Thermodynamics of horizons in a globally regular spherically symmetric spacetime

DOI10.1134/S0202289312030048zbMath1258.83014OpenAlexW1978390131MaRDI QIDQ1933357

I. G. Dymnikova

Publication date: 23 January 2013

Published in: Gravitation \& Cosmology (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1134/s0202289312030048

zbMATH Keywords

thermodynamicshorizonanisotropic vacuum fluidasymptotically de Sitter

Mathematics Subject Classification ID

Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Classical and relativistic thermodynamics (80A10) Exact solutions to problems in general relativity and gravitational theory (83C15)

Cites Work

• Unnamed Item
• Vacuum dark fluid
• Quantum cooling evaporation process in regular black holes
• The generalized uncertainty principle and black hole remnants
• Spherically symmetric space-time with two cosmological constants.
• The cosmological term as a source of mass
• Nonsingular vacuum cosmologies with a variable cosmological term
• Quantum field theory with and without conical singularities: black holes with a cosmological constant and the multi-horizon scenario
• Classical and quantum thermodynamics of horizons in spherically symmetric spacetimes
• Spin foam models for quantum gravity
• The world as a hologram
• Black Holes and Entropy
• Regular homogeneous T-models with vacuum dark fluid
• SPHERICALLY SYMMETRIC SPACE–TIME WITH REGULAR DE SITTER CENTER
• The algebraic structure of a cosmological term in spherically symmetric solutions

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