{"total":15,"items":[{"citing_arxiv_id":"2606.01071","ref_index":21,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Modular theory and affine representations on the Rindler horizon","primary_cat":"hep-th","submitted_at":"2026-05-31T07:31:33+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Affine group symmetries on the light ray, with dilations implementing modular flow, provide the minimal structure for thermality on the Rindler horizon via the Mellin transform bridge between Minkowski and Rindler modes.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.00142","ref_index":8,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Relativistic deceleration vs acceleration, Unruh effect observation, and the Schott energy","primary_cat":"physics.class-ph","submitted_at":"2026-05-29T01:49:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Finite relativistic deceleration requires boundary Schott energy changes in the LAD equation to conserve energy, and the LCHK estimate for extreme deceleration exceeds sustainable limits for uniform proper deceleration.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.29923","ref_index":26,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Black Hole Photon Rings Saturate the Quantum Chaos Bound","primary_cat":"hep-th","submitted_at":"2026-05-28T13:34:39+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Photon rings around black holes saturate the quantum chaos bound via Lyapunov exponents of null geodesics and OTOCs in the near-ring region.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.29503","ref_index":18,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Polyakov-loop potential of accelerated gluonic matter and subtlety in thermodynamics","primary_cat":"hep-ph","submitted_at":"2026-05-28T07:28:17+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Real acceleration strengthens deconfining properties of gluonic matter per the one-loop Polyakov-loop potential minimized in the optical metric, while imaginary acceleration yields a confined phase.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.09947","ref_index":15,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"The Free Particle--Oscillator--Inverted Oscillator Triangle: Conformal Bridges, Metaplectic Rotations and $\\mathfrak{osp}(1|2)$ Structure","primary_cat":"hep-th","submitted_at":"2026-05-11T03:51:09+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"The free particle, harmonic oscillator, and inverted oscillator are unified as parabolic, elliptic, and hyperbolic realizations of the same conformal module, with explicit mappings between their states, coherent states, and scattering data via metaplectic rotations and Mellin transforms.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Fulling,\"Nonuniqueness of canonical field quantization in Riemannian space-time,\" Phys. Rev. D7(1973) 2850. [12] P. C. W. Davies,\"Scalar production in Schwarzschild and Rindler metrics,\"J. Phys. A: Math. Gen.8(1975) 609. [13] W. G. Unruh,\"Notes on black-hole evaporation,\"Phys. Rev. D14(1976) 870. [14] S. W. Hawking,\"Particle creation by black holes,\"Commun. Math. Phys.43, 199 (1975). [15] L. C. B. Crispino, A. Higuchi, and G. E. A. Matsas,\"The Unruh effect and its applications,\" Rev. Mod. Phys.80, 787 (2008); [arXiv:0710.5373 [gr-qc]]. [16] M. R. Douglas, I. R. Klebanov, D. Kutasov, J. Maldacena, E. Martinec and N. Seiberg, \"A New Hat for thec = 1Matrix Model,\"in From Fields to Strings: Circumnavigating Theoretical Physics, World Scientific (2005) 1758-1827; [arXiv:hep-th/0307195]."},{"citing_arxiv_id":"2604.23849","ref_index":35,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Weyl anomaly induced transport in hydrodynamics","primary_cat":"hep-th","submitted_at":"2026-04-26T19:37:58+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"The Weyl anomaly induces a new non-dissipative current in accelerated fluids that fixes the electromagnetic-acceleration coupling at second order in hydrodynamics.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Without a boundary, the contribu- tions from virtual particle-antiparticle pairs cancel, and no net effect can be observed. This naturally leads to the question: what happens if the horizon in an accelerated frame, namely the Rindler horizon, is treated as such a boundary? To apply this framework to an accelerated observer, we consider Rindler spacetime [35] corresponding to motion along thez-axis. The metric is given byds 2 =ρ 2dθ2 − dx2−dy 2−dρ2, where the Rindler coordinatesρandθare related to the Minkowski coordinates byz=ρcoshθand t=ρsinhθ. The hypersurfaceρ= 0 corresponds to the horizon, sinceg 00(ρ= 0) = 0. The radiation associated with this horizon is the well-known Unruh effect [35, 36]. Thus,ρcorresponds to the distance from the horizon,"},{"citing_arxiv_id":"2604.15926","ref_index":68,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Exact expectation values in a boost-invariant fluid of Dirac fermions with finite spin density","primary_cat":"hep-th","submitted_at":"2026-04-17T10:32:13+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Exact calculations in a boost-invariant free Dirac fermion fluid show spin polarization arises only from finite spin potential, with shear-induced polarization and spin Hall effect absent.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Tτ0 h(τ0,p) n− F (τ0,p) \u0015 , D : bA† s(p)bB† s′(−p) : E = m2 Tτ0 j(τ0,p) 2ε(τ0,p) \u0002 n− F (τ0,p) +n + F (τ0,p) \u0003 δ3 p−p ′\u0001 (σx)s′s , D : bBs(−p)bAs′(p) : E = m2 Tτ0 j∗(τ0,p) 2ε(τ0,p) \u0002 n− F (τ0,p) +n + F (τ0,p) \u0003 δ3 p−p ′\u0001 (σx)ss′ . (4.13) We conclude this section with an important remark. The Bogoliubov transforma- tion (4.5) is reminiscent of the Unruh effect [68] for accelerated observers and of particle production in genuinely curved space-times. However, as discussed in [54], this analogy can be misleading, as the underlying physics is fundamentally different. Although the four- velocity field we consider has non-vanishing acceleration, the quantization is performed on a connected patch of Minkowski space-time."},{"citing_arxiv_id":"2604.14453","ref_index":23,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Thermality Breakdown in Null-Shifted Rindler Wedges","primary_cat":"hep-th","submitted_at":"2026-04-15T22:13:16+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Massive fields in null-shifted Rindler wedges produce non-thermal spectra for accelerated observers, as mass eliminates the exponential Bogoliubov mixing that creates thermality.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.02422","ref_index":8,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Cavity-controlled Inhibition of Decoherence in Accelerated Quantum Detectors","primary_cat":"gr-qc","submitted_at":"2026-04-02T18:00:08+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Moderate acceleration of an Unruh-DeWitt detector in a cylindrical cavity suppresses decoherence more effectively than the inertial case by smearing resonant modes and replacing off-resonant decay with oscillations.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"field-which allows one to translate field fluctuations into quantum observables associated with the detector. Although the conceptual underpinning of the Unruh ef- fect is profound, owing to its parallels with the Hawking effect, the direct observation of Unruh effect in a realis- tic experimental settings remains a challenge, casting a shadow of uncertainty on this otherwise powerful frame- work [8]. The accelerations required to produce observ- able transition rates are typically huge, and the resulting detector responses are often exceedingly small at achiev- able scales [9-12]. These challenges have motivated the ∗ harkirat221@gmail.com † shagun.kaushal@vit.ac.in ‡ kinjalk@iisermohali.ac.in exploration of alternative strategies to amplify or con-"},{"citing_arxiv_id":"2603.26121","ref_index":3,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Probing Unruh Effect from Enhanced Decoherence","primary_cat":"gr-qc","submitted_at":"2026-03-27T07:13:02+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Decoherence rate of an Unruh-DeWitt detector scales as a^{2Δ-1} in the long-time limit, increasing with the scaling dimension Δ of the coupled field and offering a more sensitive probe of the Unruh effect.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2603.01754","ref_index":6,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Spatially inhomogeneous confinement-deconfinement phase transition in accelerated gluodynamics","primary_cat":"hep-lat","submitted_at":"2026-03-02T11:25:51+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Lattice simulations find spatially inhomogeneous confinement-deconfinement transition in weakly accelerated SU(3) gluodynamics, with phase boundary following TE prediction and unchanged critical temperature.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2602.20970","ref_index":6,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Spatial confinement-deconfinement transition in accelerated gluodynamics within lattice simulation","primary_cat":"hep-lat","submitted_at":"2026-02-24T14:51:57+00:00","verdict":"CONDITIONAL","verdict_confidence":"MODERATE","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Lattice simulations in Rindler spacetime show that acceleration turns the confinement-deconfinement transition in gluodynamics into a spatial crossover that approximately follows the Tolman-Ehrenfest law, while the critical temperature stays unchanged.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2510.18670","ref_index":13,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Decay of uniformly rotating particles","primary_cat":"gr-qc","submitted_at":"2025-10-21T14:24:27+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Uniformly rotating particles decay via emission of negative-energy quanta due to the lack of a global vacuum for such observers, implying none can be regarded as stable.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2504.12521","ref_index":72,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Lectures on the Bondi--Metzner--Sachs group and related topics in infrared physics","primary_cat":"gr-qc","submitted_at":"2025-04-16T22:47:28+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"Lecture notes that build the BMS group from prerequisites to applications in soft theorems, memory effects, and new material on asymptotic conformal Killing horizons.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"meant in the full metric, not in the background Minkowski metric). Then a spacetime with a smooth conformal boundary has RµUV U = O r −4\u0001 (4.46) 11This follows from the fact that d ⃗x (p)\u000e du = d⃗x (p)\u000e dt , since ⃗x (p)(t) is a function of time only . 35 Lectures on the BMS Group Aguiar Alves as r → +∞ with constant U. This is a subcase of the so-called peeling property [72, 104, 227, 228]. In the scattering discussed above, one actually has [59] RµUV U = O r −4 log r \u0001 , (4.47) meaning the decay is too slow for the spacetime to admit a conformal compactification. Let us then take a different approach to asymptotic flatness, which was originally taken by Bondi, Van der Burg, and Metzner [34] and Sachs [204, 205] and takes the name of Bondi-Sachs formalism"},{"citing_arxiv_id":"2405.06002","ref_index":4,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Poincar\\'e invariance and the Unruh effect","primary_cat":"physics.gen-ph","submitted_at":"2024-05-09T14:24:46+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"Acceleration has no effect on a causality-enforcing trivial vacuum, so the Unruh effect is absent and standard calculations omit a cancelling contribution from Lorentz transformations acting on the detector.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}