Gowdy Cosmological Models from Stringy Black Holes

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1. Verfasser: A. Herrera-Aguilar
Format: Artículo científico
Sprache:en
Veröffentlicht: Sociedad Mexicana de Física A.C. 2007
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author A. Herrera-Aguilar
author_facet A. Herrera-Aguilar
contents Gowdy Cosmological Models from Stringy Black Holes A. Herrera-Aguilar J.C. Mejía-Ambriz V. Rojas-Macías T. Cisneros-Pérez Física, Astronomía y Matemáticas rotating black holes low–energy string theory coordinate transformation Gowdy and Kantowski–Sachs cosmological models In the framework of 4D Einstein–Maxwell Dilaton–Axion theory we show how to obtain a family of both unpolarized and polarized S1£S2Gowdy cosmological models endowed with nontrivial axion, dilaton and electromagnetic fields from a solitonic rotating black hole–typesolution by interchanging the r and t coordinates in the region located between the horizons of the black hole configuration. We also obtaina family of Kantowski–Sachs cosmologies with topology R1 £S2 from the polarized Gowdy cosmological models by decompactifying oneof the compact dimensions. 2007 artículo científico 0035-001X https://www.redalyc.org/articulo.oa?id=57066210 https://www.redalyc.org/journal/570/57066210/ https://www.redalyc.org/journal/570/57066210/html/ https://www.redalyc.org/journal/570/57066210/57066210.epub https://www.redalyc.org/journal/570/57066210/movil en http://www.redalyc.org/revista.oa?id=570 Revista Mexicana de Física application/pdf Sociedad Mexicana de Física A.C. Revista Mexicana de Física (México) Num.2 Vol.53
format Artículo científico
id redalyc_57066210
institution Redalyc
language en
publishDate 2007
publisher Sociedad Mexicana de Física A.C.
spellingShingle Gowdy Cosmological Models from Stringy Black Holes
A. Herrera-Aguilar
Física, Astronomía y Matemáticas
rotating black holes
low–energy string theory
coordinate transformation
Gowdy and Kantowski–Sachs cosmological models
Gowdy Cosmological Models from Stringy Black Holes A. Herrera-Aguilar J.C. Mejía-Ambriz V. Rojas-Macías T. Cisneros-Pérez Física, Astronomía y Matemáticas rotating black holes low–energy string theory coordinate transformation Gowdy and Kantowski–Sachs cosmological models In the framework of 4D Einstein–Maxwell Dilaton–Axion theory we show how to obtain a family of both unpolarized and polarized S1£S2Gowdy cosmological models endowed with nontrivial axion, dilaton and electromagnetic fields from a solitonic rotating black hole–typesolution by interchanging the r and t coordinates in the region located between the horizons of the black hole configuration. We also obtaina family of Kantowski–Sachs cosmologies with topology R1 £S2 from the polarized Gowdy cosmological models by decompactifying oneof the compact dimensions. 2007 artículo científico 0035-001X https://www.redalyc.org/articulo.oa?id=57066210 https://www.redalyc.org/journal/570/57066210/ https://www.redalyc.org/journal/570/57066210/html/ https://www.redalyc.org/journal/570/57066210/57066210.epub https://www.redalyc.org/journal/570/57066210/movil en http://www.redalyc.org/revista.oa?id=570 Revista Mexicana de Física application/pdf Sociedad Mexicana de Física A.C. Revista Mexicana de Física (México) Num.2 Vol.53
title Gowdy Cosmological Models from Stringy Black Holes
topic Física, Astronomía y Matemáticas
rotating black holes
low–energy string theory
coordinate transformation
Gowdy and Kantowski–Sachs cosmological models
url https://www.redalyc.org/articulo.oa?id=57066210
https://www.redalyc.org/journal/570/57066210/
https://www.redalyc.org/journal/570/57066210/html/
https://www.redalyc.org/journal/570/57066210/57066210.epub
https://www.redalyc.org/journal/570/57066210/movil