TY - JOUR
T1 - JT gravity coupled to fermions
AU - Banks, Tom
AU - Draper, Patrick
AU - Zhang, Bingnan
N1 - PD acknowledges support from the US Department of Energy under Grant number DE-SC0015655. The work of TB and BZ was partially supported by the US Department of Energy under Grant No. DE-SC0010008. We thank Juan Maldacena for comments on an earlier version of the manuscript. We particularly thank L. Susskind for incisive comments that led to the Matrix model interpretation of our results. The connection with his use of the same quantum model as a toy model of de Sitter space is fascinating and remains to be explored.
PY - 2023
Y1 - 2023
N2 - We argue that two-dimensional dilaton gravity models can all be derived from an analog of Jacobson’s covariant version of the first law of thermodynamics.We then specialize to the JT gravity model and couple it to massless fermions. This model is exactly soluble in quantum field theory, and we present a new derivation of that result. The field theory model violates two principles one might want to impose on a quantum theory of gravity describing the near horizon region of an extremal charged black hole in four dimensions: finite- ness of the entropy for finite causal diamonds, and the absence of global conservation laws. It preserves an infinite number of con- servation laws that one would have expected to be violated, since the fermion state on each side of the AdS2 wormhole is unavoid- ably thermal. We describe a cutoff version of the model, with extra interactions, which cures these difficulties. Our UV completion of the model depends on the AKK[3] map of non-relativistic fermions in an inverted oscillator potential to Weyl fermions in Minkowski space. We argue that gauging the Z2 symmetry of the oscillator model, using a density matrix with temperature that depends on the oscillator coordinates, and inserting chaotic interactions at (al-most) infinite oscillator coordinate, we obtain a model with prop- erties expected of quantum gravity in the near horizon region of an extremal charged black hole in four dimensions.
AB - We argue that two-dimensional dilaton gravity models can all be derived from an analog of Jacobson’s covariant version of the first law of thermodynamics.We then specialize to the JT gravity model and couple it to massless fermions. This model is exactly soluble in quantum field theory, and we present a new derivation of that result. The field theory model violates two principles one might want to impose on a quantum theory of gravity describing the near horizon region of an extremal charged black hole in four dimensions: finite- ness of the entropy for finite causal diamonds, and the absence of global conservation laws. It preserves an infinite number of con- servation laws that one would have expected to be violated, since the fermion state on each side of the AdS2 wormhole is unavoid- ably thermal. We describe a cutoff version of the model, with extra interactions, which cures these difficulties. Our UV completion of the model depends on the AKK[3] map of non-relativistic fermions in an inverted oscillator potential to Weyl fermions in Minkowski space. We argue that gauging the Z2 symmetry of the oscillator model, using a density matrix with temperature that depends on the oscillator coordinates, and inserting chaotic interactions at (al-most) infinite oscillator coordinate, we obtain a model with prop- erties expected of quantum gravity in the near horizon region of an extremal charged black hole in four dimensions.
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U2 - 10.4310/ATMP.2023.v27.n2.a2
DO - 10.4310/ATMP.2023.v27.n2.a2
M3 - Article
AN - SCOPUS:85174678248
SN - 1095-0761
VL - 27
SP - 483
EP - 522
JO - Advances in Theoretical and Mathematical Physics
JF - Advances in Theoretical and Mathematical Physics
IS - 2
ER -