An Evaluation of Cosmological Models from the Expansion and Growth of Structure Measurements
Abstract
Here, we compare a large suite of theoretical cosmological models to observational data from the cosmic microwave background, baryon acoustic oscillation measurements of expansion, Type Ia supernova measurements of expansion, redshift space distortion measurements of the growth of structure, and the local Hubble constant. Our theoretical models include parametrizations of dark energy as well as physical models of dark energy and modified gravity. We determine the constraints on the model parameters, incorporating the redshift space distortion data directly in the analysis. To determine whether models can be ruled out, we evaluate the p-value (the probability under the model of obtaining data as bad or worse than the observed data). In our comparison, we find the well-known tension of H0 with the other data; no model resolves this tension successfully. Among the models we consider, the large-scale growth of structure data does not affect the modified gravity models as a category particularly differently from dark energy models; it matters for some modified gravity models but not others, and the same is true for dark energy models. We compute predicted observables for each model under current observational constraints, and identify models for which future observational constraints will be particularly informative.
- Authors:
-
[1];
[1];
- New York Univ. (NYU), NY (United States). Dept. of Physics and Center for Cosmology and Particle Physics
- Brookhaven National Lab. (BNL), Upton, NY (United States)
- Publication Date:
- Research Org.:
- Brookhaven National Laboratory (BNL), Upton, NY (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP); National Science Foundation (NSF)
- OSTI Identifier:
- 1433939
- Report Number(s):
- BNL-203497-2018-JAAM
Journal ID: ISSN 1538-4357; TRN: US1802810
- Grant/Contract Number:
- SC0012704; F8670; NSF-AST-1615997; NSF-AST- 1109432
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astrophysical Journal (Online)
- Additional Journal Information:
- Journal Name: The Astrophysical Journal (Online); Journal Volume: 850; Journal Issue: 2; Journal ID: ISSN 1538-4357
- Publisher:
- Institute of Physics (IOP)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; large scale structure of universe; dark energy
Citation Formats
Zhai, Zhongxu, Blanton, Michael, Slosar, Anze, and Tinker, Jeremy. An Evaluation of Cosmological Models from the Expansion and Growth of Structure Measurements. United States: N. p., 2017.
Web. doi:10.3847/1538-4357/aa9888.
Zhai, Zhongxu, Blanton, Michael, Slosar, Anze, & Tinker, Jeremy. An Evaluation of Cosmological Models from the Expansion and Growth of Structure Measurements. United States. https://doi.org/10.3847/1538-4357/aa9888
Zhai, Zhongxu, Blanton, Michael, Slosar, Anze, and Tinker, Jeremy. Fri .
"An Evaluation of Cosmological Models from the Expansion and Growth of Structure Measurements". United States. https://doi.org/10.3847/1538-4357/aa9888. https://www.osti.gov/servlets/purl/1433939.
@article{osti_1433939,
title = {An Evaluation of Cosmological Models from the Expansion and Growth of Structure Measurements},
author = {Zhai, Zhongxu and Blanton, Michael and Slosar, Anze and Tinker, Jeremy},
abstractNote = {Here, we compare a large suite of theoretical cosmological models to observational data from the cosmic microwave background, baryon acoustic oscillation measurements of expansion, Type Ia supernova measurements of expansion, redshift space distortion measurements of the growth of structure, and the local Hubble constant. Our theoretical models include parametrizations of dark energy as well as physical models of dark energy and modified gravity. We determine the constraints on the model parameters, incorporating the redshift space distortion data directly in the analysis. To determine whether models can be ruled out, we evaluate the p-value (the probability under the model of obtaining data as bad or worse than the observed data). In our comparison, we find the well-known tension of H0 with the other data; no model resolves this tension successfully. Among the models we consider, the large-scale growth of structure data does not affect the modified gravity models as a category particularly differently from dark energy models; it matters for some modified gravity models but not others, and the same is true for dark energy models. We compute predicted observables for each model under current observational constraints, and identify models for which future observational constraints will be particularly informative.},
doi = {10.3847/1538-4357/aa9888},
journal = {The Astrophysical Journal (Online)},
number = 2,
volume = 850,
place = {United States},
year = {Fri Dec 01 00:00:00 EST 2017},
month = {Fri Dec 01 00:00:00 EST 2017}
}
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