Hiding neutrino mass in modified gravity cosmologies

Cosmological observables show a dependence with the neutrino mass, which is partially degenerate with parameters of extended models of gravity. We study and explore this degeneracy in Horndeski generalized scalar-tensor theories of gravity. Using forecasted cosmic microwave background and galaxy pow...

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Main Authors: Bellomo, N, Bellini, E, Hu, B, Jimenez, R, Pena-Garay, C, Verde, L
Format: Journal article
Published: Institute of Physics 2017
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author Bellomo, N
Bellini, E
Hu, B
Jimenez, R
Pena-Garay, C
Verde, L
author_facet Bellomo, N
Bellini, E
Hu, B
Jimenez, R
Pena-Garay, C
Verde, L
author_sort Bellomo, N
collection OXFORD
description Cosmological observables show a dependence with the neutrino mass, which is partially degenerate with parameters of extended models of gravity. We study and explore this degeneracy in Horndeski generalized scalar-tensor theories of gravity. Using forecasted cosmic microwave background and galaxy power spectrum datasets, we find that a single parameter in the linear regime of the effective theory dominates the correlation with the total neutrino mass. For any given mass, a particular value of this parameter approximately cancels the power suppression due to the neutrino mass at a given redshift. The extent of the cancellation of this degeneracy depends on the cosmological large-scale structure data used at different redshifts. We constrain the parameters and functions of the effective gravity theory and determine the influence of gravity on the determination of the neutrino mass from present and future surveys.
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spelling oxford-uuid:1676aad5-88c9-48d2-bac4-18769aa111862022-03-26T10:31:32ZHiding neutrino mass in modified gravity cosmologiesJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:1676aad5-88c9-48d2-bac4-18769aa11186Symplectic Elements at OxfordInstitute of Physics2017Bellomo, NBellini, EHu, BJimenez, RPena-Garay, CVerde, LCosmological observables show a dependence with the neutrino mass, which is partially degenerate with parameters of extended models of gravity. We study and explore this degeneracy in Horndeski generalized scalar-tensor theories of gravity. Using forecasted cosmic microwave background and galaxy power spectrum datasets, we find that a single parameter in the linear regime of the effective theory dominates the correlation with the total neutrino mass. For any given mass, a particular value of this parameter approximately cancels the power suppression due to the neutrino mass at a given redshift. The extent of the cancellation of this degeneracy depends on the cosmological large-scale structure data used at different redshifts. We constrain the parameters and functions of the effective gravity theory and determine the influence of gravity on the determination of the neutrino mass from present and future surveys.
spellingShingle Bellomo, N
Bellini, E
Hu, B
Jimenez, R
Pena-Garay, C
Verde, L
Hiding neutrino mass in modified gravity cosmologies
title Hiding neutrino mass in modified gravity cosmologies
title_full Hiding neutrino mass in modified gravity cosmologies
title_fullStr Hiding neutrino mass in modified gravity cosmologies
title_full_unstemmed Hiding neutrino mass in modified gravity cosmologies
title_short Hiding neutrino mass in modified gravity cosmologies
title_sort hiding neutrino mass in modified gravity cosmologies
work_keys_str_mv AT bellomon hidingneutrinomassinmodifiedgravitycosmologies
AT bellinie hidingneutrinomassinmodifiedgravitycosmologies
AT hub hidingneutrinomassinmodifiedgravitycosmologies
AT jimenezr hidingneutrinomassinmodifiedgravitycosmologies
AT penagarayc hidingneutrinomassinmodifiedgravitycosmologies
AT verdel hidingneutrinomassinmodifiedgravitycosmologies