The neutrino ground state in a neutron star

Details The neutrino ground state in a neutron star The neutrino ground state in a neutron star

1998-07-18

arxiv.org/abs/hep-ph/9807412v1

Nucl.Phys.Proc.Suppl. 77 (1999) 445-449

Physics

High Energy Physics

High Energy Physics - Phenomenology

5 pages, 3 figures, Latex (uses espcrc2.sty); contribution to the proceedings of Neutrino 98, Takayama, Japan, 4-9 June, 1998

Scientific paper

10.1016/S0920-5632(99)00464-8

We address a recent claim that the stability of neutron stars implies a lower bound on the mass of the neutrino. We argue that the result obtained by some previous authors is due to an improper summation of an infrared-sensitive series and that a non-perturbative "resummation" of the series yields a finite and well-behaved result. The stability of neutron stars thus gives no lower bound on the mass of the neutrino.

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