Local resolution of the Hubble tension: The impact of screened fifth forces on the cosmic distance ladder
Abstract
The discrepancy between the values of the Hubble constant H0 derived from the local distance ladder and the cosmic microwave background provides a tantalizing hint of new physics. We explore a potential resolution involving screened fifth forces in the local Universe, which alter the Cepheid calibration of supernova distances. In particular, if the Cepheids with direct distance measurements from parallax or water masers are screened but a significant fraction of those in other galaxies are not, neglecting the difference between their underlying period–luminosity relations biases the local H0 measurement high. This difference derives from a reduction in the Cepheid pulsation period and possible increase in luminosity under a fifth force. We quantify the internal and environmental gravitational properties of the Riess et al. distance ladder galaxies to assess their degrees of screening under a range of phenomenological models, and propagate this information into the H0 posterior as a function of fifth force strength. We consider well-studied screening models in scalar–tensor gravity theories such as chameleon, K-mouflage and Vainshtein, along with a recently-proposed mechanism based on baryon–dark matter interactions in which screening is governed by the local dark matter density. We find that a fifth force strength ~5%–30% that of gravitymore »
- Authors:
-
[1];
[2]
- Univ. of Oxford (United Kingdom)
- Univ. of Pennsylvania, Philadelphia, PA (United States)
- Publication Date:
- Research Org.:
- Univ. of Pennsylvania, Philadelphia, PA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC)
- OSTI Identifier:
- 1610996
- Alternate Identifier(s):
- OSTI ID: 1559085
- Grant/Contract Number:
- SC0007901
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physical Review. D.
- Additional Journal Information:
- Journal Volume: 100; Journal Issue: 4; Journal ID: ISSN 2470-0010
- Publisher:
- American Physical Society (APS)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; Astronomy & Astrophysics; Physics; Alternative gravity theories; Astrophysical studies of gravity; Cosmological parameters; Cosmology; Dark energy; Hydrostatic stellar nucleosynthesis; Novae & supernovae
Citation Formats
Desmond, Harry, Jain, Bhuvnesh, and Sakstein, Jeremy. Local resolution of the Hubble tension: The impact of screened fifth forces on the cosmic distance ladder. United States: N. p., 2019.
Web. doi:10.1103/physrevd.100.043537.
Desmond, Harry, Jain, Bhuvnesh, & Sakstein, Jeremy. Local resolution of the Hubble tension: The impact of screened fifth forces on the cosmic distance ladder. United States. https://doi.org/10.1103/physrevd.100.043537
Desmond, Harry, Jain, Bhuvnesh, and Sakstein, Jeremy. Wed .
"Local resolution of the Hubble tension: The impact of screened fifth forces on the cosmic distance ladder". United States. https://doi.org/10.1103/physrevd.100.043537. https://www.osti.gov/servlets/purl/1610996.
@article{osti_1610996,
title = {Local resolution of the Hubble tension: The impact of screened fifth forces on the cosmic distance ladder},
author = {Desmond, Harry and Jain, Bhuvnesh and Sakstein, Jeremy},
abstractNote = {The discrepancy between the values of the Hubble constant H0 derived from the local distance ladder and the cosmic microwave background provides a tantalizing hint of new physics. We explore a potential resolution involving screened fifth forces in the local Universe, which alter the Cepheid calibration of supernova distances. In particular, if the Cepheids with direct distance measurements from parallax or water masers are screened but a significant fraction of those in other galaxies are not, neglecting the difference between their underlying period–luminosity relations biases the local H0 measurement high. This difference derives from a reduction in the Cepheid pulsation period and possible increase in luminosity under a fifth force. We quantify the internal and environmental gravitational properties of the Riess et al. distance ladder galaxies to assess their degrees of screening under a range of phenomenological models, and propagate this information into the H0 posterior as a function of fifth force strength. We consider well-studied screening models in scalar–tensor gravity theories such as chameleon, K-mouflage and Vainshtein, along with a recently-proposed mechanism based on baryon–dark matter interactions in which screening is governed by the local dark matter density. We find that a fifth force strength ~5%–30% that of gravity can alleviate the H0 tension in many scenarios, around the sensitivity level at which tests based on other distance ladder data can constrain this strength. Here, our most successful models achieve consistency with Planck at the ~1.5σ level. Although our analysis is exploratory and based on screening models that are not necessarily realized in full theories, our results demonstrate that new physics-based local resolutions of the H0 tension are possible, supplementing those already known in the prerecombination era.},
doi = {10.1103/physrevd.100.043537},
journal = {Physical Review. D.},
number = 4,
volume = 100,
place = {United States},
year = {Wed Aug 28 00:00:00 EDT 2019},
month = {Wed Aug 28 00:00:00 EDT 2019}
}
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