Gravitational stability of boson stars

Fjodor V. Kusmartsev, Eckehard W. Mielke, and Franz E. Schunck
Phys. Rev. D 43, 3895 – Published 15 June 1991
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Abstract

We investigate the stability of general-relativistic boson stars by classifying singularities of differential mappings and compare our results with those of perturbation theory. Depending on the particle number, the star has the following regimes of behavior: stable, metastable, pulsation, and collapse.

  • Received 29 May 1990

DOI:https://doi.org/10.1103/PhysRevD.43.3895

©1991 American Physical Society

Authors & Affiliations

Fjodor V. Kusmartsev

  • Institute for Theoretical Physics, University of Cologne, D-5000 Köln 41, Federal Republic of Germany and L. D. Landau Institute for Theoretical Physics, Moscow 117334, U.S.S.R.

Eckehard W. Mielke and Franz E. Schunck

  • Institute for Theoretical Physics, University of Cologne, D-5000 Köln 41, Federal Republic of Germany

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Issue

Vol. 43, Iss. 12 — 15 June 1991

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