Abstract
Abstract
An old black hole can tunnel into a white hole/firewall by emitting large baby universes. This phenomenon was investigated in Jackiw-Teitelboim (JT) gravity for genus one. In this paper, the focus is on higher genus corresponding to emitting more than one baby universe (n > 1). The probability of encountering a firewall or tunneling into a white hole after emitting n baby universes is proportional to $$ {e}^{-2 nS(E)}{e}^{4\pi \sqrt{E}\left(n-1\right)}{E}^{2{n}^2-n-9/2}{t}^{4{n}^2-2n-5} $$
e
−
2
nS
E
e
4
π
E
n
−
1
E
2
n
2
−
n
−
9
/
2
t
4
n
2
−
2
n
−
5
, where t is the age of the black hole, and S and E represent the entropy and energy of the black hole, respectively.
Publisher
Springer Science and Business Media LLC