K-essence in the DGP brane-world cosmology
We analyze a Dvali-Gabadadze-Porrati (DGP) brane filled with a k-essence field and assume the k field evolving linearly with the cosmic time of the brane. We then solve analytically the Friedmann equation and deduce the different behavior of the brane at the low- and the high-energy regimes. The asy...
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2010
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| LEADER | 09487caa a22008297a 4500 | ||
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| 003 | AR-BaUEN | ||
| 005 | 20230518203716.0 | ||
| 008 | 190411s2010 xx ||||fo|||| 00| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-78651264219 | |
| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 030 | |a PRVDA | ||
| 100 | 1 | |a Bouhmadi-López, M. | |
| 245 | 1 | 0 | |a K-essence in the DGP brane-world cosmology |
| 260 | |c 2010 | ||
| 270 | 1 | 0 | |m Bouhmadi-López, M.; Centro Multidisciplinar de Astrofísica-CENTRA, Departamento de Física, Instituto Superior Técnico, Av. Rovisco Pais 1, 1049-001 Lisboa, Portugal; email: mariam.bouhmadi@ist.utl.pt |
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| 520 | 3 | |a We analyze a Dvali-Gabadadze-Porrati (DGP) brane filled with a k-essence field and assume the k field evolving linearly with the cosmic time of the brane. We then solve analytically the Friedmann equation and deduce the different behavior of the brane at the low- and the high-energy regimes. The asymptotic behavior can be quite different involving accelerating branes, big bangs, big crunches, big rips, or quiescent singularities. The latter correspond to a type of sudden singularity. © 2010 The American Physical Society. |l eng | |
| 593 | |a Centro Multidisciplinar de Astrofísica-CENTRA, Departamento de Física, Instituto Superior Técnico, Av. Rovisco Pais 1, 1049-001 Lisboa, Portugal | ||
| 593 | |a Departamento de Física, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Ciudad Universitaria, Pabellón I, 1428 Buenos Aires, Argentina | ||
| 700 | 1 | |a Chimento, L.P. | |
| 773 | 0 | |d 2010 |g v. 82 |k n. 10 |p Phys Rev D Part Fields Gravit Cosmol |x 15507998 |t Physical Review D - Particles, Fields, Gravitation and Cosmology | |
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