Modified gravity inside astrophysical bodies

Ryo Saito, Daisuke Yamauchi, Shuntaro Mizuno, Jérôme Gleyzes, David Langlois

研究成果: Article査読

68 被引用数 (Scopus)

抄録

Many theories of modified gravity, including the well studied Horndeski models, are characterized by a screening mechanism that ensures that standard gravity is recovered near astrophysical bodies. In a recently introduced class of gravitational theories that goes beyond Horndeski, it has been found that new derivative interactions lead to a partial breaking of the Vainshtein screening mechanism inside any gravitational source, although not outside. We study the impact of this new type of deviation from standard gravity on the density profile of a spherically symmetric matter distribution, in the nonrelativistic limit. For simplicity, we consider a polytropic equation of state and derive the modifications to the standard Lane-Emden equations. We also show the existence of a universal upper bound on the amplitude of this type of modified gravity, independently of the details of the equation of state.

本文言語English
論文番号008
ジャーナルJournal of Cosmology and Astroparticle Physics
2015
6
DOI
出版ステータスPublished - 2015 6 1

ASJC Scopus subject areas

  • 天文学と天体物理学

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