Gravitational Phase Transition in Neutron Stars

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dc.creatorLano, R. P.
dc.date1996-11-10
dc.date.accessioned2026-07-07T03:31:22Z
dc.date.available2026-07-07T03:31:22Z
dc.descriptionThe possibility of a gravitational phase transition, especially with respect to neutron stars is investigated. First, a semiclassical treatment is given, predicting a gravitational London penetration depth of 12km for neutron stars. Second, the problem is considered from a Ginzburg-Landau point of view. A gravitational Meissner effect, a gravitational Aharanov-Bohm type effect and a gravitational ferromagnetic type phase are predicted. Finally, a field theoretic consideration predicts a mass term for the graviton below a certain critical temperature.
dc.description19 pages, standard LaTeX
dc.identifierhttps://arxiv.org/abs/gr-qc/9611023
dc.identifierhttp://arxiv.org/abs/gr-qc/9611023
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35837
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleGravitational Phase Transition in Neutron Stars
dc.typetext

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