{"total":14,"items":[{"citing_arxiv_id":"2607.02086","ref_index":51,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"$\\Lambda$ hyperons in core-collapse supernovae: Equilibration and neutrino opacities","primary_cat":"hep-ph","submitted_at":"2026-07-02T12:26:28+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Lambda hyperons equilibrate rapidly in post-collapse proto-neutron stars through nonleptonic NN to N Lambda processes and enhance low-energy muon neutrino opacities beyond nucleonic contributions.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.29576","ref_index":87,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Quark and hybrid stars with renormalization group improvement of NNLO perturbative QCD","primary_cat":"nucl-th","submitted_at":"2026-06-28T19:42:10+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"RGOPT-resummed NNLO pQCD EoS for massive quarks in beta equilibrium is fitted and applied to construct pure quark stars (X=3.08-3.58) and hybrid stars (X~2-2.98) compatible with PSR J0740+6620 and GW190814.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.27425","ref_index":35,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Impact of neutrino-electron scattering and an improved treatment of pair processes on binary neutron star mergers","primary_cat":"astro-ph.HE","submitted_at":"2026-06-25T18:00:02+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Improved Monte Carlo neutrino transport in BNS merger simulations that includes inelastic electron scattering and refined pair processes produces lower heavy-lepton neutrino energies/luminosities and 50% higher ejecta mass.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.23929","ref_index":76,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"As above, so below: assessing extremeness of the neutron-star equation of state based on the unstable branch","primary_cat":"nucl-th","submitted_at":"2026-06-22T20:49:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Requiring causal stable thermodynamically consistent extensions of neutron-star EOS models to perturbative QCD constrains high-density behavior and disfavors purely nucleonic descriptions for all stable stars.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.06580","ref_index":38,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Neutrino mass ordering from the next Galactic supernova at DUNE, HK, and JUNO","primary_cat":"hep-ph","submitted_at":"2026-06-04T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Neutronization burst and accretion-phase rise-time observables from a 10 kpc core-collapse supernova enable DUNE, HK and JUNO to discriminate neutrino mass ordering at 3-6 sigma using multiple progenitor simulations.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.21578","ref_index":42,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Gravitational wave detectability range informed by external messengers","primary_cat":"astro-ph.HE","submitted_at":"2026-05-20T18:00:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"The Targeted Detectability Range (TDR) incorporates sky localization, inclination constraints, and mass bounds from external messengers to evaluate gravitational-wave detectability for gamma-ray bursts observed during LIGO-Virgo-KAGRA's first three runs.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.18972","ref_index":64,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Flavor Conversion Enhances or Suppresses Supernova Explodability Independent of the Progenitor Mass","primary_cat":"astro-ph.HE","submitted_at":"2026-05-18T18:00:49+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Neutrino flavor conversion in supernova cores can enhance or suppress explodability depending on the conversion location, independent of progenitor mass.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.16504","ref_index":66,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Neutrino Flavor Conversion Shapes the Rate of Failed Core-collapse Supernovae","primary_cat":"astro-ph.HE","submitted_at":"2026-05-15T18:01:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Simulations of 195 stellar progenitors indicate that neutrino flavor conversion alters explodability and remnant mass distributions, particularly for stars of 16-30 solar masses.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.04896","ref_index":108,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Parameter Estimation Horizon of Core-Collapse Supernovae with Current and Next-Generation Gravitational-Wave Detectors","primary_cat":"astro-ph.HE","submitted_at":"2026-05-06T13:27:04+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Machine learning extracts core rotation and signal properties from CCSN gravitational waves, with next-generation detectors constraining rotation beyond 100 kpc for favorable orientations despite some uncertainties.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.03947","ref_index":64,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Effects of magnetically driven shocks on nucleosynthesis and kilonovae from neutron star mergers","primary_cat":"astro-ph.HE","submitted_at":"2026-05-05T16:32:23+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Magnetically driven shocks from neutron star merger remnants can reheat ejecta to nuclear statistical equilibrium, alter r-process yields, and produce observable changes in kilonova color and light curves.","context_count":1,"top_context_role":"method","top_context_polarity":"use_method","context_text":"2: Initial launch of a blast wave in the early-launch scenario with maximum Lorentz factorγ max = 2.0. Shown in color is the magnetization parameterσ, at different timestafter launch, relative to the inner cloud radius crossing timer 0/c. White streamlines denote the in-plane magnetic field. We use the tabulated finite-temperature SFHo equation of state [64] from the CompOSE database, consistent with modern merger calculations [24, 65]. Our simulation domain consists of a Cartesian static-mesh-refinement grid. For the early-launch models, the computational do- main extends to±1,002r 0 and employs 7 equally spaced refinement levels in total. For the late-launch models, the domain extends to±7,991r 0 and employs 9 equally"},{"citing_arxiv_id":"2604.06404","ref_index":104,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Neutrino transport and flavor instabilities in a post-merger disk","primary_cat":"astro-ph.HE","submitted_at":"2026-04-07T19:37:20+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"In post-merger disks, electron-lepton-number crossings drive fast flavor instabilities that enhance heavy lepton neutrino fluxes, while collisional instabilities are subdominant and asymmetrically raise heavy-flavor antineutrino energies.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"2628 [hep-ph]. [100] C. Volpe, International Journal of Modern Physics E 24, 1541009 (2015). [101] H. Nagakura and M. Zaizen, Phys. Rev. Lett.129, 261101 (2022), arXiv:2206.04097 [astro-ph.HE]. [102] H. Nagakura, Phys. Rev. D108, 103014 (2023), arXiv:2306.10108 [astro-ph.HE]. [103] D. N. Blaschke and V. Cirigliano, Physical Review D 94, 033009 (2016). [104] S. A. Richers, G. C. McLaughlin, J. P. Kneller, and A. Vlasenko, Phys. Rev. D99, 123014 (2019), [Erratum: Phys.Rev.D 109, 129902 (2024)], arXiv:1903.00022 [astro-ph.HE]. [105] J. M. Miller, B. R. Ryan, and J. C. Dolence, Astro- phys. J. Suppl.241, 30 (2019), arXiv:1903.09273 [astro- ph.IM]. [106] S. De and D. M. Siegel, The Astrophysical Journal921,"},{"citing_arxiv_id":"2603.08843","ref_index":55,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Matter- and magnetically-driven flavor conversion of neutrinos in magnetorotational collapses","primary_cat":"astro-ph.HE","submitted_at":"2026-03-09T19:00:04+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"In magnetorotational stellar collapses, neutrinos undergo resonant flavor conversion in matter plus magnetic-moment-driven chirality flipping for Majorana neutrinos, producing orientation-dependent event rates at detectors that peak 400-600 ms after bounce.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2509.13322","ref_index":72,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Axion-photon conversion in transient compact stars: Systematics, constraints, and opportunities","primary_cat":"hep-ph","submitted_at":"2025-09-16T17:59:59+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Analytical expressions for ALP-photon conversion in transient compact stars yield an updated bound g_aγ < 5×10^{-12} GeV^{-1} for m_a ≲ 10^{-9} eV from SN 1987A, plus sensitivity forecasts for future Galactic SN and NSM observations.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"We use these models as reference cases, facilitating comparison with the results of other authors. These simulations were performed in spherical symmetry with thePrometheus-Vertexcode with general-relativistic corrections and six-species neutrino transport, solving iteratively the two-moment equations for neutrino energy and momentum with a Boltzmann closure [72] and using the full set of neutrino processes listed in Refs. [66, 73]. PNS convection was taken into account by a mixing- length treatment and explosions were manually triggered a few 100 ms after bounce at the progenitor's Fe/Si or Si/O composition interface as described in Ref. [74]. The models were all evolved until 10 s post bounce and they are publicly available upon request [75]."},{"citing_arxiv_id":"2302.12089","ref_index":34,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Time integration for neutrino radiation transport using minimally implicit Runge-Kutta methods","primary_cat":"astro-ph.HE","submitted_at":"2023-02-23T15:23:57+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Minimally implicit Runge-Kutta methods enable stable, explicit-cost integration of neutrino-matter reaction equations in radiation hydrodynamics, tested on problems and core-collapse supernova simulations.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}