z-logo
open-access-imgOpen Access
A black hole instability in five dimensions?
Author(s) -
Donald Marolf,
Amitabh Virmani
Publication year - 2005
Publication title -
journal of high energy physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.998
H-Index - 261
eISSN - 1126-6708
pISSN - 1029-8479
DOI - 10.1088/1126-6708/2005/11/026
Subject(s) - physics , angular momentum , black hole (networking) , merge (version control) , instability , rotating black hole , extremal black hole , classical mechanics , horizon , mechanics , computer network , routing protocol , routing (electronic design automation) , astronomy , computer science , information retrieval , link state routing protocol
We study the moduli-space scattering of a two-charge supertube in thebackground of a rotating BPS D1-D5-P black hole in 4+1 dimensions, extendingthe static analysis of Bena and Kraus (hep-th/0402144). While the magneticforces associated with this motion change the details considerably, the finalconclusion is similar to that of the static analysis: we find that one canbring the supertube to the horizon, so that the BMPV black hole and thesupertube merge. However, our analysis shows that this can occur even atsignificantly larger values of the angular momentum than was indicated by thestatic analysis. For a range of parameters, conservation laws and the areatheorem forbid the result of the merger from being any single known object:neither near-extremal black holes nor non-supersymmetric black rings areallowed. Such results suggest that the merger triggers an instability of therotating D1-D5-P black hole, perhaps leading to bifurcation into a pair ofblack objects.Comment: 25 pages, 4 figures; v2: references adde

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom