No nonminimally coupled massless scalar hair for spherically symmetric neutral reflecting stars
arXiv:1709.01933 · doi:10.1103/PhysRevD.96.024019
Abstract
It has recently been proved that horizonless compact stars with reflecting boundary conditions {\it cannot} support spatially regular matter configurations made of minimally coupled scalar fields, vector fields, and tensor fields. In the present paper we extend this intriguing no-hair property to the physically interesting regime of scalar fields with {\it nonminimal} coupling to gravity. In particular, we prove that static spherically symmetric configurations made of nonminimally coupled massless scalar fields cannot be supported by compact reflecting stars.
6 pages
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Cited by in corpus (11)
- No hair for spherically symmetric neutral black holes: nonminimally coupled massive scalar fields
- No hair for spherically symmetric neutral reflecting stars: nonminimally coupled massive scalar fields
- Ultra-spinning exotic compact objects supporting static massless scalar field configurations
- Scalarization of compact stars in the scalar-Gauss-Bonnet gravity
- No hair theorem for spherically symmetric regular compact stars with Dirichlet boundary conditions
- No hair theorem for bound-state massless static scalar fields outside horizonless Neumann compact stars
- No-go theorem for spatially regular boson stars made of static nonminimally coupled massive scalar fields
- Charged reflecting shells supporting non-minimally coupled massless scalar field configurations
- No scalar hair in nonminimal derivative coupling model for Neumann and Dirichlet reflecting star
- A no-go theorem for scalar fields with couplings from Ginzburg-Landau models
- No scalar condensations outside reflecting stars with coupling terms from Ginzburg-Landau models