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Title: Slinky inflation

Journal Article · · Physics Letters, (Section) B
OSTI ID:15017240

We present a new approach to quintessential inflation, in which both dark energy and inflation are explained by the evolution of a single scalar field. We start from a simple scalar potential with both oscillatory and exponential behavior.We employ the conventional reheating mechanism of new inflation, in which the scalar decays to light fermions with a decay width that is proportional to the scalar mass. Because our scalar mass is proportional to the Hubble rate, this gives adequate reheating at early times while shutting off at late times to preserve quintessence and satisfy nucleosynthesis constraints. We discuss a simple model which solves the horizon, flatness, and ''why now'' problems. Without any additional tuning of parameters, this model satisfies all constraints from CMB, large scale structure, and nucleosynthesis. The predictions for the inflationary spectral indices are n{sub S} = n{sub T} = 1. In this model we are currently beginning the third cosmic epoch of accelerated expansion.

Research Organization:
Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
Sponsoring Organization:
USDOE
DOE Contract Number:
AC02-76CH03000
OSTI ID:
15017240
Report Number(s):
FERMILAB-PUB-05-039-T; PYLBAJ; arXiv eprint number astro-ph/0504090; TRN: US0602539
Journal Information:
Physics Letters, (Section) B, Vol. 633; ISSN 0370-2693
Country of Publication:
United States
Language:
English

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