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Supernova neutrino burst detection with the Deep Underground Neutrino Experiment

dc.contributor.authorAcero, M. A.
dc.contributor.otherAndringa, S
dc.contributor.otherAntonova, M
dc.contributor.otherBiagi, S
dc.contributor.otherBonesini, M
dc.contributor.otherCalvez, S
dc.contributor.otherChen, M
dc.date.accessioned2022-12-19T21:06:55Z
dc.date.available2022-12-19T21:06:55Z
dc.date.issued2021-05-15
dc.date.submitted2020-08-15
dc.identifier.citationAbi, B., Acciarri, R., Acero, M.A. et al. Supernova neutrino burst detection with the Deep Underground Neutrino Experiment. Eur. Phys. J. C 81, 423 (2021). https://doi.org/10.1140/epjc/s10052-021-09166-wspa
dc.identifier.urihttps://hdl.handle.net/20.500.12834/1147
dc.description.abstractThe Deep Underground Neutrino Experiment (DUNE), a 40-kton underground liquid argon time projection chamber experiment, will be sensitive to the electronneutrino flavor component of the burst of neutrinos expected from the next Galactic core-collapse supernova. Such an observation will bring unique insight into the astrophysics of core collapse as well as into the properties of neutrinos. The general capabilities of DUNE for neutrino detection in the relevant few- to few-tens-of-MeV neutrino energy range will be described. As an example, DUNE’s ability to constrain the νe spectral parameters of the neutrino burst will be considered.spa
dc.format.mimetypeapplication/pdfspa
dc.language.isoengspa
dc.rights.urihttp://creativecommons.org/licenses/by-nc/4.0/*
dc.sourceThe European Phisical Journal Cspa
dc.titleSupernova neutrino burst detection with the Deep Underground Neutrino Experimentspa
dc.title.alternativeSupernova neutrino burst detection with the Deep Underground Neutrino Experimentspa
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