Cited by 483Cosmology and Gravitation TheoriesBlack Holes and Theoretical PhysicsNoncommutative and Quantum Gravity Theories

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Probable Values of the Cosmological Constant in a Holographic Theory

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Hořava, Petr, Minic, Djordje·2000·Physical Review Letters

Abstract

We point out that for a large class of universes, holography implies that the most probable value for the cosmological constant is zero. In four space-time dimensions, the probability distribution takes the Baum-Hawking form, $\mathrm{dP}\ensuremath{\sim}\mathrm{exp}({\mathrm{cM}}_{p}^{2}/\ensuremath{\Lambda})d\ensuremath{\Lambda}$.

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Research works printed but not linked: 22

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Metadata

Authors
Hořava, P., & Minic, D.
Affiliations
University of Southern California (US)
Venue
Physical Review Letters
Published
2000-08-21
Volume
85
Issue
8
Pages
1610-1613
ISSN
  • 0031-9007 (ISSN-L)
  • 1079-7114
OpenAlex
W2164044686
Cited by
483
References
3
Citations by year
2026: 16 · 2025: 20 · 2024: 30 · 2023: 26 · 2022: 31 · 2021: 31 · 2020: 25 · 2019: 28 · 2018: 15 · 2017: 9 · 2016: 17 · 2015: 15 · 2014: 20 · 2013: 25 · 2012: 18
FWCI
4.70
Type
journal article
Language
en
Open access
Locations
  • Physical Review Letters (publishedVersion)
  • PubMed (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • CaltechAUTHORS (California Institute of Technology) (submittedVersion)
  • CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
  • arXiv (Cornell University)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
  • Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Black Holes and Theoretical Physics
  • Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Noncommutative and Quantum Gravity Theories
Keywords
cosmological constant, holography, probability distributions, vacuum energy, four-dimensional spacetime, Bekenstein-Hawking entropy, string theory, vacuum selection

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