Black Holes, Oscillating Instantons, and the Hawking-Moss transition
arXiv:2003.04927 · doi:10.1007/JHEP07(2020)024
Abstract
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.
arXiv comment24 pages, 10 figures, version accepted for publication in JHEP
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