{"total":11,"items":[{"citing_arxiv_id":"2605.13970","ref_index":14,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"A Tale of Two Hartle-Hawking Wave Functions: Fully Gravitational vs Partially Frozen","primary_cat":"hep-th","submitted_at":"2026-05-13T18:00:07+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"In AdS the fully gravitational Hartle-Hawking wave function acquires a nontrivial one-loop phase while the partially frozen version stays real and positive; a partially frozen de Sitter sphere shows phase cancellation.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.03037","ref_index":18,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Generalized Free Fields in de Sitter from 1D CFT","primary_cat":"hep-th","submitted_at":"2026-05-04T18:05:58+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Pairs of large-N 1D CFTs encode generalized free fields on a timelike geodesic in de Sitter space via large-N factorization, 1D conformal symmetry, and split representations of dS Green functions.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Let us compute the two point function via the spectral representation. This gives for the two-point function, defined as the expectation value in the energy eigenstate|E 0⟩ O∆(τ)O ∆(0) = Z dE eG(E)e −(E−E0)τ (64) eG(E) =ρ(E) ⟨E O∆ E0⟩ 2 Here, following [6], we used the fine-grained energy constraint. The matrix elements between energy eigenstates in SQM are exactly known [18]. Intro- ducings= √ Eands 0 = √E0 eG(E) =b ∆ Γ(∆±is±is 0) Γ(1−∆±is±is 0) Γ(2is)Γ(1−2is)Γ(2is 0)Γ(1−2is 0) (65) =b ∆ sinh(2πs) sinh(2πs0) sin π(∆±is±is 0) \u0001 - 18 - withb ∆ = 2∆ sinh 2∆. Here we included a factor ofρ(E 0) for normalization. Lets 0 = √E0 = π/βand writings=s 0 +ω, we have eG(E)≃ b∆ sin π(∆±iω) \u0001 (66) Fourier transforming and normalizing gives the anti-podal 3D de Sitter Green function"},{"citing_arxiv_id":"2605.03015","ref_index":21,"ref_count":4,"confidence":0.9,"is_internal_anchor":false,"paper_title":"The Fate of Nucleated Black Holes in de Sitter Quantum Gravity","primary_cat":"hep-th","submitted_at":"2026-05-04T18:00:08+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Nucleated black holes in de Sitter space evaporate via standard Hawking radiation back to the empty vacuum, rendering nucleation a temporary fluctuation.","context_count":2,"top_context_role":"method","top_context_polarity":"use_method","context_text":"they use a 2d dilaton-gravity model along the temporal and radial directions to describe fluctuations in the metric and matter fields inside the static patch. Regarding the leading- order classical solution, we show that their approach is completely equivalent to dS2 Jackiw- Teitelboim (JT) gravity [48, 49] with a linear dilaton potential on a background with a slightly inhomogeneous dilaton profile [21, 50]. The dilatonϕin this description is proportional to the difference between the transverseS 2 area and its Nariai value, which is small inside the static patch. For the quantum analysis, it is important to keep the leading correction quadratic inϕto the strict JT limit inherited from the four-dimensional picture. The resulting action then takes the form in the near-Nariai regime"},{"citing_arxiv_id":"2604.07449","ref_index":42,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Quantum Fluctuations and Newton-Cartan Geometry for Non-Relativistic de Sitter space","primary_cat":"hep-th","submitted_at":"2026-04-08T18:00:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"The one-loop partition function for non-relativistic de Sitter gravity yields a T² prefactor consistent with four symmetry generators, and the bulk admits a torsionless Newton-Cartan geometry satisfying the non-relativistic JT equations.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"section, we will require the fluctuations around the saddle-point solution ofv to be real; as such,v′will turn out to receive only a complex shift due to the boundary conditions above. We believe that this is reminiscent of the choices of complex contours in discussions surrounding the treatment of the boundary theory of two-dimensionalrelativisticde Sitter [42, 43]. Having specified the boundary conditions, we now expand the action to first order in the fluctuations. Requiring the first variation to vanish, then yields the equations of motion for the background fields. We obtain I(1) EdS−G=−2 ∫ dt { ∂t [ c1 ( ¯s′+ ¯s′′ ¯v′ ) +c 0 ( ¯v′−¯v′′′ ¯v′2−¯v′′2 ¯v′3 )] δv+c1∂t ( ¯v′−¯v′′ ¯v′ ) δs } . (2.34) From this, we may read off the equations of motion, which are given by"},{"citing_arxiv_id":"2602.01096","ref_index":14,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Replica Phase Transition with Quantum Gravity Corrections","primary_cat":"hep-th","submitted_at":"2026-02-01T08:22:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"The boundary theory of near-extremal RN black holes shows a replica phase transition controlled by temperature and the couplings C, K, and E.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2512.23656","ref_index":47,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Ordering-Independent Wheeler-DeWitt Equation for Flat Minisuperspace Models","primary_cat":"hep-th","submitted_at":"2025-12-29T18:08:29+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Path-integral measures determine operator orderings for the Wheeler-DeWitt equation in flat minisuperspace models, with all consistent choices yielding identical physical observables via field redefinition Jacobians.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2511.03867","ref_index":35,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Limits on the Statistical Description of Charged de Sitter Black Holes","primary_cat":"hep-th","submitted_at":"2025-11-05T21:22:35+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Adopting the Bousso-Hawking observer normalization for RNdS black holes produces finite heat capacity near the Nariai limit while confirming vanishing capacity in cold and ultracold limits, limiting statistical descriptions.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2509.03930","ref_index":30,"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":"2508.03236","ref_index":83,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Timelike Liouville theory and AdS$_3$ gravity at finite cutoff","primary_cat":"hep-th","submitted_at":"2025-08-05T09:05:10+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Proposes that AdS3 gravity at finite cutoff is dual to a CFT2 coupled to timelike Liouville theory deformed by a marginal operator, with checks via semiclassical partition functions and EOM matching.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2505.03068","ref_index":23,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"M\\\"obius randomness in the Hartle-Hawking state","primary_cat":"hep-th","submitted_at":"2025-05-05T23:22:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"The Hartle-Hawking state for toroidal quantum cosmologies is expressed in the Langlands decomposition as a sum over zeta zeros whose near-singularity dynamics follow the Hilbert-Pólya Hamiltonian and as a Möbius average of CFT partition functions.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Stanford,Operator Dictionaries and Wave Functions in AdS/CFT and dS/CFT, arXiv:1104.2621. [21] D. Anninos,De Sitter Musings, Int. J. Mod. Phys. A27 (2012) 1230013, [arXiv:1205.3855]. [22] D. Anninos, T. Anous, D. Z. Freedman, and G. Konstantinidis,Late-time Structure of the Bunch-Davies De Sitter Wavefunction, JCAP 11 (2015) 048, [arXiv:1406.5490]. [23] J. Maldacena, G. J. Turiaci, and Z. Yang,Two dimensional Nearly de Sitter gravity, JHEP 01 (2021) 139, [arXiv:1904.01911]. - 56 - [24] R. L. Arnowitt, S. Deser, and C. W. Misner,The Dynamics of general relativity, Gen. Rel. Grav. 40 (2008) 1997-2027, [gr-qc/0405109]. [25] B. S. DeWitt,Quantum Theory of Gravity. 1. The Canonical Theory, Phys. Rev."},{"citing_arxiv_id":"1911.11977","ref_index":48,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Replica wormholes and the black hole interior","primary_cat":"hep-th","submitted_at":"2019-11-27T06:30:56+00:00","verdict":"CONDITIONAL","verdict_confidence":"MODERATE","novelty_score":9.0,"formal_verification":"none","one_line_summary":"Replica wormhole geometries justify the replica trick computation of the Page curve in holographic black hole models and support entanglement wedge reconstruction via the Petz map.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}