Abstract / Description of output
We construct an explicit scenario whereby the same material driving inflation in the early Universe can comprise dark matter in the present Universe, using a simple quadratic potential. Following inflation and preheating, the density of inflaton/dark matter particles is reduced to the observed level by a period of thermal inflation, of a duration already invoked in the literature for other reasons. Within the context of the string landscape, one can further argue for a non-zero vacuum energy of this field, thus unifying inflation, dark matter and dark energy into a single fundamental field.
Original language | English |
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Article number | 121301(R) |
Number of pages | 5 |
Journal | Physical Review D |
Volume | 77 |
Issue number | 12 |
DOIs | |
Publication status | Published - 19 Jun 2008 |