D-brane decay and Hawking radiation - INSPIRE

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D-brane decay and Hawking radiation

Sumit R. Das
(
- Tata Inst.
)

Jun, 1997

9 pages

Part of Strings. Proceedings, International Conference, Strings'97, Amsterdam, Netherlands, June 16-21, 1997, 119-127

Published in:

Nucl.Phys.B Proc.Suppl. 68 (1998) 119-127

Contribution to:

Strings 97 Meeting, 119-127

e-Print:

hep-th/9709206 [hep-th]

DOI:

10.1016/S0920-5632(98)00146-7

Report number:

TIFR-TH-97-52

View in:

ADS Abstract Service

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Abstract:

Tree level decay amplitudes of near-BPS D-brane configurations are known to exactly reproduce Hawking radiation rates from corresponding black holes at low energies even though the brane configurations describe semiclassical black holes only when the open string couplings are large. We show that a large class of one (open string) loop corrections to emission processes from D-branes vanish at low energies and nonvanishing loop contributions have an energy dependence consistent with black hole answers, thus providing a justification for the agreement of the tree level results with semiclassical answers.

talk: Amsterdam 1997/06/16
membrane model: D-brane
decay: D-brane
amplitude analysis: decay
radiation: Hawking
black hole: semiclassical
cross section: absorption
string: open
correction: higher-order
bibliography

References(64)

Figures(0)

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