Black Hole Astrophysics in AdS Braneworlds View Full Text


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Article Info

DATE

2003-01-31

AUTHORS

Roberto Emparan, Juan García-Bellido, Nemanja Kaloper

ABSTRACT

We consider astrophysics of large black holes localized on the brane in the infinite Randall-Sundrum model. Using their description in terms of a conformal field theory (CFT) coupled to gravity, deduced in ref. [1], we show that they undergo a period of rapid decay via Hawking radiation of CFT modes. For example, a black hole of mass few × M⊙ would shed most of its mass in ~ 104−105 years if the AdS radius is L ~ 10−1 mm, currently the upper bound from table-top experiments. Since this is within the mass range of X-ray binary systems containing a black hole, the evaporation enhanced by the hidden sector CFT modes could cause the disappearance of X-ray sources on the sky. This would be a striking signature of RS2 with a large AdS radius. Alternatively, for shorter AdS radii, the evaporation would be slower. In such cases, the persistence of X-ray binaries with black holes already implies an upper bound on the AdS radius of L10−2 mm, an order of magnitude better than the bounds from table-top experiments. The observation of primordial black holes with a mass in the MACHO range M ~ 0.1−0.5 M⊙ and an age comparable to the age of the universe would further strengthen the bound on the AdS radius to Lfew × 10−6 mm. More... »

PAGES

079

References to SciGraph publications

  • 2001-08-06. Holography and phenomenology in JOURNAL OF HIGH ENERGY PHYSICS
  • 1999-09. Evidence of a supernova origin for the black hole in the system GRO J1655 - 40 in NATURE
  • 1975-08. Particle creation by black holes in COMMUNICATIONS IN MATHEMATICAL PHYSICS
  • 1998-04. Microquasars in our Galaxy in NATURE
  • 2002-08-27. Quantum Black Holes as Holograms in AdS Braneworlds in JOURNAL OF HIGH ENERGY PHYSICS
  • Identifiers

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    http://scigraph.springernature.com/pub.10.1088/1126-6708/2003/01/079

    DOI

    http://dx.doi.org/10.1088/1126-6708/2003/01/079

    DIMENSIONS

    https://app.dimensions.ai/details/publication/pub.1052622948


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    41 schema:description We consider astrophysics of large black holes localized on the brane in the infinite Randall-Sundrum model. Using their description in terms of a conformal field theory (CFT) coupled to gravity, deduced in ref. [1], we show that they undergo a period of rapid decay via Hawking radiation of CFT modes. For example, a black hole of mass few × M⊙ would shed most of its mass in ~ 104−105 years if the AdS radius is L ~ 10−1 mm, currently the upper bound from table-top experiments. Since this is within the mass range of X-ray binary systems containing a black hole, the evaporation enhanced by the hidden sector CFT modes could cause the disappearance of X-ray sources on the sky. This would be a striking signature of RS2 with a large AdS radius. Alternatively, for shorter AdS radii, the evaporation would be slower. In such cases, the persistence of X-ray binaries with black holes already implies an upper bound on the AdS radius of L10−2 mm, an order of magnitude better than the bounds from table-top experiments. The observation of primordial black holes with a mass in the MACHO range M ~ 0.1−0.5 M⊙ and an age comparable to the age of the universe would further strengthen the bound on the AdS radius to Lfew × 10−6 mm.
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