Comparing decay rates for black holes and D-branes

Sumit R. Das; Samir D. Mathur

doi:10.1016/0550-3213(96)00453-1

Comparing decay rates for black holes and D-branes

Sumit R. Das
, Samir D. Mathur

Producción científica: Article › revisión exhaustiva

271 Citas (Scopus)

Resumen

We compute the leading order (in coupling) rate of emission of low energy quanta from a slightly non-extremal system of 1-D-and 5-D-branes. We also compute the classical cross-section, and hence the Hawking emission rate, for low energy scalar quanta for the black hole geometry that corresponds to these branes (at sufficiently strong coupling). These rates are found to agree with each other.

Idioma original	English
Páginas (desde-hasta)	561-576
Número de páginas	16
Publicación	Nuclear Physics B
Volumen	478
N.º	3
DOI	https://doi.org/10.1016/0550-3213(96)00453-1
Estado	Published - nov 4 1996

ASJC Scopus subject areas

Nuclear and High Energy Physics

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10.1016/0550-3213(96)00453-1

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title = "Comparing decay rates for black holes and D-branes",

abstract = "We compute the leading order (in coupling) rate of emission of low energy quanta from a slightly non-extremal system of 1-D-and 5-D-branes. We also compute the classical cross-section, and hence the Hawking emission rate, for low energy scalar quanta for the black hole geometry that corresponds to these branes (at sufficiently strong coupling). These rates are found to agree with each other.",

author = "Das, \{Sumit R.\} and Mathur, \{Samir D.\}",

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AU - Mathur, Samir D.

PY - 1996/11/4

Y1 - 1996/11/4

N2 - We compute the leading order (in coupling) rate of emission of low energy quanta from a slightly non-extremal system of 1-D-and 5-D-branes. We also compute the classical cross-section, and hence the Hawking emission rate, for low energy scalar quanta for the black hole geometry that corresponds to these branes (at sufficiently strong coupling). These rates are found to agree with each other.

AB - We compute the leading order (in coupling) rate of emission of low energy quanta from a slightly non-extremal system of 1-D-and 5-D-branes. We also compute the classical cross-section, and hence the Hawking emission rate, for low energy scalar quanta for the black hole geometry that corresponds to these branes (at sufficiently strong coupling). These rates are found to agree with each other.

UR - https://www.scopus.com/pages/publications/0030569235

UR - https://www.scopus.com/pages/publications/0030569235#tab=citedBy

U2 - 10.1016/0550-3213(96)00453-1

DO - 10.1016/0550-3213(96)00453-1

M3 - Article

AN - SCOPUS:0030569235

SN - 0550-3213

VL - 478

SP - 561

EP - 576

JO - Nuclear Physics B

JF - Nuclear Physics B

IS - 3

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Comparing decay rates for black holes and D-branes

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