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Title: Swampland conjectures and late-time cosmology

Abstract

We discuss the cosmological implications of the string swampland conjectures for late-time cosmology, and test them against a wide range of state of the art cosmological observations. The refined de Sitter conjecture constrains either the minimal slope or the curvature of the scalar potential, and depends on two dimensionless constants. For constants of size one or larger, tension exists between observations, especially the Hubble constant, and the slope and curvature conjectures at a level of 4.5σ and 2.3σ, respectively. Smaller values of the constants are permitted by observations, and we determine upper bounds at varying confidence levels. We also derive and constrain the relationship between cosmological observables and the scalar field excursion during the acceleration epoch, thereby testing the distance conjecture.

Authors:
; ;
Publication Date:
Research Org.:
Univ. of Chicago, IL (United States)
Sponsoring Org.:
USDOE Office of Science (SC), High Energy Physics (HEP); National Science Foundation (NSF)
OSTI Identifier:
1507604
Alternate Identifier(s):
OSTI ID: 1593891
Grant/Contract Number:  
SC0009924; FG02-13ER41958; NNX15AK22G; PHY-1316960
Resource Type:
Published Article
Journal Name:
Physical Review. D.
Additional Journal Information:
Journal Name: Physical Review. D. Journal Volume: 99 Journal Issue: 8; Journal ID: ISSN 2470-0010
Publisher:
American Physical Society (APS)
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; Alternative gravity theories; Cosmic microwave background; Dark energy; String phenomenology

Citation Formats

Raveri, Marco, Hu, Wayne, and Sethi, Savdeep. Swampland conjectures and late-time cosmology. United States: N. p., 2019. Web. doi:10.1103/PhysRevD.99.083518.
Raveri, Marco, Hu, Wayne, & Sethi, Savdeep. Swampland conjectures and late-time cosmology. United States. https://doi.org/10.1103/PhysRevD.99.083518
Raveri, Marco, Hu, Wayne, and Sethi, Savdeep. Thu . "Swampland conjectures and late-time cosmology". United States. https://doi.org/10.1103/PhysRevD.99.083518.
@article{osti_1507604,
title = {Swampland conjectures and late-time cosmology},
author = {Raveri, Marco and Hu, Wayne and Sethi, Savdeep},
abstractNote = {We discuss the cosmological implications of the string swampland conjectures for late-time cosmology, and test them against a wide range of state of the art cosmological observations. The refined de Sitter conjecture constrains either the minimal slope or the curvature of the scalar potential, and depends on two dimensionless constants. For constants of size one or larger, tension exists between observations, especially the Hubble constant, and the slope and curvature conjectures at a level of 4.5σ and 2.3σ, respectively. Smaller values of the constants are permitted by observations, and we determine upper bounds at varying confidence levels. We also derive and constrain the relationship between cosmological observables and the scalar field excursion during the acceleration epoch, thereby testing the distance conjecture.},
doi = {10.1103/PhysRevD.99.083518},
journal = {Physical Review. D.},
number = 8,
volume = 99,
place = {United States},
year = {Thu Apr 18 00:00:00 EDT 2019},
month = {Thu Apr 18 00:00:00 EDT 2019}
}

Journal Article:
Free Publicly Available Full Text
Publisher's Version of Record
https://doi.org/10.1103/PhysRevD.99.083518

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Cited by: 45 works
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