Intersecting M-branes as four-dimensional black holes

I. R. Klebanov; A. A. Tseytlin

doi:10.1016/0550-3213(96)00338-0

Intersecting M-branes as four-dimensional black holes

I. R. Klebanov, A. A. Tseytlin

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Abstract

We present two 1/8 supersymmetric intersecting p-brane solutions of 11-dimensional supergravity which upon compactification to four dimensions reduce to extremal dyonic black holes with finite area of horizon. The first solution is a configuration of three intersecting 5-branes with an extra momentum flow along the common string. The second describes a system of two 2-branes and two 5-branes. Related (by compactification and T-duality) solution of type IIB theory corresponds to a completely symmetric configuration of four intersecting 3-branes. We suggest methods for counting the BPS degeneracy of three intersecting 5-branes which, in the macroscopic limit, reproduce the Bekenstein-Hawking entropy.

Original language	English (US)
Pages (from-to)	179-192
Number of pages	14
Journal	Nuclear Physics B
Volume	475
Issue number	1-2
DOIs	https://doi.org/10.1016/0550-3213(96)00338-0
State	Published - Sep 9 1996

All Science Journal Classification (ASJC) codes

Nuclear and High Energy Physics

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10.1016/0550-3213(96)00338-0

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@article{02f104b09b2141de8e0956098326e551,

title = "Intersecting M-branes as four-dimensional black holes",

abstract = "We present two 1/8 supersymmetric intersecting p-brane solutions of 11-dimensional supergravity which upon compactification to four dimensions reduce to extremal dyonic black holes with finite area of horizon. The first solution is a configuration of three intersecting 5-branes with an extra momentum flow along the common string. The second describes a system of two 2-branes and two 5-branes. Related (by compactification and T-duality) solution of type IIB theory corresponds to a completely symmetric configuration of four intersecting 3-branes. We suggest methods for counting the BPS degeneracy of three intersecting 5-branes which, in the macroscopic limit, reproduce the Bekenstein-Hawking entropy.",

author = "Klebanov, {I. R.} and Tseytlin, {A. A.}",

note = "Funding Information: We are grateful to V. Balasubramanian, C. Callan and M. Cveti~ for useful discussions. I.R.K. was supported in part by DOE grant DE-FG02-91ER40671, the NSF Presidential Young Investigator Award PHY-9157482, and the James S. McDonnell Foundation grant No. 91-48. A.A.T. would like to acknowledge the support of PPARC, ECC grant SC1{"}-CT92-0789 and NATO grant CRG 940870.",

year = "1996",

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doi = "10.1016/0550-3213(96)00338-0",

language = "English (US)",

volume = "475",

pages = "179--192",

journal = "Nuclear Physics B",

issn = "0550-3213",

publisher = "Elsevier",

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T1 - Intersecting M-branes as four-dimensional black holes

AU - Klebanov, I. R.

AU - Tseytlin, A. A.

N1 - Funding Information: We are grateful to V. Balasubramanian, C. Callan and M. Cveti~ for useful discussions. I.R.K. was supported in part by DOE grant DE-FG02-91ER40671, the NSF Presidential Young Investigator Award PHY-9157482, and the James S. McDonnell Foundation grant No. 91-48. A.A.T. would like to acknowledge the support of PPARC, ECC grant SC1"-CT92-0789 and NATO grant CRG 940870.

PY - 1996/9/9

Y1 - 1996/9/9

N2 - We present two 1/8 supersymmetric intersecting p-brane solutions of 11-dimensional supergravity which upon compactification to four dimensions reduce to extremal dyonic black holes with finite area of horizon. The first solution is a configuration of three intersecting 5-branes with an extra momentum flow along the common string. The second describes a system of two 2-branes and two 5-branes. Related (by compactification and T-duality) solution of type IIB theory corresponds to a completely symmetric configuration of four intersecting 3-branes. We suggest methods for counting the BPS degeneracy of three intersecting 5-branes which, in the macroscopic limit, reproduce the Bekenstein-Hawking entropy.

AB - We present two 1/8 supersymmetric intersecting p-brane solutions of 11-dimensional supergravity which upon compactification to four dimensions reduce to extremal dyonic black holes with finite area of horizon. The first solution is a configuration of three intersecting 5-branes with an extra momentum flow along the common string. The second describes a system of two 2-branes and two 5-branes. Related (by compactification and T-duality) solution of type IIB theory corresponds to a completely symmetric configuration of four intersecting 3-branes. We suggest methods for counting the BPS degeneracy of three intersecting 5-branes which, in the macroscopic limit, reproduce the Bekenstein-Hawking entropy.

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U2 - 10.1016/0550-3213(96)00338-0

DO - 10.1016/0550-3213(96)00338-0

M3 - Article

AN - SCOPUS:0030576771

SN - 0550-3213

VL - 475

SP - 179

EP - 192

JO - Nuclear Physics B

JF - Nuclear Physics B

IS - 1-2

ER -

Intersecting M-branes as four-dimensional black holes

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