Constraints on Modified Gravity Models from White Dwarfs
arXiv:1705.01048 · doi:10.1088/1475-7516/2017/10/004
Abstract
Modified gravity theories can introduce modifications to the Poisson equation in the Newtonian limit. As a result, we expect to see interesting features of these modifications inside stellar objects. White dwarf stars are one of the most well studied stars in stellar astrophysics. We explore the effect of modified gravity theories inside white dwarfs. We derive the modified stellar structure equations and solve them to study the mass-radius relationships for various modified gravity theories. We also constrain the parameter space of these theories from observations.
27 pages, 22 figures, 1 Table; Matches the version published in JCAP
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