Neutrostriction in Neutron stars

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dc.creatorIgnatovich, V. K.
dc.date2003-11-20
dc.date2006-06-29
dc.date.accessioned2026-07-07T06:34:37Z
dc.date.available2026-07-07T06:34:37Z
dc.descriptionIt is demonstrated that not only gravity, but also neutrostriction forces due to optical potential created by coherent elastic neutron-neutron scattering can hold a neutron star together. The latter forces can be stronger than gravitational ones. The effect of these forces on mass, radius and structure of the neutron star is estimated.
dc.description11 pages 4 fig added Updated historical part of paper. Communications with Dr. Blume
dc.identifierhttps://arxiv.org/abs/astro-ph/0311471
dc.identifierhttp://arxiv.org/abs/astro-ph/0311471
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/99579
dc.subjectAstrophysics
dc.titleNeutrostriction in Neutron stars
dc.typetext

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