Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2009-05-18
Phys.Lett.B678:157-163,2009
Physics
High Energy Physics
High Energy Physics - Phenomenology
8 pages, 2 figures
Scientific paper
10.1016/j.physletb.2009.06.025
A model is presented in which a single scalar field is responsible for both primordial inflation at early times and then dark energy at late times. This field is coupled to a second scalar field which becomes unstable and starts to oscillate after primordial inflation, thus driving a reheating phase that can create a high post-inflation temperature. This model easily avoids overproduction of gravity waves, which is a problem in the original quintessential inflation model in which reheating occurs via gravitational particle production.
Bastero-Gil Mar
Berera Arjun
Jackson Brendan M.
Taylor Andy
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