Superconductivity, generalized random phase approximation and linear scaling methods
Sebastiano Peotta

TL;DR
This paper reviews superfluid weight calculations in superconductors, emphasizing the importance of including effective field dependence on twisted boundary conditions, and introduces a generalized RPA approach and linear scaling methods for improved analysis.
Contribution
It introduces a generalized random phase approximation accounting for effective field dependence and reformulates mean-field theory as a minimization problem for linear scaling applications.
Findings
Including effective field dependence yields more accurate superfluid weight calculations.
Derived explicit superfluid weight expression within the generalized RPA.
Reformulated mean-field theory for linear scaling methods in superconductivity.
Abstract
The superfluid weight is an important observable of superconducting materials since it is related to the London penetration depth of the Meissner effect. It can be computed from the change in the grand potential (or free energy) in response to twisted boundary conditions in a torus geometry. Here we review the Bardeen-Cooper-Schrieffer mean-field theory emphasizing its origin as a variational approximation for the grand potential. The variational parameters are the effective fields that enter in the mean-field Hamiltonian, namely the Hartree-Fock potential and the pairing potential. The superfluid weight is usually computed by ignoring the dependence of the effective fields on the twisted boundary conditions. However, it has been pointed out in recent works that this can lead to unphysical results, particularly in the case of lattice models with flat bands. As a first result, we show…
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Taxonomy
TopicsPhysics of Superconductivity and Magnetism · Theoretical and Computational Physics · Quantum many-body systems
