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Title: Greybody factors and charges in Kerr/CFT

Abstract

We compute greybody factors for near extreme Kerr black holes in D = 4 and D = 5. In D = 4 we include four charges so that our solutions can be continuously deformed to the BPS limit. In D = 5 we include two independent angular momenta so Left-Right symmetry is incorporated. We discuss the CFT interpretation of our emission amplitudes, including the overall frequency dependence and the dependence on all black hole parameters. We find that all additional parameters can be incorporated Kerr/CFT, with central charge independent of U(1) charges.

Authors:
 [1];  [2]
  1. Univ. of Pennsylvania, Philadelphia, PA (United States)
  2. Michigan Center for Theoretical Physics, Ann Arbor, MI (United States)
Publication Date:
Research Org.:
Univ. of Pennsylvania, Philadelphia, PA (United States)
Sponsoring Org.:
USDOE
OSTI Identifier:
1196561
Grant/Contract Number:  
FG02-95ER40893
Resource Type:
Accepted Manuscript
Journal Name:
Journal of High Energy Physics (Online)
Additional Journal Information:
Journal Name: Journal of High Energy Physics (Online); Journal Volume: 2009; Journal Issue: 09; Journal ID: ISSN 1029-8479
Publisher:
Springer Berlin
Country of Publication:
United States
Language:
English
Subject:
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; greybody factors

Citation Formats

Cvetič, Mirjam, and Larsen, Finn. Greybody factors and charges in Kerr/CFT. United States: N. p., 2009. Web. doi:10.1088/1126-6708/2009/09/088.
Cvetič, Mirjam, & Larsen, Finn. Greybody factors and charges in Kerr/CFT. United States. doi:10.1088/1126-6708/2009/09/088.
Cvetič, Mirjam, and Larsen, Finn. Tue . "Greybody factors and charges in Kerr/CFT". United States. doi:10.1088/1126-6708/2009/09/088. https://www.osti.gov/servlets/purl/1196561.
@article{osti_1196561,
title = {Greybody factors and charges in Kerr/CFT},
author = {Cvetič, Mirjam and Larsen, Finn},
abstractNote = {We compute greybody factors for near extreme Kerr black holes in D = 4 and D = 5. In D = 4 we include four charges so that our solutions can be continuously deformed to the BPS limit. In D = 5 we include two independent angular momenta so Left-Right symmetry is incorporated. We discuss the CFT interpretation of our emission amplitudes, including the overall frequency dependence and the dependence on all black hole parameters. We find that all additional parameters can be incorporated Kerr/CFT, with central charge independent of U(1) charges.},
doi = {10.1088/1126-6708/2009/09/088},
journal = {Journal of High Energy Physics (Online)},
number = 09,
volume = 2009,
place = {United States},
year = {2009},
month = {9}
}

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Cited by: 51 works
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