Neutrino ground state in a dense star

Abstract

It has recently been argued that long range forces due to the exchange of massless neutrinos give rise to a very large self-energy in a dense, finite-ranged, weakly-charged medium. Such an effect, if real, would destabilize a neutron star. To address this issue we have studied the related problem of a massless neutrino field in the presence of an external, static electroweak potential of finite range. To be precise, we have computed to one loop the exact vacuum energy for the case of a spherical square well potential of depth alpha and radius R. For small wells, the vacuum energy is reliably determined by a perturbative expansion in the external potential. For large wells, however, the perturbative expansion breaks down. A manifestation of this breakdown is that the vacuum carries a non-zero neutrino charge. The energy and neutrino charge of the ground state are, to a good approximation for large wells, those of a neutrino condensate with chemical potential mu=alpha. Our results demonstrate explicitly that long-range forces due to the exchange of massless neutrinos do not threaten the stability of neutron stars.

27 pages, 7 figures, revtex; several typos corrected; a few references added; title changed slightly; includes a "note added in proof"; version to appear in Phys. Rev. D

References in corpus (4)

• Neutrino self-energy and pair creation in neutron stars
• Coherent Neutrino Interactions in a Dense Medium
• Finite-size effects on multibody neutrino exchange
• Multibody neutrino exchange in a neutron star: neutrino sea and border effects

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• Finite-size effects on multibody neutrino exchange
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• Addendum to Finite-size effects on multibody neutrino exchange
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