Supernova neutrino burst detection with the Deep Underground Neutrino Experiment

Agradecimentos: 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...

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Detalhes bibliográficos
Autor principal: Holanda, Pedro Cunha de, 1973- (author)
Outros Autores: Gelli, Bruno Passarelli, 1995- (author), Guzzo, Marcelo Moraes, 1963- (author), Kemp, Ernesto, 1965- (author), Machado, Ana Amélia Bergamini (author), Peres, Orlando Luís Goulart, 1969- (author), Prakash, Suprabh (author), Guzzo, Marina Reggiani, 1994- (author), Segreto, Ettore, 1973- (author), Nunes, Mônica Soares, 1987- (author), Vanegas Forero, David, 1983- (author), Souza, Henrique Vieira de, 1990- (author)
Formato: article
Publicado em: 2021
Assuntos:
Texto completo:https://hdl.handle.net/20.500.12733/714
País:Brasil
Oai:oai:http://www.repositorio.unicamp.br/:1168895
Descrição
Resumo:Agradecimentos: 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?TAK, 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