{"total":22,"items":[{"citing_arxiv_id":"2607.00866","ref_index":10,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Dissipative hydrodynamic actions and horizon symmetries in gravity","primary_cat":"hep-th","submitted_at":"2026-07-01T12:31:32+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A new prescription computes the dissipative action for holographic hydrodynamics in AdS4 to first order in derivatives and reproduces known Green's functions via horizon diffeomorphisms.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.30043","ref_index":8,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Nonlinear nature of near-equilibrium viscous fluids","primary_cat":"hep-th","submitted_at":"2026-06-29T09:36:04+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Nonlinear analysis of relativistic viscous fluid relaxation yields an asymptotic attractor with frequency locking to n times the fundamental and amplitude cascading J_n = α_J^{n-1} J_1^n fixed by EOS and viscosity.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.14115","ref_index":23,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Hydrodynamics of Nonminimal $F^{(a)\\alpha \\beta } F^{(a)\\gamma \\lambda } R_{\\alpha \\gamma } R_{\\beta \\lambda }$ AdS Black Brane","primary_cat":"hep-th","submitted_at":"2026-06-12T04:53:54+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Perturbative holographic calculation yields σ = 1 − q₂(9κQ²/(L² r_h⁴) + 7κ²Q⁴/(4 r_h⁸)) and η/s = (1/(4π))(1 + q₂ 7κ²Q⁴/(2 r_h⁸)) for a nonminimal AdS black brane.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.11984","ref_index":145,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Modular quantization and black holes","primary_cat":"hep-th","submitted_at":"2026-06-10T12:07:41+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Modular quantization of a single holographic CFT reproduces exact Hartle-Hawking correlators of smooth BTZ black holes in the semiclassical limit while yielding non-smooth stretched-horizon descriptions at finite GN.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"in our present study within AdS/CFT, the construction ofH edge suggests a holographic descrip- tion of black holes directly in terms of 'horizon edge modes'. Several evidences in the literature support such near horizon holography perspective. These include membrane paradigm [139]- [143], as well as related fluid/gravity correspondence in AdS/CFT [144], [145], the near horizon conformal symmetry with analogous structure of a single copy of the \"near-horizon Virasoro algebra\" [146]- [151], as noticed in [56], Kerr/CFT correspondence [152], Carrolian description of near horizon physics [153]- [155], which may provide a natural holographic framework for non-extremal black holes, even beyond the AdS setting."},{"citing_arxiv_id":"2606.10526","ref_index":34,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Tensor Decomposition for Energy-Momentum Correlation Functions","primary_cat":"hep-ph","submitted_at":"2026-06-09T07:55:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"Energy-momentum tensor correlator is reduced to fewer spectral functions via rotational symmetry decomposition and conservation-derived differential relations at zero and finite temperature.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.01486","ref_index":19,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Approximate higher-form symmetries and dualities of massive p-forms in the holographic bulk","primary_cat":"hep-th","submitted_at":"2026-05-31T23:01:48+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Develops a holographic realization of approximate higher-form symmetries via massive antisymmetric tensor fields and derives dualities between boundary theories from bulk Hodge dualities, including constraints on current-current correlators for self-dual cases.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.28753","ref_index":6,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"GR from RG, $2d$ Example: JT-Gravity Induced from Renormalization Group Flow","primary_cat":"hep-th","submitted_at":"2026-05-27T17:12:13+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Holographic RG flow on a 2D CFT induces JT gravity with bulk lapse as dilaton and recovers TTbar deformation in the Fefferman-Graham limit.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.18978","ref_index":4,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"After the Fluid: Subexponential Decay in AdS$_4$","primary_cat":"hep-th","submitted_at":"2026-05-18T18:01:08+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Real-analytic perturbations of AdS4 black branes exhibit stretched-exponential decay exp(-c t^{5/6}) controlled by the large-k tail of the quasinormal mode spectrum.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.15797","ref_index":9,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"A fluid dual to charged large D membrane paradigm","primary_cat":"hep-th","submitted_at":"2026-05-15T09:54:08+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"The leading-order dynamics of charged large D membranes dual to asymptotically flat black holes correspond to a relativistic charged fluid localized on the membrane, with transport coefficients extracted in Eckart and Landau frames showing negative thermal conductivity and heat capacity for enforced","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.01807","ref_index":19,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Relativistic BDNK MHD Evolution in a Boost-Invariant Medium and Its Impact on Dilepton Production","primary_cat":"nucl-th","submitted_at":"2026-05-03T10:23:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Coupled BDNK MHD evolution in boost-invariant flow enhances cooling and suppresses the low-mass dilepton spectrum via magnetic-thermal feedback.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"88, 062302 (2002), [Er- ratum: Phys.Rev.Lett. 89, 159901 (2002)], arXiv:nucl- th/0104064. [17] G. S. Denicol, H. Niemi, E. Molnar, and D. H. Rischke, Phys. Rev. D85, 114047 (2012), [Erratum: Phys.Rev.D 91, 039902 (2015)], arXiv:1202.4551 [nucl-th]. [18] R. Baier, P. Romatschke, D. T. Son, A. O. Starinets, and M. A. Stephanov, JHEP04, 100, arXiv:0712.2451 [hep-th]. [19] S. Bhattacharyya, V. E. Hubeny, S. Minwalla, and M. Rangamani, JHEP02, 045, arXiv:0712.2456 [hep-th]. [20] A. Jaiswal, Phys. Rev. C88, 021903 (2013), arXiv:1305.3480 [nucl-th]. [21] S. Grozdanov and N. Kaplis, Phys. Rev. D93, 066012 (2016), arXiv:1507.02461 [hep-th]. [22] G. S. Denicol, T. Kodama, T. Koide, and P. Mota, J. Phys. G35, 115102 (2008), arXiv:0807."},{"citing_arxiv_id":"2604.18675","ref_index":54,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"All-order fluctuating hydrodynamics of the SYK lattice","primary_cat":"hep-th","submitted_at":"2026-04-20T18:00:00+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":8.0,"formal_verification":"none","one_line_summary":"Derives the all-order fluctuating hydrodynamics effective action and transport coefficients for the SYK lattice from its microscopic pseudo-Goldstone boson action.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Jeon,Hydrodynamic transport coefficients in relativistic scalar field theory,Phys. Rev. D52 (1995) 3591-3642, [hep-ph/9409250]. [52] R. A. Janik and R. B. Peschanski,Asymptotic perfect fluid dynamics as a consequence of Ads/CFT,Phys. Rev. D73(2006) 045013, [hep-th/0512162]. [53] S. Bhattacharyya, S. Lahiri, R. Loganayagam and S. Minwalla,Large rotating AdS black holes from fluid mechanics,JHEP09(2008) 054, [0708.1770]. [54] S. Bhattacharyya, V. E. Hubeny, S. Minwalla and M. Rangamani,Nonlinear Fluid Dynamics from Gravity,JHEP02(2008) 045, [0712.2456]. [55] R. Baier, P. Romatschke, D. T. Son, A. O. Starinets and M. A. Stephanov,Relativistic viscous hydrodynamics, conformal invariance, and holography,JHEP04(2008) 100, [0712.2451]. [56] S. Grozdanov and N. Kaplis,Constructing higher-order hydrodynamics: The third order,Phys."},{"citing_arxiv_id":"2604.13975","ref_index":32,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Universal analytic dependence of the stress-energy tensor at thermodynamic equilibrium in curved space-time","primary_cat":"hep-th","submitted_at":"2026-04-15T15:24:07+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"The analytic part of the stress-energy tensor at thermodynamic equilibrium has a universal covariant form independent of specific curved spacetime geometry for the massless scalar field, argued to hold for any quantum field theory.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"However, regularity requirements limit the nature of quantum states that can be considered. For instance it is well known that the presence of a cosmological horizon is strongly linked to the emergence of thermodynamical properties, namely the Gibbons-Hawking temperature [31], which will be discussed in a dedicated section. Finite temperature quantum field theory in the static patch of dS has been considered in [32]. The exact stress- energy tensor for a conformally coupled scalar field has been calculated in [33] and reads: ⟨bTµν⟩ren = κ4 960π2 gµν + \u0012 π2 90 T 4 0 − κ4 1440π2 \u0013\u0012 1 1−κ 2r2 \u00132 (−gµν + 4uµuν).(54) Thus, removing the trace anomaly just like in AdS case: dist κ2=0 ⟨bTµν⟩= \u0012 π2 90 T 4 0 − κ4 1440π2 \u0013\u0012 1 1−κ 2r2 \u00132 (−gµν + 4uµuν).(55) which corresponds to the analytic distillate (47) in AdS with the transformationκ 2 → −κ 2, thus confirming the"},{"citing_arxiv_id":"2604.13516","ref_index":1,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Quasinormal Modes of pp-Wave Spacetimes and Zero Temperature Dissipation","primary_cat":"gr-qc","submitted_at":"2026-04-15T06:00:59+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Scalar quasinormal modes on pp-wave spacetimes show zero-temperature dissipation for d >= 3 via an irregular singular point acting as absorber, with exact non-dissipative spectrum for d=2 and gapped modes proven by reduction to Bessel equation.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"6 Numerical QNM Spectrum 19 6.1 Numerical method 19 6.2 QNM spectra across dimensions 21 6.3 Structure of the QNM spectrum 22 6.4 Transverse dispersion relation 24 7 Conclusions and discussions 25 7.1 Summary of results 25 7.2 Physical interpretation 26 7.3 Future directions 28 - 1 - A Numerical Method Details 29 1 Introduction The fluid/gravity correspondence [1, 2] provides a powerful framework for understanding the dynamics of strongly coupled quantum field theories at finite temperature within the AdSd+1/CFTd correspondence [3] (see [4, 5] for reviews of holographic applications to con- densed matter). In this framework, the quasinormal modes (QNMs) of black holes in anti-de Sitter (AdS) spacetimes encode the relaxation spectrum of the dual thermal plasma [6, 7]:"},{"citing_arxiv_id":"2602.11806","ref_index":8,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"GR from RG: Gravity Is Induced From Renormalization Group Flow In The Infrared","primary_cat":"hep-th","submitted_at":"2026-02-12T10:38:42+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Holographic RG flow induces gravity by evolving boundary conditions from rigid Dirichlet to mixed Dirichlet-Neumann, generating an Einstein-Hilbert term and evading the Weinberg-Witten theorem.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2602.05130","ref_index":73,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Holographic pressure and volume for black holes","primary_cat":"hep-th","submitted_at":"2026-02-04T23:31:47+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Introduces a holographic pressure and volume for static spherically symmetric black holes via quasi-local thermodynamics, showing large black holes become extensive in the large-system limit while small ones do not.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"[70] V. Iyer and R. M. Wald,Some properties of noether charge and a proposal for dynamical black hole entropy,Physical Review D50(1994) 846-864. [71] L. McGough, M. Mezei and H. Verlinde,Moving the CFT into the bulk withT T, JHEP04(2018) 010, [1611.03470]. [72] K. S. Thorne, R. H. Price and D. A. MacDonald,Black holes: The membrane paradigm. 1986. [73] S. Bhattacharyya, V. E. Hubeny, S. Minwalla and M. Rangamani,Nonlinear Fluid Dynamics from Gravity,JHEP02(2008) 045, [0712.2456]. [74] I. Bredberg, C. Keeler, V. Lysov and A. Strominger,From Navier-Stokes To Einstein, JHEP07(2012) 146, [1101.2451]. [75] G. Compere, P. McFadden, K. Skenderis and M. Taylor,The Holographic fluid dual to vacuum Einstein gravity,JHEP07(2011) 050, [1103."},{"citing_arxiv_id":"2512.25053","ref_index":13,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Fluid dynamics as intersection problem","primary_cat":"hep-th","submitted_at":"2025-12-31T18:48:16+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Fluid dynamics is formulated as an intersection problem on a symplectic manifold associated with spacetime, yielding a geometric derivation of covariant hydrodynamics and extensions to multicomponent and anomalous fluids.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2510.07467","ref_index":32,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Weakly turbulent saturation of the nonlinear scalar ergoregion instability","primary_cat":"gr-qc","submitted_at":"2025-10-08T19:15:23+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Time-domain evolutions demonstrate that the nonlinear scalar ergoregion instability saturates via a weakly turbulent direct cascade transferring energy to small scales and populating higher-order azimuthal modes on the stable light ring.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2509.03656","ref_index":19,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Loops Outside a Black Hole","primary_cat":"hep-th","submitted_at":"2025-09-03T19:06:54+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Conjecture reducing bulk loop discontinuity integrals in black hole Schwinger-Keldysh geometry to exterior real-time finite-temperature loop integrals, checked at one to three loops for low-point functions.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2508.01446","ref_index":20,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Radiation in Fluid/Gravity and the Flat Limit","primary_cat":"hep-th","submitted_at":"2025-08-02T17:28:33+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Establishes a holographic link between bulk gravitational radiation and dissipative corrections plus entropy production in boundary fluids, then constructs Carrollian analogues and celestial observables in the flat limit.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"built out of the extrinsic curvatureT ij 2, the bulk Einstein equations in AdS4 impose3 ∇(0) i T ij = 0 g(0) ij T ij = 0. (1.1) These equations express the diffeomorphisms and conformal invariance of the boundary theory, respectively [10, 18, 19]. They also admit a natural interpretation in terms of the Navier-Stokes equations for a conformal relativistic fluid living at the boundary [20]. This is the starting point of the fluid/gravity correspondence [20-36], which posits that (Einstein) gravity in the bulk of an asymptotically AdS spacetime is dual to a conformal relativistic fluid in one dimension less. The fluid/gravity correspondence can clearly be understood as a coarse-graining of the microscopic boundary CFT, and thus of AdS/CFT itself, which"},{"citing_arxiv_id":"2202.04702","ref_index":35,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Carrollian Perspective on Celestial Holography","primary_cat":"hep-th","submitted_at":"2022-02-09T19:52:15+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A 3d sourced conformal Carrollian field theory is proposed to holographically capture 4d flat gravity kinematics, with Ward identities matching 2d celestial CFT after relating operators.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"1907.02974","ref_index":15,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Ricci cosmology","primary_cat":"gr-qc","submitted_at":"2019-07-05T18:00:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Ricci cosmology adds curvature-matter coupling terms to the stress-energy tensor, enabling analytic inflationary solutions in standard flat FLRW cosmology without Lambda or new scalar fields.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"0905.2975","ref_index":117,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Quasinormal modes of black holes and black branes","primary_cat":"gr-qc","submitted_at":"2009-05-19T05:15:43+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"Quasinormal modes are eigenmodes of dissipative gravitational systems whose spectra encode near-equilibrium transport coefficients in dual quantum field theories and enable tests of general relativity through gravitational wave observations.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"mode gravitational channel of a generic black brane [114] re veals universality, related to the universality of the shear viscosity to entropy density r atio in dual gauge theories. This and further developments [115, 116] also point to a sign ificance of the QNM spectrum in the context of the BH membrane paradigm (for a rec ent review of the membrane paradigm approach, see [117]). •2008-2009 - QNM spectra are computed in applications of the g auge-gravity duality to condensed matter theory [37, 38]. 1.2. Notation and conventions Unless otherwise and explicitly stated, we use geometrized units where G =c = 1, so that energy and time have units of length. We also adopt the ( − + ++) convention for the metric. For reference, the following is a list of symb ols that are used often"}],"limit":50,"offset":0}