Dark Energy and the BOOMERANG Data
- 8 January 2001
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review Letters
- Vol. 86 (2) , 196-199
- https://doi.org/10.1103/physrevlett.86.196
Abstract
The recent high-quality BOOMERANG data allow the testing of many competing cosmological models. Here I present a seven-parameter likelihood analysis of dark energy models with exponential potential and explicit coupling to dark matter. The BOOMERANG data constrain the dimensionless coupling to be smaller than 0.1, an order of magnitude better than previous limits. In terms of the constant of nonminimally coupled theories, this amounts to On the other hand, BOOMERANG does not have enough sensitivity to put constraints on the potential slope.
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This publication has 28 references indexed in Scilit:
- Dark Energy and the Cosmic Microwave Background RadiationPhysical Review Letters, 2000
- A flat Universe from high-resolution maps of the cosmic microwave background radiationNature, 2000
- Interactions in scalar field cosmologyPhysical Review D, 2000
- Cosmic Concordance and QuintessenceThe Astrophysical Journal, 2000
- Self-similar cosmological solutions with a nonminimally coupled scalar fieldPhysical Review D, 2000
- Measurements of Ω and Λ from 42 High‐Redshift SupernovaeThe Astrophysical Journal, 1999
- Quintessence and the Rest of the World: Suppressing Long-Range InteractionsPhysical Review Letters, 1998
- Cosmological Imprint of an Energy Component with General Equation of StatePhysical Review Letters, 1998
- Cosmology with Ultralight Pseudo Nambu-Goldstone BosonsPhysical Review Letters, 1995
- Exponential Potentials, Scaling Solutions and InflationAnnals of the New York Academy of Sciences, 1993