Analytic Lifshitz black holes in higher dimensions

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We generalize the four-dimensional R 2-corrected z = 3/2 Lifshitz black hole to a two-parameter family of black hole solutions for any dynamical exponent z and for any dimension D. For a particular relation between the parameters, we find the first example of an extremal Lifshitz black hole. An asym...

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Autor principal: Ayón-Beato, E.
Otros Autores: Garbarz, A., Giribet, G., Hassaïne, M.
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: 2010
Acceso en línea:Registro en Scopus
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Biblioteca Central Dr. Luis F. Leloir (FCEN) de Universidad de Buenos Aires
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100 1 |a Ayón-Beato, E. 
245 1 0 |a Analytic Lifshitz black holes in higher dimensions 
260 |c 2010 
270 1 0 |m Ayón-Beato, E.; Departamento de Física, CINVESTAV-IPN, Apdo. Postal 14-740, 07000, México D.F., Mexico; email: ayon-beato@fis.cinvestav.mx 
506 |2 openaire  |e Política editorial 
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504 |a Myung, Y.S., Kim, Y.-W., Park, Y.-J., Dilaton Gravity Approach to Three Dimensional Lifshitz Black Hole, , arXiv: 0910.4428 [SPIRES] 
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520 3 |a We generalize the four-dimensional R 2-corrected z = 3/2 Lifshitz black hole to a two-parameter family of black hole solutions for any dynamical exponent z and for any dimension D. For a particular relation between the parameters, we find the first example of an extremal Lifshitz black hole. An asymptotically Lifshitz black hole with a logarithmic decay is also exhibited for a specific critical exponent depending on the dimension. We extend this analysis to the more general quadratic curvature corrections for which we present three new families of higher-dimensional D ≥ 5 analytic Lifshitz black holes for generic z. One of these higher-dimensional families contains as critical limits the z = 3 three-dimensional Lifshitz black hole and a new z = 6 four-dimensional black hole. The variety of analytic solutions presented here encourages to explore these gravity models within the context of non-relativistic holographic correspondence. © SISSA 2010.  |l eng 
593 |a Departamento de Física, CINVESTAV-IPN, Apdo. Postal 14-740, 07000, México D.F., Mexico 
593 |a Departamento de Física, Universidad de Buenos Aires FCEN - UBA, Ciudad Universitaria, Pabellón 1, 1428, Buenos Aires, Argentina 
593 |a Departamento de Física, Universidad de Buenos Aires FCEN - UBA and CONICET, Ciudad Universitaria, Pabellón 1, 1428, Buenos Aires, Argentina 
593 |a Instituto de Matemática y Física, Universidad de Talca, Casilla 747, Talca, Chile 
690 1 0 |a ADS-CFT CORRESPONDENCE 
690 1 0 |a BLACK HOLES 
700 1 |a Garbarz, A. 
700 1 |a Giribet, G. 
700 1 |a Hassaïne, M. 
773 0 |d 2010  |g v. 2010  |k n. 4  |p J. High Energy Phys.  |x 11266708  |t Journal of High Energy Physics 
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856 4 0 |u https://doi.org/10.1007/JHEP04(2010)030  |y DOI 
856 4 0 |u https://hdl.handle.net/20.500.12110/paper_11266708_v2010_n4_p_AyonBeato  |y Handle 
856 4 0 |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_11266708_v2010_n4_p_AyonBeato  |y Registro en la Biblioteca Digital 
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