Is the cosmological singularity thermodynamically possible?

DOI10.1007/BF00670342zbMath0703.53085OpenAlexW2048192939WikidataQ56505165 ScholiaQ56505165MaRDI QIDQ916123

Jacob D. Bekenstein

Publication date: 1989

Published in: International Journal of Theoretical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf00670342

zbMATH Keywords

Friedmann initial singularity

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Applications of global differential geometry to the sciences (53C80)

Related Items (13)

Thermodynamics of conformal fields in topologically non-trivial space-time backgrounds ⋮ Holography and the generalized second law of thermodynamics in \((2+1)\)-dimensional cosmology ⋮ Generalized second law in string cosmology ⋮ Relating Friedmann equation to Cardy formula in universes with cosmological constant ⋮ CFT, holography, and causal entropy bound ⋮ Universe explosions ⋮ The holographic principle ⋮ INFLATION AS A RESPONSE TO PROTECT THE HOLOGRAPHIC PRINCIPLE ⋮ Singularity theorems and their consequences ⋮ Entropy generation and inflation in wave collision induced pre-big-bang cosmology ⋮ Holography, Cosmology, and the Second Law of Thermodynamics ⋮ Generalized Second Law in Cosmology from Causal Boundary Entropy ⋮ Bekenstein–Hawking entropy in expanding universes from black hole theorems

Cites Work

• The singularities of gravitational collapse and cosmology
• Black Holes and Entropy
• Inflationary universe: A possible solution to the horizon and flatness problems
• Singularities in Closed Universes
• The Large Scale Structure of Space-Time
• Unnamed Item
• Unnamed Item

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