Perturbation theory for self-gravitating gauge fields: The odd-parity sector
Physical Review D - Particles, Fields, Gravitation and Cosmology, ISSN: 0556-2821, Vol: 62, Issue: 8, Page: 1-24
2000
- 10Citations
- 7Captures
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Article Description
A gauge- and coordinate-invariant perturbation theory for self-gravitating non-Abelian gauge fields with the gauge group SU(2) is developed and used to analyze local uniqueness and linear stability properties of non-Abelian equilibrium configurations. It is shown that all admissible stationary odd-parity excitations of the static and spherically symmetric Einstein-Yang-Mills soliton and black hole solutions have a total angular momentum number l=1, and are characterized by nonvanishing asymptotic flux integrals. Local uniqueness and stability results with respect to non-Abelian perturbations are also established for the Schwarzschild and Reissner-Nordström solutions. Finally, unstable modes with l=1 are excluded for the static and spherically symmetric non-Abelian solitons and black holes. ©2000 The American Physical Society.
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=16644374012&origin=inward; http://dx.doi.org/10.1103/physrevd.62.084001; https://link.aps.org/doi/10.1103/PhysRevD.62.084001; http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.62.084001/fulltext; http://link.aps.org/article/10.1103/PhysRevD.62.084001
American Physical Society (APS)
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