Supersymmetric rotating black holes and attractors

Journal Article · Fri Feb 28 23:00:00 EST 1997 · Physical Review, D

DOI:https://doi.org/10.1103/PhysRevD.55.R3246· OSTI ID:520950

Kallosh, R ^[1]; Rajaraman, A ^[2]; Kai Wong, W ^[1]

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1. Physics Department, Stanford University, Stanford, California 94305-4060 (United States)
2. Stanford Linear Accelerator Center, Stanford University, Stanford, California 94309 (United States)

Five-dimensional stringy rotating black holes are embedded into N=2 supergravity interacting with one vector multiplet. The existence of an unbroken supersymmetry of the rotating solution is proved directly by solving the Killing spinor equations. The asymptotic enhancement of supersymmetry near the horizon in the presence of rotation is established via the calculation of the supercurvature. The area of the horizon of the rotating supersymmetric black holes is found to be {radical}(Z{sub fix}{sup 3}{minus}J{sup 2}), where Z{sub fix} is the extremal value of the central charge in moduli space. {copyright} {ital 1997} {ital The American Physical Society}

• Research Organization: Stanford Linear Accelerator Center
• DOE Contract Number: AC03-76SF00515
• OSTI ID: 520950
• Journal Information: Physical Review, D, Journal Name: Physical Review, D Journal Issue: 6 Vol. 55; ISSN PRVDAQ; ISSN 0556-2821
• Country of Publication: United States
• Language: English

Related Subjects

66 PHYSICS
ATTRACTORS
BLACK HOLES
MANY-DIMENSIONAL CALCULATIONS
MULTIPLETS
ROTATION
STRING MODELS
SUPERGRAVITY
SUPERSYMMETRY
VECTORS