Classical hair for Kerr-Newman black holes in string gravity

Bruce A. Campbell; Nemanja Kaloper; Keith A. Olive

doi:10.1016/0370-2693(92)91452-F

Classical hair for Kerr-Newman black holes in string gravity

Bruce A. Campbell, Nemanja Kaloper, Keith A. Olive

Physics and Astronomy (Twin Cities)

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76 Scopus citations

Abstract

We compute the external field strength hair present for black holes in string gravity. We retain all couplings in the effective lagrangian for string gravity through first order in α′, the string tension. We work in general black hole backgrounds, both rotating and charged, and compute both dilaton and axion hair to that order, thus expanding and systematizing previous treatments.

Original language	English (US)
Pages (from-to)	199-205
Number of pages	7
Journal	Physics Letters B
Volume	285
Issue number	3
DOIs	https://doi.org/10.1016/0370-2693(92)91452-F
State	Published - Jul 9 1992

Bibliographical note

Funding Information:
The work of B.A.C. was supported in part by the Natural Sciences and Engineering Research Council of Canada. The work of N.K. and K.A.O. was supported in part by DOE grant DE-AC02-83ER-40105. In addition the work of K.A.O. was also supported in part by a Presidential Young Investigator Award. The work of N.K. was supported in part by the University of Minnesota Doctoral Dissertation Fellowship.

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AU - Kaloper, Nemanja

AU - Olive, Keith A.

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N2 - We compute the external field strength hair present for black holes in string gravity. We retain all couplings in the effective lagrangian for string gravity through first order in α′, the string tension. We work in general black hole backgrounds, both rotating and charged, and compute both dilaton and axion hair to that order, thus expanding and systematizing previous treatments.

AB - We compute the external field strength hair present for black holes in string gravity. We retain all couplings in the effective lagrangian for string gravity through first order in α′, the string tension. We work in general black hole backgrounds, both rotating and charged, and compute both dilaton and axion hair to that order, thus expanding and systematizing previous treatments.

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ER -

Classical hair for Kerr-Newman black holes in string gravity

Abstract

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