Effect of scalar field mass on gravitating charged scalar solitons and black holes in a cavity

Abstract

We study soliton and black hole solutions of Einstein charged scalar field theory in cavity. We examine the effect of introducing a scalar field mass on static, spherically symmetric solutions of the field equations. We focus particularly on the spaces of soliton and black hole solutions, as well as studying their stability under linear, spherically symmetric perturbations of the metric, electromagnetic field, and scalar field.

Minor changes, 7 pages, 7 figures

References in corpus (1)

• Dynamical formation of a Reissner-Nordström black hole with scalar hair in a cavity

Cited by in corpus (9)

• Spinning Kerr black holes with stationary massive scalar clouds: The large-coupling regime
• Hawking--Page phase transitions of the black holes in a cavity
• No-go theorem for static boson stars
• Phase Structures and Transitions of Quintessence Surrounding RN Black Holes in a Grand Canonical Ensemble
• On the dual relation in the Hawking--Page phase transition of the black holes in a cavity
• Phase diagram of the charged black hole bomb system
• Thermal phase transition in $F(R)$-charged $Ad{S}_4$-scalar theory
• Boson stars and solitons confined in a Minkowski box
• The Joule--Thomson and Joule--Thomson-like effects of the black holes in a cavity