\(\langle\phi^2\rangle\) in the spacetime of a cylindrical black hole

DOI10.1023/A:1026734521256zbMath0932.83027arXivgr-qc/9804032OpenAlexW1589859410MaRDI QIDQ1964551

Andrew DeBenedictis

Publication date: 20 February 2000

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/9804032

zbMATH Keywords

black holesvacuum polarizationanti-de SitterHartle-Hawking vacuum state

Mathematics Subject Classification ID

Black holes (83C57) Quantum field theory on curved space or space-time backgrounds (81T20) Methods of quantum field theory in general relativity and gravitational theory (83C47)

Related Items (4)

Vacuum currents in partially compactified Rindler spacetime with an application to cylindrical black holes ⋮ Characteristics of quantum radiation as tunneling from a cylindrically symmetric black hole ⋮ Vacuum polarization on topological black holes ⋮ Quantum statistical entropy of black hole

Cites Work

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• Anti-de Sitter space, thermal phase transition, and confinement in gauge theories.
• Semiclassical effects in black hole interiors
• Stress-energy tensor of quantized scalar fields in static spherically symmetric spacetimes
• Some special solutions of the equations of axially symmetric gravitational fields
• Formation of naked singularities: The violation of cosmic censorship
• Black hole in three-dimensional spacetime
• Quantum Fields in Curved Space

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