The superfluidity of fermions coupled to gravity
G. Vlasov (Moscow Aviat., Landau)

TL;DR
This paper explores how relativistic fermionic superfluidity is influenced by gravitational interactions, highlighting the dominant role of metric coefficients in forming the excitation gap.
Contribution
It introduces a theoretical analysis of superfluidity in relativistic fermions coupled to gravity, emphasizing the impact of metric coefficients on the excitation spectrum.
Findings
Superfluidity occurs at specific ratios of Fermi momentum, mass, and coupling constant.
Metric coefficients significantly influence the excitation gap.
Gravitational interaction modifies the superfluid excitation spectrum.
Abstract
We investigate superfluidity of the relativistic fermi-gas with gravitational interaction. The excitation spectrum is obtained within the linearized theory. While superfluidity may take place at a definite ratio of the Fermi momentum, rest mass and coupling constant, the metric coefficients play predominant role forming the gap of excitation spectrum.
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Taxonomy
TopicsCosmology and Gravitation Theories · Pulsars and Gravitational Waves Research · Black Holes and Theoretical Physics
