On the radial linear stability of nonrelativistic -boson stars
arXiv:2302.00717 · doi:10.1103/PhysRevD.107.084001
Abstract
We study the linear stability of nonrelativistic -boson stars, describing static, spherically symmetric configurations of the Schrödinger-Poisson system with multiple wave functions having the same value of the angular momentum . In this work we restrict our analysis to time-dependent perturbations of the radial profiles of the wave functions, keeping their angular dependency fixed. Based on a combination of analytic and numerical methods, we find that for each , the ground state is linearly stable, whereas the 'th excited states possess unstable (exponentially in time growing) modes. Our results also indicate that all excited states correspond to saddle points of the conserved energy functional of the theory.
21+1 pages, 7 figures, 5 tables
References in corpus (14)
- Cosmic Structure as the Quantum Interference of a Coherent Dark Wave
- Understanding the Core-Halo Relation of Quantum Wave Dark Matter, DM, from 3D Simulations
- Axion dark matter, solitons, and the cusp-core problem
- Boson Stars and Oscillatons: A Review
- Scalar Field Dark Matter: non-spherical collapse and late time behavior
- Bosonic gas as a Galactic Dark Matter Halo
- Multi-field, multi-frequency bosonic stars and a stabilization mechanism
- Critical Behavior in the Gravitational Collapse of a Scalar Field with Angular Momentum in Spherical Symmetry
- Dynamical -boson stars: generic stability and evidence for non-spherical solutions
- Head-on collisions of -boson stars
- Boson stars and their relatives in semiclassical gravity
- Extreme -boson stars
- Horndeski stars
- On the linear stability of -boson stars with respect to radial perturbations
Cited by in corpus (9)
- Bayesian analysis for rotational curves with -boson stars as a dark matter component
- On the linear stability of nonrelativistic selfinteracting boson stars
- Total light bending in non-asymptotically flat black hole spacetimes
- Are nonrelativistic ground state -boson stars only stable for and ?
- Scaling of highly excited Schrödinger-Poisson eigenstates and universality of their rotation curves
- Nonrelativistic Proca stars: Spherical stationary and multi-frequency states
- Noble gravitational atoms: Self-gravitating black hole scalar wigs with angular momentum number
- Linear stability of nonrelativistic Proca stars
- -Boson stars in anti-de Sitter spacetime