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arXiv:1304.0849 · The European Physical Journal B

Electron-hole symmetry and solutions of Richardson pairing model

W. V. Pogosov, Nansheng Lin, Vyacheslav R. Misko

Published May 1, 2013• 6 citations
arXivHTMLPDF
DOI
10.1140/epjb/e2013-40234-9

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We address a generalized Richardson model (Russian doll BCS model), which is characterized by the breaking of time-reversal symmetry. This model is known to be exactly solvable and integrable. We point out that the Russian doll BCS model, on the level of Hamiltonian, is also particle-hole symmetric. This implies that the same state can be expressed both in the particle and hole representations with two different sets of Bethe roots. We then derive exact relations between Bethe roots in the two representations, which can hardly be obtained staying on the level of Bethe equations. In a quasi-classical limit, similar identities for usual Richardson model, known from literature, are recovered from our results. We also show that these relations for Richardson roots take a remarkably simple form at half-filling and for a symmetric with respect to the middle of the interaction band distribution of one-body energy levels, since, in this special case, the rapidities in the particle and hole representations up to the translation satisfy the same system of equations.
A type of electron pairing model with spin-orbit interactions or Zeeman coupling is solved exactly in the framework of the Richardson ansatz. Based on the exact solutions for the case with spin-orbit interactions, it is shown rigorously that the pairing symmetry is of the p + ip wave and the ground state possesses time-reversal symmetry, regardless of the strength of the pairing interaction. Intriguingly, how Majorana fermions can emerge in the system is also elaborated. Exact results are illustrated for two systems, respectively, with spin-orbit interactions and Zeeman coupling.
Chapter 10 deals with the exact solution to the BCS problem, as obtained by analytically solving Richardson-Gaudin equations. The chapter first provides a simple derivation of these equations and shows how to solve them for arbitrary N. The explicit N dependence of the N–Cooper pair energy obtained from this resolution provides invaluable insights into the role of the Pauli exclusion principle in paired fermion systems because the reduced BCS potential does not directly act between Cooper pairs. Revelation of this subtle point makes it possible to understand (i) why Cooper pairs can strongly overlap without breaking, whereas, at large density, an exciton system dissociates into an electron-hole plasma, and (ii) why the gap energy is far larger than the average pair energy. This understanding is further supported by the Cooper pair many-body parameter, which has the same form as the ones for Wannier or Frenkel excitons do.