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dc.contributor.authorAbi, B.
dc.contributor.authorAcciarri, R.
dc.contributor.authorAcero, M. A
dc.contributor.authorAdamov, G.
dc.contributor.authorAdams, D.
dc.contributor.authorAdinolfi, M.
dc.contributor.authorAhmad, Z.
dc.contributor.authorAhmed, J.
dc.contributor.authorAlion, T.
dc.contributor.authorAlonso Monsalve, S.
dc.contributor.authorAlt, C.
dc.contributor.authorAnderson, J.
dc.contributor.authorAndreopoulos, C.
dc.contributor.authorAndrews, M. P
dc.contributor.authorAndrianala, F.
dc.contributor.authorAndringa, S.
dc.contributor.authorAnkowski, A.
dc.contributor.authorAntonova, M.
dc.contributor.authorAntusch, S.
dc.contributor.authorAranda-Fernandez, A.
dc.date.accessioned2021-10-27T16:17:17Z
dc.date.available2021-10-27T16:17:17Z
dc.date.issued2021-05-15
dc.identifier.urihttps://hdl.handle.net/1721.1/133149
dc.description.abstractAbstract The deep underground neutrino experiment (DUNE), a 40-kton underground liquid argon time projection chamber experiment, will be sensitive to the electron-neutrino 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 $$\nu _e$$ ν e spectral parameters of the neutrino burst will be considered.en_US
dc.publisherSpringer Berlin Heidelbergen_US
dc.relation.isversionofhttps://doi.org/10.1140/epjc/s10052-021-09166-wen_US
dc.rightsCreative Commons Attributionen_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_US
dc.sourceSpringer Berlin Heidelbergen_US
dc.titleSupernova neutrino burst detection with the deep underground neutrino experimenten_US
dc.typeArticleen_US
dc.identifier.citationThe European Physical Journal C. 2021 May 15;81(5):423en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physics
dc.identifier.mitlicensePUBLISHER_CC
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2021-05-16T03:11:25Z
dc.language.rfc3066en
dc.rights.holderThe Author(s)
dspace.embargo.termsN
dspace.date.submission2021-05-16T03:11:25Z
mit.licensePUBLISHER_CC
mit.metadata.statusAuthority Work and Publication Information Neededen_US


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