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The evolution of discontinuities in radiating spheres in the diffusion approximation
dc.rights.license | http://creativecommons.org/licenses/by-nc-sa/3.0/ve/ | |
dc.contributor.author | Barreto Acevedo, Willians | es_VE |
dc.contributor.author | Núñez, Luis | es_VE |
dc.contributor.author | Herrera, L. | es_VE |
dc.date | 2005-12-08 | es_VE |
dc.date.accessioned | 2005-12-08T09:00:00Z | |
dc.date.available | 2005-12-08T09:00:00Z | |
dc.date.created | 1991-07-10 | es_VE |
dc.date.issued | 2005-12-08T09:00:00Z | es_VE |
dc.identifier.other | T016300002554/0 | es_VE |
dc.identifier.uri | http://www.saber.ula.ve/handle/123456789/16868 | |
dc.description.abstract | The evolution of discontinuities in radiating spheres in the diffusion approximation (Barreto Acevedo, Willians; Herrera, L.; Núñez, Luis) Abstract The evolution of discontinuities in a general relativistic sphere free of singularities is studied. The energy transport mechanism through fluid is diffusive. The distribution of matter is divided by a shock wave front in two regions. The equations of state at both sides of the shock are different, and the solutions are matched on it via the Rankine-Hugoniot conditions. The outer metric joins the Vaidya solution at the boundary surface of the sphere. Exploding models are obtained, and their dynamics are studied using a generalized compressibility coefficient for nonadiabatic systems. Artículo publicado en: The Astrophysical Journal, 375:663-673,1991 July 10 | es_VE |
dc.format.extent | 1160305 | es_VE |
dc.language.iso | es | es_VE |
dc.publisher | SABER ULA | es_VE |
dc.rights | info:eu-repo/semantics/openAccess | |
dc.subject | Astrofísica | es_VE |
dc.subject | Distribuciones autogravitantes | es_VE |
dc.title | The evolution of discontinuities in radiating spheres in the diffusion approximation | es_VE |
dc.type | info:eu-repo/semantics/article | |
dc.description.email | wbarreto@ula.ve | es_VE |
dc.description.email | nunez@ula.ve | es_VE |
dc.description.email | laherrera@telcel.net.ve | es_VE |
dc.description.tiponivel | Nivel monográfico | es_VE |
dc.subject.facultad | Facultad de Ciencias. | es_VE |
dc.subject.keywords | Diffusion relativity | es_VE |
dc.subject.keywords | Shock waves | es_VE |
dc.subject.keywords | Astrophysics | es_VE |
dc.subject.keywords | Radiation distribution | es_VE |
dc.subject.keywords | Rankine-Hugoniot relation | es_VE |
dc.subject.keywords | Relativity | es_VE |
dc.subject.keywords | Shock discontinuity | es_VE |
dc.subject.keywords | Approximation | es_VE |
dc.subject.keywords | Diffusion | es_VE |
dc.subject.keywords | Heat transmission | es_VE |
dc.subject.keywords | Spheres | es_VE |
dc.subject.laboratorio | Laboratorio de Física Teórica | es_VE |
dc.subject.tipo | Artículos | es_VE |