phtavncSilePHtrans

class sisl.io.tbtrans.phtavncSilePHtrans(filename, mode='r', lvl=0, access=1, *args, **kwargs)[source]

PHtrans file object

Attributes

E

Sampled energy-points in file

a_buf

Atomic indices (0-based) of device atoms

a_dev

Atomic indices (0-based) of device atoms

base_file

File of the current Sile

cell

Unit cell in file

chemical_potential

current

current_parameter

elecs

List of electrodes

electron_temperature

fano

file

File of the current Sile

geom

The associated geometry from this file

geometry

The associated geometry from this file

k

Sampled k-points in file

kpt

Sampled k-points in file

lasto

Last orbital of corresponding atom

nE

Number of energy-points in file

na

Returns number of atoms in the cell

na_b

Number of atoms in the buffer region

na_buffer

Number of atoms in the buffer region

na_d

Number of atoms in the device region

na_dev

Number of atoms in the device region

na_u

Returns number of atoms in the cell

ne

Number of energy-points in file

nk

Number of k-points in file

nkpt

Always return 1, this is to signal other routines

no

Returns number of orbitals in the cell

no_d

Number of orbitals in the device region

no_u

Returns number of orbitals in the cell

noise_power

o_dev

Orbital indices (0-based) of device orbitals

shot_noise

wk

Weights of k-points in file

wkpt

Always return [1.], this is to signal other routines

xa

Atomic coordinates in file

xyz

Atomic coordinates in file

Methods

ADOS(self[, elec, E, kavg, atom, orbital, …])

Spectral density of states (DOS) (1/eV).

Adensity_matrix(self, elec, E[, kavg, isc, …])

Spectral function density matrix at energy E (1/eV)

BDOS(self[, elec, E, kavg, sum, norm])

Bulk density of states (DOS) (1/eV).

DOS(self[, E, kavg, atom, orbital, sum, norm])

Green function density of states (DOS) (1/eV).

Eindex(self, E)

Return the closest energy index corresponding to the energy E

__init__(self, filename[, mode, lvl, access])

Initialize self.

a2p(self, atom)

Return the pivoting orbital indices (0-based) for the atoms

atom_ACOHP(self, elec, E[, kavg, isc, uc])

Atomic COHP curve of the spectral function

atom_ACOOP(self, elec, E[, kavg, isc, uc])

Atomic COOP curve of the spectral function

atom_COHP(self, E[, kavg, isc, uc])

Atomic COHP curve of the Green function

atom_COHP_from_orbital(self, COHP[, uc])

Calculate the atomic COHP curve from the orbital COHP

atom_COOP(self, E[, kavg, isc, uc])

Atomic COOP curve of the Green function

atom_COOP_from_orbital(self, COOP[, uc])

Calculate the atomic COOP curve from the orbital COOP

atom_current(self, elec, E[, kavg, activity])

Atomic current of atoms

atom_current_from_orbital(self, Jij[, activity])

Atomic current of atoms by passing the orbital current

bond_current(self, elec, E[, kavg, isc, …])

Bond-current between atoms (sum of orbital currents)

bond_current_from_orbital(self, Jij[, only, uc])

Bond-current between atoms (sum of orbital currents) from an external orbital current

btd(self[, elec])

Block-sizes for the BTD method

close(self)

density_matrix(self, E[, kavg, isc, geometry])

Density matrix from the Green function at energy E (1/eV)

dir_file(self[, filename])

File of the current Sile

eta(self[, elec])

The imaginary part used when calculating the self-energies in eV (or for the device

exist(self)

Query whether the file exists

info(self[, elec])

Information about the calculated quantities available for extracting in this file

iter(self[, group, dimension, variable, …])

Iterator on all groups, variables and dimensions.

kT(self, elec)

Electron bath temperature [eV]

kindex(self, k)

Return the index of the k-point that is closests to the queried k-point (in reduced coordinates)

mu(self, elec)

Return the chemical potential associated with the electrode elec

n_btd(self[, elec])

Number of blocks in the BTD partioning

norm(self[, atom, orbital, norm])

Normalization factor depending on the input

o2p(self, orbital)

Return the pivoting indices (0-based) for the orbitals

orbital_ACOHP(self, elec, E[, kavg, isc])

Orbital resolved COHP analysis of the spectral function

orbital_ACOOP(self, elec, E[, kavg, isc])

Orbital COOP analysis of the spectral function

orbital_COHP(self, E[, kavg, isc])

Orbital resolved COHP analysis of the Green function

orbital_COOP(self, E[, kavg, isc])

Orbital COOP analysis of the Green function

orbital_current(self, elec, E[, kavg, isc, only])

Orbital current originating from elec as a sparse matrix

pivot(self[, in_device, sort])

Pivoting orbitals for the full system

read(self, \*args, \*\*kwargs)

Generic read method which should be overloaded in child-classes

read_data(self, \*args, \*\*kwargs)

Read specific type of data.

read_geometry(self, \*args, \*\*kwargs)

Returns Geometry object from this file

read_supercell(self)

Returns SuperCell object from this file

reflection(self[, elec, kavg, from_single])

Reflection into electrode elec

transmission(self[, elec_from, elec_to, kavg])

Transmission from elec_from to elec_to.

transmission_bulk(self[, elec, kavg])

Bulk transmission for the elec electrode

transmission_eig(self[, elec_from, elec_to, …])

Transmission eigenvalues from elec_from to elec_to.

vector_current(self, elec, E[, kavg, only])

Vector for each atom describing the mean path for the current travelling through the atom

vector_current_from_bond(self, Jab)

Vector for each atom being the sum of bond-current times the normalized bond between the atoms

write(self, \*args, \*\*kwargs)

Generic write method which should be overloaded in child-classes

write_geometry(self, \*args, \*\*kwargs)

This is not meant to be used

write_tbtav(self, \*args, \*\*kwargs)

Wrapper for writing the k-averaged TBT.AV.nc file.

ADOS(self, elec=0, E=None, kavg=True, atom=None, orbital=None, sum=True, norm='none')

Spectral density of states (DOS) (1/eV).

Extract the spectral DOS from electrode elec on a selected subset of atoms/orbitals in the device region

\[\mathrm{ADOS}_\mathfrak{el}(E) = \frac{1}{2\pi N} \sum_{\nu\in \mathrm{atom}/\mathrm{orbital}} [\mathbf{G}(E)\Gamma_\mathfrak{el}\mathbf{G}^\dagger]_{\nu\nu}(E)\]

The normalization constant (\(N\)) is defined in the routine norm and depends on the arguments.

Parameters
elec: str, int, optional

electrode originating spectral function

Efloat or int, optional

optionally only return the DOS of atoms at a given energy point

kavg: bool, int, optional

whether the returned DOS is k-averaged, or an explicit (unweighed) k-point is returned

atomarray_like of int or bool, optional

only return for a given set of atoms (default to all). NOT allowed with orbital keyword

orbitalarray_like of int or bool, optional

only return for a given set of orbitals (default to all) NOT allowed with atom keyword

sumbool, optional

whether the returned quantities are summed or returned as is, i.e. resolved per atom/orbital.

norm{‘none’, ‘atom’, ‘orbital’, ‘all’}

how the normalization of the summed DOS is performed (see norm routine).

See also

DOS

the total density of states (including bound states)

BDOS

the bulk density of states in an electrode

Adensity_matrix(self, elec, E, kavg=True, isc=None, geometry=None)

Spectral function density matrix at energy E (1/eV)

The density matrix can be used to calculate the LDOS in real-space.

The \(\mathrm{LDOS}(E, \mathbf r)\) may be calculated using the density routine. Basically the LDOS in real-space may be calculated as

\[\rho_{\mathbf A_{\mathfrak{el}}}(E, \mathbf r) = \frac{1}{2\pi}\sum_{\nu\mu}\phi_\nu(\mathbf r)\phi_\mu(\mathbf r) \Re[\mathbf A_{\mathfrak{el}, \nu\mu}(E)]\]

where \(\phi\) are the orbitals. Note that the broadening used in the TBtrans calculations ensures the broadening of the density, i.e. it should not be necessary to perform energy averages over the density matrices.

Parameters
elec: str or int

the electrode of originating electrons

Efloat or int

the energy or the energy index of density matrix. If an integer is passed it is the index, otherwise the index corresponding to Eindex(E) is used.

kavg: bool, int, optional

whether the returned density matrix is k-averaged, or an explicit (unweighed) k-point is returned

isc: array_like, optional

the returned density matrix from unit-cell ([None, None, None]) to the given supercell, the default is all density matrix elements for the supercell. To only get unit cell orbital currents, pass [0, 0, 0].

geometry: Geometry, optional

geometry that will be associated with the density matrix. By default the geometry contained in this file will be used. However, then the atomic species are probably incorrect, nor will the orbitals contain the basis-set information required to generate the required density in real-space.

Returns
DensityMatrix

object containing the Geometry and the density matrix elements

See also

density_matrix

Green function density matrix

BDOS(self, elec=0, E=None, kavg=True, sum=True, norm='none')

Bulk density of states (DOS) (1/eV).

Extract the bulk DOS from electrode elec on a selected subset of atoms/orbitals in the device region

\[\mathrm{BDOS}_\mathfrak{el}(E) = -\frac{1}{\pi} \Im\mathbf{G}(E)\]
Parameters
elec: str, int, optional

electrode where the bulk DOS is returned

Efloat or int, optional

optionally only return the DOS of atoms at a given energy point

kavg: bool, int, optional

whether the returned DOS is k-averaged, or an explicit (unweighed) k-point is returned

sumbool, optional

whether the returned quantities are summed or returned as is, i.e. resolved per atom/orbital.

norm{‘none’, ‘atom’, ‘orbital’, ‘all’}

whether the returned quantities are summed or normed by total number of orbitals. Currently one cannot extract DOS per atom/orbital.

See also

DOS

the total density of states (including bound states)

ADOS

the spectral density of states from an electrode

DOS(self, E=None, kavg=True, atom=None, orbital=None, sum=True, norm='none')

Green function density of states (DOS) (1/eV).

Extract the DOS on a selected subset of atoms/orbitals in the device region

\[\mathrm{DOS}(E) = -\frac{1}{\pi N} \sum_{\nu\in \mathrm{atom}/\mathrm{orbital}} \Im \mathbf{G}_{\nu\nu}(E)\]

The normalization constant (\(N\)) is defined in the routine norm and depends on the arguments.

Parameters
Efloat or int, optional

optionally only return the DOS of atoms at a given energy point

kavg: bool, int, optional

whether the returned DOS is k-averaged, or an explicit (unweighed) k-point is returned

atomarray_like of int or bool, optional

only return for a given set of atoms (default to all). NOT allowed with orbital keyword

orbitalarray_like of int or bool, optional

only return for a given set of orbitals (default to all) NOT allowed with atom keyword

sumbool, optional

whether the returned quantities are summed or returned as is, i.e. resolved per atom/orbital.

norm{‘none’, ‘atom’, ‘orbital’, ‘all’}

how the normalization of the summed DOS is performed (see norm routine)

See also

ADOS

the spectral density of states from an electrode

BDOS

the bulk density of states in an electrode

property E

Sampled energy-points in file

Eindex(self, E)

Return the closest energy index corresponding to the energy E

Parameters
Efloat or int

if int, return it-self, else return the energy index which is closests to the energy.

a2p(self, atom)

Return the pivoting orbital indices (0-based) for the atoms

This is equivalent to:

>>> p = self.o2p(self.geom.a2o(atom, True))

Will warn if an atom requested is not in the device list of atoms.

Parameters
atomarray_like or int

atomic indices (0-based)

property a_buf

Atomic indices (0-based) of device atoms

property a_dev

Atomic indices (0-based) of device atoms

atom_ACOHP(self, elec, E, kavg=True, isc=None, uc=False)

Atomic COHP curve of the spectral function

Parameters
elec: str or int

the electrode of the spectral function

E: float or int

the energy or the energy index of COHP. If an integer is passed it is the index, otherwise the index corresponding to Eindex(E) is used.

kavg: bool, int, optional

whether the returned COHP is k-averaged, or an explicit (unweighed) k-point is returned

isc: array_like, optional

the returned COHP from unit-cell ([None, None, None]) to the given supercell, the default is all COHP for the supercell. To only get unit cell orbital currents, pass [0, 0, 0].

ucbool, optional

whether the returned COHP are only in the unit-cell. If True this will return a sparse matrix of shape = (self.na, self.na), else, it will return a sparse matrix of shape = (self.na, self.na * self.n_s). One may figure out the connections via sc_index.

See also

orbital_COHP

orbital resolved COHP analysis of the Green function

atom_COHP_from_orbital

transfer an orbital COHP to atomic COHP

atom_COHP

atomic COHP analysis of the Green function

atom_ACOOP

atomic COOP analysis of the spectral function

atom_ACOOP(self, elec, E, kavg=True, isc=None, uc=False)

Atomic COOP curve of the spectral function

Parameters
elec: str or int

the electrode of the spectral function

E: float or int

the energy or the energy index of COOP. If an integer is passed it is the index, otherwise the index corresponding to Eindex(E) is used.

kavg: bool, int, optional

whether the returned COOP is k-averaged, or an explicit (unweighed) k-point is returned

isc: array_like, optional

the returned COOP from unit-cell ([None, None, None]) to the given supercell, the default is all COOP for the supercell. To only get unit cell orbital currents, pass [0, 0, 0].

ucbool, optional

whether the returned COOP are only in the unit-cell. If True this will return a sparse matrix of shape = (self.na, self.na), else, it will return a sparse matrix of shape = (self.na, self.na * self.n_s). One may figure out the connections via sc_index.

See also

orbital_COOP

orbital resolved COOP analysis of the Green function

atom_COOP_from_orbital

transfer an orbital COOP to atomic COOP

atom_COOP

atomic COOP analysis of the Green function

atom_ACOHP

atomic COHP analysis of the spectral function

atom_COHP(self, E, kavg=True, isc=None, uc=False)

Atomic COHP curve of the Green function

Parameters
E: float or int

the energy or the energy index of COHP. If an integer is passed it is the index, otherwise the index corresponding to Eindex(E) is used.

kavg: bool, int, optional

whether the returned COHP is k-averaged, or an explicit (unweighed) k-point is returned

isc: array_like, optional

the returned COHP from unit-cell ([None, None, None]) to the given supercell, the default is all COHP for the supercell. To only get unit cell orbital currents, pass [0, 0, 0].

ucbool, optional

whether the returned COHP are only in the unit-cell. If True this will return a sparse matrix of shape = (self.na, self.na), else, it will return a sparse matrix of shape = (self.na, self.na * self.n_s). One may figure out the connections via sc_index.

See also

orbital_COHP

orbital resolved COHP analysis of the Green function

atom_COHP_from_orbital

transfer an orbital COHP to atomic COHP

atom_ACOHP

atomic COHP analysis of the spectral function

atom_COOP

atomic COOP analysis of the Green function

atom_COHP_from_orbital(self, COHP, uc=False)

Calculate the atomic COHP curve from the orbital COHP

The atomic COHP are a sum over all orbital COHP:

\[\mathrm{COHP}_{\alpha\beta} = \sum_{\nu\in\alpha}\sum_{\mu\in\beta} \mathrm{COHP}_{\nu\mu}\]
Parameters
COHPscipy.sparse.csr_matrix

the orbital COHP as retrieved from orbital_COHP or orbital_ACOHP

ucbool, optional

whether the returned COHP are only in the unit-cell. If True this will return a sparse matrix of shape = (self.na, self.na), else, it will return a sparse matrix of shape = (self.na, self.na * self.n_s). One may figure out the connections via sc_index.

See also

orbital_COHP

orbital resolved COHP analysis of the Green function

orbital_ACOHP

orbital resolved COHP analysis of the spectral function

atom_COHP

atomic COHP analysis of the Green function

atom_COOP(self, E, kavg=True, isc=None, uc=False)

Atomic COOP curve of the Green function

Parameters
E: float or int

the energy or the energy index of COOP. If an integer is passed it is the index, otherwise the index corresponding to Eindex(E) is used.

kavg: bool, int, optional

whether the returned COOP is k-averaged, or an explicit (unweighed) k-point is returned

isc: array_like, optional

the returned COOP from unit-cell ([None, None, None]) to the given supercell, the default is all COOP for the supercell. To only get unit cell orbital currents, pass [0, 0, 0].

ucbool, optional

whether the returned COOP are only in the unit-cell. If True this will return a sparse matrix of shape = (self.na, self.na), else, it will return a sparse matrix of shape = (self.na, self.na * self.n_s). One may figure out the connections via sc_index.

See also

orbital_COOP

orbital resolved COOP analysis of the Green function

atom_COOP_from_orbital

transfer an orbital COOP to atomic COOP

atom_ACOOP

atomic COOP analysis of the spectral function

atom_COHP

atomic COHP analysis of the Green function

atom_COOP_from_orbital(self, COOP, uc=False)

Calculate the atomic COOP curve from the orbital COOP

The atomic COOP are a sum over all orbital COOP:

\[\mathrm{COOP}_{\alpha\beta} = \sum_{\nu\in\alpha}\sum_{\mu\in\beta} \mathrm{COOP}_{\nu\mu}\]
Parameters
COOPscipy.sparse.csr_matrix

the orbital COOP as retrieved from orbital_COOP or orbital_ACOOP

ucbool, optional

whether the returned COOP are only in the unit-cell. If True this will return a sparse matrix of shape = (self.na, self.na), else, it will return a sparse matrix of shape = (self.na, self.na * self.n_s). One may figure out the connections via sc_index.

See also

orbital_COOP

orbital resolved COOP analysis of the Green function

orbital_ACOOP

orbital resolved COOP analysis of the spectral function

atom_COOP

atomic COOP analysis of the Green function

atom_current(self, elec, E, kavg=True, activity=True)

Atomic current of atoms

Short hand function for calling orbital_current and atom_current_from_orbital.

Parameters
elec: str, int

the electrode of originating electrons

E: float or int

the energy or energy index of the atom current.

kavg: bool, int, optional

whether the returned atomic current is k-averaged, or an explicit (unweighed) k-point is returned

activity: bool, optional

whether the activity current is returned, see atom_current_from_orbital for details.

See also

orbital_current

the orbital current between individual orbitals

bond_current_from_orbital

transfer the orbital current to bond current

bond_current

the bond current (orbital current summed over orbitals)

vector_current

an atomic field current for each atom (Cartesian representation of bond-currents)

atom_current_from_orbital(self, Jij, activity=True)

Atomic current of atoms by passing the orbital current

The atomic current is a single number specifying a figure of the magnitude current flowing through each atom. It is thus not a quantity that can be related to the physical current flowing in/out of atoms but is merely a number that provides an idea of how much current this atom is redistributing.

The atomic current may have two meanings based on these two equations

\[\begin{split}J_\alpha^{|a|} &=\frac{1}{2} \sum_\beta \Big| \sum_{\nu\in \alpha}\sum_{\mu\in \beta} J_{\nu\mu} \Big| \\ J_\alpha^{|o|} &=\frac{1}{2} \sum_\beta \sum_{\nu\in \alpha}\sum_{\mu\in \beta} \big| J_{\nu\mu} \big|\end{split}\]

If the activity current is requested (activity=True) \(J_\alpha^{\mathcal A} = \sqrt{ J_\alpha^{|a|} J_\alpha^{|o|} }\) is returned.

If activity=False \(J_\alpha^{|a|}\) is returned.

For geometries with all atoms only having 1-orbital, they are equivalent.

Generally the activity current is a more rigorous figure of merit for the current flowing through an atom. More so than than the summed absolute atomic current due to the following reasoning. The activity current is a geometric mean of the absolute bond current and the absolute orbital current. This means that if there is an atom with a large orbital current it will have a larger activity current.

Parameters
Jij: scipy.sparse.csr_matrix

the orbital currents as retrieved from orbital_current

activity: bool, optional

True to return the activity current, see explanation above

Examples

>>> Jij = tbt.orbital_current(0, -1.03) # orbital current @ E = -1 eV originating from electrode ``0``
>>> Ja = tbt.atom_current_from_orbital(Jij)
property base_file

File of the current Sile

bond_current(self, elec, E, kavg=True, isc=None, only='+', uc=False)

Bond-current between atoms (sum of orbital currents)

Short hand function for calling orbital_current and bond_current_from_orbital.

Parameters
elecstr, int

the electrode of originating electrons

Efloat or int

A float for energy in eV, int for explicit energy index Unlike orbital_current this may not be None as the down-scaling of the orbital currents may not be equivalent for all energy points.

kavgbool, int, optional

whether the returned bond current is k-averaged, or an explicit (unweighed) k-point is returned

iscarray_like, optional

the returned bond currents from the unit-cell ([None, None, None]) (default) to the given supercell. If [None, None, None] is passed all bond currents are returned.

only{‘+’, ‘-‘, ‘all’}

If “+” is supplied only the positive orbital currents are used, for “-“, only the negative orbital currents are used, else return the sum of both. Please see discussion in orbital_current.

ucbool, optional

whether the returned bond-currents are only in the unit-cell. If True this will return a sparse matrix of shape = (self.na, self.na), else, it will return a sparse matrix of shape = (self.na, self.na * self.n_s). One may figure out the connections via sc_index.

See also

orbital_current

the orbital current between individual orbitals

bond_current_from_orbital

transfer the orbital current to bond current

atom_current

the atomic current for each atom (scalar representation of bond-currents)

vector_current

an atomic field current for each atom (Cartesian representation of bond-currents)

Examples

>>> Jij = tbt.orbital_current(0, -1.0, only='+') # orbital current @ E = -1 eV originating from electrode ``0``
>>> Jab1 = tbt.bond_current_from_orbital(Jij)
>>> Jab2 = tbt.bond_current(0, -1.0)
>>> Jab1 == Jab2
True
bond_current_from_orbital(self, Jij, only='+', uc=False)

Bond-current between atoms (sum of orbital currents) from an external orbital current

Conversion routine from orbital currents into bond currents.

The bond currents are a sum over all orbital currents:

\[J_{\alpha\beta} = \sum_{\nu\in\alpha}\sum_{\mu\in\beta} J_{\nu\mu}\]

where if

  • only='+': only \(J_{\nu\mu} > 0\) are summed onto the corresponding atom,

  • only='-': only \(J_{\nu\mu} < 0\) are summed onto the corresponding atom,

  • only='all': all \(J_{\nu\mu}\) are summed onto the corresponding atom.

Parameters
Jijscipy.sparse.csr_matrix

the orbital currents as retrieved from orbital_current

only{‘+’, ‘-‘, ‘all’}

If “+” is supplied only the positive orbital currents are used, for “-“, only the negative orbital currents are used, else return both.

ucbool, optional

whether the returned bond-currents are only in the unit-cell. If True this will return a sparse matrix of shape = (self.na, self.na), else, it will return a sparse matrix of shape = (self.na, self.na * self.n_s). One may figure out the connections via sc_index.

See also

orbital_current

the orbital current between individual orbitals

bond_current

the bond current (orbital current summed over orbitals)

atom_current

the atomic current for each atom (scalar representation of bond-currents)

vector_current

an atomic field current for each atom (Cartesian representation of bond-currents)

Examples

>>> Jij = tbt.orbital_current(0, -1.0) # orbital current @ E = -1 eV originating from electrode ``0``
>>> Jab = tbt.bond_current_from_orbital(Jij)
>>> Jab[2,3] # bond current between atom 3 and 4
btd(self, elec=None)

Block-sizes for the BTD method

Parameters
elecstr or int, optional

if None the number of blocks in the device region BTD matrix. Else the number of BTD blocks in the electrode down-folding.

property cell

Unit cell in file

chemical_potential = None
close(self)
current = None
current_parameter = None
density_matrix(self, E, kavg=True, isc=None, geometry=None)

Density matrix from the Green function at energy E (1/eV)

The density matrix can be used to calculate the LDOS in real-space.

The \(\mathrm{LDOS}(E, \mathbf r)\) may be calculated using the density routine. Basically the LDOS in real-space may be calculated as

\[\rho_{\mathbf G}(E, \mathbf r) = -\frac{1}{\pi}\sum_{\nu\mu}\phi_\nu(\mathbf r)\phi_\mu(\mathbf r) \Im[\mathbf G_{\nu\mu}(E)]\]

where \(\phi\) are the orbitals. Note that the broadening used in the TBtrans calculations ensures the broadening of the density, i.e. it should not be necessary to perform energy averages over the density matrices.

Parameters
Efloat or int

the energy or the energy index of density matrix. If an integer is passed it is the index, otherwise the index corresponding to Eindex(E) is used.

kavg: bool, int, optional

whether the returned density matrix is k-averaged, or an explicit (unweighed) k-point is returned

isc: array_like, optional

the returned density matrix from unit-cell ([None, None, None]) to the given supercell, the default is all density matrix elements for the supercell. To only get unit cell orbital currents, pass [0, 0, 0].

geometry: Geometry, optional

geometry that will be associated with the density matrix. By default the geometry contained in this file will be used. However, then the atomic species are probably incorrect, nor will the orbitals contain the basis-set information required to generate the required density in real-space.

Returns
DensityMatrix

object containing the Geometry and the density matrix elements

See also

Adensity_matrix

spectral function density matrix

dir_file(self, filename=None)

File of the current Sile

property elecs

List of electrodes

electron_temperature = None
eta(self, elec=None)

The imaginary part used when calculating the self-energies in eV (or for the device

Parameters
elecstr, int, optional

electrode to extract the eta value from. If not specified (or None) the device region eta will be returned.

exist(self)

Query whether the file exists

fano = None
property file

File of the current Sile

property geom

The associated geometry from this file

property geometry

The associated geometry from this file

info(self, elec=None)

Information about the calculated quantities available for extracting in this file

Parameters
elecstr or int

the electrode to request information from

iter(self, group=True, dimension=True, variable=True, levels=-1, root=None)

Iterator on all groups, variables and dimensions.

This iterator iterates through all groups, variables and dimensions in the Dataset

The generator sequence will _always_ be:

  1. Group

  2. Dimensions in group

  3. Variables in group

As the dimensions are generated before the variables it is possible to copy groups, dimensions, and then variables such that one always ensures correct dependencies in the generation of a new SileCDF.

Parameters
groupbool (True)

whether the iterator yields Group instances

dimensionbool (True)

whether the iterator yields Dimension instances

variablebool (True)

whether the iterator yields Variable instances

levelsint (-1)

number of levels to traverse, with respect to root variable, i.e. number of sub-groups this iterator will return.

rootstr (None)

the base root to start iterating from.

Examples

Script for looping and checking each instance.

>>> for gv in self.iter():
...     if self.isGroup(gv):
...         # is group
...     elif self.isDimension(gv):
...         # is dimension
...     elif self.isVariable(gv):
...         # is variable
property k

Sampled k-points in file

kT(self, elec)

Electron bath temperature [eV]

kindex(self, k)

Return the index of the k-point that is closests to the queried k-point (in reduced coordinates)

Parameters
karray_like of float

the queried k-point in reduced coordinates \(]-0.5;0.5]\).

property kpt

Sampled k-points in file

property lasto

Last orbital of corresponding atom

mu(self, elec)

Return the chemical potential associated with the electrode elec

property nE

Number of energy-points in file

n_btd(self, elec=None)

Number of blocks in the BTD partioning

Parameters
elecstr or int, optional

if None the number of blocks in the device region BTD matrix. Else the number of BTD blocks in the electrode down-folding.

property na

Returns number of atoms in the cell

property na_b

Number of atoms in the buffer region

property na_buffer

Number of atoms in the buffer region

property na_d

Number of atoms in the device region

property na_dev

Number of atoms in the device region

property na_u

Returns number of atoms in the cell

property ne

Number of energy-points in file

property nk

Number of k-points in file

property nkpt

Always return 1, this is to signal other routines

property no

Returns number of orbitals in the cell

property no_d

Number of orbitals in the device region

property no_u

Returns number of orbitals in the cell

noise_power = None
norm(self, atom=None, orbital=None, norm='none')

Normalization factor depending on the input

The normalization can be performed in one of the below methods. In the following \(N\) refers to the normalization constant that is to be used (i.e. the divisor):

'none'

\(N=1\)

'all'

\(N\) equals the number of orbitals in the total device region.

'atom'

\(N\) equals the total number of orbitals in the selected atoms. If orbital is an argument a conversion of orbital to the equivalent unique atoms is performed, and subsequently the total number of orbitals on the atoms is used. This makes it possible to compare the fraction of orbital DOS easier.

'orbital'

\(N\) is the sum of selected orbitals, if atom is specified, this is equivalent to the ‘atom’ option.

Parameters
atomarray_like of int or bool, optional

only return for a given set of atoms (default to all). NOT allowed with orbital keyword

orbitalarray_like of int or bool, optional

only return for a given set of orbitals (default to all) NOT allowed with atom keyword

norm{‘none’, ‘atom’, ‘orbital’, ‘all’}

how the normalization of the summed DOS is performed (see norm routine)

o2p(self, orbital)

Return the pivoting indices (0-based) for the orbitals

Will warn if an orbital requested is not in the device list of orbitals.

Parameters
orbitalarray_like or int

orbital indices (0-based)

property o_dev

Orbital indices (0-based) of device orbitals

orbital_ACOHP(self, elec, E, kavg=True, isc=None)

Orbital resolved COHP analysis of the spectral function

This will return a sparse matrix, see scipy.sparse.csr_matrix for details. Each matrix element of the sparse matrix corresponds to the COHP of the underlying geometry.

The COHP analysis can be written as:

\[\mathrm{COHP}^{\mathbf A}_{\nu\mu} = \frac{1}{2\pi} \Re\big[\mathbf A_{\nu\mu} \mathbf H_{\nu\mu} \big]\]
Parameters
elec: str or int

the electrode of the spectral function

E: float or int

the energy or the energy index of COHP. If an integer is passed it is the index, otherwise the index corresponding to Eindex(E) is used.

kavg: bool, int, optional

whether the returned COHP is k-averaged, or an explicit (unweighed) k-point is returned

isc: array_like, optional

the returned COHP from unit-cell ([None, None, None]) to the given supercell, the default is all COHP for the supercell. To only get unit cell orbital currents, pass [0, 0, 0].

See also

orbital_COHP

orbital resolved COHP analysis of the Green function

atom_COHP_from_orbital

atomic COHP analysis from an orbital COHP

atom_COHP

atomic COHP analysis of the Green function

atom_ACOHP

atomic COHP analysis of the spectral function

orbital_COOP

orbital resolved COOP analysis of the Green function

atom_COOP_from_orbital

transfer an orbital COOP to atomic COOP

atom_COOP

atomic COOP analysis of the Green function

orbital_ACOOP

orbital resolved COOP analysis of the spectral function

atom_ACOOP

atomic COOP analysis of the spectral function

orbital_ACOOP(self, elec, E, kavg=True, isc=None)

Orbital COOP analysis of the spectral function

This will return a sparse matrix, see csr_matrix for details. Each matrix element of the sparse matrix corresponds to the COOP of the underlying geometry.

The COOP analysis can be written as:

\[\mathrm{COOP}^{\mathbf A}_{\nu\mu} = \frac{1}{2\pi} \Re\big[\mathbf A_{\nu\mu} \mathbf S_{\mu\nu} \big]\]

The sum of the COOP DOS is equal to the DOS:

\[\mathrm{ADOS}_{\nu} = \sum_\mu \mathrm{COOP}^{\mathbf A}_{\nu\mu}\]

One can calculate the (diagonal) balanced COOP analysis, see JPCM 15 (2003), 7751-7761 for details. The DBCOOP is given by:

\[\begin{split}D &= \sum_\nu \mathrm{COOP}^{\mathbf A}_{\nu\nu} \\ \mathrm{DBCOOP}^{\mathbf A}_{\nu\mu} &= \mathrm{COOP}^{\mathbf A}_{\nu\mu} / D\end{split}\]

The BCOOP can be looked up in the reference above.

Parameters
elec: str or int

the electrode of the spectral function

E: float or int

the energy or the energy index of COOP. If an integer is passed it is the index, otherwise the index corresponding to Eindex(E) is used.

kavg: bool, int, optional

whether the returned COOP is k-averaged, or an explicit (unweighed) k-point is returned

isc: array_like, optional

the returned COOP from unit-cell ([None, None, None]) to the given supercell, the default is all COOP for the supercell. To only get unit cell orbital currents, pass [0, 0, 0].

See also

orbital_COOP

orbital resolved COOP analysis of the Green function

atom_COOP_from_orbital

transfer an orbital COOP to atomic COOP

atom_COOP

atomic COOP analysis of the Green function

atom_ACOOP

atomic COOP analysis of the spectral function

orbital_COHP

orbital resolved COHP analysis of the Green function

atom_COHP_from_orbital

atomic COHP analysis from an orbital COHP

atom_COHP

atomic COHP analysis of the Green function

orbital_ACOHP

orbital resolved COHP analysis of the spectral function

atom_ACOHP

atomic COHP analysis of the spectral function

Examples

>>> ACOOP = tbt.orbital_ACOOP(0, -1.0) # COOP @ E = -1 eV from ``0`` spectral function
>>> ACOOP[10, 11] # COOP value between the 11th and 12th orbital
>>> ACOOP.sum(1).A[tbt.o_dev, 0] == tbt.ADOS(0, sum=False)[tbt.Eindex(-1.0)]
>>> D = ACOOP.diagonal().sum()
>>> ADBCOOP = ACOOP / D
orbital_COHP(self, E, kavg=True, isc=None)

Orbital resolved COHP analysis of the Green function

This will return a sparse matrix, see scipy.sparse.csr_matrix for details. Each matrix element of the sparse matrix corresponds to the COHP of the underlying geometry.

The COHP analysis can be written as:

\[\mathrm{COHP}^{\mathbf G}_{\nu\mu} = \frac{-1}{2\pi} \Im\big[(\mathbf G - \mathbf G^\dagger)_{\nu\mu} \mathbf H_{\mu\nu} \big]\]
Parameters
E: float or int

the energy or the energy index of COHP. If an integer is passed it is the index, otherwise the index corresponding to Eindex(E) is used.

kavg: bool, int, optional

whether the returned COHP is k-averaged, or an explicit (unweighed) k-point is returned

isc: array_like, optional

the returned COHP from unit-cell ([None, None, None]) to the given supercell, the default is all COHP for the supercell. To only get unit cell orbital currents, pass [0, 0, 0].

See also

atom_COHP_from_orbital

atomic COHP analysis from an orbital COHP

atom_COHP

atomic COHP analysis of the Green function

orbital_ACOHP

orbital resolved COHP analysis of the spectral function

atom_ACOHP

atomic COHP analysis of the spectral function

orbital_COOP

orbital resolved COOP analysis of the Green function

atom_COOP_from_orbital

transfer an orbital COOP to atomic COOP

atom_COOP

atomic COOP analysis of the Green function

orbital_ACOOP

orbital resolved COOP analysis of the spectral function

atom_ACOOP

atomic COOP analysis of the spectral function

Examples

>>> COHP = tbt.orbital_COHP(-1.0) # COHP @ E = -1 eV 
>>> COHP[10, 11] # COHP value between the 11th and 12th orbital
orbital_COOP(self, E, kavg=True, isc=None)

Orbital COOP analysis of the Green function

This will return a sparse matrix, see scipy.sparse.csr_matrix for details. Each matrix element of the sparse matrix corresponds to the COOP of the underlying geometry.

The COOP analysis can be written as:

\[\mathrm{COOP}^{\mathbf G}_{\nu\mu} = \frac{-1}{2\pi} \Im\big[(\mathbf G - \mathbf G^\dagger)_{\nu\mu} \mathbf S_{\mu\nu} \big]\]

The sum of the COOP DOS is equal to the DOS:

\[\mathrm{DOS}_{\nu} = \sum_\mu \mathrm{COOP}^{\mathbf G}_{\nu\mu}\]

One can calculate the (diagonal) balanced COOP analysis, see JPCM 15 (2003), 7751-7761 for details. The DBCOOP is given by:

\[\begin{split}D &= \sum_\nu \mathrm{COOP}^{\mathbf G}_{\nu\nu} \\ \mathrm{DBCOOP}^{\mathbf G}_{\nu\mu} &= \mathrm{COOP}^{\mathbf G}_{\nu\mu} / D\end{split}\]

The BCOOP can be looked up in the reference above.

Parameters
E: float or int

the energy or the energy index of COOP. If an integer is passed it is the index, otherwise the index corresponding to Eindex(E) is used.

kavg: bool, int, optional

whether the returned COOP is k-averaged, or an explicit (unweighed) k-point is returned

isc: array_like, optional

the returned COOP from unit-cell ([None, None, None]) to the given supercell, the default is all COOP for the supercell. To only get unit cell orbital currents, pass [0, 0, 0].

See also

atom_COOP_from_orbital

transfer an orbital COOP to atomic COOP

atom_COOP

atomic COOP analysis of the Green function

orbital_ACOOP

orbital resolved COOP analysis of the spectral function

atom_ACOOP

atomic COOP analysis of the spectral function

orbital_COHP

orbital resolved COHP analysis of the Green function

atom_COHP_from_orbital

atomic COHP analysis from an orbital COHP

atom_COHP

atomic COHP analysis of the Green function

orbital_ACOHP

orbital resolved COHP analysis of the spectral function

atom_ACOHP

atomic COHP analysis of the spectral function

Examples

>>> COOP = tbt.orbital_COOP(-1.0) # COOP @ E = -1 eV 
>>> COOP[10, 11] # COOP value between the 11th and 12th orbital
>>> COOP.sum(1).A[tbt.o_dev, 0] == tbt.DOS(sum=False)[tbt.Eindex(-1.0)]
>>> D = COOP.diagonal().sum()
>>> DBCOOP = COOP / D
orbital_current(self, elec, E, kavg=True, isc=None, only='all')

Orbital current originating from elec as a sparse matrix

This will return a sparse matrix, see scipy.sparse.csr_matrix for details. Each matrix element of the sparse matrix corresponds to the orbital indices of the underlying geometry.

When requesting orbital-currents it is vital to consider how the data needs to be analysed before extracting the data. For instance, if only local currents are interesting one should use only='+'. While if one is interested in the transmission between subset of orbitals, only='all' is the correct method.

For inexperienced users it is adviced to try out all three values of only to ensure the correct physics is obtained.

This becomes even more important when the orbital currents are calculated with magnetic fields. With \(\mathbf B\) fields local current loops may form and current does not necessarily flow along the transport direction.

Parameters
elec: str, int

the electrode of originating electrons

E: float or int

the energy or the energy index of the orbital current. If an integer is passed it is the index, otherwise the index corresponding to Eindex(E) is used.

kavg: bool, int, optional

whether the returned orbital current is k-averaged, or an explicit (unweighed) k-point is returned

isc: array_like, optional

the returned bond currents from the unit-cell ([None, None, None]) to the given supercell, the default is all orbital currents for the supercell. To only get unit cell orbital currents, pass [0, 0, 0].

only{‘all’, ‘+’, ‘-‘}

which orbital currents to return, all, positive or negative values only. Default to 'all' because it can then be used in the subsequent default arguments for bond_current_from_orbital and atom_current_from_orbital.

See also

bond_current_from_orbital

transfer the orbital current to bond current

bond_current

the bond current (orbital current summed over orbitals)

atom_current_from_orbital

transfer the orbital current to atomic current

atom_current

the atomic current for each atom (scalar representation of bond-currents)

vector_current

an atomic field current for each atom (Cartesian representation of bond-currents)

Examples

>>> Jij = tbt.orbital_current(0, -1.0) # orbital current @ E = -1 eV originating from electrode ``0``
>>> Jij[10, 11] # orbital current from the 11th to the 12th orbital
pivot(self, in_device=False, sort=False)

Pivoting orbitals for the full system

Parameters
in_devicebool, optional

whether the pivoting elements are with respect to the device region

sortbool, optional

whether the pivoting elements are sorted

read(self, *args, **kwargs)

Generic read method which should be overloaded in child-classes

Parameters
kwargs :

keyword arguments will try and search for the attribute read_<> and call it with the remaining **kwargs as arguments.

read_data(self, *args, **kwargs)

Read specific type of data.

This is a generic routine for reading different parts of the data-file.

Parameters
geom: bool, optional

return the geometry

atom_current: bool, optional

return the atomic current flowing through an atom (the activity current)

vector_current: bool, optional

return the orbital currents as vectors

read_geometry(self, *args, **kwargs)

Returns Geometry object from this file

read_supercell(self)

Returns SuperCell object from this file

reflection(self, elec=0, kavg=True, from_single=False)

Reflection into electrode elec

The reflection into electrode elec is calculated as:

\[R(E) = T_{\mathrm{bulk}}(E) - \sum_{\mathrm{to}} T_{\mathrm{elec}\to\mathrm{to}}(E)\]

Another way of calculating the reflection is via:

\[R(E) = T_{\mathrm{bulk}}(E) - \big\{i \mathrm{Tr}[(\mathbf G-\mathbf G^\dagger)\boldsymbol\Gamma_{\mathrm{elec}}] - \mathrm{Tr}[\mathbf G\boldsymbol\Gamma_{\mathrm{elec}}\mathbf G^\dagger\boldsymbol\Gamma_{\mathrm{elec}}]\big\}\]

Both are identical, however, numerically they may be different. Particularly when the bulk transmission is very large compared to the transmission to the other electrodes one should prefer the first equation.

Parameters
elec: str, int, optional

the backscattered electrode

kavg: bool, int, optional

whether the returned reflection is k-averaged, or an explicit (unweighed) k-point is returned

from_single: bool, optional

whether the reflection is calculated using the Green function and a single scattering matrix Eq. (2) above (true), otherwise Eq. (1) will be used (false).

See also

transmission

the total transmission

transmission_eig

the transmission decomposed in eigenchannels

transmission_bulk

the total transmission in a periodic lead

shot_noise = None
transmission(self, elec_from=0, elec_to=1, kavg=True)

Transmission from elec_from to elec_to.

The transmission between two electrodes may be retrieved from the Sile.

The transmission is calculated as:

\[T(E) = \mathrm{Tr}[\mathbf{G}\boldsymbol\Gamma_{\mathrm{from}}\mathbf{G}^\dagger\boldsymbol\Gamma_{\mathrm{to}}]\]

where all quantities are energy dependent.

Parameters
elec_from: str, int, optional

the originating electrode

elec_to: str, int, optional

the absorbing electrode (different from elec_from)

kavg: bool, int, optional

whether the returned transmission is k-averaged, or an explicit (unweighed) k-point is returned

See also

transmission_eig

the transmission decomposed in eigenchannels

transmission_bulk

the total transmission in a periodic lead

reflection

total reflection back into the electrode

transmission_bulk(self, elec=0, kavg=True)

Bulk transmission for the elec electrode

The bulk transmission is equivalent to creating a 2 terminal device with electrode elec tiled 3 times.

Parameters
elec: str, int, optional

the bulk electrode

kavg: bool, int, optional

whether the returned transmission are k-averaged, or an explicit (unweighed) k-point is returned

See also

transmission

the total transmission

transmission_eig

the transmission decomposed in eigenchannels

reflection

total reflection back into the electrode

transmission_eig(self, elec_from=0, elec_to=1, kavg=True)

Transmission eigenvalues from elec_from to elec_to.

Parameters
elec_from: str, int, optional

the originating electrode

elec_to: str, int, optional

the absorbing electrode (different from elec_from)

kavg: bool, int, optional

whether the returned transmission eigenvalues are k-averaged, or an explicit (unweighed) k-point is returned

See also

transmission

the total transmission

transmission_bulk

the total transmission in a periodic lead

vector_current(self, elec, E, kavg=True, only='+')

Vector for each atom describing the mean path for the current travelling through the atom

See vector_current_from_bond for details.

Parameters
elec: str or int

the electrode of originating electrons

E: float or int

the energy or energy index of the vector current. Unlike orbital_current this may not be None as the down-scaling of the orbital currents may not be equivalent for all energy points.

kavg: bool, int, optional

whether the returned vector current is k-averaged, or an explicit (unweighed) k-point is returned

only{‘+’, ‘-‘, ‘all’}

By default only sum outgoing vector currents ('+'). The incoming vector currents may be retrieved by '-', while the average incoming and outgoing direction can be obtained with 'all'. In the last case the vector currents are divided by 2 to ensure the length of the vector is compatibile with the other options given a pristine system.

Returns
numpy.ndarray

array of vectors per atom in the Geometry (only non-zero for device atoms)

See also

orbital_current

the orbital current between individual orbitals

bond_current_from_orbital

transfer the orbital current to bond current

bond_current

the bond current (orbital current summed over orbitals)

atom_current

the atomic current for each atom (scalar representation of bond-currents)

vector_current_from_bond(self, Jab)

Vector for each atom being the sum of bond-current times the normalized bond between the atoms

The vector current is defined as:

\[\mathbf J_\alpha = \sum_\beta \frac{r_\beta - r_\alpha}{|r_\beta - r_\alpha|} \cdot J_{\alpha\beta}\]

Where \(J_{\alpha\beta}\) is the bond current between atom \(\alpha\) and \(\beta\) and \(r_\alpha\) are the atomic coordinates.

Parameters
Jab: scipy.sparse.csr_matrix

the bond currents as retrieved from bond_current

Returns
numpy.ndarray

array of vectors per atom in the Geometry (only non-zero for device atoms)

See also

orbital_current

the orbital current between individual orbitals

bond_current_from_orbital

transfer the orbital current to bond current

bond_current

the bond current (orbital current summed over orbitals)

atom_current

the atomic current for each atom (scalar representation of bond-currents)

property wk

Weights of k-points in file

property wkpt

Always return [1.], this is to signal other routines

write(self, *args, **kwargs)

Generic write method which should be overloaded in child-classes

Parameters
**kwargs :

keyword arguments will try and search for the attribute write_ and call it with the remaining **kwargs as arguments.

write_geometry(self, *args, **kwargs)

This is not meant to be used

write_tbtav(self, *args, **kwargs)

Wrapper for writing the k-averaged TBT.AV.nc file.

This write requires the TBT.nc Sile object passed as the first argument, or as the keyword from=tbt argument.

Parameters
fromtbtncSileTBtrans

the TBT.nc file object that has the k-sampled quantities.

property xa

Atomic coordinates in file

property xyz

Atomic coordinates in file