| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1770951 | Astroparticle Physics | 2012 | 7 Pages |
Abstract
⺠Inflation and Dark Matter takes place via a single scalar field. ⺠We have only 4 free parameters, 2 in V (lambda and m) and 2 couplings. ⺠Same parameters are present in models of inflation reheating without DM. ⺠Parameters g,m are in models of WIMP DM without inflation or reheating. ⺠We do not increase the number of parameters and have unification for free.
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Authors
A. de la Macorra,