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Black Holes, Oscillating Instantons, and the Hawking-Moss transition

Static oscillating bounces in Schwarzschild de Sitter spacetime are investigated. The oscillating bounce with many oscillations gives a super-thick bubble wall, for which the total vacuum energy increases while the mass of the black hole decreases due to the conservation of Arnowitt-Deser-Misner (ADM) mass. We show that the transition rate of such an "up-tunneling" consuming the seed black hole is higher than that of the Hawking-Moss transition. The correspondence of analyses in the static and global coordinates in the Euclidean de Sitter space is also investigated.

preprint2020arXivOpen access
Ruth GregoryIan G. MossNaritaka Oshita
gr-qchep-th
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Ruth GregoryIan G. MossNaritaka Oshita

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