A New Look to Massive Neutron Cores

dc.creatorBel, Ll.
dc.date2002-10-17
dc.date.accessioned2026-07-07T03:27:15Z
dc.date.available2026-07-07T03:27:15Z
dc.descriptionWe reconsider the problem of modelling static spherically symmetric perfect fluid configurations with an equation of state from a point of view of that requires the use of the concept of principal transform of a 3-dimensional Riemannian metric. We discuss from this new point of view the meaning of those familiar quantities that we call density, pressure and geometry in a relativistic context. This is not simple semantics. To prove it we apply the new ideas to recalculate the maximum mass that a massive neutron core can have. This limit is found to be of the order of 3.8 $M_\odot$ substantially larger than the Oppenheimer and Volkoff limit.
dc.description14 pages, Latex
dc.identifierhttps://arxiv.org/abs/gr-qc/0210057
dc.identifierhttp://arxiv.org/abs/gr-qc/0210057
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34360
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleA New Look to Massive Neutron Cores
dc.typetext

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