BCS approximation to the effective vector vertex of superfluid fermions
arXiv:0804.0841 · doi:10.1103/PhysRevC.78.015502
Abstract
We examine the effective interaction of nonrelativistic fermions with an external vector field in superfluid systems. In contrast to the complicated vertex equation, usually used in this case, we apply the approach which does not employ an explicit form of the pairing interaction. This allows to obtain a simple analytic expression for the vertex function only in terms of the order parameter and other macroscopic parameters of the system. We use this effective vertex to analyze the linear response function of the superfluid medium at finite temperatures. At the time-like momentum transfer, the imaginary part of the response function is found to be proportional to the fourth power of small Fermi velocity, i.e. the energy losses through vector currents are strongly suppressed. As an application, we calculate the neutrino energy losses through neutral weak currents caused by the pair recombination in the superfluid neutron matter at temperatures lower than the critical one for S-wave pairing. This approach confirms a strong suppression of the neutrino energy losses as predicted in Ref.[4].
19 pages, no figures
References in corpus (5)
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- Vector current conservation and neutrino emission from singlet-paired baryons in neutron stars
- Vertex renormalization in weak decays of Cooper pairs and cooling compact stars
- Neutrino scattering off pair-breaking and collective excitations in superfluid neutron matter and in color-flavor locked quark matter
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- Superfluid phases of triplet pairing and neutrino emission from neutron stars
- Transport equations and linear response of superfluid Fermi mixtures in neutron stars
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- Neutrino emission from Cooper pairs at finite temperatures
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- Coupling between superfluid neutrons and superfluid protons in the elementary excitations of neutron star matter