Abstract
We find a simple inflationary solution in an inhomogeneous spacetime with heat flux. The heat flux obeys a causal transport equation, and counteracts the inflationary decrease of energy density. At late times, the heat flux tends to zero and thefluid approaches the equation of state p =–ρ.
Original language | English |
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Pages (from-to) | 815-819 |
Journal | General Relativity and Gravitation |
Volume | 31 |
Issue number | 6 |
DOIs | |
Publication status | Published - Jun 1999 |
Keywords
- cosmology
- inflation
- nonequilibrium thermodynamics