On the radial linear stability of nonrelativistic $\ell$-boson stars
Armando A. Roque, Emmanuel Ch\'avez Nambo, Olivier Sarbach

TL;DR
This paper investigates the linear stability of nonrelativistic $ ext{l}$-boson stars, revealing that ground states are stable while excited states have multiple unstable modes, using combined analytical and numerical methods.
Contribution
It provides the first detailed stability analysis of $ ext{l}$-boson stars, identifying stability properties of ground and excited states within the Schrödinger-Poisson framework.
Findings
Ground states are linearly stable.
Excited states have $2n$ unstable modes.
All excited states are saddle points of the energy functional.
Abstract
We study the linear stability of nonrelativistic -boson stars, describing static, spherically symmetric configurations of the Schr\"odinger-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.
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Taxonomy
TopicsCold Atom Physics and Bose-Einstein Condensates · Quantum, superfluid, helium dynamics · Pulsars and Gravitational Waves Research
