State transitions in black hole Xray binaries are likely caused by gas evaporation from a thin accretion disk into a hot corona. We present a heightintegrated version of this process, which is suitable for analytical and numerical studies. With radius
We propose a new model of the spherical symmetric quantum black hole in the reduced phase space formulation. We deparametrize gravity by coupling to the Gaussian dust which provides the material coordinates. The foliation by dust coordinates covers both the interior and exterior of the black hole. After the spherical symmetry reduction, our model is a 1 + 1 dimensional field theory containing infinitely many degrees of freedom. The effective dynamics of the quantum black hole is generated by an improved physical Hamiltonian
 Award ID(s):
 1912278
 NSFPAR ID:
 10361710
 Publisher / Repository:
 IOP Publishing
 Date Published:
 Journal Name:
 Classical and Quantum Gravity
 Volume:
 39
 Issue:
 3
 ISSN:
 02649381
 Page Range / eLocation ID:
 Article No. 035011
 Format(s):
 Medium: X
 Sponsoring Org:
 National Science Foundation
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