Instability of compact stars with a nonminimal scalar-derivative coupling

Abstract

For a theory in which a scalar field ϕ has a nonminimal derivative coupling to the Einstein tensor Gμ ν of the form ϕ Gμ ν∇μ∇ν ϕ, it is known that there exists a branch of static and spherically-symmetric relativistic stars endowed with a scalar hair in their interiors. We study the stability of such hairy solutions with a radial field dependence ϕ(r) against odd- and even-parity perturbations. We show that, for the star compactness \U0001d49e smaller than 1/3, they are prone to Laplacian instabilities of the even-parity perturbation associated with the scalar-field propagation along an angular direction. Even for \U0001d49e>1/3, the hairy star solutions are subject to ghost instabilities. We also find that even the other branch with a vanishing background field derivative is unstable for a positive perfect-fluid pressure, due to nonstandard propagation of the field perturbation δ ϕ inside the star. Thus, there are no stable star configurations in derivative coupling theory without a standard kinetic term, including both relativistic and nonrelativistic compact objects.