Linear stability of Einstein-Skyrme black holes

Details Linear stability of Einstein-Skyrme black holes Linear stability of Einstein-Skyrme black holes

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992phlb..285...21h&link_type=abstract

Physics Letters B, Volume 285, Issue 1-2, p. 21-26.

Physics

49

Scientific paper

We analyze the linear stability of black hole solutions of the Einstein-Skyrme system. These solutions, which we have recently found numerically, provide counter examples to the ``no hair'' conjecture for black holes of non-linear matter models. We show that there exist only oscillating radial modes (satisfying the necessary boundary conditions at the horizon and at infinity), with the possible exception of a small region of the two-dimensional parameter space of the black hole configurations. Some numerical evidence for non-linear stability is also discussed.

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