abinit/doc/topics/_CalcUJ.md

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---
description: How to calculate the effective Coulomb interaction
authors: BAmadon
---
<!--- This is the source file for this topics. Can be edited. -->
This page gives hints on how to calculate the effective Coulomb interaction with the ABINIT package.
## Introduction
DFT+U as well as DFT+DMFT requires as input values the effective Coulomb
interaction. Two ways to compute them are available in ABINIT.
Firstly, the constrained Random Phase Approximation [[cite:Aryasetiawan2004]]
[[ucrpa]] allows one to take into account the screening of the Coulomb
interaction between correlated electrons, by non-interacting electrons. For
non-entangled bands ([[ucrpa]]= 1), the bands excluded from the polarisability
can be specified either by a band index ([[ucrpa_bands]]) or an energy window
([[ucrpa_window]]) [[cite:Amadon2014]].
For entangled bands ([[ucrpa]]= 2}), the scheme used in ABINIT
[[cite:Shih2012]], [[cite:Sakuma2013]],[[cite:Amadon2014]] uses a band and
k-point dependent weight to define the polarisability, using Wannier orbitals
as correlated orbitals.
This method is well adapted to compute the effective interaction for the same
orbitals used in DFT+DMFT. To use the same orbitals as in DFT+U, the Wannier
functions can be ajusted such that the bare interaction is close to the bare
interaction of atomic orbitals as used in DFT+ _U_ (see tutorial).
Secondly, a linear response method [[cite:Cococcioni2005]] is implemented. The
implementation is not yet in production. The implementation in ABINIT takes
into account the truncated atomic orbitals from PAW and therefore differs from
the original work [[cite:Cococcioni2005]] treating full atomic orbitals. In
particular, considerably higher effective values for U are found.
## Related Input Variables
{{ related_variables }}
## Selected Input Files
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## Tutorials
* The [[tutorial:ucalc_crpa|tutorial on the calculation of effective interactions U and J by the cRPA method]] shows how to determine the U value with the constrained Random Phase Approximation [[cite:Aryasetiawan2004]] using projected Wannier orbitals. Prerequisite: DFT+U.
* The [[tutorial:lruj|tutorial on the computation of U from linear response]] for DFT+U shows how to determine the U value with the linear response method [[cite:Cococcioni2005]], to be used in the DFT+U approach. Prerequisite: DFT+U.