Oscillatory and Power-law Mass Inflation in Non-Abelian Black Holes
arXiv:gr-qc/9712024
Abstract
Interior structure of non-Abelian black holes is shown to exhibit in a general case either an oscillating mass-inflationary behavior, or power-law behavior with a divergent mass function. In both cases no Cauchy horizon forms.
LaTeX, 3 pages, 1 eps figure; uses mprocl.sty and epsf.tex. To appear in the Proceedings of the 8th Marcel Grossmann Meeting on General Relativity