0000000000305845

AUTHOR

Volodymyr Takhistov

showing 2 related works from this author

SNEWS 2.0 : a next-generation supernova early warning system for multi-messenger astronomy

2021

The next core-collapse supernova in the Milky Way or its satellites will represent a once-in-a-generation opportunity to obtain detailed information about the explosion of a star and provide significant scientific insight for a variety of fields because of the extreme conditions found within. Supernovae in our galaxy are not only rare on a human timescale but also happen at unscheduled times, so it is crucial to be ready and use all available instruments to capture all possible information from the event. The first indication of a potential stellar explosion will be the arrival of a bright burst of neutrinos. Its observation by multiple detectors worldwide can provide an early warning for t…

Milky WayAstrophysics::High Energy Astrophysical PhenomenasatelliteFOS: Physical sciencesGeneral Physics and Astronomy01 natural sciencesHigh Energy Physics - Experiment010305 fluids & plasmasHigh Energy Physics - Experiment (hep-ex)Astronomi astrofysik och kosmologistar0103 physical sciencessupernova[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Astronomy Astrophysics and Cosmology010306 general physicssupernova neutrinoscaptureAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Astroparticle physicsPhysicsWarning systemSupernova Early Warning SystembackgroundAstronomysensitivityGalaxySupernovaelectromagneticNeutrino detectorsupernova neutrinos; multi-messenger astronomy; particle astrophysicsneutrino: burstgalaxyNeutrinoAstrophysics - High Energy Astrophysical Phenomenamulti-messenger astronomy[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]particle astrophysics
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New opportunities at the next-generation neutrino experiments I: BSM neutrino physics and dark matter

2020

Abstract The combination of the high intensity proton beam facilities and massive detectors for precision measurements of neutrino oscillation parameters including the charge-parity violating (CPV) phase will open the door to help make beyond the standard model (BSM) physics reachable even in low energy regimes in the accelerator-based experiments. Large-mass detectors with highly precise tracking and energy measurements, excellent timing resolution, and low energy thresholds will enable the searches for BSM phenomena from cosmogenic origin, as well. Therefore, it is also conceivable that BSM topics in the next-generation neutrino experiments could be the dominant physics topics in the fore…

PhysicsParticle physicsSterile neutrinoPhysics beyond the Standard ModelDark matterGeneral Physics and AstronomyScale (descriptive set theory)Tracking (particle physics)01 natural sciences0103 physical sciencesDeep Underground Neutrino ExperimentHigh Energy Physics::ExperimentNeutrino010306 general physicsNeutrino oscillationReports on Progress in Physics
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