Charged Schroedinger black holes

Journal Article · Tue Dec 15 04:00:00 EST 2009 · Physical Review. D, Particles Fields

DOI:https://doi.org/10.1103/PHYSREVD.80.125018· OSTI ID:21316569

Adams, Allan ^[1]; Brown, Charles Max; DeWolfe, Oliver; Rosen, Christopher ^[2]

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1. Center for Theoretical Physics, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139 (United States)
2. Department of Physics 390 UCB, University of Colorado, Boulder, Colorado 80309 (United States)

We construct charged and rotating asymptotically Schroedinger black hole solutions of type IIB supergravity. We begin by obtaining a closed-form expression for the null Melvin twist of a broad class of type IIB backgrounds, including solutions of minimal five-dimensional gauged supergravity, and identify the resulting five-dimensional effective action. We use these results to demonstrate that the near-horizon physics and thermodynamics of asymptotically Schroedinger black holes obtained in this way are essentially inherited from their anti-de Sitter (AdS) progenitors, and verify that they admit zero-temperature extremal limits with AdS{sub 2} near-horizon geometries. Notably, the AdS{sub 2} radius is parametrically larger than that of the asymptotic Schroedinger space.

• OSTI ID: 21316569
• Journal Information: Physical Review. D, Particles Fields, Journal Name: Physical Review. D, Particles Fields Journal Issue: 12 Vol. 80; ISSN PRVDAQ; ISSN 0556-2821
• Country of Publication: United States
• Language: English

Related Subjects

72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
79 ASTRONOMY AND ASTROPHYSICS
ANTI DE SITTER SPACE
ASYMPTOTIC SOLUTIONS
BLACK HOLES
SCHROEDINGER EQUATION
SUPERGRAVITY
THERMODYNAMICS