{"total":15,"items":[{"citing_arxiv_id":"2607.01319","ref_index":64,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"What's the Matter with 3D Gravity?","primary_cat":"hep-th","submitted_at":"2026-07-01T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Using worldline formalism and geometric quantization, the partition function for 3D gravity with matter on thermal AdS3 is computed via equivariant localization, reproducing the Wilson spool and conjecturing the all-orders result.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.30725","ref_index":47,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Constrained particle on a group: from propagators to correlators","primary_cat":"hep-th","submitted_at":"2026-06-29T18:00:02+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Develops a constrained particle-on-group formulation of super-JT gravity that yields super-Schwarzian actions, physical supercharges, and explicit N=2/N=4 three-point functions plus zero-energy OTOCs.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.26241","ref_index":62,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"An observer's quantization of 3d de Sitter","primary_cat":"hep-th","submitted_at":"2026-06-24T18:00:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Proposes an SL(2,Z) sum of Kerr-lens geometries in 3d dS gravity whose spectral density is computed via crosscap amplitudes in CLS ⊗ CLS, matching semi-classical predictions and reducing in a simple case to GΣ ⊗ GΣ on the observer worldline.","context_count":1,"top_context_role":"background","top_context_polarity":"support","context_text":"development of this proposed twisted version of the SYK model to future work. Finally, we comment on the possibility of relating the Kerr-lens geometries to matrix integrals. For pc, dq \" p0,1q, the chiral amplitude (5.31) is the disk spectrum of the matrix model dual toCLS [33,152]. Whenpc, dq \" p'2,1q, the chiral spectrum matches the DSSYK spectral density, and the disk amplitude of the ETH matrix model [62]. For generalpc, dq, consider decomposing (5.25) as follows: ρpc,dq CLS pα`q \" `8ÿ n\"'8 ψpc,dq cap pnqZ trumpetpα`, nq.(6.14) Here,Z trumpetpα`, nqis the sine dilaton trumpet [53,141], andψ cappnqit called the cap amplitude [153]: ψpc,dq cap pnq \" 1?'c e dℏ 8c n2 e' ℏ 4c n sin ˆ πpa'nq c ˙ , Z trumpetpα;nq \"cos ' nα 2 ¯ .(6.15) It is possible to associate to a cap amplitudeψ cappnqa random matrix model computing a set of discrete"},{"citing_arxiv_id":"2606.18739","ref_index":42,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"ASEP/DSSYK duality and strange correlator","primary_cat":"hep-th","submitted_at":"2026-06-17T06:33:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Moments of the DSSYK transfer matrix equal an ASEP stationary-product state overlap, presented as analogous to the strange correlator in topological state-sum models.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.23880","ref_index":37,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Not all black holes decohere quantum superpositions","primary_cat":"hep-th","submitted_at":"2026-05-22T17:39:41+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Near-extremal charged black holes make decoherence of charged particle superpositions vanish at late times via a spin-induced energy gap from quantum metric fluctuations.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.13956","ref_index":180,"ref_count":4,"confidence":0.9,"is_internal_anchor":false,"paper_title":"q-Askey Deformations of Double-Scaled SYK","primary_cat":"hep-th","submitted_at":"2026-05-13T18:00:01+00:00","verdict":null,"verdict_confidence":null,"novelty_score":null,"formal_verification":null,"one_line_summary":null,"context_count":2,"top_context_role":"method","top_context_polarity":"use_method","context_text":"Multitrace correlators and geometric wormholesWe would like to perform further checks on the correspondence between the q-Askey deformation of the SYK model with sine dilaton gravity. In particular, it was explained in [14] that one can evaluate a double trumpet amplitude in sine dilaton gravity (which we illustrate in Fig. 14) using the ETH matrix model of Jafferis-Kolchmeyer-Mukhametzhanov-Sonner [179, 180], which takes the form ˜Z(β1,β2)≡ ⣨ Tr ( e−β1 ˆHETH ) Tr ( e−β2 ˆHETH )⟩ conn ,(5.1) where ˆHETH represents the Hamiltonian matrix used in [179, 180] (see also [37, 81, 181-184]) as one of the two types of matrices in the model, and the subindex conn represents connected contributions of two pairs of Hamiltonians in the two different traces inside the expectation"},{"citing_arxiv_id":"2604.12784","ref_index":37,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Quantum chaos and the holographic principle","primary_cat":"quant-ph","submitted_at":"2026-04-14T14:19:21+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":1.0,"formal_verification":"none","one_line_summary":"A review of the chaos-assisted holographic correspondence linking the SYK model to 2D JT gravity, including the need for string theory corrections at fine quantum scales.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"the cited literature, and we felt that a notation emphasizing parametric connections over numerical accuracy should have priority in this review. Finally, there are several directions, which we cannot adequately cover in this short review. Specifically, we will not attempt to review the periodic-orbit/trace-formula approach to JT/matrix-theory physics [35, 36] and the growing literature on coupling matter to JT gravity [37, 38, 39]; either of these fascinating topics would require a substantial separate discussion. For a review focused on JT gravity, we refer to [40]. Before delving in, let us briefly outline the tale of two-dimensional holography for the benefit of those who have not heard of it before: 2D gravity is concerned with the geometry of surfaces. These surfaces can have holes (think of a torus), or boundaries (a cylinder), or"},{"citing_arxiv_id":"2602.06113","ref_index":296,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Deforming the Double-Scaled SYK & Reaching the Stretched Horizon From Finite Cutoff Holography","primary_cat":"hep-th","submitted_at":"2026-02-05T19:00:00+00:00","verdict":null,"verdict_confidence":null,"novelty_score":null,"formal_verification":null,"one_line_summary":null,"context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"recurring to a mixed boundary condition interpretation in the bulk. It would be interesting to generalize the previous work of [36] to explore how this type of interpretation works in a ma- trix model dual to the sine dilaton gravity model with a higher genus expansion, which is not well developed. It might also be interesting to perform theT2 deformation of the two-matrix model of [295, 296] that reproduces certain DSSYK amplitudes (and which has been further developed in [297-299]), to compare with our findings on semiclassical thermodynamics in Sec. 2.3, and possibly to investigate recent connections between JT gravity at finite cutoff with matrix models [42]. Charged DSSYK model and JT deformationsIn line with our analysis ofT 2 defor-"},{"citing_arxiv_id":"2512.10101","ref_index":28,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"The von Neumann algebraic quantum group $\\mathrm{SU}_q(1,1)\\rtimes \\mathbb{Z}_2$ and the DSSYK model","primary_cat":"math-ph","submitted_at":"2025-12-10T21:46:07+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":8.0,"formal_verification":"none","one_line_summary":"The DSSYK model emerges as the dynamics on the quantum homogeneous space of the von Neumann algebraic quantum group SU_q(1,1) ⋊ Z2.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2511.03779","ref_index":286,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Cosmological Entanglement Entropy from the von Neumann Algebra of Double-Scaled SYK & Its Connection with Krylov Complexity","primary_cat":"hep-th","submitted_at":"2025-11-05T19:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Algebraic entanglement entropy from type II1 algebras in double-scaled SYK is matched via triple-scaling limits to Ryu-Takayanagi areas in (A)dS2, reproducing Bekenstein-Hawking and Gibbons-Hawking formulas for specific regions while depending on Krylov complexity of the Hartle-Hawking state.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Vassilevich,Flat space holography and the complex Sachdev-Ye-Kitaev model,Phys. Rev. D101(2020) 086024 [1911.05739]. [284] H. Afshar and B. Oblak,Flat JT gravity and the BMS-Schwarzian,JHEP11(2022) 172 [2112.14609]. [285] D.L. Jafferis, D.K. Kolchmeyer, B. Mukhametzhanov and J. Sonner,Matrix Models for Eigenstate Thermalization,Phys. Rev. X13(2023) 031033 [2209.02130]. [286] D.L. Jafferis, D.K. Kolchmeyer, B. Mukhametzhanov and J. Sonner,Jackiw-Teitelboim gravity with matter, generalized eigenstate thermalization hypothesis, and random matrices,Phys. Rev. D108(2023) 066015 [2209.02131]. [287] M.M. Faruk, E. Morvan and J.P. van der Schaar,Static sphere observers and geodesics in Schwarzschild-de Sitter spacetime,JCAP05(2024) 118 [2312."},{"citing_arxiv_id":"2510.07804","ref_index":13,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Exploring the Spectral Edge in SYK Models","primary_cat":"hep-th","submitted_at":"2025-10-09T05:30:34+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Numerical confirmation that SYK models reproduce RMT spectral edge statistics, yielding power-law quenched entropy at low T and enabling large-N entanglement entropy calculations for supersymmetric wormholes.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2509.15295","ref_index":64,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Living on the edge: a non-perturbative resolution to the negativity of bulk entropies","primary_cat":"hep-th","submitted_at":"2025-09-18T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Summing non-perturbative contributions in the gravitational path integral, extended via matrix integral saddles including one- and two-eigenvalue instantons, resolves negativity of bulk entropies in two-sided black holes.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"operator, ¯EandδEare the average energy and width of the band,f O( ¯E) is the micro- canonical expectation value ofO,g( ¯E, δE) the square root of the microcanonical two-point function, andR ij is a random variable. In the original ETH formulation,R ij is simply taken to be Gaussian-distributed, but this ansatz can (and must) be refined to include non-Gaussianities [64, 65], as we will discuss in Appendix C. For CFTs, ETH is equivalent to the statement that light-heavy-heavy OPE coefficients behave erratically and can be approximated by random variables drawn from an appropriate ensemble [50]. ETH sug- gests that matter operators can also be modeled by random matrices [64]. One can then expect gravitational theories to be generically described (with the caveats explained above)"},{"citing_arxiv_id":"2509.03930","ref_index":5,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Cap amplitudes in random matrix models","primary_cat":"hep-th","submitted_at":"2025-09-04T06:40:07+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Introduces cap amplitude ψ(b) in one-matrix models and interprets the dilaton equation for discrete volumes N_{g,n} as boundary gluing that reduces n by one.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2507.20983","ref_index":108,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Fiducial observers and the thermal atmosphere in the black hole quantum throat","primary_cat":"hep-th","submitted_at":"2025-07-28T16:45:02+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A semiclassical construction of fiducial observers in JT gravity, fixed by conformal isometry flow, is extended to the quantum regime to compute wormhole contributions yielding finite thermal entropy and a quantum description of the stretched horizon.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"differently, at least conceptually, as something akin to quenched rather than an annealed disorder in the system and summarize this approach via the simple mantra: Simplify first, extend later. 17Of course the full von Neumann entropy of the total system should still be well-defined. - 27 - Let us exemplify some of the consequences of this choice and contrast this approach to different options like the two-matrix model pioneered in [108, 109]. As a first example, take the two-point function on the disk (see Fig. 11 for an example). A priori, one may Figure 11. Self-intersections can always be trivialized on the disk. This is no longer true on higher topology due to topologically supported loops. choose the path integral to include or exclude self-intersecting configurations of the matter"},{"citing_arxiv_id":"2411.12050","ref_index":55,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Long-time Freeness in the Kicked Top","primary_cat":"cond-mat.stat-mech","submitted_at":"2024-11-18T20:43:11+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"In the fully chaotic regime of the kicked top, long-time freeness is reached exponentially fast, accompanied by a hierarchy of time scales indicating a multifractal approach.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}