Author:
Oshita Naritaka,Ueda Kazushige,Yamaguchi Masahide
Abstract
Abstract
We investigate a vacuum decay around a spinning seed black hole by using the Israel junction condition and conclude that the spin of black hole would suppress a vacuum decay rate compared to that for a non-spinning case, provided that the surface of vacuum bubble has its ellipsoidal shape characterized by the Kerr geometry. We also find out that in the existence of a near-extremal black hole, a false vacuum state can be more stabilized than the case of the Coleman-de Luccia solution. A few necessary assumptions to carry the calculations are discussed.
Publisher
Springer Science and Business Media LLC
Subject
Nuclear and High Energy Physics
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