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U duality, D-branes, and black hole emission rates: Agreements and disagreements
Physics Review D
  • F Dowker
  • David Kastor, University of Massachusetts - Amherst
  • Jennie Traschen, University of Massachusetts - Amherst
Publication Date
1998
Abstract
An expression for the spacetime absorption coefficient of a scalar field in a five-dimensional, near-extremal black hole background is derived, which has the same form as that presented by Maldacena and Strominger, but is valid over a larger, U-duality invariant region of parameter space and in general disagrees with the corresponding D-brane result. We develop an argument, based on D-brane thermodynamics, which specifies the range of parameters over which agreement should be expected. For neutral emission, the spacetime and D-brane results agree over this range. However, for charged emission, we find disagreement in the “fat black hole” regime, in which charge is quantized in smaller units on the brane than in the bulk of spacetime. We indicate a possible problem with the D-brane model in this regime. We also use the Born approximation to study the high frequency limit of the absorption coefficient and find that it approaches unity, for large black hole backgrounds, at frequencies still below the string scale, again in disagreement with D-brane results.
Comments
This is the pre-published version harvested from ArXiv. The published version is located at http://prd.aps.org/abstract/PRD/v58/i12/e124025
Citation Information
F Dowker, David Kastor and Jennie Traschen. "U duality, D-branes, and black hole emission rates: Agreements and disagreements" Physics Review D Vol. 58 Iss. 12 (1998)
Available at: http://works.bepress.com/david_kastor/31/