PT Journal
AU Maso-Ferrando, A
   Sanchis-Gual, N
   Font, JA
   Olmo, GJ
TI Boson stars in Palatini f(R) gravity
SO Classical and Quantum Gravity
JI Class. Quantum Gravity
PY 2021
BP 194003
EP 25pp
VL 38
IS 19
DI 10.1088/1361-6382/ac1fd0
LA English
DE boson stars; Palatini formalism; modified gravity
AB We explore equilibrium solutions of spherically symmetric boson stars in the Palatini formulation of f (R) gravity. We account for the modifications introduced in the gravitational sector by using a recently established correspondence between modified gravity with scalar matter and general relativity with modified scalar matter. We focus on the quadratic theory f (R) = R + xi R-2 and compare its solutions with those found in general relativity, exploring both positive and negative values of the coupling parameter xi. As matter source, a complex, massive scalar field with and without self-interaction terms is considered. Our results show that the existence curves of boson stars in Palatini f (R) gravity are fairly similar to those found in general relativity. Major differences are observed for negative values of the coupling parameter which results in a repulsive gravitational component for high enough scalar field density distributions. Adding self-interactions makes the degeneracy between f (R) and general relativity even more pronounced, leaving very little room for observational discrimination between the two theories.
ER