Supernova neutrino burst detection with the Deep Underground Neutrino Experiment

Simple item page
dc.contributor.authorabi, babak
dc.contributor.authorAcciarri, Roberto
dc.contributor.authorAcero O, Mario A
dc.contributor.authorAdamov, G
dc.contributor.authorAdams, David
dc.contributor.authorAdinolfi, M
dc.contributor.authorAhmad, Z
dc.contributor.authorSzczerbinska, Barbara
dc.creator.orcidhttp://orcid.org/0000-0003-4477-4350en_US
dc.creator.orcidhttp://orcid.org/0000-0003-4477-4350
dc.date.accessioned2022-10-12T21:02:01Z
dc.date.available2022-10-12T21:02:01Z
dc.date.issued2021-05-15
dc.description.abstractThe 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 νe spectral parameters of the neutrino burst will be considered.en_US
dc.description.sponsorshipFunded by SCOAP3. This document was prepared by the DUNE collaboration using the resources of the Fermi National Accelerator Laboratory (Fermilab), a U.S. Department of Energy, Office of Science, HEP User Facility. Fermilab is managed by Fermi Research Alliance, LLC (FRA), acting under Contract No. DE-AC02-07CH11359. This work was supported by CNPq, FAPERJ, FAPEG and FAPESP, Brazil; CFI, IPP and NSERC, Canada; CERN; MŠMT, Czech Republic; ERDF, H2020-EU and MSCA, European Union; CNRS/IN2P3 and CEA, France; INFN, Italy; FCT, Portugal; NRF, South Korea; CAM, Fundación “La Caixa” and MICINN, Spain; SERI and SNSF, Switzerland; TÜB˙ITAK, Turkey; The Royal Society and UKRI/STFC, United Kingdom; DOE and NSF, United States of America. This research used resources of the National Energy Research Scientific Computing Center (NERSC), a U.S. Department of Energy Office of Science User Facility operated under Contract No. DE-AC02-05CH11231.en_US
dc.identifier.citationAbi, B., Acciarri, R., Acero, M.A., Szczerbinska, B., 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-wen_US
dc.identifier.doihttps://doi.org/10.1140/epjc/s10052-021-09166-w
dc.identifier.urihttps://hdl.handle.net/1969.6/94077
dc.language.isoen_USen_US
dc.rightsAttribution 4.0 International*
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/*
dc.subjectdeep underground neutrino experimenten_US
dc.subjectduneen_US
dc.subjectastrophysicsen_US
dc.subjectsupernovaen_US
dc.titleSupernova neutrino burst detection with the Deep Underground Neutrino Experimenten_US
dc.title.alternativeDUNE collaborationen_US
dc.typeArticleen_US

Files

Original bundle

Now showing 1 - 1 of 1
Thumbnail Image
Name:
Supernova Neutrino Burst Detection with the Deep Underground Neutrino Experiment.pdf
Size:
2.68 MB
Format:
Adobe Portable Document Format
Description:
Download

License bundle

Now showing 1 - 1 of 1
No Thumbnail Available
Name:
license.txt
Size:
1.72 KB
Format:
Item-specific license agreed upon to submission
Description:
Download

Collections

COS Faculty Works