dc.contributor.author | Abi, B. | |
dc.contributor.author | García Gámez, Diego | |
dc.contributor.author | Zamorano García, Bruno | |
dc.contributor.author | Dune Collaboration | |
dc.date.accessioned | 2021-06-01T12:17:15Z | |
dc.date.available | 2021-06-01T12:17:15Z | |
dc.date.issued | 2021-05-15 | |
dc.identifier.citation | Abi, 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-w] | es_ES |
dc.identifier.uri | http://hdl.handle.net/10481/68974 | |
dc.description | 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. | es_ES |
dc.description | Data Availability Statement This manuscript has no associated data
or the data will not be deposited. [Authors’ comment: This manuscript
describes sensitivity studies for the DUNE experiment using simulation
only, and as such there are no experimental data to report.] | es_ES |
dc.description.abstract | 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 νe spectral parameters of the neutrino burst will be considered. | es_ES |
dc.description.sponsorship | Commissariat à l'Énergie Atomique et aux Énergies Alternatives
CEA | es_ES |
dc.description.sponsorship | Fundação de Amparo à Pesquisa do Estado de São Paulo
FAPESP | es_ES |
dc.description.sponsorship | U.S. Department of Energy
DE-AC02-05CH11231 USDOE | es_ES |
dc.description.sponsorship | Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro
FAPERJ | es_ES |
dc.description.sponsorship | Ministerstvo Školství, Mládeže a Tělovýchovy
MŠMT | es_ES |
dc.description.sponsorship | Fundação para a Ciência e a Tecnologia
FCT | es_ES |
dc.description.sponsorship | Royal Society | es_ES |
dc.description.sponsorship | Ministerio de Ciencia e Innovación
MICINN | es_ES |
dc.description.sponsorship | Natural Sciences and Engineering Research Council of Canada
NSERC | es_ES |
dc.description.sponsorship | UK Research and Innovation
UKRI | es_ES |
dc.description.sponsorship | Instituto Nazionale di Fisica Nucleare
INFN | es_ES |
dc.description.sponsorship | Centre National de la Recherche Scientifique
CNRS | es_ES |
dc.description.sponsorship | Conselho Nacional de Desenvolvimento Científico e Tecnológico
CNPq | es_ES |
dc.description.sponsorship | National Research Foundation of Korea
NRF | es_ES |
dc.description.sponsorship | Institut National de Physique Nucléaire et de Physique des Particules
IN2P3 | es_ES |
dc.description.sponsorship | H2020-EU | es_ES |
dc.description.sponsorship | European Commission
EC | es_ES |
dc.description.sponsorship | European Regional Development Fund
ERDF | es_ES |
dc.description.sponsorship | TÜBİTAK | es_ES |
dc.description.sponsorship | CERN | es_ES |
dc.description.sponsorship | U.S. Department of Energy
USDOE | es_ES |
dc.description.sponsorship | Fundação de Amparo à Pesquisa do Estado de Goiás
FAPEG | es_ES |
dc.description.sponsorship | Multiple Sclerosis Center of Atlanta
MSCA | es_ES |
dc.description.sponsorship | Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung
SNF | es_ES |
dc.description.sponsorship | Singapore Eye Research Institute
SERI | es_ES |
dc.description.sponsorship | Fermi Research Alliance, LLC DE-AC02-07CH11359 | es_ES |
dc.description.sponsorship | National Science Foundation
NSF | es_ES |
dc.description.sponsorship | Science and Technology Facilities Council
STFC | es_ES |
dc.language.iso | eng | es_ES |
dc.publisher | Springer Nature | es_ES |
dc.rights | Atribución 3.0 España | * |
dc.rights.uri | http://creativecommons.org/licenses/by/3.0/es/ | * |
dc.title | Supernova neutrino burst detection with the deep underground neutrino experiment: DUNE Collaboration | es_ES |
dc.type | journal article | es_ES |
dc.rights.accessRights | open access | es_ES |
dc.identifier.doi | 10.1140/epjc/s10052-021-09166-w | |
dc.type.hasVersion | VoR | es_ES |