TY - JOUR
T1 - Stability of non-Abelian black holes and catastrophe theory
AU - Maeda, K.
AU - Tachizawa, T.
AU - Torii, T.
AU - Maki, T.
N1 - Copyright:
Copyright 2015 Elsevier B.V., All rights reserved.
PY - 1994
Y1 - 1994
N2 - Two types of self-gravitating particle solutions found in several theories with non-Abelian fields are smoothly connected by a family of nontrivial black holes. There exists a maximum point of the black hole entropy where the stability of solutions changes. This criterion is universal, and the changes in stability follow from a catastrophe-theoretic analysis of the potential function defined by black hole entropy.
AB - Two types of self-gravitating particle solutions found in several theories with non-Abelian fields are smoothly connected by a family of nontrivial black holes. There exists a maximum point of the black hole entropy where the stability of solutions changes. This criterion is universal, and the changes in stability follow from a catastrophe-theoretic analysis of the potential function defined by black hole entropy.
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U2 - 10.1103/PhysRevLett.72.450
DO - 10.1103/PhysRevLett.72.450
M3 - Article
AN - SCOPUS:0001548267
SN - 0031-9007
VL - 72
SP - 450
EP - 453
JO - Physical Review Letters
JF - Physical Review Letters
IS - 4
ER -