{"total":23,"items":[{"citing_arxiv_id":"2607.01190","ref_index":44,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Semi-regularised three-body pseudopotential for mean-field and beyond-mean-field calculations","primary_cat":"nucl-th","submitted_at":"2026-07-01T17:22:18+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Derives general local leading-order semi-regularised three-body pseudopotential for nuclear EDF in particle-hole and particle-particle channels with expressions for infinite matter and spherical systems.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2607.00036","ref_index":14,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Gravitating Tubes Beyond World Line Paradigm In General Relativity","primary_cat":"gr-qc","submitted_at":"2026-06-28T07:09:41+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"The work constructs timelike tubes foliated by hypersurfaces with a brane-like action whose collective stress-energy is smooth, violates the strong energy condition inside the tube, and reduces to a point-particle action plus self-force term in the vanishing-radius limit.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.13539","ref_index":8,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Conformally Invariant Corrections to the Anomaly-Induced Effective Action and Black Hole Evaporation in Four Dimensions","primary_cat":"hep-th","submitted_at":"2026-06-11T16:23:37+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Conformally invariant corrections to the anomaly-induced effective action produce a one-parameter family of quantum hair for Schwarzschild black holes that modifies the near-horizon stress tensor in a static approximation.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.04631","ref_index":4,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Analisys of $0^-$ excitations in $^{16}$O from inelastic scattering of polarized protons of intermediate energy","primary_cat":"nucl-th","submitted_at":"2026-06-03T09:03:19+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"Calculations of 0- excitations in 16O via inelastic proton scattering are compared to experimental data to assess antisymmetrization effects and possible pion condensation.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.29370","ref_index":8,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"High-Quality Axion Dark Matter without Isocurvature Problem","primary_cat":"hep-ph","submitted_at":"2026-05-28T05:14:43+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A discrete gauge symmetry protecting the axion induces a large effective mass during inflation via a gauge-invariant PQ-violating operator, suppressing isocurvature fluctuations and addressing both quality and isocurvature issues.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.23654","ref_index":22,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Probing nuclear interactions \\`a la Rutherford: Insights on $^4$He from $\\alpha$ scattering","primary_cat":"nucl-ex","submitted_at":"2026-05-22T14:07:18+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"New 4He+4He scattering data and analysis using electron-scattering densities yields a reasonable description of the 4He resonance within existing nuclear interaction models.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.16014","ref_index":231,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Advances in laser-assisted nuclear decay and nuclear excitation","primary_cat":"physics.plasm-ph","submitted_at":"2026-05-15T14:47:24+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"Lasers influence alpha decay, proton radioactivity, and nuclear excitations in isotopes such as 229Th, 83Kr, and 45Sc through methods including the time-dependent Schrödinger equation and Fermi's golden rule.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"nuclear systems, related electron-mediated coupling mechanisms may provide sensitive probes for testing fundamental symmetries, such as parity violation and time-reversal invariance, offering possible insights into beyond-standard-model physics [141,142]. 7.3.1. Nuclear excitation by electron capture (NEEC) NEEC is a resonant process first proposed by Goldanskii and Namiot in the 1970s [231]. It involves the capture of a free electron into a bound atomic state, where the electron transfers its energy directly to the nucleus, exciting it to a higher energy state. Unlike photon-mediated nuclear excitation, NEEC relies on the interaction between the electron, nucleus, and the quantized radiation field, without the emission of real photons."},{"citing_arxiv_id":"2605.11623","ref_index":73,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Cosmology of f(Q,L_m) gravity with Holographic Ricci Dark Energy: Early-Time Inflation and Late-Time Acceleration and RGUP Corrected Observables","primary_cat":"gr-qc","submitted_at":"2026-05-12T06:49:11+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"A single f(Q, L_m) gravity model with HRDE produces Starobinsky-like inflation at high curvature and late-time acceleration, with RGUP corrections keeping n_s and r consistent with Planck while shifting the running of the spectral index.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"cutoff, naturally incorporates local spacetime dynamics through the Hubble parameter and its derivatives while avoiding the causality problems and the coincidence problem of dark energy. Thus, HRDE models have been widely investigated [59-67] as potential solutions to other problems in modern cos- mology. Discussions arising from string theory [68-72], black-hole thermodynam- ics [73], and doubly special relativity [74-76] point to a breakdown of the standard Heisenberg uncertainty relation [77] and the appearance of a mini- mum measurable length [78] or a maximum observable momentum at energy scales [79] that are close to the Planck mass. Several Generalized Uncertainty Principle (GUP) proposals [80-84], which alter canonical commutation rela-"},{"citing_arxiv_id":"2605.11323","ref_index":37,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Characterizing quantum correlations and quantum teleportation in $gg \\to t\\bar{t}$ and $q\\bar{q} \\to t\\bar{t}$ processes under noisy channels","primary_cat":"quant-ph","submitted_at":"2026-05-11T23:20:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Quantum teleportation using noisy top-quark pairs stays above the classical fidelity threshold of 2/3.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"science/article/pii/S0370269313005261. [35] I. Bigi, Y . Dokshitzer, V . Khoze, J. K¨uhn, and P. Zerwas, Physics Letters B181, 157 (1986), ISSN 0370-2693, URLhttps://www. sciencedirect.com/science/article/pii/037026938691275X. [36] G. L. Kane, G. A. Ladinsky, and C. P. Yuan, Phys. Rev. D45, 124 (1992), URLhttps://link.aps.org/doi/10.1103/PhysRevD. 45.124. [37] A. Brandenburg, Z. Si, and P. Uwer, Physics Letters B539, 235 (2002), ISSN 0370-2693, URLhttps://www.sciencedirect.com/ science/article/pii/S0370269302020981. [38] W. Bernreuther, A. Brandenburg, Z. G. Si, and P. Uwer, Phys. Rev. Lett.87, 242002 (2001), URLhttps://link.aps.org/doi/10. 1103/PhysRevLett.87.242002. [39] W. Bernreuther, A. Brandenburg, and P."},{"citing_arxiv_id":"2605.07826","ref_index":121,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Hadronic parity violation: successes, challenges, and future prospects","primary_cat":"nucl-th","submitted_at":"2026-05-08T14:54:10+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"A review of hadronic parity violation covers observed effects, theoretical and experimental progress, and prospects for extending few-nucleon precision studies to nuclei and new physics searches.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"nuclear spin operator,αis the Dirac matrix vector, andρ(r) is the normalized nuclear density. In an APV experiment, the anapole moment cannot be measured in pure isolation. The experimentally extracted NSD parameter,κ total, is a linear combination of several overlapping Hadronic parity violation: successes, challenges, and future prospects15 effects: κtotal =κ a +κ Z +κ hf .(33) Here,κ a is the anapole moment contribution [121] (see also Fig. 5 (c)),κ Z represents the tree-level electroweakZ 0 exchange between the electron and the unpaired nucleon [122] (see also Fig. 5 (b)), andκ hf accounts for hyperfine-induced mixing of the much larger NSI weak charge [123, 124]. Beyond the SM contributions could also be present; see Fig. 5 (d) and the discussion ofZ ′ sensitivity above."},{"citing_arxiv_id":"2605.04393","ref_index":14,"ref_count":2,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Medium Characterization with Hard Probes: From Cherenkov Light in QED to Jet Drift in QCD","primary_cat":"nucl-th","submitted_at":"2026-05-06T01:32:26+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"The work presents a dispersive fit for the refractive index of liquid argon incorporating anomalous dispersion and proposes jet drift in simulations of heavy-ion collisions as a way to disentangle medium properties from energy loss.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"onds after the Big Bang, the Cosmic Neutrino Background (CNB) carries information from a much earlier epoch of the universe compared to the well-known Cosmic Microwave Back- ground (CMB) counterpart (which formed 380,000 years later) [12, 13]. Neutrinos may also carry answers to questions of leptogenesis related to the observed asymmetry between matter and antimatter [14]. Many fundamental questions still remain about neutrinos, including their absolute masses (despite the∼eV upper limits set by experiments like KATRIN [15]). Whether they are Majorana or Dirac fermions and whether beyond the Standard Model \"sterile neutrinos\" exist, neutrinos persist as a focal point for the most significant enduring 4 questions in modern physics."},{"citing_arxiv_id":"2605.00780","ref_index":7,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Breakdown of Semiclassical Gravity in Four-Dimensional Black Hole Evaporation","primary_cat":"hep-th","submitted_at":"2026-05-01T16:54:38+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Semiclassical black hole evaporation in four dimensions produces a thunderbolt singularity signaling breakdown of the effective theory at large distances.","context_count":1,"top_context_role":"method","top_context_polarity":"use_method","context_text":"with the complexity of the four-dimensional semiclassical Einstein equations, has held back progress toward a definitive description of four-dimensional black hole evaporation. In the present paper, we revisit the back-reaction problem using a four-dimensional semi- classical model that retains full diffeomorphism invariance and exactly reproduces the one- looptraceanomaly. ThemodelisbasedontheRiegertanomaly-inducedaction[7]coupledto Einstein gravity, which can be viewed as a controlled truncation of the full one-loop effective action. While not complete, this framework captures essential quantum effects associated with conformal matter fields and provides a concrete setting in which semiclassical back- reaction can be studied dynamically. Earlier literature on this effective action, and some"},{"citing_arxiv_id":"2604.23224","ref_index":13,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Parametric Resonance in $\\phi^4$ Preheating: An Exact Numerical Study","primary_cat":"astro-ph.CO","submitted_at":"2026-04-25T09:31:06+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":"in inflation.Phys. Rev. D, 50:7222-7232, Dec 1994. URL:https://link.aps.org/doi/10.1103/ PhysRevD.50.7222,doi:10.1103/PhysRevD.50.7222. [12] G.D. Coughlan and G.G. Ross. Initial conditions for inflation.Physics Letters B, 157(2):151- 156, 1985. URL:https://www.sciencedirect.com/science/article/pii/0370269385915369, doi:10.1016/0370-2693(85)91536-9. 19 [13] A.D. Linde. Initial conditions for inflation.Physics Letters B, 162(4):281-286, 1985. URL:https://www.sciencedirect.com/science/article/pii/0370269385909232,doi:10. 1016/0370-2693(85)90923-2. [14] Andreas Albrecht and Robert H. Brandenberger. Realization of new inflation.Phys. Rev. D, 31:1225-1231, Mar 1985. URL:https://link.aps.org/doi/10.1103/PhysRevD."},{"citing_arxiv_id":"2604.20792","ref_index":108,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Irreducible Gravitational Wave Background as a Particle Detector","primary_cat":"hep-ph","submitted_at":"2026-04-22T17:17:40+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":"unclear","context_text":"Rev. Lett.89, 091302 (2002), hep-ph/0203118. [106] T. Bringmann, P. F. Depta, M. Hufnagel, J. T. Rud- erman, and K. Schmidt-Hoberg, Phys. Rev. Lett.127, 191802 (2021), 2103.16572. [107] J. Preskill, M. B. Wise, and F. Wilczek, Physics Letters B120, 127 (1983), ISSN 0370-2693, URL https://www.sciencedirect.com/science/article/ pii/0370269383906378. [108] L. F. Abbott and P. Sikivie, Phys. Lett. B120, 133 (1983). [109] M. Dine and W. Fischler, Phys. Lett. B120, 137 (1983). [110] M. S. Turner, Phys. Rev. D28, 1243 (1983). [111] O. Lebedev, JCAP02, 032 (2023), 2210.02293. [112] D. Feiteira and O. Lebedev (2025), 2503.14652. [113] A. Ghoshal, D. Paul, and S. Pal (2025), 2506.17568. [114] A. Ghoshal, D."},{"citing_arxiv_id":"2604.07950","ref_index":4,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Classification of Pati--Salam Asymmetric $\\mathbb{Z}_2 \\times \\mathbb{Z}_2$ Heterotic String Orbifolds","primary_cat":"hep-th","submitted_at":"2026-04-09T08:15:08+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Asymmetric orbifold actions in Pati-Salam heterotic strings yield 24 classes with 0-12 moduli, enabling exophobic three-generation models with moduli-independent doublet-triplet splitting.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"B258 (1985), pp. 46-74. [2] I. Antoniadis, J. Ellis, J. Hagelin, and D. V. Nanopoulos. \"The flippedSU(5)×U(1) string model revamped\". In:Physics Letters B231 (1989), pp. 65-74. [3] A. E. Faraggi, D. V. Nanopoulos, and K. Yuan. \"A standard-like model in the four-dimensional free fermionic string formulation\". In:Nuclear Physics335 (1990), pp. 347-362. [4] I. Antoniadis, G. Leontaris, and J. Rizos. \"A three-generationSU(4)×O(4) string model\". In:Phys. Lett.B245 (1990), pp. 161-168.issn: 03702693.doi:10.1016/ 0370- 2693(90)90127- R.url:http://linkinghub.elsevier.com/retrieve/ pii/037026939090127R. [5] A. E. Faraggi. \"A New standard - like model in the four-dimensional free fermionic string formulation\"."},{"citing_arxiv_id":"2602.04313","ref_index":30,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Critical behavior of isotropic systems with strong dipole-dipole interaction from the functional renormalization group","primary_cat":"cond-mat.stat-mech","submitted_at":"2026-02-04T08:28:10+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"FRG in the LPA' approximation identifies the Aharony fixed point for strong dipolar magnets and yields critical exponents numerically close to but distinct from the O(3) Heisenberg class.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2512.16329","ref_index":30,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Modeling Ultra-High-Energy Cosmic Rays propagation using the input from Configuration Interaction Shell Model","primary_cat":"nucl-th","submitted_at":"2025-12-18T09:11:06+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"CI-SM calculations supply new E1 photon strength function predictions for light nuclei that are fed into UHECR propagation simulations for a 40Ca source.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2512.00864","ref_index":8,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Poly-vector deformations of heterotic supergravity solutions","primary_cat":"hep-th","submitted_at":"2025-11-30T12:25:40+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Bi- and uni-vector deformations of heterotic supergravity solutions are constructed using gauged double field theory together with a generalized open/closed map.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2508.00807","ref_index":31,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Proper-time functional renormalization in $O(N)$ scalar models coupled to gravity","primary_cat":"hep-th","submitted_at":"2025-08-01T17:39:46+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Proper-time FRG applied to gravity-coupled O(N) scalars largely reproduces scaling solutions and critical properties found with the effective average action, with some quantitative differences at finite and large N depending on improved schemes.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2506.02142","ref_index":89,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Gravitons on Nariai Edges","primary_cat":"hep-th","submitted_at":"2025-06-02T18:13:18+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"The one-loop graviton path integral on S² × S^{d-1} factorizes into a bulk thermal graviton gas partition function in Nariai geometry and an edge contribution from shift-symmetric fields on S^{d-1}.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2501.17912","ref_index":103,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"De Sitter Horizon Edge Partition Functions","primary_cat":"hep-th","submitted_at":"2025-01-29T19:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Edge partition functions for totally symmetric tensors in dS_{d+1} are decomposed under so(d), with the linearized gravity case receiving contributions from shift-symmetric fields on S^{d-1} suggesting an embedded brane interpretation.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"S. Fradkin and A. A. Tseytlin, \"One Loop Effective Potential in Gauged O(4) Supergravity,\" Nucl. Phys. B 234 (1984) 472. [101] B. Allen, \"Phase Transitions in de Sitter Space,\" Nucl. Phys. B 226 (1983) 228-252. [102] T. R. Taylor and G. Veneziano, \"Quantum Gravity at Large Distances and the Cosmological Constant,\" Nucl. Phys. B 345 (1990) 210-230. [103] P. A. Griffin and D. A. Kosower, \"Curved spacetime one-loop gravity in a physical gauge,\" Physics Letters B 233 no. 3, (1989) 295-300. https://www.sciencedirect.com/science/article/pii/0370269389913130. [104] P. O. Mazur and E. Mottola, \"ABSENCE OF PHASE IN THE SUM OVER SPHERES,\". [105] D. V. Vassilevich, \"One loop quantum gravity on de Sitter space,\" Int."},{"citing_arxiv_id":"2501.13328","ref_index":9,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Physics on manifolds with exotic differential structures","primary_cat":"hep-th","submitted_at":"2025-01-23T02:18:07+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Exotic differential structures on S^7 produce different Dirac operator spectra for specific symmetric gauge potentials in the Kaluza-Klein limit, implying different physical laws on topologically identical manifolds.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"1907.04402","ref_index":61,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Lectures on Reheating after Inflation","primary_cat":"astro-ph.CO","submitted_at":"2019-07-09T20:36:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":0.0,"formal_verification":"none","one_line_summary":"Lecture notes providing a generic introduction to reheating after inflation, covering its theoretical, phenomenological, and observational aspects.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"These kinds of rapid decay are called preheating, with the decay products in a highly non-thermal state. Finally, we discuss the implications from coupling these decay products to additional matter fields for the energy transfer from the inflaton condensate. 5.1 Perturbative treatment of reheating Originally, reheating was studied as a perturbative process [61] in which individual in- flaton particles were assumed to decay independently of each other. Interaction rates and decay rates were calculated in the usual manner, using perturbative coupling expan- sions. For illustrative purposes we consider inflaton interactions of the form Smatter ⊃∫ d4x√−g(−σφχ2− hφ ¯ψψ), where χ and ψ are some scalar and fermion decay products."}],"limit":50,"offset":0}