LORENTZIAN WORMHOLES IN THE FRIEDMAN–ROBERTSON–WALKER UNIVERSE
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Publication:3430047
DOI10.1142/S0218271806008851zbMath1119.83041arXivgr-qc/0606049OpenAlexW3123657768MaRDI QIDQ3430047
Behrouz Mirza, Shahram Dehdashti, Madjid Eshaghi-Gordji
Publication date: 20 March 2007
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/gr-qc/0606049
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The cosmological model with a wormhole and Hawking temperature near apparent horizon ⋮ Evolution of cosmological horizons of wormhole cosmology
Cites Work
- Reissner-Nordstrom metric in the Friedman-Robertson-Walker universe
- How much negative energy does a wormhole need?
- Topological censorship
- Wormhole cosmology and the horizon problem
- Null Energy Condition in Dynamic Wormholes
- Wormholes in spacetime and their use for interstellar travel: A tool for teaching general relativity
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