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Supernova neutrino burst detection with the Deep Underground Neutrino Experiment

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Title: Supernova neutrino burst detection with the Deep Underground Neutrino Experiment
Authors: Abi, B
Acciarri, R
Acero, MA
Adamov, G
Adams, D
Adinolfi, M
Ahmad, Z
Ahmed, J
Alion, T
Monsalve, SA
Alt, C
Anderson, J
Andreopoulos, C
Andrews, MP
Andrianala, F
Andringa, S
Ankowski, A
Antonova, M
Antusch, S
Aranda-Fernandez, A
Ariga, A
Arnold, LO
Arroyave, MA
Asaadi, J
Aurisano, A
Aushev, V
Autiero, D
Azfar, F
Back, H
Back, JJ
Backhouse, C
Baesso, P
Bagby, L
Bajou, R
Balasubramanian, S
Baldi, P
Bambah, B
Barao, F
Barenboim, G
Barker, GJ
Barkhouse, W
Barnes, C
Barr, G
Barranco Monarca, J
Barros, N
Barrow, JL
Bashyal, A
Basque, V
Bay, F
Bazo Alba, JL
Beacom, JF
Bechetoille, E
Behera, B
Bellantoni, L
Bellettini, G
Bellini, V
Beltramello, O
Belver, D
Benekos, N
Neves, FB
Berger, J
Berkman, S
Bernardini, P
Berner, RM
Berns, H
Bertolucci, S
Betancourt, M
Bezawada, Y
Bhattacharjee, M
Bhuyan, B
Biagi, S
Bian, J
Biassoni, M
Biery, K
Bilki, B
Bishai, M
Bitadze, A
Blake, A
Siffert, BB
Blaszczyk, FDM
Blazey, GC
Blucher, E
Boissevain, J
Bolognesi, S
Bolton, T
Bonesini, M
Bongrand, M
Bonini, F
Booth, A
Booth, C
Bordoni, S
Borkum, A
Boschi, T
Bostan, N
Bour, P
Boyd, SB
Boyden, D
Bracinik, J
Braga, D
Brailsford, D
Brandt, A
Bremer, J
Brew, C
Brianne, E
Brice, SJ
Brizzolari, C
Bromberg, C
Brooijmans, G
Brooke, J
Bross, A
Brunetti, G
Buchanan, N
Budd, H
Caiulo, D
Calafiura, P
Calcutt, J
Calin, M
Calvez, S
Calvo, E
Camilleri, L
Caminata, A
Campanelli, M
Caratelli, D
Carini, G
Carlus, B
Carniti, P
Terrazas, IC
Carranza, H
Castillo, A
Castromonte, C
Cattadori, C
Cavalier, F
Cavanna, F
Centro, S
Cerati, G
Cervelli, A
Cervera Villanueva, A
Chalifour, M
Chang, C
Chardonnet, E
Chatterjee, A
Chattopadhyay, S
Chaves, J
Chen, H
Chen, M
Chen, Y
Cherdack, D
Chi, C
Childress, S
Chiriacescu, A
Cho, K
Choubey, S
Christensen, A
Christian, D
Christodoulou, G
Church, E
Clarke, P
Coan, TE
Cocco, AG
Coelho, JAB
Conley, E
Conrad, JM
Convery, M
Corwin, L
Cotte, P
Cremaldi, L
Cremonesi, L
Crespo-Anadon, J
Cristaldo, E
Cross, R
Cuesta, C
Cui, Y
Cussans, D
Dabrowski, M
Da Motta, H
Peres, LDS
David, C
David, Q
Davies, GS
Davini, S
Dawson, J
De, K
De Almeida, RM
Debbins, P
De Bonis, I
Decowski, MP
De Gouvea, A
De Holanda, PC
Astiz, ILDI
Deisting, A
De Jong, P
Delbart, A
Delepine, D
Delgado, M
Dell-Acqua, A
De Lurgio, P
De Mello Neto, JRT
DeMuth, DM
Dennis, S
Densham, C
Deptuch, G
De Roeck, A
De Romeri, V
De Vries, JJ
Dharmapalan, R
Dias, M
Diaz, F
Diaz, JS
Di Domizio, S
Di Giulio, L
Ding, P
Di Noto, L
Distefano, C
Diurba, R
Diwan, M
Djurcic, Z
Dokania, N
Dolinski, MJ
Domine, L
Douglas, D
Drielsma, F
Duchesneau, D
Duffy, K
Dunne, P
Durkin, T
Duyang, H
Dvornikov, O
Dwyer, DA
Dyshkant, AS
Eads, M
Edmunds, D
Eisch, J
Emery, S
Ereditato, A
Escobar, CO
Sanchez, LE
Evans, JJ
Ewart, E
Ezeribe, AC
Fahey, K
Falcone, A
Farnese, C
Farzan, Y
Felix, J
Fernandez-Martinez, E
Fernandez Menendez, P
Ferraro, F
Fields, L
Filkins, A
Filthaut, F
Fitzpatrick, RS
Flanagan, W
Fleming, B
Flight, R
Fowler, J
Fox, W
Franc, J
Francis, K
Franco, D
Freeman, J
Freestone, J
Fried, J
Friedland, A
Fuess, S
Furic, I
Furmanski, AP
Gago, A
Gallagher, H
Gallego-Ros, A
Gallice, N
Galymov, V
Gamberini, E
Gamble, T
Gandhi, R
Gandrajula, R
Gao, S
Garcia-Gamez, D
Garcia-Peris, MA
Gardiner, S
Gastler, D
Ge, G
Gelli, B
Gendotti, A
Gent, S
Ghorbani-Moghaddam, Z
Gibin, D
Gil-Botella, I
Girerd, C
Giri, AK
Gnani, D
Gogota, O
Gold, M
Gollapinni, S
Gollwitzer, K
Gomes, RA
Gomez Bermeo, L
Gomez Fajardo, LS
Gonnella, F
Gonzalez-Cuevas, JA
Goodman, MC
Goodwin, O
Goswami, S
Gotti, C
Goudzovski, E
Grace, C
Graham, M
Gramellini, E
Gran, R
Granados, E
Grant, A
Grant, C
Gratieri, D
Green, P
Green, S
Greenler, L
Greenwood, M
Greer, J
Griffith, WC
Groh, M
Grudzinski, J
Grzelak, K
Gu, W
Guarino, V
Guenette, R
Guglielmi, A
Guo, B
Guthikonda, KK
Gutierrez, R
Guzowski, P
Guzzo, MM
Gwon, S
Habig, A
Hackenburg, A
Hadavand, H
Haenni, R
Hahn, A
Haigh, J
Haiston, J
Hamernik, T
Hamilton, P
Han, J
Harder, K
Harris, DA
Hartnell, J
Hasegawa, T
Hatcher, R
Hazen, E
Heavey, A
Heeger, KM
Heise, J
Hennessy, K
Henry, S
Hernandez Morquecho, MA
Herner, K
Hertel, L
Hesam, AS
Hewes, J
Higuera, A
Hill, T
Hillier, SJ
Himmel, A
Hoff, J
Hohl, C
Holin, A
Hoppe, E
Horton-Smith, GA
Hostert, M
Hourlier, A
Howard, B
Howell, R
Huang, J
Huang, J
Hugon, J
Iles, G
Ilic, N
Iliescu, AM
Illingworth, R
Ioannisian, A
Itay, R
Izmaylov, A
James, E
Jargowsky, B
Jediny, F
Jesus-Valls, C
Ji, X
Jiang, L
Jimenez, S
Jipa, A
Joglekar, A
Johnson, C
Johnson, R
Jones, B
Jones, S
Jung, CK
Junk, T
Jwa, Y
Kabirnezhad, M
Kaboth, A
Kadenko, I
Kamiya, F
Karagiorgi, G
Karcher, A
Karolak, M
Karyotakis, Y
Kasai, S
Kasetti, SP
Kashur, L
Kazaryan, N
Kearns, E
Keener, P
Kelly, KJ
Kemp, E
Ketchum, W
Kettell, SH
Khabibullin, M
Khotjantsev, A
Khvedelidze, A
Kim, D
King, B
Kirby, B
Kirby, M
Klein, J
Koehler, K
Koerner, LW
Kohn, S
Koller, PP
Kordosky, M
Kosc, T
Kose, U
Kostelecky, VA
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Krennrich, F
Kreslo, I
Kudenko, Y
Kudryavtsev, VA
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Kumar, J
Kumar, R
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Kutter, T
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Miotto, GL
Lehnert, R
Leigui de Oliveira, MA
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Liao, H
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Littlejohn, BR
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Item Type: Journal Article
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.
Issue Date: 1-May-2021
Date of Acceptance: 21-Apr-2021
URI: http://hdl.handle.net/10044/1/89969
DOI: 10.1140/epjc/s10052-021-09166-w
ISSN: 1124-1861
Publisher: EDP Sciences
Start Page: 1
End Page: 26
Journal / Book Title: European Physical Journal C: Particles and Fields
Volume: 81
Issue: 5
Copyright Statement: © The Author(s) 2021. Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/.
Sponsor/Funder: Science and Technology Facilities Council (STFC)
Funder's Grant Number: ST/S003630/1
Keywords: Science & Technology
Physical Sciences
Physics, Particles & Fields
Physics
CORE-COLLAPSE
SASI ACTIVITY
SENSITIVITY
ACCRETION
PHYSICS
SYSTEM
SIGNAL
Science & Technology
Physical Sciences
Physics, Particles & Fields
Physics
CORE-COLLAPSE
SASI ACTIVITY
SENSITIVITY
ACCRETION
PHYSICS
SYSTEM
SIGNAL
hep-ex
hep-ex
astro-ph.IM
astro-ph.SR
nucl-ex
physics.ins-det
Nuclear & Particles Physics
0202 Atomic, Molecular, Nuclear, Particle and Plasma Physics
0206 Quantum Physics
Publication Status: Published
Open Access location: https://link.springer.com/article/10.1140/epjc/s10052-021-09166-w
Article Number: ARTN 423
Online Publication Date: 2021-05-15
Appears in Collections:Physics
High Energy Physics



This item is licensed under a Creative Commons License Creative Commons