Black Holes and Nonrelativistic Quantum Systems

We describe black holes in d+3 dimensions, whose thermodynamic properties correspond to those of a scale-invariant nonrelativistic (d+1)-dimensional quantum system with a dynamical exponent z=2. The gravitational model involves a massive Abelian vector field and a scalar field, in addition to the me...

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Main Authors: Nickel, Marcel Dominik Johannes, Kovtun, Pavel
其他作者: Massachusetts Institute of Technology. Center for Theoretical Physics
格式: 文件
语言:en_US
出版: American Physical Society 2010
在线阅读:http://hdl.handle.net/1721.1/51771
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author Nickel, Marcel Dominik Johannes
Kovtun, Pavel
author2 Massachusetts Institute of Technology. Center for Theoretical Physics
author_facet Massachusetts Institute of Technology. Center for Theoretical Physics
Nickel, Marcel Dominik Johannes
Kovtun, Pavel
author_sort Nickel, Marcel Dominik Johannes
collection MIT
description We describe black holes in d+3 dimensions, whose thermodynamic properties correspond to those of a scale-invariant nonrelativistic (d+1)-dimensional quantum system with a dynamical exponent z=2. The gravitational model involves a massive Abelian vector field and a scalar field, in addition to the metric. The energy per particle in the dual theory is |μ|d/(d+2) at any temperature (μ is the chemical potential). The ratio of shear viscosity to entropy density is ℏ/4π in any dimension d≥2.
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spelling mit-1721.1/517712022-10-02T06:33:43Z Black Holes and Nonrelativistic Quantum Systems Nickel, Marcel Dominik Johannes Kovtun, Pavel Massachusetts Institute of Technology. Center for Theoretical Physics Nickel, Marcel Dominik Johannes Nickel, Marcel Dominik Johannes We describe black holes in d+3 dimensions, whose thermodynamic properties correspond to those of a scale-invariant nonrelativistic (d+1)-dimensional quantum system with a dynamical exponent z=2. The gravitational model involves a massive Abelian vector field and a scalar field, in addition to the metric. The energy per particle in the dual theory is |μ|d/(d+2) at any temperature (μ is the chemical potential). The ratio of shear viscosity to entropy density is ℏ/4π in any dimension d≥2. NSERC of Canada German Research Foundation (DFG) Department of Energy 2010-02-17T16:36:39Z 2010-02-17T16:36:39Z 2009-01 2008-09 Article http://purl.org/eprint/type/JournalArticle 0031-9007 http://hdl.handle.net/1721.1/51771 Kovtun, Pavel , and Dominik Nickel. “Black Holes and Nonrelativistic Quantum Systems.” Physical Review Letters 102.1 (2009): 011602. © 2009 The American Physical Society. en_US http://dx.doi.org/10.1103/PhysRevLett.102.011602 Physical Review Letters Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. application/pdf American Physical Society APS
spellingShingle Nickel, Marcel Dominik Johannes
Kovtun, Pavel
Black Holes and Nonrelativistic Quantum Systems
title Black Holes and Nonrelativistic Quantum Systems
title_full Black Holes and Nonrelativistic Quantum Systems
title_fullStr Black Holes and Nonrelativistic Quantum Systems
title_full_unstemmed Black Holes and Nonrelativistic Quantum Systems
title_short Black Holes and Nonrelativistic Quantum Systems
title_sort black holes and nonrelativistic quantum systems
url http://hdl.handle.net/1721.1/51771
work_keys_str_mv AT nickelmarceldominikjohannes blackholesandnonrelativisticquantumsystems
AT kovtunpavel blackholesandnonrelativisticquantumsystems