The cosmological constant is back
1995; Springer Science+Business Media; Volume: 27; Issue: 11 Linguagem: Inglês
10.1007/bf02108229
ISSN1572-9532
AutoresLawrence M. Krauss, Michael S. Turner,
Tópico(s)Relativity and Gravitational Theory
ResumoA diverse set of observations now compellingly suggest that Universe possesses a nonzero cosmological constant. In the context of quantum-field theory a cosmological constant corresponds to the energy density of the vacuum, and the wanted value for the cosmological constant corresponds to a very tiny vacuum energy density. We discuss future observational tests for a cosmological constant as well as the fundamental theoretical challenges---and opportunities---that this poses for particle physics and for extending our understanding of the evolution of the Universe back to the earliest moments.
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