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Title: Neutron stars in f(R) gravity with perturbative constraints

Journal Article · · Physical Review. D, Particles Fields
; ;  [1]
  1. Department of Physics, University of Arizona, Tucson, Arizona 85721 (United States)

We study the structure of neutron stars in f(R) gravity theories with perturbative constraints. We derive the modified Tolman-Oppenheimer-Volkov equations and solve them for a polytropic equation of state. We investigate the resulting modifications to the masses and radii of neutron stars and show that observations of surface phenomena alone cannot break the degeneracy between altering the theory of gravity versus choosing a different equation of state of neutron-star matter. On the other hand, observations of neutron-star cooling, which depends on the density of matter at the stellar interior, can place significant constraints on the parameters of the theory.

OSTI ID:
21421175
Journal Information:
Physical Review. D, Particles Fields, Vol. 82, Issue 6; Other Information: DOI: 10.1103/PhysRevD.82.064033; (c) 2010 American Institute of Physics; ISSN 0556-2821
Country of Publication:
United States
Language:
English