{"total":11,"items":[{"citing_arxiv_id":"2607.08175","ref_index":18,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Transformer-based machine learning using low-level calorimeter signals for collimated photon identification at collider experiments","primary_cat":"hep-ph","submitted_at":"2026-07-09T07:21:11+00:00","verdict":"ACCEPT","verdict_confidence":"HIGH","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Cell-level Transformers classify collimated ALP photon-jets versus single photons with AUC 0.98 and regress diphoton mass to ~64 MeV, beating shower-shape and other ML baselines in an ATLAS-like GEANT4 simulation.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2607.07158","ref_index":38,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Weakly supervised machine learning for model-agnostic searches of new phenomena in the $\\gamma$-ray sky","primary_cat":"astro-ph.HE","submitted_at":"2026-07-08T08:50:25+00:00","verdict":"CONDITIONAL","verdict_confidence":"MODERATE","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Weakly supervised classifiers trained on background-versus-mixture samples can identify anomalous gamma-ray sources without labeled signal templates, approaching supervised performance in controlled benchmarks.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.27878","ref_index":7,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Prospects for probing neutral vector-like leptons via pair production at muon collider","primary_cat":"hep-ph","submitted_at":"2026-06-26T09:21:34+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"Simulations indicate a 6 TeV muon collider with 4 ab^{-1} can reach >5σ significance for neutral doublet VLLs of 1.3-3 TeV mass using 4j2μ and 2ℓ2μ + missing energy channels under polarized beams.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.17176","ref_index":41,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Tracing Ultra Light Axions in Post-reionization, Lyman-$\\alpha$ and CMB Missions","primary_cat":"astro-ph.CO","submitted_at":"2026-06-15T18:15:02+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"Fisher forecasts indicate joint post-reionization LSS cross-spectra and CMB-S4-like data can reach O(10^{-4}) uncertainty on ultra-light axion fraction for m_a ≲ 10^{-28} eV, with peak sensitivity near 10^{-25} eV.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.30411","ref_index":14,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Axions Create Singularities on Extremal Horizons","primary_cat":"hep-th","submitted_at":"2026-05-28T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Axions cause singularities on the horizons of extremal rotating charged black holes for almost all axion mass and coupling values.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.22696","ref_index":21,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Dimming of Photon Ring due to Photon-Axion Conversion around Kerr Black Holes","primary_cat":"gr-qc","submitted_at":"2026-05-21T16:38:45+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Photon-axion conversion near Kerr black holes produces dimming of photon spectral luminosity that increases with black hole spin, magnetic field strength, and photon-axion coupling, most efficiently at high frequencies.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.15820","ref_index":24,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"A Near-Cutoff Waveguide Haloscope for sub-meV Dark Matter","primary_cat":"hep-ph","submitted_at":"2026-05-15T10:19:29+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"A novel waveguide haloscope concept using near-cutoff slow-wave response for sub-meV bosonic dark matter, projecting dark photon sensitivity of ε≈2.1×10^{-15} at 0.1 meV.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.13181","ref_index":20,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Searching for axions with quantum interferometry","primary_cat":"hep-ph","submitted_at":"2026-04-14T18:03:42+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Axion-photon coupling imprints measurable Aharonov-Bohm and Berry phases in superconducting circuits and interferometers, projecting sensitivity to g_aγγ ~ 7.8e-14 GeV^{-1} at m_a ~ 1e-10 eV.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"The physics case for Weakly Interacting Slim Particles,\"arXiv:2603.03433 [hep-ph]. [18] G. Bertone and T. Tait, M. P., \"A new era in the search for dark matter,\"Nature562no. 7725, (2018) 51-56,arXiv:1810.01668 [astro-ph.CO]. 17 [19] F. Chadha-Day, J. Ellis, and D. J. E. Marsh, \"Axion dark matter: What is it and why now?,\"Sci. Adv.8 no. 8, (2022) abj3618,arXiv:2105.01406 [hep-ph]. [20] C. A. J. O'Hare, \"Cosmology of axion dark matter,\" PoSCOSMICWISPers(2024) 040, arXiv:2403.17697 [hep-ph]. [21] S. J. Asztalos, G. Carosi, C. Hagmann, D. Kinion, K. van Bibber, M. Hotz, L. J. Rosenberg, G. Rybka, J. Hoskins, J. Hwang, P. Sikivie, D. B. Tanner, R. Bradley, J. Clarke, and ADMX Collaboration, \"SQUID-Based Microwave Cavity Search for Dark-Matter Axions,\"Phys."},{"citing_arxiv_id":"2603.22864","ref_index":18,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"A search for heavy axion-like particles in light-by-light scattering at the FCC-hh","primary_cat":"hep-ph","submitted_at":"2026-03-24T07:05:47+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"Computes production cross sections and sensitivity limits for heavy ALPs in light-by-light scattering at FCC-hh across pp, pPb, and PbPb modes.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Wilczek, Cosmology of the invisible axion , Phys. Lett. B 120, 127 (1983). [15] L.F. Abbott and P. Sikivie, A cosmological bound on the invisible axion , Phys. Lett. B 120, 113 (1983). [16] M. Dine and W. Fischler, The not so harmless axion , Phys. Lett. B 120, 137 (1983). [17] D.J.E. Marsh, Axion cosmology , Phys. Rep. 643, 1 (2016) [arXiv:1510.07633] [18] F. Chadha-Day, J. Ellis and D.J.E. Marsh, Axion dark matter: what is it and why now? , Sci. Adv. 8, eabj3618 (2022) [arXiv:2105.01406]. [19] Z.-Y. Yan and J. Feng, Axion-like particle search with a light-shining- through-walls setup at a γγ collider, arXiv:2512.15192. [20] M.A. Akg¨ um¨ us et al.,A new limit for axion dark matter with SPACE , arXiv:2506."},{"citing_arxiv_id":"2603.10189","ref_index":20,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Searching for axions with time resolved pulsar polarimetry","primary_cat":"hep-ph","submitted_at":"2026-03-10T19:32:25+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Time-resolved optical polarimetry of the Crab pulsar is used to place bounds on the axion-photon coupling via oscillating axion fields induced by the pulsar's magnetic field.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2512.14110","ref_index":13,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Any Light Particle Searches with ALPS II: first science results","primary_cat":"hep-ex","submitted_at":"2025-12-16T05:45:34+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"ALPS II reports no detection of axion-like particles and establishes improved 95% CL upper limits on di-photon couplings of 1.5e-9 GeV^-1 for masses below 0.1 meV, plus limits for scalar, vector, and tensor bosons.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}