Gravitational field energy contribution to the neutron star mass

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dc.creatorDyrda, M.
dc.creatorKinasiewicz, B.
dc.creatorKutschera, M.
dc.creatorSzmaglinski, A.
dc.date2006-01-16
dc.date.accessioned2026-07-07T06:58:04Z
dc.date.available2026-07-07T06:58:04Z
dc.descriptionNeutron stars are discussed as laboratories of physics of strong gravitational fields. The mass of a neutron star is split into matter energy and gravitational field energy contributions. The energy of the gravitational field of neutron stars is calculated with three different approaches which give the same result. It is found that up to one half of the gravitational mass of maximum mass neutron stars is comprised by the gravitational field energy. Results are shown for a number of realistic equations of state of neutron star matter.
dc.description19 pages, 18 figures
dc.identifierhttps://arxiv.org/abs/gr-qc/0601061
dc.identifierhttp://arxiv.org/abs/gr-qc/0601061
dc.identifierActa Phys.Polon. B37 (2006) 357-376
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/107214
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleGravitational field energy contribution to the neutron star mass
dc.typetext

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