Unified Model for Inflation and Dark Energy with Planck-Scale Pseudo-Goldstone Bosons
arXiv:astro-ph/0602166 · doi:10.1088/1475-7516/2006/02/012
Abstract
We present a model with a complex and a real scalar fields and a potential whose symmetry is explicitly broken by Planck-scale physics. For exponentially small breaking, the model accounts for the period of inflation in the early universe and for the period of acceleration of the late universe.
arXiv comment15 pages, 4 figures, RevTeX4; some references added
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Cited by in corpus (9)
- Cosmic microwave background and large-scale structure constraints on a simple quintessential inflation model
- Neutrino Condensate as Origin of Dark Energy
- Low-scale inflation in a model of dark energy and dark matter
- Majorana Neutrino Superfluidity and Stability of Neutrino Dark Energy
- Neutrino Phenomenology, Dark Energy and Leptogenesis from pseudo-Nambu-Goldstone Bosons
- Radiative Inflation and Dark Energy RIDEs Again after BICEP2
- Radiative Inflation and Dark Energy
- Unified Model for Inflation and Dark Matter
- Unified Model for Inflation and the Dark Side of the Universe