Observation of cosmic acceleration and determining the fate of the universe

Glenn Starkman, Mark Trodden, Tanmay Vachaspati

Research output: Contribution to journalArticle

26 Citations (Scopus)

Abstract

Current observations of type-la supernovae provide evidence for cosmic acceleration out to a redshift of z ≲ 1, leading to the possibility that the universe is entering an inflationary epoch. However, inflation can take place only if vacuum energy (or other sufficiently slowly redshifting source of energy density) dominates the energy density of a region of physical radius 1/H. We argue that, for the best-fit values of ΩΛ = 0.8 and Ωm = 0.2 inferred from the supernovae data, one must confirm cosmic acceleration out to at least z ≃ 1.8 to infer that our portion of the universe is inflating. If ΩΛ < 0.736 then no present-day measurement can confirm or falsify that inference.

Original languageEnglish (US)
Pages (from-to)1510-1513
Number of pages4
JournalPhysical Review Letters
Volume83
Issue number8
StatePublished - Aug 23 1999
Externally publishedYes

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supernovae
flux density
universe
inflating
inference
time measurement
vacuum
radii
energy

ASJC Scopus subject areas

  • Physics and Astronomy(all)

Cite this

Observation of cosmic acceleration and determining the fate of the universe. / Starkman, Glenn; Trodden, Mark; Vachaspati, Tanmay.

In: Physical Review Letters, Vol. 83, No. 8, 23.08.1999, p. 1510-1513.

Research output: Contribution to journalArticle

Starkman, Glenn ; Trodden, Mark ; Vachaspati, Tanmay. / Observation of cosmic acceleration and determining the fate of the universe. In: Physical Review Letters. 1999 ; Vol. 83, No. 8. pp. 1510-1513.
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