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Gravitational Stability of Boson Stars
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Gravitational Stability of Boson Stars
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We investigate the stability of general-relativistic boson stars by classifying singularities of differential mappings and compare it with the results of perturbation theory. Depending on the particle number, the star has the following regimes of behavior: stable, metastable, pulsation, and collapse.
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Cited by 1 Pith paper
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Boson Stars in $D \ge 4$ Dimensions: Stability, Oscillation Frequencies, and Dynamical Evolutions
Self-interacting boson stars in D=5,6 and solitonic boson stars in D=5 can be radially stable, as shown by generalized pulsation equations and nonlinear spherical evolutions.
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