Screened fifth forces mediated by dark matter-baryon interactions: Theory and astrophysical probes

We derive the details of a new screening mechanism where the interactions of baryons and dark matter can be screened according to the local dark matter density. In this mechanism, the value of Newton’s constant is dark matter-density dependent, allowing for the possibility that astrophysical phenome...

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Main Authors: Sakstein, J, Desmond, H, Jain, B
Format: Journal article
Language:English
Published: American Physical Society 2019
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author Sakstein, J
Desmond, H
Jain, B
author_facet Sakstein, J
Desmond, H
Jain, B
author_sort Sakstein, J
collection OXFORD
description We derive the details of a new screening mechanism where the interactions of baryons and dark matter can be screened according to the local dark matter density. In this mechanism, the value of Newton’s constant is dark matter-density dependent, allowing for the possibility that astrophysical phenomena are very different in galaxies less dense than the Milky Way. The parametrized post-Newtonian parameter γ , which quantifies the difference between kinematical and lensing probes, also depends on dark matter density. We calculate the effects of varying G on various stages of stellar evolution, focusing on observables that impact cosmology: the Cepheid period-luminosity relation and the supernova Ia magnitude-redshift relation. Other potential tests of the model are also investigated including main-sequence, post-main-sequence, and low-mass dwarf stars. Finally, we discuss how extragalactic tests of γ could provide complementary constraints.
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spelling oxford-uuid:2aad0ad9-c55d-4ac5-8c57-44257650e64f2022-03-26T12:26:29ZScreened fifth forces mediated by dark matter-baryon interactions: Theory and astrophysical probesJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:2aad0ad9-c55d-4ac5-8c57-44257650e64fEnglishSymplectic ElementsAmerican Physical Society2019Sakstein, JDesmond, HJain, BWe derive the details of a new screening mechanism where the interactions of baryons and dark matter can be screened according to the local dark matter density. In this mechanism, the value of Newton’s constant is dark matter-density dependent, allowing for the possibility that astrophysical phenomena are very different in galaxies less dense than the Milky Way. The parametrized post-Newtonian parameter γ , which quantifies the difference between kinematical and lensing probes, also depends on dark matter density. We calculate the effects of varying G on various stages of stellar evolution, focusing on observables that impact cosmology: the Cepheid period-luminosity relation and the supernova Ia magnitude-redshift relation. Other potential tests of the model are also investigated including main-sequence, post-main-sequence, and low-mass dwarf stars. Finally, we discuss how extragalactic tests of γ could provide complementary constraints.
spellingShingle Sakstein, J
Desmond, H
Jain, B
Screened fifth forces mediated by dark matter-baryon interactions: Theory and astrophysical probes
title Screened fifth forces mediated by dark matter-baryon interactions: Theory and astrophysical probes
title_full Screened fifth forces mediated by dark matter-baryon interactions: Theory and astrophysical probes
title_fullStr Screened fifth forces mediated by dark matter-baryon interactions: Theory and astrophysical probes
title_full_unstemmed Screened fifth forces mediated by dark matter-baryon interactions: Theory and astrophysical probes
title_short Screened fifth forces mediated by dark matter-baryon interactions: Theory and astrophysical probes
title_sort screened fifth forces mediated by dark matter baryon interactions theory and astrophysical probes
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AT desmondh screenedfifthforcesmediatedbydarkmatterbaryoninteractionstheoryandastrophysicalprobes
AT jainb screenedfifthforcesmediatedbydarkmatterbaryoninteractionstheoryandastrophysicalprobes