The cosmological model with a wormhole and Hawking temperature near apparent horizon

DOI10.1016/J.PHYSLETB.2018.03.005zbMath1390.83032arXiv1801.07989OpenAlexW2791463443WikidataQ130173333 ScholiaQ130173333MaRDI QIDQ1750572

Sung-Won Kim

Publication date: 22 May 2018

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1801.07989

Mathematics Subject Classification ID

Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (1)

Revisiting the evolving Lorentzian wormhole: a general perspective

Cites Work

• Reissner-Nordstrom metric in the Friedman-Robertson-Walker universe
• New coordinates for de Sitter space and de Sitter radiation
• The Hawking temperature of a dynamical black hole in de Sitter spacetime
• Cosmological black holes: a black hole in the Einstein-de Sitter universe
• WORMHOLES IN SPACETIMES WITH COSMOLOGICAL HORIZONS
• Hawking radiation of an apparent horizon in a FRW universe
• LORENTZIAN WORMHOLES IN THE FRIEDMAN–ROBERTSON–WALKER UNIVERSE
• Wormhole cosmology and the horizon problem
• Wormholes in spacetime and their use for interstellar travel: A tool for teaching general relativity
• Unified first law of black-hole dynamics and relativistic thermodynamics
• Hawking Radiation As Tunneling

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