The quantum gravity dynamics of near extremal black holes
By Zhenbin Yang. Journal of High Energy Physics, 2018
190 citations recorded by the source corpus.
We study the quantum effects of Near-Extremal black holes near their horizons. The gravitational dynamics in such backgrounds are closely connected to a particle in AdS2 with constant electric field. We use this picture to solve the theory exactly. We will give a formula to calculate all correlation functions with quantum gravity backreactions as well as the exact Wheeler-DeWitt wavefunction. Using the WdW wavefunction, we investigate the complexity growth in quantum gravity.
Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/31bcfa642813c2872d58702f7cc88c32750fbe7b
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Astronomy and Astrophysics
In Atomic and Molecular Physics, and Optics
In Nuclear and High Energy Physics
Citations in the corpus
- JT gravity and the ensembles of random matrix theory (2019, methodology): “The contribution of a particular topology to the path (1)This has included many different derivations of the exact path integral [12, 13, 14, 15, 16, 17, 18, 19, 20], studies of the Hilbert space structure [21, 18, 22, 23], correlation functions [24, 25, 26], the physical symmetry charges [27], and ”
- The statistical mechanics of near-BPS black holes (2020, methodology): “The terms of order ε include couplings between matter and gravity, through the Schwarzian mode [96].”
- The entropy of bulk quantum fields and the entanglement wedge of an evaporating black hole (2019, background): “being highly entangled (entropy S 0) only with Land the other factor being entangled only with B. Such a picture is also suggested by the semiclassical analysis of the JT gravity density of states in [45]. In that case, (3.24) would violate both unitarity and the Araki-Lieb bound. We will discuss su”
- Late Time Correlation Functions, Baby Universes, and ETH in JT Gravity (2019, methodology): “We begin with setup, describing the calculation of the early time behavior of the correlator from [21], and discussing the geometry responsible for the ramp behavior.”
- Replica wormholes and the black hole interior (2019, methodology): “only the exterior boundaries of the hyperbolic polygon has nontrivial measure. To get the expression of I n, we can glue multiple copies of I 3 along the inner boundaries. Using the formula of I 3 in [58], we get the expression of I n: I n= (‘ 12;‘ 23;:::‘ n1) = 2 n 1 0 dsˆ(s)K 2is(4e ‘12 2 ):::K 2i”
- JT gravity as a matrix integral (2019, methodology): “The resulting path integral is the partition function of the Schwarzian theory, which has been computed by several different methods [20, 21, 22, 23, 24, 25] and it leads to the expression2”