DOE PAGES title logo U.S. Department of Energy
Office of Scientific and Technical Information

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

Abstract

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.

Authors:
 [1];  [1]
  1. California Inst. of Technology (CalTech), Pasadena, CA (United States). Walter Burke Inst. for Theoretical Physics
Publication Date:
Research Org.:
California Institute of Technology (CalTech), Pasadena, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC), High Energy Physics (HEP); National Science Foundation (NSF); Betty Moore Foundation
OSTI Identifier:
1596472
Alternate Identifier(s):
OSTI ID: 1180062
Grant/Contract Number:  
SC0011632; DGE-1144469; 776
Resource Type:
Accepted Manuscript
Journal Name:
Physical Review. D, Particles, Fields, Gravitation and Cosmology
Additional Journal Information:
Journal Volume: 90; Journal Issue: 6; Journal ID: ISSN 1550-7998
Publisher:
American Physical Society (APS)
Country of Publication:
United States
Language:
English
Subject:
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS

Citation Formats

Remmen, Grant N., and Carroll, Sean M. How many e-folds should we expect from high-scale inflation?. United States: N. p., 2014. Web. doi:10.1103/PhysRevD.90.063517.
Remmen, Grant N., & Carroll, Sean M. How many e-folds should we expect from high-scale inflation?. United States. https://doi.org/10.1103/PhysRevD.90.063517
Remmen, Grant N., and Carroll, Sean M. Mon . "How many e-folds should we expect from high-scale inflation?". United States. https://doi.org/10.1103/PhysRevD.90.063517. https://www.osti.gov/servlets/purl/1596472.
@article{osti_1596472,
title = {How many e-folds should we expect from high-scale inflation?},
author = {Remmen, Grant N. and Carroll, Sean M.},
abstractNote = {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 1016 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)=m2Φ2/2 with m=2×1013 GeV and cutoff at MPl=2.4×1018 GeV, we find an expectation value of 2×1010 e-folds on the set of Friedmann-Robertson-Walker trajectories. For cosine inflation V(Φ)=Λ4[1-cos(Φ/f)] with f=1.5×1019 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.},
doi = {10.1103/PhysRevD.90.063517},
journal = {Physical Review. D, Particles, Fields, Gravitation and Cosmology},
number = 6,
volume = 90,
place = {United States},
year = {Mon Sep 22 00:00:00 EDT 2014},
month = {Mon Sep 22 00:00:00 EDT 2014}
}

Journal Article:

Citation Metrics:
Cited by: 37 works
Citation information provided by
Web of Science

Save / Share:

Works referenced in this record:

Natural Chaotic Inflation in Supergravity
journal, October 2000


Attractor solutions in scalar-field cosmology
journal, October 2013


Natural inflation in supergravity and beyond
journal, August 2014


Rescuing quadratic inflation
journal, February 2014

  • Ellis, John; Fairbairn, Malcolm; Sueiro, Maria
  • Journal of Cosmology and Astroparticle Physics, Vol. 2014, Issue 02
  • DOI: 10.1088/1475-7516/2014/02/044

Extranatural Inflation
journal, June 2003


Recent progress in the inflationary universe scenario
journal, January 1985


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

  • Adams, Fred C.; Bond, J. Richard; Freese, Katherine
  • Physical Review D, Vol. 47, Issue 2
  • DOI: 10.1103/PhysRevD.47.426

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


Works referencing / citing this record:

Global dynamics and inflationary center manifold and slow-roll approximants
journal, January 2015

  • Alho, Artur; Uggla, Claes
  • Journal of Mathematical Physics, Vol. 56, Issue 1
  • DOI: 10.1063/1.4906081

Misalignment & Co.: (pseudo-)scalar and vector dark matter with curvature couplings
journal, February 2020

  • Alonso-Álvarez, Gonzalo; Hugle, Thomas; Jaeckel, Joerg
  • Journal of Cosmology and Astroparticle Physics, Vol. 2020, Issue 02
  • DOI: 10.1088/1475-7516/2020/02/014

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

  • Clough, Katy; Lim, Eugene A.; DiNunno, Brandon S.
  • Journal of Cosmology and Astroparticle Physics, Vol. 2017, Issue 09
  • DOI: 10.1088/1475-7516/2017/09/025

Robustness of inflation to large tensor perturbations
journal, May 2018

  • Clough, Katy; Flauger, Raphael; Lim, Eugene A.
  • Journal of Cosmology and Astroparticle Physics, Vol. 2018, Issue 05
  • DOI: 10.1088/1475-7516/2018/05/065

Global dynamics and asymptotics for monomial scalar field potentials and perfect fluids
journal, June 2015


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