$\ell$-Boson stars in anti-de Sitter spacetime

Abstract

In previous work, we introduced the $\ell$-boson stars, a generalization of standard boson stars, which are parameterized by an angular momentum number $\ell$, while still preserving the spacetime's spherical symmetry. In this article, we present and study the properties of $\ell$-boson stars in spacetimes with a negative cosmological constant, such that they are asymptotically anti-de Sitter.

13 pages, 5 figures. Final version as published in PRD

References in corpus (19)

• Cosmic Structure as the Quantum Interference of a Coherent Dark Wave
• Light ring stability in ultra-compact objects
• Dilute and dense axion stars
• Boson Stars and Oscillatons: A Review
• Accretion disk onto boson stars: a way to supplant black holes candidates
• Constraining scalar fields with stellar kinematics and collisional dark matter
• Stellar and substellar objects in modified gravity
• Dynamical $\ell$-boson stars: generic stability and evidence for non-spherical solutions
• Head-on collisions of $\ell$-boson stars
• Boson stars and their relatives in semiclassical gravity
• Extreme $\ell$-boson stars
• Horndeski stars
• Scalar field confinement as a model for accreting systems
• Long-term stable nonlinear evolutions of ultracompact black-hole mimickers
• On the radial linear stability of nonrelativistic $\ell$-boson stars
• Are nonrelativistic ground state $\ell$-boson stars only stable for $\ell =0$ and $\ell =1$?
• Large-Charge Limit of AdS Boson Stars with Mixed Boundary Conditions
• Gravitational atoms beyond the test field limit: The case of Sgr A* and ultralight dark matter
• Noble gravitational atoms: Self-gravitating black hole scalar wigs with angular momentum number