{"total":14,"items":[{"citing_arxiv_id":"2607.00840","ref_index":37,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Dark matter energy exchange in stars orbiting supermassive black holes","primary_cat":"hep-ph","submitted_at":"2026-07-01T12:06:57+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Orbit-averaged DM energy exchange for S4714 reaches stellar luminosity at σ_χp ~ 10^{-36} cm² (MeV-GeV) and σ_χe ~ 5×10^{-38} cm² (sub-MeV) for spiked DM profiles.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.07008","ref_index":8,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Macroscopic Quantum Interference in Dark Matter Wave Scattering with MICROSCOPE","primary_cat":"hep-ph","submitted_at":"2026-06-05T07:53:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Nested cylinders in MICROSCOPE act as a dark-matter-wave interferometer, producing rotation-modulated signals that yield leading constraints on quadratic DM-nucleon couplings for masses 10^{-3}--10^{-2} eV.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.03396","ref_index":17,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Shedding Stray Light on Decaying Light Dark Matter: Constraints from NuSTAR X-ray Observations","primary_cat":"hep-ph","submitted_at":"2026-06-02T09:39:19+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"NuSTAR stray-light data yields the strongest indirect bounds on decaying electrophilic scalar, ALP, and dark photon DM in the 6-70 keV range, plus inelastic DM with mass splittings 3-100 keV.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.16869","ref_index":14,"ref_count":2,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Gauge-invariant cosmological perturbations in Type 3 New General Relativity and background-hierarchy bounds","primary_cat":"gr-qc","submitted_at":"2026-05-16T08:15:03+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Derives background-hierarchy bounds for scalar, transverse-vector and tensor modes in Type 3 NGR around flat FLRW, identifying viable parameter regions where linear perturbation theory remains consistent.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.13042","ref_index":10,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"The Gravitational Spectral Radio Forest: A Signature of Primordial Black Holes","primary_cat":"gr-qc","submitted_at":"2026-05-13T05:54:23+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Asteroid-mass primordial black holes induce a Riemann tidal splitting of the 2P_{3/2} hydrogen state, turning the 9.9 GHz line into a ~2 GHz bandwidth gravitational spectral radio forest in H II regions with accretion-enhanced emission measure.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Bertone and D. Hooper, Rev. Mod. Phys.90, 045002 (2018), arXiv:1605.04909 [astro- ph.CO]. [7] V. C. Rubin and W. K. Ford, Jr., Astrophys. J.159, 379 (1970). 10 [8] V. C. Rubin, N. Thonnard, and W. K. Ford, Jr., Astrophys. J.238, 471 (1980). [9] L. Roszkowski, E. M. Sessolo, and S. Trojanowski, Rept. Prog. Phys.81, 066201 (2018), arXiv:1707.06277 [hep-ph]. [10] J. Billardet al., Rept. Prog. Phys.85, 056201 (2022), arXiv:2104.07634 [hep-ex]. [11] Y. Kahn and T. Lin, Rept. Prog. Phys.85, 066901 (2022), arXiv:2108.03239 [hep-ph]. [12] C. P' erez de los Heros, Symmetry12, 1648 (2020), arXiv:2008.11561 [astro-ph.HE]. [13] M. Misiaszek and N. Rossi, Symmetry16, 201 (2024), arXiv:2310.20472 [hep-ph]. [14] Y. B."},{"citing_arxiv_id":"2605.11097","ref_index":122,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Two-loop neutrino mass model with modular $S_4$ symmetry","primary_cat":"hep-ph","submitted_at":"2026-05-11T18:03:31+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A two-loop neutrino mass model with modular S4 and Z3 symmetries reproduces charged lepton masses and normal-ordering neutrino data while predicting observable LFV and viable DM candidates.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"to the leptonic Dirac CP violating phaseδ CP. where all leptonic Yukawa couplings are taken to be real. Assumptions over scalar quartic couplings will be discussed in Sec. VI. For a given input vector, we minimize the standardχ2 function [121] defined in terms of the calculated observables and their corresponding best experimental values arising from neutrino oscillation experimental data [122]. In addition, all accepted points are required to satisfy the cosmological bounds [123, 124] X i mνi ≤0.04−0.3 eV, (30) the Higgs into di-photon rateR γγ, the SM vector boson couplingκ V [118] and vacuum stability conditions. In the numerical results presented below we take the input parameters in the following ranges: Re(τ)∈[−1/2,1/2],Im(τ)∈[0,4],|τ| ≥1,"},{"citing_arxiv_id":"2605.11082","ref_index":80,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Dark Matter as a Source for Lepton Flavor Violation","primary_cat":"hep-ph","submitted_at":"2026-05-11T18:00:08+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"A dark matter fermion is shown to simultaneously explain the relic density, satisfy direct detection and collider bounds, and produce observable rates for muon-to-electron transitions in a viable parameter region.","context_count":1,"top_context_role":"method","top_context_polarity":"use_method","context_text":"182(2011) 842-856, [1004.1092]. [78] G. Belanger, F. Boudjema, A. Pukhov, and A. Semenov,micrOMEGAs 3: A program for calculating dark matter observables,Comput. Phys. Commun.185(2014) 960-985, [1305.0237]. [79] G. B' elanger, F. Boudjema, A. Pukhov, and A. Semenov,micrOMEGAs4.1: two dark matter candidates,Comput. Phys. Commun.192(2015) 322-329, [1407.6129]. [80] A. Belyaev, N. D. Christensen, and A. Pukhov,CalcHEP 3.4 for collider physics within and beyond the Standard Model,Comput. Phys. Commun.184(2013) 1729-1769, [1207.6082]. [81] G. Alguero, G. Belanger, F. Boudjema, S. Chakraborti, A. Goudelis, S. Kraml, A. Mjallal, and A. Pukhov,micrOMEGAs 6.0: N-component dark matter,Comput. Phys. Commun.299(2024) 109133, [2312."},{"citing_arxiv_id":"2604.10257","ref_index":4,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"DREAMuS: Dark matter REsearch with Advanced Muon Source","primary_cat":"hep-ph","submitted_at":"2026-04-11T15:49:07+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"DREAMuS proposes a muon-beam fixed-target setup at HIAF to probe GeV-scale muon-philic dark matter with sensitivity to couplings around 10^{-4} using background-suppressed signatures from a light flavor-violating mediator.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"015014 (2009). [2] J. Billardet al., Direct detection of dark mat- ter-APPEC committee report*, Rept. Prog. Phys.85, 056201 (2022), arXiv:2104.07634 [hep-ex]. [3] E. Izaguirre, G. Krnjaic, P. Schuster, and N. Toro, Test- ing GeV-Scale Dark Matter with Fixed-Target Miss- ing Momentum Experiments, Phys. Rev. D91, 094026 (2015), arXiv:1411.1404 [hep-ph]. [4] P. Agrawal, Z. Chacko, and C. B. Verhaaren, Leptophilic Dark Matter and the Anomalous Magnetic Moment of the Muon, JHEP08, 147, arXiv:1402.7369 [hep-ph]. [5] G. Bickendorf and M. Drees, Constraints on light lep- tophilic dark matter mediators from decay experiments, Eur. Phys. J. C82, 1163 (2022), arXiv:2206.05038 [hep- ph]. [6] J. P. Leveille, The second-order weak correction to (g−2)"},{"citing_arxiv_id":"2604.07618","ref_index":22,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Multi Component Dark Matter in a Minimal Model","primary_cat":"hep-ph","submitted_at":"2026-04-08T21:39:30+00:00","verdict":null,"verdict_confidence":null,"novelty_score":null,"formal_verification":null,"one_line_summary":null,"context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2511.02023","ref_index":3,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Underground Production of Electromagnetic Dark States by MeV-scale Electron Beams and Detection with CCDs","primary_cat":"hep-ph","submitted_at":"2025-11-03T19:52:20+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Proposes underground MeV-scale electron-beam production of millicharged or dipole fermions followed by CCD detection to access unconstrained parameter space.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2509.08043","ref_index":109,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Testing Viability of Benchmark Dark Matter Models for the Galactic Center Excess","primary_cat":"hep-ph","submitted_at":"2025-09-09T18:00:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Updated constraints on two simplified dark matter models for the Galactic Center Excess leave unconstrained parameter space after applying recent multi-experiment data.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"ants of the 2HDM model, such as a type-II 2HDM model with an extended Yukawa struc- ture [107], have been explored to explain several persistent flavor anomalies, including potential deviations from the SM predictions observed inb→cτ −νandb→sl +l− tran- sitions [102, 108]. Other loop-induced processes likeb→sγrequire a relatively heavy charged Higgs (typicallyM H ± ≳600GeV in Type II scenarios) [109]. The mass of the charged Higgs is not the main focus of this paper; we require the charged Higgs to be heavy enough to evade the other constraints while preserving the perturbativity of the 2HDM+amodel. 3.2.5 Invisible Higgs decay In the 2HDM+amodel, it is possible for the SM-like Higgshto decay into dark sector particles, thereby creating an invisible Higgs decay."},{"citing_arxiv_id":"2509.06892","ref_index":26,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Asymmetric Cannibal Dark Matter: Constraints from Neutron Star","primary_cat":"hep-ph","submitted_at":"2025-09-08T17:11:20+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Asymmetric cannibal dark matter with Z3-symmetric 3→2 interactions depletes in neutron star cores, producing observable heating signatures that constrain dark matter parameters beyond standard annihilation models.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2509.03388","ref_index":7,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Probing Heavy Dark Matter in Red Giants","primary_cat":"hep-ph","submitted_at":"2025-09-03T15:06:45+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Red-giant luminosity observations at the tip of the branch are used to set upper limits on dark-matter masses near 10^11 GeV and spin-independent cross sections near 10^{-37} cm² by requiring that DM-induced core heating does not cause premature helium ignition.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2507.11376","ref_index":52,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"GeV-scale thermal dark matter from dark photons: tightly constrained, yet allowed","primary_cat":"hep-ph","submitted_at":"2025-07-15T14:48:22+00:00","verdict":"CONDITIONAL","verdict_confidence":"MODERATE","novelty_score":5.0,"formal_verification":"none","one_line_summary":"In a dark-photon-mediated Dirac fermionic DM model, only narrow resonant regions with small dark-sector coupling allow the candidate to saturate the full relic density while evading current direct and indirect detection bounds.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":", a photon or a jet) is recoiling against a sizeable amount of missing transverse momentum,pmiss T , (commonly referred to as mono-X searches) [45-51], as well as precision measurements of electroweak (EW) observables. Combining current leading direct and indirect DM searches, GeV-scale thermal relics appear to be excluded up to masses of several tens of GeV [52, 53]. However, care has to be taken when applying these bounds to a specific model, since the relic density is a function of the input parameters. This can result in regions of the parameter space where the cosmological abundance of a particular DM candidate,Ωh2 χ, is smaller than the total observed cold DM - 2 - relic abundance, Ωh2 CDM (in such a case, DM would be multicomponent)."}],"limit":50,"offset":0}