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Title: Gravitational waves and the scale of inflation

Journal Article · · Physical Review. D, Particles, Fields, Gravitation and Cosmology
 [1];  [2];  [2];  [1]
  1. Institute for Advanced Study, Princeton, NJ (United States)
  2. Stanford Univ., Stanford, CA (United States)

Here, we revisit alternative mechanisms of gravitational wave production during inflation and argue that they generically emit a non-negligible amount of scalar fluctuations. We find the scalar power is larger than the tensor power by a factor of order 1/ε2. For an appreciable tensor contribution, the associated scalar emission completely dominates the zero-point fluctuations of the inflaton, resulting in a tensor-to-scalar ratio r ~ ε2. A more quantitative result can be obtained if one further assumes that gravitational waves are emitted by localized subhorizon processes, giving rmax ≃ 0.3ε2. However, ε is generally time dependent, and this result for r depends on its instantaneous value during the production of the sources, rather than just its average value, somewhat relaxing constraints from the tilt ns. We calculate the scalar 3-point correlation function in the same class of models and show that non-Gaussianity cannot be made arbitrarily small, i.e. fNL ≳ 1, independently of the value of r. Possible exceptions in multifield scenarios are discussed.

Research Organization:
Stanford Univ., CA (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP)
Grant/Contract Number:
SC0008078; FG02-12ER41854
OSTI ID:
1491084
Alternate ID(s):
OSTI ID: 1180012
Journal Information:
Physical Review. D, Particles, Fields, Gravitation and Cosmology, Vol. 91, Issue 6; ISSN 1550-7998
Publisher:
American Physical Society (APS)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 46 works
Citation information provided by
Web of Science

References (39)

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New Sources of Gravitational Waves during Inflation text January 2011
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Gravity waves and non-Gaussian features from particle production in a sector gravitationally coupled to the inflaton text January 2012
Gauge Fields and Inflation: Chiral Gravitational Waves, Fluctuations and the Lyth Bound text January 2013
Inflation Physics from the Cosmic Microwave Background and Large Scale Structure text January 2013
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Statistics of Cosmic Microwave Background Polarization text January 1996

Cited By (7)

A model with cosmological Bell inequalities: A model with cosmological Bell inequalities journal December 2015
On the validity of the perturbative description of axions during inflation journal April 2016
Gravitational waves at interferometer scales and primordial black holes in axion inflation journal December 2016
Exploring cosmic origins with CORE: Inflation journal April 2018
Erratum: On the validity of the perturbative description of axions during inflation journal October 2016
On the validity of the perturbative description of axions during inflation text January 2015
Gravitational waves at interferometer scales and primordial black holes in axion inflation text January 2016

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