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Attractor Behaviour of Non-Supersymmetric Black Holes for type IIB Compactification

Journal Article · · AIP Conference Proceedings
DOI:https://doi.org/10.1063/1.2803802· OSTI ID:21035950
 [1]
  1. Department of Physics, IIT Roorkee (India)

We look for possible non-supersymmetric black hole attractor solutions for type IIB compactified on (the mirror of) CY{sub 3}(2,128) expressed as a degree-12 hypersurface in WCP{sup 4}[1,1,2,2,6], for points away from the conifold locus, and for points near the conifold locus. We also discuss application of Kallosh's attractor equations (which are equivalent to the extremization of the effective black-hole potential) for nonsupersymmetric attractors and show that (a) for points away from the conifold locus, the attractor equations demand that the attractor solutions be independent of one of the two complex structure moduli, and (b) for points near the conifold locus, the attractor equations imply switching off of one of the six components of the fluxes. Both these features are more obvious using the atractor equations than the extremization of the black hole potential.

OSTI ID:
21035950
Journal Information:
AIP Conference Proceedings, Journal Name: AIP Conference Proceedings Journal Issue: 1 Vol. 939; ISSN 0094-243X; ISSN APCPCS
Country of Publication:
United States
Language:
English

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