4.7 Article

Hybrid quintessential inflation

期刊

PHYSICS LETTERS B
卷 678, 期 2, 页码 157-163

出版社

ELSEVIER
DOI: 10.1016/j.physletb.2009.06.025

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资金

  1. M.E.C. [FIS2007-63364]
  2. Junta de Andalucia [101]
  3. STFC
  4. Science and Technology Facilities Council [ST/G000522/1] Funding Source: researchfish
  5. STFC [ST/G000522/1] Funding Source: UKRI

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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. (C) 2009 Elsevier B.V. All rights reserved.

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