Galaxy Clusters and Modified Gravity

Saltas, Ippocratis D.; Pizzuti, Lorenzo

doi:10.1007/978-3-030-83715-0_36

Cited by 1 publication

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“…Earlier works constraining the fifth-force coupling Y were carried out in the context of white dwarfs (Jain et al 2016;Saltas et al 2018), red and brown dwarfs (Sakstein 2015a,b;Kozak et al 2022), main-sequence stars , relativistic compact objects (Babichev et al 2016), galaxy clusters (Sakstein et al 2016;Pizzuti et al 2019Pizzuti et al , 2021Laudato et al 2022;Haridasu et al 2021), the Hulse-Taylor pulsar (Dima & Vernizzi 2018), gravitational waves (Creminelli & Vernizzi 2017;Ezquiaga & Zumalacárregui 2017;Baker et al 2017;Sakstein & Jain 2017;Creminelli et al 2018), and the Solar System (Crisostomi et al 2019) 1 . All constraints from stellar scales have thus far imposed Y < O(0.1) at 2σ.…”

Section: Introductionmentioning

confidence: 99%

Searching for dark energy with the Sun

Saltas

Christensen‐Dalsgaard

2022

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General extensions of general relativity (GR) based on bona fide degrees of freedom predict a fifth force which operates within massive objects, opening up an exciting opportunity to perform precision tests of gravity at stellar scales. Here, focussing on general scalar-tensor theories for dark energy, we utilise the Sun as our laboratory and search for imprints of the fifth-force effect on the solar equilibrium structure. With analytic results and numerical simulations, we explain how the different solar regions offer powerful ways to test gravity. Accounting for the delicate interplay between the fifth force and solar microphysics such as opacity, diffusion, equation of state, and metallicity, we demonstrate that the fifth force still leaves a sharp signature on the solar sound speed, in a region where simple estimates of input physics uncertainties become negligible. For general scalar-field extensions of GR, known as (U-)DHOST, based solely on the observational helioseismic errors, our analysis at the equilibrium level allows us to place an approximate constraint on the fifth-force coupling strength of −10 −3 Y 5 • 10 −4 at 2σ. This result improves previous stellar constraints by ∼ 3 orders of magnitude, and should be confirmed and improved by future helioseismic inversions in modified gravity, combined with an elaborate accounting of theoretical uncertainties. Our analysis can be applied to a wide set of theories beyond GR, and also paves the way for helioseismic analyses in this context. In this regard, we discuss how the solar radiative and convective zone can be employed as promising laboratories to test generic theories of gravity.

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