Supernova neutrino burst detection with the Deep Underground Neutrino Experiment-Reference-Cited by-同舟云学术

Supernova neutrino burst detection with the Deep Underground Neutrino Experiment

Published:2021-05 Issue:5 Volume:81 Page:
ISSN:1434-6044
Container-title:The European Physical Journal C
language:en
Short-container-title:Eur. Phys. J. C

Author:

Abi B.,Acciarri R.,Acero M. A.,Adamov G.,Adams D.,Adinolfi M.,Ahmad Z.,Ahmed J.,Alion T.,Alonso Monsalve S.,Alt C.,Anderson J.,Andreopoulos C.,Andrews M. P.,Andrianala F.,Andringa S.,Ankowski A.,Antonova M.,Antusch S.,Aranda-Fernandez A.,Ariga A.,Arnold L. O.,Arroyave M. A.,Asaadi J.,Aurisano A.,Aushev V.,Autiero D.,Azfar F.,Back H.,Back J. J.,Backhouse C.,Baesso P.,Bagby L.,Bajou R.,Balasubramanian S.,Baldi P.,Bambah B.,Barao F.,Barenboim G.,Barker G. J.,Barkhouse W.,Barnes C.,Barr G.,Barranco Monarca J.,Barros N.,Barrow J. L.,Bashyal A.,Basque V.,Bay F.,Alba J. L. Bazo,Beacom J. F.,Bechetoille E.,Behera B.,Bellantoni L.,Bellettini G.,Bellini V.,Beltramello O.,Belver D.,Benekos N.,Bento Neves F.,Berger J.,Berkman S.,Bernardini P.,Berner R. M.,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.,Blanco Siffert B.,Blaszczyk F. D. M.,Blazey G. C.,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 S. B.,Boyden D.,Bracinik J.,Braga D.,Brailsford D.,Brandt A.,Bremer J.,Brew C.,Brianne E.,Brice S. J.,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.,Caro Terrazas I.,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 T. E.,Cocco A. G.,Coelho J. A. B.,Conley E.,Conrad J. M.,Convery M.,Corwin L.,Cotte P.,Cremaldi L.,Cremonesi L.,Crespo-Anadón J. I.,Cristaldo E.,Cross R.,Cuesta C.,Cui Y.,Cussans D.,Dabrowski M.,da Motta H.,Da Silva Peres L.,David C.,David Q.,Davies G. S.,Davini S.,Dawson J.,De K.,De Almeida R. M.,Debbins P.,De Bonis I.,Decowski M. P.,de Gouvêa A.,De Holanda P. C.,De Icaza Astiz I. L.,Deisting A.,De Jong P.,Delbart A.,Delepine D.,Delgado M.,Dell-Acqua A.,De Lurgio P.,de Mello Neto J. R. T.,DeMuth D. M.,Dennis S.,Densham C.,Deptuch G.,De Roeck A.,De Romeri V.,De Vries J. J.,Dharmapalan R.,Dias M.,Diaz F.,Díaz J. S.,Di Domizio S.,Di Giulio L.,Ding P.,Di Noto L.,Distefano C.,Diurba R.,Diwan M.,Djurcic Z.,Dokania N.,Dolinski M. J.,Domine L.,Douglas D.,Drielsma F.,Duchesneau D.,Duffy K.,Dunne P.,Durkin T.,Duyang H.,Dvornikov O.,Dwyer D. A.,Dyshkant A. S.,Eads M.,Edmunds D.,Eisch J.,Emery S.,Ereditato A.,Escobar C. O.,Escudero Sanchez L.,Evans J. J.,Ewart E.,Ezeribe A. 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M.,Penichot Y.,Pennacchio E.,Penzo A.,Peres O. L. G.,Perry J.,Pershey D.,Pessina G.,Petrillo G.,Petta C.,Petti R.,Piastra F.,Pickering L.,Pietropaolo F.,Pillow J.,Pinzino J.,Plunkett R.,Poling R.,Pons X.,Poonthottathil N.,Pordes S.,Potekhin M.,Potenza R.,Potukuchi B. V. K. S.,Pozimski J.,Pozzato M.,Prakash S.,Prakash T.,Prince S.,Prior G.,Pugnere D.,Qi K.,Qian X.,Raaf J. L.,Raboanary R.,Radeka V.,Rademacker J.,Radics B.,Rafique A.,Raguzin E.,Rai M.,Rajaoalisoa M.,Rakhno I.,Rakotondramanana H. T.,Rakotondravohitra L.,Ramachers Y. A.,Rameika R.,Ramirez Delgado M. A.,Ramson B.,Rappoldi A.,Raselli G.,Ratoff P.,Ravat S.,Razafinime H.,Real J. S.,Rebel B.,Redondo D.,Reggiani-Guzzo M.,Rehak T.,Reichenbacher J.,Reitzner S. D.,Renshaw A.,Rescia S.,Resnati F.,Reynolds A.,Riccobene G.,Rice L. C. J.,Rielage K.,Rigaut Y.,Rivera D.,Rochester L.,Roda M.,Rodrigues P.,Rodriguez Alonso M. J.,Rodriguez Rondon J.,Roeth A. 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Abstract

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

$$\nu _e$$

ν e spectral parameters of the neutrino burst will be considered.

Publisher

Springer Science and Business Media LLC

Subject

Physics and Astronomy (miscellaneous),Engineering (miscellaneous)

Link

https://link.springer.com/content/pdf/10.1140/epjc/s10052-021-09166-w.pdf

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