Gravitational Meissner Effect

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dc.creatorLano, R. P.
dc.date1996-03-12
dc.date.accessioned2026-07-07T04:21:57Z
dc.date.available2026-07-07T04:21:57Z
dc.descriptionThe gravitational analogue of the electromagnetic Meissner effect is investigated. Starting from the post-Newtonian approximation to general relativity we arrive at gravitational London equations, predicting a gravitational Meissner effect. Applied to neutron stars we arrive at a London penetration depth of 12km, which is about the size of a neutron star.
dc.descriptionSubmitted to Phys. Rev. D
dc.identifierhttps://arxiv.org/abs/hep-th/9603077
dc.identifierhttp://arxiv.org/abs/hep-th/9603077
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/54531
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleGravitational Meissner Effect
dc.typetext

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