Abstract
We examine the possibility that a significant component of the energy density of the Universe has an equation of state different from that of matter, radiation, or cosmological constant (Λ). An example is a cosmic scalar field evolving in a potential, but our treatment is more general. Including this component alters cosmic evolution in a way that fits current observations well. Unlike Λ, it evolves dynamically and develops fluctuations, leaving a distinctive imprint on the microwave background anisotropy and mass power spectrum.
Original language | English (US) |
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Pages (from-to) | 1582-1585 |
Number of pages | 4 |
Journal | Physical review letters |
Volume | 80 |
Issue number | 8 |
DOIs | |
State | Published - Feb 23 1998 |
Externally published | Yes |
All Science Journal Classification (ASJC) codes
- General Physics and Astronomy