| Revue: | Revista mexicana de física |
| Base de datos: | PERIÓDICA |
| Número de sistema: | 000404273 |
| ISSN: | 0035-001X |
| Autores: | García Aspeitia, M.A1 Ortiz, C2 López Domínguez, J.C2 Hinojosa Ruiz, S2 Reyes Ibarra, M.J3 |
| Instituciones: | 1Consejo Nacional de Ciencia y Tecnología, Ciudad de México. México 2Universidad Autónoma de Zacatecas, Unidad Académica de Física, Zacatecas. México 3Instituto Politécnico Nacional, Centro de Investigación y de Estudios Avanzados, Ciudad de México. México |
| Año: | 2016 |
| Periodo: | May-Jun |
| Volumen: | 62 |
| Número: | 3 |
| Paginación: | 199-205 |
| País: | México |
| Idioma: | Inglés |
| Tipo de documento: | Artículo |
| Enfoque: | Analítico, teórico |
| Resumen en inglés | This paper is dedicated to revisit the modifications caused by branes in the collapse of a stellar structure under the Snyder-Oppenheimer scheme. Due to the homogeneity and isotropy of the model, we choose study the case of a closed geometry described by k = 1, through the tool of dynamical systems. We revisit the different components of the star and its evolution during the stellar collapse, paying particular attention to the non-local effects and the quadratic terms of the energy momentum tensor that come from branes corrections. In the same vein we realize a phase portrait together with a stability analysis with the aim of obtain information about the attractors or saddle points of the dynamical system under different initial conditions in the density parameters, remarking the parameters that come from branes contributions |
| Disciplinas: | Física y astronomía |
| Palabras clave: | Astronomía, Física, Astrofísica, Branas, Colapso gravitacional |
| Keyword: | Physics and astronomy, Astronomy, Physics, Astrophysics, Branes, Gravitational collapse |
| Texte intégral: | Texto completo (Ver PDF) |
