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Title: Inflation in a scale-invariant universe

Journal Article · · Physical Review D

A scale-invariant universe can have a period of accelerated expansion at early times: inflation. We use a frame-invariant approach to calculate inflationary observables in a scale-invariant theory of gravity involving two scalar fields: the spectral indices, the tensor-to-scalar ratio, the level of isocurvature modes, and non-Gaussianity. We show that scale symmetry leads to an exact cancellation of isocurvature modes and that, in the scale symmetry–broken phase, this theory is well described by a single scalar-field theory. Lastly, ee find the predictions of this theory strongly compatible with current observations.

Research Organization:
Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP)
Grant/Contract Number:
AC02-07CH11359
OSTI ID:
1437397
Alternate ID(s):
OSTI ID: 1454351
Report Number(s):
FERMILAB-PUB-18-079-T; arXiv:1802.06069; PRVDAQ; 1655609; TRN: US1900321
Journal Information:
Physical Review D, Vol. 97, Issue 12; ISSN 2470-0010
Publisher:
American Physical Society (APS)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 31 works
Citation information provided by
Web of Science

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Cited By (7)

Palatini inflation in models with an R 2 term journal November 2018
Inflation as a spontaneous symmetry breaking of Weyl symmetry journal January 2019
Nonminimal Coleman-Weinberg inflation with an R 2 term journal February 2019
Scale-independent R 2 inflation journal December 2019
Spectral Noncommutative Geometry Standard Model and all that journal July 2019
Nonminimal Coleman--Weinberg Inflation with an $R^2$ term text January 2018
Spectral Noncommutative Geometry, Standard Model and all that text January 2019

Figures / Tables (2)


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