Geant4 simulation finds neutron capture positions statistically enhance IBD neutrino directionality in water Cherenkov detectors from ~10 MeV to hundreds of MeV despite diffusion.
Supernova Neutrino Neutrino Astronomy
2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
abstract
Modern neutrino facilities will be able to detect a large number of neutrinos from the next Galactic supernova. We investigate the viability of the triangulation method to locate a core-collapse supernova by employing the neutrino arrival time differences at various detectors. We perform detailed numerical fits in order to determine the uncertainties of these time differences for the cases when the core collapses into a neutron star or a black hole. We provide a global picture by combining all the relevant current and future neutrino detectors. Our findings indicate that in the scenario of a neutron star formation, supernova can be located with precision of 1.5 and 3.5 degrees in declination and right ascension, respectively. For the black hole scenario, sub-degree precision can be reached.
years
2026 2representative citing papers
New reactor antineutrino data from CONUS germanium detectors improve upper limits on neutrino magnetic moment to 5.18e-11 mu_B, millicharge to 1.76e-12 e0, NSI scale to 145 GeV, and yield sin^2 theta_W = 0.28 +0.03/-0.04 at ~10 MeV.
citing papers explorer
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Improving the Angular Resolution of IBD Events Using Neutron Capture Information in Super-Kamiokande
Geant4 simulation finds neutron capture positions statistically enhance IBD neutrino directionality in water Cherenkov detectors from ~10 MeV to hundreds of MeV despite diffusion.
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New constraints on physics within and beyond the standard model from the latest CONUS datasets
New reactor antineutrino data from CONUS germanium detectors improve upper limits on neutrino magnetic moment to 5.18e-11 mu_B, millicharge to 1.76e-12 e0, NSI scale to 145 GeV, and yield sin^2 theta_W = 0.28 +0.03/-0.04 at ~10 MeV.