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Title: How many e -folds should we expect from high-scale inflation?

Journal Article · · Physical Review. D, Particles, Fields, Gravitation and Cosmology
 [1];  [1]
  1. California Inst. of Technology (CalTech), Pasadena, CA (United States). Walter Burke Inst. for Theoretical Physics

In this study, we address the issue of how many e -folds we would naturally expect if inflation occurred at an energy scale of order 10 16 GeV . We use the canonical measure on trajectories in classical phase space, specialized to the case of flat universes with a single scalar field. While there is no exact analytic expression for the measure, we are able to derive conditions that determine its behavior. For a quadratic potential V ( Φ ) = m 2 Φ 2 / 2 with m = 2 × 10 13 GeV and cutoff at M Pl = 2.4 × 10 18 GeV , we find an expectation value of 2 × 10 10 e -folds on the set of Friedmann-Robertson-Walker trajectories. For cosine inflation V ( Φ ) = Λ 4 [ 1 - cos ( Φ / f ) ] with f = 1.5 × 10 19 GeV , we find that the expected total number of e -folds is 50, which would just satisfy the observed requirements of our own Universe; if f is larger, more than 50 e -folds are generically attained. Finally, we conclude that one should expect a large amount of inflation in large-field models and more limited inflation in small-field (hilltop) scenarios.

Research Organization:
California Institute of Technology (CalTech), Pasadena, CA (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP); National Science Foundation (NSF); Betty Moore Foundation
Grant/Contract Number:
SC0011632; DGE-1144469; 776
OSTI ID:
1596472
Alternate ID(s):
OSTI ID: 1180062
Journal Information:
Physical Review. D, Particles, Fields, Gravitation and Cosmology, Vol. 90, Issue 6; ISSN 1550-7998
Publisher:
American Physical Society (APS)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 37 works
Citation information provided by
Web of Science

References (14)

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Detection of B -Mode Polarization at Degree Angular Scales by BICEP2 journal June 2014
A natural measure on the set of all universes journal February 1987
Natural inflation: Particle physics models, power-law spectra for large-scale structure, and constraints from the Cosmic Background Explorer journal January 1993
Ultraviolet-Protected Inflation journal April 2011
Natural inflation with pseudo Nambu-Goldstone bosons journal December 1990
Difficulties with Inflationary Cosmology journal December 1989
Measure problem in cosmology journal March 2008
Chaotic inflation journal March 1988

Cited By (13)

Global dynamics and inflationary center manifold and slow-roll approximants journal January 2015
Misalignment & Co.: (pseudo-)scalar and vector dark matter with curvature couplings journal February 2020
Case for kinetically dominated initial conditions for inflation journal July 2019
Initial conditions for inflation — A short review journal January 2017
Constraining the kinetically dominated universe journal July 2019
Robustness of inflation to inhomogeneous initial conditions journal September 2017
Robustness of inflation to large tensor perturbations journal May 2018
Global dynamics and asymptotics for monomial scalar field potentials and perfect fluids journal June 2015
Global dynamics and inflationary center manifold and slow-roll approximants text January 2014
Global dynamics and asymptotics for monomial scalar field potentials and perfect fluids preprint January 2015
Robustness of Inflation to Large Tensor Perturbations text January 2017
A case for kinetically dominated initial conditions for inflation text January 2018
TeV scale leptogenesis, inflaton dark matter and neutrino mass in a scotogenic model text January 2018

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