf, direction='toLocal',shells=shells_type)
        # G_loc can now also be used to look at orbitally-resolved quantities
          for ish in range(n_shells):
            for bname, gf in G_loc[ish]:  # loop over spins
                DOSproj[ish][bname] = -gf.data.imag.trace(axis1=1, axis2=2) / numpy.pi
                DOSproj_orb[ish][bname][
                      :, :, :] += (1.0j*(gf-gf.conjugate().transpose())/2.0/numpy.pi).data[:,:,:]

        # Write to files
        if save_to_file and mpi.is_master_node():
            for sp in spn:
                f = open('DOS_%s.dat' % sp, 'w')
                for iom in range(n_om):
                    f.write("%s    %s\n" % (mesh_val[iom], DOS[sp][iom]))
                f.close()
                # Partial
                if(proj_type!=None):
                  for ish in range(n_shells):
                    f = open('DOS_' + proj_type +  '_%s_proj%s.dat' % (sp, ish), 'w')
                    for iom in range(n_om):
                        f.write("%s    %s\n" %
                                (mesh_val[iom], DOSproj[ish][sp][iom]))
                    f.close()
                    # Orbitally-resolved
                    for i in range(dims[ish]):
                        for j in range(dims[ish]):
                            #For Elk with parproj - skip off-diagonal elements
                            #if(proj_type=='elk') and (i!=j): continue
                            f = open('DOS_' + proj_type + '_' + sp + '_proj' + str(ish) +
                                     '_' + str(i) + '_' + str(j) + '.dat', 'w')
                            for iom in range(n_om):
                                f.write("%s    %s    %s\n" % (
                                    mesh_val[iom], DOSproj_orb[ish][sp][iom, i, j].real,DOSproj_orb[ish][sp][iom, i, j].imag))
                            f.close()

        return DOS, DOSproj, DOSproj_orb


    def proj_type_G_loc(self, G_latt, G_inp, ik, ish, proj_type=None):
        """
        Internal routine which calculates the project Green's function subject to the 
        proj_type input.
        Parameters
        ----------
        G_latt   : Gf
                   block of lattice Green's functions to be projected/downfolded
        G_inp    : Gf
                   block of local Green's functions used as a template for G_proj
        ik       : integer
                   integer specifing k-point index.
        ish      : integer
                   integer specifing shell index.
        proj_type : string, optional
                   Output the orbital-projected DOS type from the following options:
                   'wann'   - Wannier DOS calculated from the Wannier projectors
                   'vasp'   - Vasp orbital-projected DOS only from Vasp inputs
                   'wien2k' - Wien2k orbital-projected DOS from the wien2k theta projectors
                   'elk'    - Elk orbital-projected DOS only from Elk inputs               
        Returns
        -------
        G_proj   : Gf
                   projected/downfolded lattice Green's function
                   Contains the band-resolved density matrices per k-point.
        """

        G_proj = G_inp.copy()
        if (proj_type == 'wann'):
           for bname, gf in G_proj:
              G_proj[bname] << self.downfold(ik, ish, bname,
                                G_latt[bname], gf)  # downfolding G
        elif (proj_type == 'vasp'):
           for bname, gf in G_latt:
              G_proj[bname] << self.downfold(ik, ish, bname, gf, G_proj[bname], shells='csc')
        elif (proj_type == 'wien2k'):
           tmp = G_proj.copy()
           for ir in range(self.n_parproj[ish]):
              tmp.zero()
              for bname, gf in tmp:
                 tmp[bname] << self.downfold(ik, ish, bname,
                                G_latt[bname], gf, shells='all', ir=ir)
              G_proj += tmp
#        elif (proj_type == 'elk'):
#           dim = self.shells[ish]['dim']
#           ntoi = self.spin_names_to_ind[self.SO]
#           for bname, gf in G_latt:
#              n_om = len(gf.data[:,0,0])
#              isp=ntoi[bname]
#              nst=self.n_orbitals[ik,isp]
#              #matrix multiply band resolved muffin density with
#              #diagonal of band resolved spectral function and fill diagonal of 
#              #DOSproj_orb orbital dimensions with the result for each frequency
#              bdm=self.band_dens_muffin[ik,isp,ish,0:dim,0:nst]
#              tmp=[numpy.matmul(bdm, gf.data[iom,:,:].diagonal())
#                         for iom in range(n_om)]
#              tmp=numpy.asarray(tmp)
#              tmp2 = numpy.zeros([n_om,dim,dim], dtype=complex)
#              if(dim==1):
#                  tmp2[:,0,0]=tmp[:,0]
#              else:
#                 [numpy.fill_diagonal(tmp2[iom,:,:],tmp[iom,:])
#                         for iom in range(n_om)]
#              G_proj[bname].data[:,:,:] = tmp2[:,:,:]

        return G_proj

    def load_parproj(self,data_type=None):
        """
        Internal routine which loads the n_parproj, proj_mat_all, rot_mat_all and 
        rot_mat_all_time_inv from parproj data from .h5 file.
        Parameters
        ----------
        data_type : string, optional
                    which data type desired to be read in. 
                    'band' - reads data converted by bands_convert()        
                    None - reads data converted by parproj_convert()
        """
        #read in the projectors
        things_to_read = ['n_parproj', 'proj_mat_all']
        if data_type == 'band':
            subgroup_present, values_not_read = self.read_input_from_hdf(
              subgrp=self.bands_data, things_to_read=things_to_read)
        else:
            subgroup_present, values_not_read = self.read_input_from_hdf(
              subgrp=self.parproj_data, things_to_read=things_to_read)
            if self.symm_op:
                self.symmpar = Symmetry(self.hdf_file, subgroup=self.symmpar_data)
        if len(values_not_read) > 0 and mpi.is_master_node:
            raise ValueError(
                'ERROR: One or more necessary SumK input properties have not been found in the given h5 archive:', self.values_not_read)
        #read general data
        things_to_read = ['rot_mat_all', 'rot_mat_all_time_inv']
        subgroup_present, values_not_read = self.read_input_from_hdf(
            subgrp=self.parproj_data, things_to_read=things_to_read)
        if len(values_not_read) > 0 and mpi.is_master_node:
            raise ValueError(
                'ERROR: One or more necessary SumK input properties have not been found in the given h5 archive:', self.values_not_read)

    def occupations(self, mu=None, with_Sigma=True, with_dc=True, save_occ=True):
        """
        Calculates the band resolved density matrices (occupations) from the Matsubara 
        frequency self-energy.
        Parameters
        ----------
        mu           : double, optional
                       Chemical potential, overrides the one stored in the hdf5 archive.
        with_Sigma   : boolean, optional
                       If True, the self energy is used for the calculation. 
                       If false, the DOS is calculated without self energy.
        with_dc      : boolean, optional
                       If True the double counting correction is used.
        save_occ     : boolean, optional
                       If True, saves the band resolved density matrix in misc_data.
        save_to_file : boolean, optional
                       If True, text files with the calculated data will be created.
        Returns
        -------
        occik        : Dict of numpy arrays
                       Contains the band-resolved density matrices per k-point.
        """

        if with_Sigma:
            mesh = self.Sigma_imp[0].mesh
        else:
            mesh = self.mesh
        assert isinstance(mesh, MeshImFreq), "SumkDFT.mesh must be real if with_Sigma is True or mesh is not given"

        if mu is None:
            mu = self.chemical_potential
        ntoi = self.spin_names_to_ind[self.SO]
        spn = self.spin_block_names[self.SO]
        occik = {}
        for sp in spn:
          #same format as gf.data ndarray  
          occik[sp] = [numpy.zeros([1, self.n_orbitals[ik, ntoi[sp]], self.n_orbitals[ik, ntoi[sp]]], numpy.double) for ik in range(self.n_k)]
        #calculate the occupations
        ikarray = numpy.array(range(self.n_k))
        for ik in range(self.n_k):
          G_latt = self.lattice_gf(
              ik=ik, mu=mu, with_Sigma=with_Sigma, with_dc=with_dc)
          for bname, gf in G_latt:
            occik[bname][ik][0,:,:] = gf.density().real
        # Collect data from mpi:
        for sp in spn:
          occik[sp] = mpi.all_reduce(occik[sp])
        mpi.barrier()
        #save to HDF5 file (if specified)
        if save_occ and mpi.is_master_node():
          things_to_save_misc = ['occik']
          # Save it to the HDF:
          ar = HDFArchive(self.hdf_file, 'a')
          if not (self.misc_data in ar):
            ar.create_group(self.misc_data)
          for it in things_to_save_misc:
            ar[self.misc_data][it] = locals()[it]
          del ar
        return occik

    # Uses .data of only GfReFreq objects.
    def spectral_contours(self, mu=None, broadening=None, mesh=None, plot_range=None, FS=True, with_Sigma=True, with_dc=True, proj_type=None, save_to_file=True):
        """
        Calculates the correlated spectral function at the Fermi level (relating to the Fermi
        surface) or at specific frequencies. 

        Parameters
        ----------
        mu           : double, optional
                       Chemical potential, overrides the one stored in the hdf5 archive.
        broadening   : double, optional
                       Lorentzian broadening of the spectra. 
                       If not given, standard value of lattice_gf is used.
        mesh         : real frequency MeshType, optional
                       Omega mesh for the real-frequency Green's function. 
                       Given as parameter to lattice_gf.
        plot_range   : list of double, optional
                       Sets the energy window for plotting to (plot_range[0],plot_range[1]). 
                       If not provided, the min and max values of the energy mesh is used.           
        FS           : boolean
                       Flag for calculating the spectral function at the Fermi level (omega ~ 0)
                       If False, the spectral function will be generated for each frequency within 
                       plot_range.
        with_Sigma   : boolean, optional
                       If True, the self energy is used for the calculation. 
                       If false, the DOS is calculated without self energy.
        with_dc      : boolean, optional
                       If True the double counting correction is used.
        proj_type    : string, optional
                       Output the orbital-projected A(k,w) type from the following:
                       'wann'   - Wannier A(k,w) calculated from the Wannier projectors                       
        save_to_file : boolean, optional
                       If True, text files with the calculated data will be created.

        Returns
        -------
        Akw          : Dict of numpy arrays
                       (Correlated) k-resolved spectral function
        pAkw      : Dict of numpy arrays
                       (Correlated) k-resolved spectral function projected to atoms. 
                       Empty if proj_type = None
        pAkw_orb  : Dict of numpy arrays
                       (Correlated) k-resolved spectral function projected to atoms and 
                       resolved into orbital contributions. Empty if proj_type = None
        """
        if(proj_type!=None):
            assert proj_type in ('wann'), "'proj_type' must be 'wann' if not None"
        #read in the energy contour energies and projectors
        things_to_read = ['n_k','bmat','BZ_n_k','BZ_iknr','BZ_vkl',
                          'n_orbitals', 'proj_mat', 'hopping']
        subgroup_present, values_not_read = self.read_input_from_hdf(
          subgrp=self.cont_data, things_to_read=things_to_read)
        if len(values_not_read) > 0 and mpi.is_master_node:
            raise ValueError(
                'ERROR: One or more necessary SumK input properties have not been found in the given h5 archive:', self.values_not_read)

        if mu is None:
            mu = self.chemical_potential
        if (with_Sigma):
            assert isinstance(self.Sigma_imp[0].mesh, MeshReFreq), "SumkDFT.mesh must be real if with_Sigma is True"
            mesh=self.Sigma_imp[0].mesh
        elif mesh is not None:
            assert isinstance(mesh, MeshReFreq), "mesh must be of form MeshReFreq"
            if broadening is None:
                broadening=0.001
        elif self.mesh is not None:
            assert isinstance(self.mesh, MeshReFreq), "self.mesh must be of form MeshReFreq"
            mesh=self.mesh
            if broadening is None:
                broadening=0.001
        else:
            assert 0, "ReFreqMesh input required for calculations without real frequency self-energy"
        mesh_val = numpy.linspace(mesh.w_min,mesh.w_max,len(mesh))
        n_om = len(mesh)
        om_minplot = mesh_val[0] - 0.001
        om_maxplot = mesh_val[-1] + 0.001
        #for Fermi Surface calculations
        if FS:
            dw = abs(mesh_val[1]-mesh_val[0])
            #ensure that a few frequencies around the Fermi level are included
            plot_range = [-2*dw, 2*dw]
            mpi.report('Generated A(k,w) will be evaluted at closest frequency to 0.0 in given mesh ')
        if plot_range is None:
            n_om = len(mesh_val[(mesh_val > om_minplot)&(mesh_val < om_maxplot)])
            mesh_val2 = mesh_val[(mesh_val > om_minplot)&(mesh_val < om_maxplot)]
        else:
            om_minplot = plot_range[0]
            om_maxplot = plot_range[1]
            n_om = len(mesh_val[(mesh_val > om_minplot)&(mesh_val < om_maxplot)])
            mesh_val2 = mesh_val[(mesh_val > om_minplot)&(mesh_val < om_maxplot)]
            #\omega ~= 0.0 index for FS file
            abs_mesh_val = [abs(i) for i in mesh_val2]
            jw=[i for i in range(len(abs_mesh_val)) if abs_mesh_val[i] == numpy.min(abs_mesh_val[:])]

        #calculate the spectral functions for the irreducible set of k-points
        [Akw, pAkw, pAkw_orb] = self.gen_Akw(mu=mu, broadening=broadening, mesh=mesh, \
                                plot_shift=0.0, plot_range=plot_range, \
                                shell_list=None, with_Sigma=with_Sigma, with_dc=with_dc, \
                                proj_type=proj_type)
   
        if save_to_file and mpi.is_master_node():
           spn = self.spin_block_names[self.SO]
           vkc = numpy.zeros(3, float)
           mesh_val2 = mesh_val[(mesh_val > om_minplot)&(mesh_val < om_maxplot)]
           if FS:
             n_om = 1
           else:
             n_om = len(mesh_val2)
           for sp in spn:
                # Open file for storage:
                for iom in range(n_om):
                  if FS:
                    f = open('Akw_FS_' + sp + '.dat', 'w')
                    jom=jw[0]
                  else:
                    f = open('Akw_omega_%s_%s.dat' % (iom, sp), 'w')
                    jom=iom
                  f.write("#Spectral function evaluated at frequency = %s\n" %mesh_val2[jom])
                  for ik in range(self.BZ_n_k):
                     jk=self.BZ_iknr[ik]
                     vkc[:] = numpy.matmul(self.bmat,self.BZ_vkl[ik,:])
                     f.write("%s    %s    %s    %s\n" % (vkc[0], vkc[1], vkc[2], Akw[sp][jk, jom]))
                  f.close()
           if (proj_type!=None):
                n_shells = len(pAkw[:])
                for iom in range(n_om):
                  for sp in spn:
                    for ish in range(n_shells):
                      if FS:
                        strng = 'Akw_FS' + '_' + proj_type + '_' + sp + '_proj' + str(ish)
                        jom=jw[0]
                      else:
                        strng = 'Akw_omega_' + str(iom) + '_' + proj_type + '_' + sp + '_proj' + str(ish)
                        jom=iom
                      f = open(strng + '.dat', 'w')
                      f.write("#Spectral function evaluated at frequency = %s\n" %mesh_val2[jom])
                      for ik in range(self.BZ_n_k):
                        jk=self.BZ_iknr[ik]
                        vkc[:] = numpy.matmul(self.bmat,self.BZ_vkl[ik,:])
                        f.write("%s    %s    %s    %s\n" % (vkc[0], vkc[1], vkc[2],
                                 pAkw[ish][sp][jk, jom]))
                      f.close()
                      dim=len(pAkw_orb[ish][sp][0, 0, 0, :])
                      for i in range(dim):
                        for j in range(dim):
                        #For Elk with parproj - skip off-diagonal elements
                          if(proj_type=='elk') and (i!=j): continue
                          strng2 = strng + '_' + str(i) + '_' + str(j)
                        # Open file for storage:
                          f = open(strng2 + '.dat', 'w')
                          for ik in range(self.BZ_n_k):
                             jk=self.BZ_iknr[ik]
                             vkc[:] = numpy.matmul(self.bmat,self.BZ_vkl[ik,:])
                             f.write("%s    %s    %s    %s\n" % (vkc[0], vkc[1], vkc[2],
                                    pAkw_orb[ish][sp][jk, jom, i, j]))
                          f.close()

        return Akw, pAkw, pAkw_orb

    # Uses .data of only GfReFreq objects.
    def spaghettis(self, mu=None, broadening=None, mesh=None, plot_shift=0.0, plot_range=None, shell_list=None, with_Sigma=True, with_dc=True, proj_type=None, save_to_file=True):
        """
        Calculates the k-resolved spectral function A(k,w) (band structure)

        Parameters
        ----------
        mu           : double, optional
                       Chemical potential, overrides the one stored in the hdf5 archive.
        broadening   : double, optional
                       Lorentzian broadening of the spectra.
                       If not given, standard value of lattice_gf is used.
        mesh         : real frequency MeshType, optional
                       Omega mesh for the real-frequency Green's function.
                       Given as parameter to lattice_gf.
        plot_shift   : double, optional
                       Offset for each A(k,w) for stacked plotting of spectra.
        plot_range   : list of double, optional
                       Sets the energy window for plotting to (plot_range[0],plot_range[1]). 
                       If not provided, the min and max values of the energy mesh is used.           
        shell_list   : list of integers, optional
                       Contains the indices of the shells of which the projected spectral function 
                       is calculated for. 
                       If shell_list = None and proj_type is not None, then the projected spectral 
                       function is calculated for all shells.
        with_Sigma   : boolean, optional
                       If True, the self energy is used for the calculation.
                       If false, the DOS is calculated without self energy.
        with_dc      : boolean, optional
                       If True the double counting correction is used.
        proj_type    : string, optional
                       Output the orbital-projected A(k,w) type from the following:
                       'wann'   - Wannier A(k,w) calculated from the Wannier projectors
                       'wien2k' - Wien2k orbital-projected A(k,w) from the wien2k theta projectors
        save_to_file : boolean, optional
                       If True, text files with the calculated data will be created.
        Returns
        -------
        Akw          : Dict of numpy arrays
                       (Correlated) k-resolved spectral function
        pAkw      : Dict of numpy arrays
                       (Correlated) k-resolved spectral function projected to atoms. 
                       Empty if proj_type = None
        pAkw_orb  : Dict of numpy arrays
                       (Correlated) k-resolved spectral function projected to atoms and 
                       resolved into orbital contributions. Empty if proj_type = None
        """

        #initialisation
        if(proj_type!=None):
            assert proj_type in ('wann', 'wien2k'), "'proj_type' must be either 'wann', 'wien2k'"
            if(proj_type!='wann'):
                assert proj_type==self.dft_code, "proj_type must be from the corresponding dft inputs."
        things_to_read = ['n_k', 'n_orbitals', 'proj_mat', 'hopping']
        subgroup_present, values_not_read = self.read_input_from_hdf(
            subgrp=self.bands_data, things_to_read=things_to_read)
        if len(values_not_read) > 0 and mpi.is_master_node:
            raise ValueError(
                'ERROR: One or more necessary SumK input properties have not been found in the given h5 archive:', self.values_not_read)
        if(proj_type=='wien2k'):
           self.load_parproj(data_type='band')

        if mu is None:
            mu = self.chemical_potential
        if (with_Sigma):
            assert isinstance(self.Sigma_imp[0].mesh, MeshReFreq), "SumkDFT.mesh must be real if with_Sigma is True"
            mesh=self.Sigma_imp[0].mesh
        elif mesh is not None:
            assert isinstance(mesh, MeshReFreq), "mesh must be of form MeshReFreq"
            if broadening is None:
                broadening=0.001
        elif self.mesh is not None:
            assert isinstance(self.mesh, MeshReFreq), "self.mesh must be of form MeshReFreq"
            mesh=self.mesh
            if broadening is None:
                broadening=0.001
        else:
            assert 0, "ReFreqMesh input required for calculations without real frequency self-energy"
        mesh_val = numpy.linspace(mesh.w_min,mesh.w_max,len(mesh))
        n_om = len(mesh)
        om_minplot = mesh_val[0] - 0.001
        om_maxplot = mesh_val[-1] + 0.001
        if plot_range is None:
            om_minplot = mesh_val[0] - 0.001
            om_maxplot = mesh_val[-1] + 0.001
        else:
            om_minplot = plot_range[0]
            om_maxplot = plot_range[1]
        n_om = len(mesh_val[(mesh_val > om_minplot)&(mesh_val < om_maxplot)])

        [Akw, pAkw, pAkw_orb] = self.gen_Akw(mu=mu, broadening=broadening, mesh=mesh, \
                                plot_shift=plot_shift, plot_range=plot_range, \
                                shell_list=shell_list, with_Sigma=with_Sigma, with_dc=with_dc, \
                                proj_type=proj_type)

        if save_to_file and mpi.is_master_node():
           mesh_val2 = mesh_val[(mesh_val > om_minplot)&(mesh_val < om_maxplot)]
           spn = self.spin_block_names[self.SO]
           for sp in spn:
                # Open file for storage:
                f = open('Akw_' + sp + '.dat', 'w')
                for ik in range(self.n_k):
                    for iom in range(n_om):
                        f.write('%s     %s      %s\n' %(ik, mesh_val2[iom], Akw[sp][ik, iom]))
                    f.write('\n')
                f.close()
           if (proj_type!=None):
                n_shells = len(pAkw[:])
                if shell_list==None:
                  shell_list=[ish for ish in range(n_shells)]
                for sp in spn:
                  for ish in range(n_shells):
                    jsh=shell_list[ish]
                    f = open('Akw_' + proj_type + '_' +
                                 sp + '_proj' + str(jsh) + '.dat', 'w')
                    for ik in range(self.n_k):
                       for iom in range(n_om):
                          f.write('%s     %s      %s\n' % (
                                 ik, mesh_val2[iom], pAkw[ish][sp][ik, iom]))
                       f.write('\n')
                    f.close()
                    #get orbital dimension from the length of dimension of the array
                    dim=len(pAkw_orb[ish][sp][0, 0, 0, :])
                    for i in range(dim):
                      for j in range(dim):
                        #For Elk with parproj - skip off-diagonal elements
                        if(proj_type=='elk') and (i!=j): continue
                        # Open file for storage:
                        f = open('Akw_' + proj_type + '_' + sp + '_proj' + str(jsh)
                                + '_' + str(i) + '_' + str(j) + '.dat', 'w')
                        for ik in range(self.n_k):
                            for iom in range(n_om):
                                f.write('%s     %s      %s\n' % (
                                            ik, mesh_val2[iom], pAkw_orb[ish][sp][ik, iom, i, j]))
                            f.write('\n')
                        f.close()

        return Akw, pAkw, pAkw_orb


    def gen_Akw(self, mu, broadening, mesh, plot_shift, plot_range, shell_list, with_Sigma, with_dc, proj_type):
        """
        Internal routine used by spaghettis and spectral_contours to Calculate the k-resolved spectral 
        function A(k,w). For advanced users only.

        Parameters
        ----------
        mu           : double
                       Chemical potential, overrides the one stored in the hdf5 archive.
        broadening   : double
                       Lorentzian broadening of the spectra.
        mesh         : real frequency MeshType, optional
                       Omega mesh for the real-frequency Green's function.
                       Given as parameter to lattice_gf.
        plot_shift   : double
                       Offset for each A(k,w) for stacked plotting of spectra.
        plot_range   : list of double
                       Sets the energy window for plotting to (plot_range[0],plot_range[1]).
        shell_list   : list of integers, optional
                       Contains the indices of the shells of which the projected spectral function
                       is calculated for.
                       If shell_list = None and proj_type is not None, then the projected spectral
                       function is calculated for all shells.
        with_Sigma   : boolean
                       If True, the self energy is used for the calculation.
                       If false, the DOS is calculated without self energy.
        with_dc      : boolean
                       If True the double counting correction is used.
        proj_type    : string
                       Output the orbital-projected A(k,w) type from the following:
                       'wann'   - Wannier A(k,w) calculated from the Wannier projectors
                       'wien2k' - Wien2k orbital-projected A(k,w) from the wien2k theta projectors
        Returns
        -------
        Akw          : Dict of numpy arrays
                       (Correlated) k-resolved spectral function
        pAkw      : Dict of numpy arrays
                       (Correlated) k-resolved spectral function projected to atoms.
                       Empty if proj_type = None
        pAkw_orb  : Dict of numpy arrays
                       (Correlated) k-resolved spectral function projected to atoms and
                       resolved into orbital contributions. Empty if proj_type = None
        """

        mesh_val = numpy.linspace(mesh.w_min,mesh.w_max,len(mesh))
        n_om = len(mesh)
        om_minplot = mesh_val[0] - 0.001
        om_maxplot = mesh_val[-1] + 0.001
        if plot_range is None:
            om_minplot = mesh_val[0] - 0.001
            om_maxplot = mesh_val[-1] + 0.001
        else:
            om_minplot = plot_range[0]
            om_maxplot = plot_range[1]
        n_om = len(mesh_val[(mesh_val > om_minplot)&(mesh_val < om_maxplot)])

        #set-up spectral functions
        spn = self.spin_block_names[self.SO]
        Akw = {sp: numpy.zeros([self.n_k, n_om], float) for sp in spn}
        pAkw = []
        pAkw_orb = []
        #set-up projected A(k,w) and parameters if required
        if (proj_type):
            if (proj_type == 'wann'):
                n_shells = self.n_corr_shells
                gf_struct = self.gf_struct_sumk.copy()
                dims = [self.corr_shells[ish]['dim'] for ish in range(n_shells)]
                shells_type = 'corr'
            elif (proj_type == 'wien2k'):
                n_shells = self.n_shells
                gf_struct = [[(sp, self.shells[ish]['dim']) for sp in spn]
                             for ish in range(n_shells)]
                dims = [self.shells[ish]['dim'] for ish in range(n_shells)]
                shells_type = 'all'
            #only outputting user specified parproj shells
            if shell_list!=None:
              for ish in shell_list:
                if(ish > n_shells) or (ish < 0):
                  raise IOError("indices in shell_list input do not correspond \
                                 to existing self.shells indices")
              n_shells = len(shell_list)
              mpi.report("calculating spectral functions for following user specified shell_list:")
              [mpi.report('%s : %s '%(ish, self.shells[ish])) for ish in shell_list]
            else:
              shell_list=[ish for ish in range(n_shells)]
            #projected Akw via projectors
            pAkw = [{} for ish in range(n_shells)]
            pAkw_orb = [{} for ish in range(n_shells)]
            #set-up Green's function object
            G_loc = []
            for ish in range(n_shells):
               jsh=shell_list[ish]
               dim = dims[ish]
               for sp in spn:
                  pAkw[ish][sp] = numpy.zeros([self.n_k, n_om], float)
                  pAkw_orb[ish][sp] = numpy.zeros([self.n_k, n_om, dim, dim], float)
               glist = [GfReFreq(target_shape=(block_dim, block_dim), mesh=mesh)
                   for block, block_dim in gf_struct[ish]]
               G_loc.append(
                   BlockGf(name_list=spn, block_list=glist, make_copies=False))
               G_loc[ish].zero()

        #calculate the spectral function
        ikarray = numpy.array(list(range(self.n_k)))
        for ik in mpi.slice_array(ikarray):
            G_latt_w = self.lattice_gf(ik=ik, mu=mu, broadening=broadening, mesh=mesh, with_Sigma=with_Sigma, with_dc=with_dc)
            # Non-projected A(k,w)
            for bname, gf in G_latt_w:
                Akw[bname][ik] = -gf.data[numpy.where((mesh_val > om_minplot) &
                                    (mesh_val < om_maxplot))].imag.trace(axis1=1, axis2=2)/numpy.pi
                # shift Akw for plotting stacked k-resolved eps(k) curves
                Akw[bname][ik] += ik * plot_shift
            #project spectral functions
            if (proj_type!=None):
                # Projected A(k,w):
                for ish in range(n_shells):
                    G_loc[ish].zero()
                    tmp = G_loc[ish].copy()
                    tmp.zero()
                    tmp << self.proj_type_G_loc(G_latt_w, tmp, ik, ish, proj_type)
                    G_loc[ish] += tmp
                # Rotate to local frame
                if (self.use_rotations):
                  for ish in range(n_shells):
                    jsh=shell_list[ish]
                    for bname, gf in G_loc[ish]:
                        G_loc[ish][bname] << self.rotloc(
                            jsh, gf, direction='toLocal', shells=shells_type)
                for ish in range(n_shells):
                    for bname, gf in G_loc[ish]:  # loop over spins
                        pAkw_orb[ish][bname][ik,:,:,:] = -gf.data[numpy.where((mesh_val > om_minplot) &
                                            (mesh_val < om_maxplot)),:,:].imag/numpy.pi
                        # shift pAkw_orb for plotting stacked k-resolved eps(k) curves
                        pAkw_orb[ish][sp][ik] += ik * plot_shift

        # Collect data from mpi
        mpi.barrier()
        for sp in spn:
          Akw[sp] = mpi.all_reduce(Akw[sp])
          if (proj_type):
            for ish in range(n_shells):
              pAkw_orb[ish][sp] = mpi.all_reduce(pAkw_orb[ish][sp])
              pAkw[ish][sp] = pAkw_orb[ish][sp].trace(axis1=2, axis2=3)
        mpi.barrier()

        return Akw, pAkw, pAkw_orb
        
    def partial_charges(self, mu=None, with_Sigma=True, with_dc=True):
        """
        Calculates the orbitally-resolved density matrix for all the orbitals considered in the input, consistent with
        the definition of Wien2k. Hence, (possibly non-orthonormal) projectors have to be provided in the partial projectors subgroup of
        the hdf5 archive.

        Parameters
        ----------

        with_Sigma : boolean, optional
                     If True, the self energy is used for the calculation. If false, partial charges are calculated without self-energy correction.
        mu : double, optional
             Chemical potential, overrides the one stored in the hdf5 archive.
        with_dc : boolean, optional
                  If True the double counting correction is used.

        Returns
        -------
        dens_mat : list of numpy array
                   A list of density matrices projected to all shells provided in the input.
        """
        assert self.dft_code in ('wien2k'), "This routine has only been implemented for wien2k inputs"

        things_to_read = ['dens_mat_below', 'n_parproj',
                          'proj_mat_all', 'rot_mat_all', 'rot_mat_all_time_inv']
        subgroup_present, values_not_read = self.read_input_from_hdf(
            subgrp=self.parproj_data, things_to_read=things_to_read)
        if len(values_not_read) > 0 and mpi.is_master_node:
            raise ValueError(
                'ERROR: One or more necessary SumK input properties have not been found in the given h5 archive:', self.values_not_read)
        if self.symm_op:
            self.symmpar = Symmetry(self.hdf_file, subgroup=self.symmpar_data)

        spn = self.spin_block_names[self.SO]
        ntoi = self.spin_names_to_ind[self.SO]
        # Density matrix in the window
        self.dens_mat_window = [[numpy.zeros([self.shells[ish]['dim'], self.shells[ish]['dim']], complex)
                                 for ish in range(self.n_shells)]
                                for isp in range(len(spn))]
        # Set up G_loc
        gf_struct_parproj = [[(sp, self.shells[ish]['dim']) for sp in spn]
                             for ish in range(self.n_shells)]
        G_loc = [BlockGf(name_block_generator=[(block, GfImFreq(target_shape=(block_dim, block_dim), mesh=self.mesh))
                                                for block, block_dim in gf_struct_parproj[ish]], make_copies=False)
                    for ish in range(self.n_shells)]
        for ish in range(self.n_shells):
            G_loc[ish].zero()

        ikarray = numpy.array(list(range(self.n_k)))
        for ik in mpi.slice_array(ikarray):

            G_latt_iw = self.lattice_gf(ik=ik, mu=mu, with_Sigma=with_Sigma, with_dc=with_dc)
            G_latt_iw *= self.bz_weights[ik]
            for ish in range(self.n_shells):
                tmp = G_loc[ish].copy()
                for ir in range(self.n_parproj[ish]):
                    for bname, gf in tmp:
                        tmp[bname] << self.downfold(ik, ish, bname, G_latt_iw[
                                                    bname], gf, shells='all', ir=ir)
                    G_loc[ish] += tmp

        # Collect data from mpi:
        for ish in range(self.n_shells):
            G_loc[ish] << mpi.all_reduce(G_loc[ish])
        mpi.barrier()

        # Symmetrize and rotate to local coord. system if needed:
        if self.symm_op != 0:
            G_loc = self.symmpar.symmetrize(G_loc)
        if self.use_rotations:
            for ish in range(self.n_shells):
                for bname, gf in G_loc[ish]:
                    G_loc[ish][bname] << self.rotloc(
                        ish, gf, direction='toLocal', shells='all')

        for ish in range(self.n_shells):
            isp = 0
            for bname, gf in G_loc[ish]:
                self.dens_mat_window[isp][ish] = G_loc[ish].density()[bname]
                isp += 1

        # Add density matrices to get the total:
        dens_mat = [[self.dens_mat_below[ntoi[spn[isp]]][ish] + self.dens_mat_window[isp][ish]
                     for ish in range(self.n_shells)]
                    for isp in range(len(spn))]

        return dens_mat

    def print_hamiltonian(self):
        """
        Prints the Kohn-Sham Hamiltonian to the text files hamup.dat and hamdn.dat (no spin orbit-coupling), or to ham.dat (with spin-orbit coupling).
        """

        if self.SP == 1 and self.SO == 0:
            f1 = open('hamup.dat', 'w')
            f2 = open('hamdn.dat', 'w')
            for ik in range(self.n_k):
                for i in range(self.n_orbitals[ik, 0]):
                    f1.write('%s    %s\n' %
                             (ik, self.hopping[ik, 0, i, i].real))
                for i in range(self.n_orbitals[ik, 1]):
                    f2.write('%s    %s\n' %
                             (ik, self.hopping[ik, 1, i, i].real))
                f1.write('\n')
                f2.write('\n')
            f1.close()
            f2.close()
        else:
            f = open('ham.dat', 'w')
            for ik in range(self.n_k):
                for i in range(self.n_orbitals[ik, 0]):
                    f.write('%s    %s\n' %
                            (ik, self.hopping[ik, 0, i, i].real))
                f.write('\n')
            f.close()