Covariant entropy bound and loop quantum cosmology

Abhay Ashtekar, Edward Wilson-Ewing

Research output: Contribution to journalArticle

29 Citations (Scopus)

Abstract

We examine Bousso's covariant entropy bound conjecture in the context of radiation filled, spatially flat, Friedmann-Robertson-Walker models. The bound is violated near the big bang. However, the hope has been that quantum gravity effects would intervene and protect it. Loop quantum cosmology provides a near ideal setting for investigating this issue. For, on the one hand, quantum geometry effects resolve the singularity and, on the other hand, the wave function is sharply peaked at a quantum corrected but smooth geometry, which can supply the structure needed to test the bound. We find that the bound is respected. We suggest that the bound need not be an essential ingredient for a quantum gravity theory but may emerge from it under suitable circumstances.

Original languageEnglish (US)
Article number064047
JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
Volume78
Issue number6
DOIs
StatePublished - Sep 18 2008

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cosmology
entropy
gravitation
geometry
ingredients
wave functions
radiation

All Science Journal Classification (ASJC) codes

  • Nuclear and High Energy Physics
  • Physics and Astronomy (miscellaneous)

Cite this

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Covariant entropy bound and loop quantum cosmology. / Ashtekar, Abhay; Wilson-Ewing, Edward.

In: Physical Review D - Particles, Fields, Gravitation and Cosmology, Vol. 78, No. 6, 064047, 18.09.2008.

Research output: Contribution to journalArticle

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