Fermionic localization of the schwarzian theory
By D. Stanford, E. Witten. Journal of High Energy Physics, 2017
453 citations recorded by the source corpus.
The SYK model is a quantum mechanical model that has been proposed to be holographically dual to a 1 + 1-dimensional model of a quantum black hole. An emergent “gravitational” mode of this model is governed by an unusual action that has been called the Schwarzian action. It governs a reparametrization of a circle. We show that the path integral of the Schwarzian theory is one-loop exact. The argument uses a method of fermionic localization, even though the model itself is purely bosonic.
Subfields: Atomic and Molecular Physics, and Optics, Nuclear and High Energy Physics, Statistical and Nonlinear Physics
View Paper: https://www.semanticscholar.org/paper/4d06ec2aa3cc2ee592e32bf3a981e4ec69bff641
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Atomic and Molecular Physics, and Optics
In Nuclear and High Energy Physics
In Statistical and Nonlinear Physics
Citations in the corpus
- The soft mode in the Sachdev-Ye-Kitaev model and its gravity dual (2017, background): “Remarkably, this expression is valid even for βJ & N , when the fluctuations of the soft mode are strong [25, 27, 28].”
- A semiclassical ramp in SYK and in gravity (2018, background): “In particular, this region of the curve has an explanation involving fluctuations about the naive saddle point in the collective field description or dual AdS2 gravity theory [22, 25].”
- Late Time Correlation Functions, Baby Universes, and ETH in JT Gravity (2019, background): “10 (8)The “smooth” density of states may have sharp edges, as in the SYK model or JT gravity [10, 13, 43, 44, 24, 45, 21] but to leading order this does not stop the decaying behavior.”
- Asymptotic fragility, near AdS2 holography and TT¯$$ T\overline{T} $$ (2017, background): “A further independent support for the semiclassical nature of the JT gravity comes from the recent observation [32] that even before taking the flat limit the Schwarzian path integral is one loop exact.”
- Eternal traversable wormhole (2018, background): “36) was already shown to describe correctly the TFD (for η = 0) [30, 31, 32].”
- The statistical mechanics of near-BPS black holes (2020, methodology): “We review the solution given by [72] using localization and the exact spectrum derived in [69].”
- The Schwarzian theory — origins (2018, methodology): “The link between Liouville theory between branes and the geometric Alekseev-Shatashvili action is made in appendix A. Stanford and Witten showed that for a suitable choice of gauge, this becomes the standard SL(2,R) ∏ t 1/ḟ(t) measure [29].”
- Black holes and random matrices (2016, methodology): “ng it dicult to evaluate Z. In fact, with the correct measure, the theory turns out to be one-loop exact. We will present a somewhat indirect derivation of this fact. A direct proof is also possible [57]. 26 Our derivation is based on an intermediate step where we think about the SYK model for large”
- Solving the Schwarzian via the conformal bootstrap (2017, methodology): “While this is obtained in [23] by performing an inverse Laplace transform, in our approach both terms have a physical origin.”
- JT gravity as a matrix integral (2019, methodology): “A useful simplification is that both path integrals are one-loop exact [22], so we can evaluate them exactly by just doing the path integral for small fluctuations.”
- Statistical mechanics of a two-dimensional black hole (2018, methodology): “) This result was derived in several ways, in particular, by solving the SYK model in the double-scaling limit [9], by evaluating the Schwarzian path integral exactly [10], and by reducing the problem to Liouville quantum mechanics [11, 12].”
- Low-dimensional de Sitter quantum gravity (2019, methodology): “int orbit of the Virasoro group [38,43] at central charge C= 6=G 2. This measure was conjectured to be the correct one for the Schwarzian model as obtained from Jackiw-Teitelboim gravity and from SYK [44], and shown to be the right measure for nearly AdS 2 gravity in [21]. The PSL(2;R) quotient may ”
- Notes on the complex Sachdev-Ye-Kitaev model (2019, background): “The density of states (DOS) and the partition function for the pure Schwarzian model are as follows [33–36], where the energy E and the temperature β−1 are measured in units of (αSN) −1:”
- The factorization problem in Jackiw-Teitelboim gravity (2018, background): “ns Foundation \It-from-Qubit" Collaboration and the MIT Department of Physics. The work of DJ is supported in part by NSFCAREER grant PHY-1352084. 19A similar analysis was done for JT gravity in [54], where it was again observed that the result is not consistent with a thermal partition functio”
- 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 ”
- Transcending the ensemble: baby universes, spacetime wormholes, and the order and disorder of black hole information (2020, background): “escribed by the Schwarzian path integral [93,94]. The Schwarzian alone is not a consistent quantum mechanics, since the path integral on the circle cannot be interpreted as Tre H for any Hamiltonian H[85,95]. This possibility arises from a quotient by residual gauge symmetries acting nontrivially on”