Accelerating Branes and Brane Temperature
arXiv:0805.3488 · doi:10.1088/0264-9381/25/17/175017
Abstract
We define the local acceleration and jerk of a relativistic brane in an ambient spacetime, and construct from them a dimensionless parameter lambda that must be small for an interpretation of brane acceleration as local Unruh temperature. As examples, we discuss (i) open rotating branes, for which lambda>1 (ii) closed spherical branes expanding in Minkowski spacetime, for which lambda=0 when the worldvolume is either an Einstein static universe or de Sitter space, in which case the brane temperature equals the Gibbons-Hawking temperature, (iii) closed spherical branes in anti-de Sitter spacetime, for which a maximally symmetric worldvolume is anti-de Sitter, Minkowski or de Sitter according to whether the magnitude of the brane acceleration is less than, equal to or greater than a `critical' value, and (iv) the BTZ black hole, viewed as a membrane.
32 pages, small corrections
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- Rindler-AdS/CFT
- Relativistic Kinematics and Stationary Motions
- Accelerated detectors and worldsheet horizons in AdS/CFT
- On the response of a particle detector in Anti-de Sitter spacetime
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- String Entanglement and D-branes as Pure States
- Local free-fall temperature of a RN-AdS black hole
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- D7-brane dynamics and thermalization in the Kuperstein-Sonnenschein model
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