Cited by 218Cosmology and Gravitation TheoriesGalaxies: Formation, Evolution, PhenomenaStellar, planetary, and galactic studies

Energy Conditions in the Epoch of Galaxy Formation

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Visser, Matt·1997·Science

Abstract

The energy conditions of Einsteinian gravity (classical general relativity) do not require one to fix a specific equation of state. In a Friedmann-Robertson-Walker universe where the equation of state for the cosmological fluid is uncertain, the energy conditions provide simple, model-independent, and robust bounds on the behavior of the density and look-back time as a function of red shift. Current observations suggest that the “strong energy condition” was violated sometime between the epoch of galaxy formation and the present. This implies that no possible combination of “normal” matter is capable of fitting the observational data.

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References 17 · Cited by 218

Authors
Visser, M.
Affiliations
Washington University in St. Louis (US)
Corresponding author
Visser, Matt
Venue
Science
Published
1997-04-04
Volume
276
Issue
5309
Pages
88-90
ISSN
  • 0036-8075 (ISSN-L)
  • 1095-9203
OpenAlex
W2037195717
Cited by
218
References
17
Citations by year
2026: 15 · 2025: 16 · 2024: 21 · 2023: 17 · 2022: 21 · 2021: 20 · 2020: 15 · 2019: 5 · 2018: 9 · 2017: 11 · 2016: 8 · 2015: 2 · 2014: 2 · 2013: 5 · 2012: 6
FWCI
2.61
Type
journal article
Language
en
Open access
Locations
  • Science (publishedVersion)
  • PubMed (publishedVersion)
  • arXiv (Cornell University) (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 › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
Keywords
energy conditions, strong energy condition, galaxy formation, FRW universe, equation of state, cosmic fluid, lookback time, density evolution

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