Abstract
Starting from a simple Ansatz for the equation of state, different solutions connecting the radiation and matter eras of a perfect fluid-filled universe and a universe possessing bulk dissipative stress are derived, as is the temperature evolution. The energy conditions are also analysed. No interchange of energy between radiation and matter is allowed.
Original language | English |
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Pages (from-to) | 753-762 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 282 |
Issue number | 3 |
DOIs | |
Publication status | Published - 1 Jan 1996 |
Keywords
- Cosmology: Theory