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The perturbation in φ (or F ) must be even with respect to reflections on the origin to maintain regularity there

We add a small perturbation to the scalar potential φ(r) (in practice, we add it to F (r)), typically a Gaussian, leaving the vector potential a(r) unchanged

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Proca stars in excited states

gr-qc · 2024-11-13 · conditional · novelty 6.0

Excited Proca stars are always unstable: under perturbations they collapse, disperse, or migrate to the ground state, with migration possible only for a narrow set of negative-binding-energy configurations.

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  • Proca stars in excited states gr-qc · 2024-11-13 · conditional · none · ref 1

    Excited Proca stars are always unstable: under perturbations they collapse, disperse, or migrate to the ground state, with migration possible only for a narrow set of negative-binding-energy configurations.