Vyasanakere, Jayantha P. ; Shenoy, Vijay B. (2012) Rashbons: properties and their significance New Journal of Physics, 14 (4). Article ID 043041. ISSN 1367-2630
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Official URL: http://iopscience.iop.org/article/10.1088/1367-263...
Related URL: http://dx.doi.org/10.1088/1367-2630/14/4/043041
Abstract
In the presence of a synthetic non-Abelian gauge field that produces a Rashba-like spin–orbit interaction, a collection of weakly interacting fermions undergoes a crossover from a Bardeen–Cooper–Schrieffer (BCS) ground state to a Bose–Einstein condensate (BEC) ground state when the strength of the gauge field is increased (Vyasanakere et al 2011 Phys. Rev. B 84 014512). The BEC that is obtained at large gauge coupling strengths is a condensate of tightly bound bosonic fermion pairs. The properties of these bosons are solely determined by the Rashba gauge field—hence called rashbons. In this paper, we conduct a systematic study of the properties of rashbons and their dispersion. This study reveals a new qualitative aspect of the problem of interacting fermions in non-Abelian gauge fields, i.e. that the rashbon state ceases to exist when the center-of-mass momentum of the fermions exceeds a critical value that is of the order of the gauge coupling strength. The study allows us to estimate the transition temperature of the rashbon BEC and suggests a route to enhance the exponentially small transition temperature of the system with a fixed weak attraction to the order of the Fermi temperature by tuning the strength of the non-Abelian gauge field. The nature of the rashbon dispersion, and in particular the absence of the rashbon states at large momenta, suggests a regime in parameter space where the normal state of the system will be a dynamical mixture of uncondensed rashbons and unpaired helical fermions. Such a state should show many novel features including pseudogap physics.
Item Type: | Article |
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Source: | Copyright of this article belongs to Institute of Physics. |
ID Code: | 106115 |
Deposited On: | 01 Feb 2018 09:52 |
Last Modified: | 01 Feb 2018 09:52 |
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