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Related papers: Supernova Neutrino Detection in LZ
200 papers
Dark matter detectors that utilize liquid xenon have now achieved tonne-scale targets, giving them sensitivity to all flavours of supernova neutrinos via coherent elastic neutrino-nucleus scattering. Considering for the first time a…
High Energy Astrophysical Phenomena · Physics
2016-12-21
Rafael F. Lang , Christopher McCabe , Shayne Reichard , Marco Selvi , Irene Tamborra
The LZ experiment is a liquid xenon time-projection chamber (TPC) searching for evidence of particle dark matter interactions. In the simplest assumption of elastic scattering, many dark matter models predict an energy spectrum which rises…
Instrumentation and Detectors · Physics
2025-09-23
J. Aalbers , D. S. Akerib , A. K. Al Musalhi , F. Alder , C. S. Amarasinghe , A. Ames , T. J. Anderson , N. Angelides , H. M. Araújo , J. E. Armstrong , M. Arthurs , A. Baker , S. Balashov , J. Bang , J. W. Bargemann , E. E. Barillier , K. Beattie , T. Benson , A. Bhatti , T. P. Biesiadzinski , H. J. Birch , E. Bishop , G. M. Blockinger , B. Boxer , C. A. J. Brew , P. Brás , S. Burdin , M. C. Carmona-Benitez , M. Carter , A. Chawla , H. Chen , Y. T. Chin , N. I. Chott , N. I. Chott , M. V. Converse , S. Contreras , R. Coronel , A. Cottle , G. Cox , D. Curran , C. E. Dahl , I. Darlington , S. Dave , A. David , J. Delgaudio , S. Dey , L. de Viveiros , L. Di Felice , C. Ding , J. E. Y. Dobson , E. Druszkiewicz , S. Dubey , C. L. Dunbar , S. R. Eriksen , A. Fan , N. M. Fearon , N. Fieldhouse , S. Fiorucci , H. Flaecher , E. D. Fraser , T. M. A. Fruth , R. J. Gaitskell , A. Geffre , J. Genovesi , C. Ghag , A. Ghosh , R. Gibbons , S. Gokhale , J. Green , M. G. D. van der Grinten , J. J. Haiston , C. R. Hall , T. Hall , S. Han , E. Hartigan-O'Connor , S. J. Haselschwardt , M. A. Hernandez , S. A. Hertel , G. J. Homenides , M. Horn , D. Q. Huang , D. Hunt , E. Jacquet , R. S. James , M. K. K , A. C. Kaboth , A. C. Kamaha , D. Khaitan , A. Khazov , J. Kim , Y. D. Kim , J. Kingston , R. Kirk , D. Kodroff , E. V. Korolkova , H. Kraus , S. Kravitz , L. Kreczko , V. A. Kudryavtsev , C. Lawes , D. S. Leonard , K. T. Lesko , C. Levy , J. Lin , A. Lindote , W. H. Lippincott , J. Long , M. I. Lopes , W. Lorenzon , C. Lu , S. Luitz , P. A. Majewski , A. Manalaysay , R. L. Mannino , C. Maupin , M. E. McCarthy , G. McDowell , D. N. McKinsey , J. McLaughlin , J. B. Mclaughlin , R. McMonigle , B. Mitra , E. Mizrachi , M. E. Monzani , E. Morrison , B. J. Mount , M. Murdy , A. St. J. Murphy , H. N. Nelson , F. Neves , A. Nguyen , C. L. O'Brien , I. Olcina , K. C. Oliver-Mallory , J. Orpwood , K. Y Oyulmaz , K. J. Palladino , J. Palmer , N. J. Pannifer , N. Parveen , S. J. Patton , B. Penning , G. Pereira , E. Perry , T. Pershing , A. Piepke , Y. Qie , J. Reichenbacher , C. A. Rhyne , G. R. C. Rischbieter , E. Ritchey , H. S. Riyat , R. Rosero , T. Rushton , D. Rynders , D. Santone , A. B. M. R. Sazzad , R. W. Schnee , G. Sehr , B. Shafer , S. Shaw , K. Shi , T. Shutt , J. J. Silk , C. Silva , G. Sinev , J. Siniscalco , A. M. Slivar , R. Smith , V. N. Solovov , P. Sorensen , J. Soria , I. Stancu , A. Stevens , T. J. Sumner , A. Swain , M. Szydagis , D. R. Tiedt , M. Timalsina , Z. Tong , D. R. Tovey , J. Tranter , M. Trask , M. Tripathi , K. Trengrove , A. Usón , A. C. Vaitkus , O. Valentino , V. Velan , A. Wang , J. J. Wang , Y. Wang , L. Weeldreyer , T. J. Whitis , K. Wild , M. Williams , W. J. Wisniewski , L. Wolf , F. L. H. Wolfs , S. Woodford , D. Woodward , C. J. Wright , Q. Xia , J. Xu , Y. Xu , M. Yeh , D. Yeum , W. Zha , H. Zhang , T. Zhang
Future large liquid-scintillator detectors can be implemented to observe neutrinos from a core-collapse supernova (SN) in our galaxy in various reaction channels: (1) The inverse beta decay $\overline{\nu}^{}_e + p \to n + e^+$; (2) The…
It has been known that neutrinos from supernova (SN) bursts can give rise to nuclear recoil (NR) signals arising from coherent elastic neutrino-nucleus scattering (CE$\nu$NS) interaction, a neutral current (NC) process, of the neutrinos…
High Energy Physics - Phenomenology · Physics
2022-08-01
Pijushpani Bhattacharjee , Abhijit Bandyopadhyay , Sovan Chakraborty , Sayan Ghosh , Kamales Kar , Satyajit Saha
Possibility to use ultra pure liquid Xenon as a low energy solar neutrino detector by means of $\nu$+e scatterings is evaluated. A possible detector with 10 tons of fiducial volume will give $\sim$14 events for pp-neutrinos and $\sim$6…
The large-volume liquid-scintillator detector LENA (Low Energy Neutrino Astronomy) will provide high-grade background discrimination and enable the detection of diffuse supernova neutrinos (DSN) in an almost background-free energy window…
Astrophysics · Physics
2008-11-26
M. Wurm , F. von Feilitzsch , M. Goeger-Neff , K. A. Hochmuth , T. Marrodan Undagoitia , L. Oberauer , W. Potzel
We have developed a neutrino detector with threshold energies from ~0.115 to 105 MeV in a clean detection mode almost completely void of accidental backgrounds. It was initially developed for the NASA $\nu$SOL project to put a solar…
Instrumentation and Detectors · Physics
2024-11-20
Nickolas Solomey , Mark Christl , Brian Doty , Jonathan Folkerts , Brooks Hartsock , Evgen Kuznetsco , Robert McTaggart , Holger Meyer , Tyler Nolan , Greg Pawloski , Daniel Reichart , Miguel Rodriguez-Otero , Dan Smith , Lisa Solomey
Low-energy neutrinos are clean messengers from supernovae explosions and probably carry unique insights into the process of stellar evolution. We estimate the expected number of events considering coherent elastic scattering of neutrinos…
High Energy Physics - Phenomenology · Physics
2020-12-22
Ana Luisa Foguel , Eduardo Souza Fraga , Carla Bonifazi
Development of large mass detectors for low-energy neutrinos and dark matter may allow supernova detection via neutrino-nucleus elastic scattering. An elastic-scattering detector could observe a few, or more, events per ton for a galactic…
Large-scale organic liquid scintillator detectors are highly efficient in the detection of MeV-scale electron antineutrinos. These signal events can be detected through inverse beta decay on protons, which produce a positron accompanied by…
Instrumentation and Detectors · Physics
2025-05-05
JUNO Collaboration , Thomas Adam , Kai Adamowicz , Shakeel Ahmad , Rizwan Ahmed , Sebastiano Aiello , Fengpeng An , Costas Andreopoulos , Giuseppe Andronico , Nikolay Anfimov , Vito Antonelli , Tatiana Antoshkina , João Pedro Athayde Marcondes de André , Didier Auguste , Weidong Bai , Nikita Balashov , Andrea Barresi , Davide Basilico , Eric Baussan , Marco Beretta , Antonio Bergnoli , Nikita Bessonov , Daniel Bick , Lukas Bieger , Svetlana Biktemerova , Thilo Birkenfeld , Simon Blyth , Anastasia Bolshakova , Mathieu Bongrand , Matteo Borghesi , Dominique Breton , Augusto Brigatti , Riccardo Brugnera , Riccardo Bruno , Marcel Büchner , Antonio Budano , Jose Busto , Anatael Cabrera , Barbara Caccianiga , Hao Cai , Xiao Cai , Yanke Cai , Zhiyan Cai , Stéphane Callier , Steven Calvez , Antonio Cammi , Chuanya Cao , Guofu Cao , Jun Cao , Yaoqi Cao , Rossella Caruso , Cédric Cerna , Vanessa Cerrone , Jinfan Chang , Yun Chang , Auttakit Chatrabhuti , Chao Chen , Guoming Chen , Jiahui Chen , Jian Chen , Jing Chen , Junyou Chen , Pingping Chen , Shaomin Chen , Shiqiang Chen , Xin Chen , Yiming Chen , Yixue Chen , Yu Chen , Ze Chen , Zhangming Chen , Zhiyuan Chen , Jie Cheng , Yaping Cheng , Yu Chin Cheng , Alexander Chepurnov , Alexey Chetverikov , Davide Chiesa , Pietro Chimenti , Po-Lin Chou , Ziliang Chu , Artem Chukanov , Gérard Claverie , Catia Clementi , Barbara Clerbaux , Claudio Coletta , Selma Conforti Di Lorenzo , Simon Csakli , Chenyang Cui , Olivia Dalager , Christophe De La Taille , Zhi Deng , Ziyan Deng , Xiaoyu Ding , Xuefeng Ding , Yayun Ding , Bayu Dirgantara , Carsten Dittrich , Sergey Dmitrievsky , David Doerflinger , Dmitry Dolzhikov , Haojie Dong , Jianmeng Dong , Evgeny Doroshkevich , Marcos Dracos , Frédéric Druillole , Ran Du , Shuxian Du , Yujie Duan , Katherine Dugas , Stefano Dusini , Hongyue Duyang , Jessica Eck , Timo Enqvist , Andrea Fabbri , Ulrike Fahrendholz , Lei Fan , Jian Fang , Wenxing Fang , Dmitry Fedoseev , Li-Cheng Feng , Qichun Feng , Federico Ferraro , Daniela Fetzer , Marcellin Fotzé , Amélie Fournier , Aaron Freegard , Feng Gao , Alberto Garfagnini , Arsenii Gavrikov , Marco Giammarchi , Nunzio Giudice , Maxim Gonchar , Guanghua Gong , Hui Gong , Yuri Gornushkin , Marco Grassi , Maxim Gromov , Vasily Gromov , Minghao Gu , Xiaofei Gu , Yu Gu , Mengyun Guan , Yuduo Guan , Nunzio Guardone , Rosa Maria Guizzetti , Cong Guo , Wanlei Guo , Caren Hagner , Hechong Han , Ran Han , Yang Han , Jinhong He , Miao He , Wei He , Xinhai He , Ziou He , Tobias Heinz , Patrick Hellmuth , Yuekun Heng , YuenKeung Hor , Shaojing Hou , Yee Hsiung , Bei-Zhen Hu , Hang Hu , Jun Hu , Tao Hu , Yuxiang Hu , Guihong Huang , Jinhao Huang , Junting Huang , Kaixuan Huang , Shengheng Huang , Tao Huang , Xin Huang , Xingtao Huang , Yongbo Huang , Jiaqi Hui , Lei Huo , Cédric Huss , Safeer Hussain , Leonard Imbert , Ara Ioannisian , Adrienne Jacobi , Arshak Jafar , Beatrice Jelmini , Xiangpan Ji , Xiaolu Ji , Huihui Jia , Junji Jia , Cailian Jiang , Wei Jiang , Xiaoshan Jiang , Xiaozhao Jiang , Yijian Jiang , Yixuan Jiang , Xiaoping Jing , Cécile Jollet , Li Kang , Rebin Karaparabil , Narine Kazarian , Ali Khan , Amina Khatun , Khanchai Khosonthongkee , Denis Korablev , Konstantin Kouzakov , Alexey Krasnoperov , Sergey Kuleshov , Sindhujha Kumaran , Nikolay Kutovskiy , Loïc Labit , Tobias Lachenmaier , Haojing Lai , Cecilia Landini , Sébastien Leblanc , Matthieu Lecocq , Frederic Lefevre , Ruiting Lei , Rupert Leitner , Jason Leung , Demin Li , Fei Li , Fule Li , Gaosong Li , Hongjian Li , Huang Li , Jiajun Li , Min Li , Nan Li , Qingjiang Li , Ruhui Li , Rui Li , Shanfeng Li , Tao Li , Teng Li , Weidong Li , Xiaonan Li , Yi Li , Yichen Li , Yifan Li , Yufeng Li , Zhaohan Li , Zhibing Li , Zi-Ming Li , Zonghai Li , An-An Liang , Jiajun Liao , Minghua Liao , Yilin Liao , Ayut Limphirat , Bo-Chun Lin , Guey-Lin Lin , Shengxin Lin , Tao Lin , Xianhao Lin , Xingyi Lin , Jiajie Ling , Xin Ling , Ivano Lippi , Caimei Liu , Fang Liu , Fengcheng Liu , Haidong Liu , Haotian Liu , Hongbang Liu , Hongjuan Liu , Hongtao Liu , Hongyang Liu , Jianglai Liu , Jiaxi Liu , Jinchang Liu , Kainan Liu , Min Liu , Qian Liu , Runxuan Liu , Shenghui Liu , Shulin Liu , Xiaowei Liu , Xiwen Liu , Xuewei Liu , Yankai Liu , Zhen Liu , Lorenzo Loi , Alexey Lokhov , Paolo Lombardi , Claudio Lombardo , Kai Loo , Haoqi Lu , Junguang Lu , Meishu Lu , Peizhi Lu , Shuxiang Lu , Xianguo Lu , Bayarto Lubsandorzhiev , Sultim Lubsandorzhiev , Livia Ludhova , Arslan Lukanov , Fengjiao Luo , Guang Luo , Jianyi Luo , Shu Luo , Wuming Luo , Xiaojie Luo , Vladimir Lyashuk , Bangzheng Ma , Bing Ma , Qiumei Ma , Si Ma , Wing Yan Ma , Xiaoyan Ma , Xubo Ma , Jihane Maalmi , Jingyu Mai , Marco Malabarba , Yury Malyshkin , Roberto Carlos Mandujano , Fabio Mantovani , Xin Mao , Stefano M. 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The next Galactic core-collapse supernova (SN) is a highly anticipated observational target for neutrino telescopes. However, even prior to collapse, massive dying stars shine copiously in "pre-supernova" (pre-SN) neutrinos, which can…
High Energy Physics - Phenomenology · Physics
2020-02-21
Nirmal Raj , Volodymyr Takhistov , Samuel J. Witte
Neutrinos produced in the hot and dense interior of the next galactic supernova would be visible at dark matter experiments in coherent elastic nuclear recoils. While studies on this channel have focused on successful core-collapse…
LENA (Low Energy Neutrino Astronomy) has been proposed as a next generation 50 kt liquid scintillator detector. Its large target mass allows to search for the Diffuse Supernova Neutrino Background (DSNB), which was generated by the…
Instrumentation and Methods for Astrophysics · Physics
2015-06-22
Randolph Möllenberg , Franz von Feilitzsch , Dominikus Hellgartner , Lothar Oberauer , Marc Tippmann , Jürgen Winter , Michael Wurm , Vincenz Zimmer
Thermal MeV neutrino emission from core-collapse supernovae offers a unique opportunity to probe physics beyond the Standard Model in the neutrino sector. The next generation of neutrino experiments, such as DUNE and Hyper-Kamiokande, can…
High Energy Physics - Phenomenology · Physics
2023-04-20
Jose Alonso Carpio , Ali Kheirandish , Kohta Murase
Electron-neutrino charged-current interactions with xenon nuclei were modeled in the nEXO neutrinoless double-$\beta$ decay detector (~5 metric ton, 90% ${}^{136}$Xe, 10% ${}^{134}$Xe) to evaluate its sensitivity to supernova neutrinos.…
High Energy Physics - Phenomenology · Physics
2024-12-02
nEXO Collaboration , S. Hedges , S. Al Kharusi , E. Angelico , J. P. Brodsky , G. Richardson , S. Wilde , A. Amy , A. Anker , I. J. Arnquist , P. Arsenault , A. Atencio , I. Badhrees , J. Bane , V. Belov , E. P. Bernard , T. Bhatta , A. Bolotnikov , J. Breslin , P. A. Breur , E. Brown , T. Brunner , E. Caden , G. F. Cao , L. Q. Cao , D. Cesmecioglu , E. Chambers , B. Chana , S. A. Charlebois , D. Chernyak , M. Chiu , R. Collister , M. Cvitan , J. Dalmasson , T. Daniels , L. Darroch , R. DeVoe , M. L. di Vacri , Y. Y. Ding , M. J. Dolinski , B. Eckert , M. Elbeltagi , R. Elmansali , L. Fabris , W. Fairbank , J. Farine , N. Fatemighomi , B. Foust , Y. S. Fu , D. Gallacher , N. Gallice , W. Gillis , D. Goeldi , A. Gorham , R. Gornea , G. Gratta , Y. D. Guan , C. A. Hardy , M. Heffner , E. Hein , J. D. Holt , E. W. Hoppe , A. House , W. Hunt , A. Iverson , P. Kachru , A. Karelin , D. Keblbeck , A. Kuchenkov , K. S. Kumar , A. Larson , M. B. Latif , K. G. Leach , B. G. Lenardo , D. S. Leonard , H. Lewis , G. Li , Z. Li , C. Licciardi , R. Lindsay , R. MacLellan , S. Majidi , C. Malbrunot , P. Martel-Dion , J. Masbou , K. McMichael , M. Medina-Peregrina , B. Mong , D. C. Moore , J. Nattress , C. R. Natzke , X. E. Ngwadla , K. Ni , A. Nolan , S. C. Nowicki , J. C. Nzobadila Ondze , J. L. Orrell , G. S. Ortega , C. T. Overman , L. Pagani , H. Peltz Smalley , A. Peña-Perez , A. Perna , A. Piepke , T. Pinto Franco , A. Pocar , J. -F. Pratte , H. Rasiwala , D. Ray , K. Raymond , S. Rescia , V. Riot , R. Ross , R. Saldanha , S. Sangiorgio , S. Schwartz , S. Sekula , J. Soderstrom , A. K. Soma , F. Spadoni , X. L. Sun , S. Thibado , A. Tidball , T. Totev , S. Triambak , R. H. M. Tsang , O. A. Tyuka , E. van Bruggen , M. Vidal , S. Viel , M. Walent , Q. D. Wang , W. Wang , Y. G. Wang , M. Watts , M. Wehrfritz , W. Wei , L. J. Wen , U. Wichoski , X. M. Wu , H. Xu , H. B. Yang , L. Yang , M. Yu , M. Yvaine , O. Zeldovich , J. Zhao
Detection of supernova relic neutrinos could provide key support for our current understanding of stellar and cosmological evolution, and precise measurements of these neutrinos could yield novel insights into the universe. In this paper,…
The coherent elastic neutrino-nucleus scattering (CEvNS) plays a crucial role at the final evolution of stars. The detection of it would be of importance in astroparticle physics. Among all available neutrino sources, galactic supernovae…
We present searches for light dark matter (DM) with masses 3-9 GeV/$c^2$ in the presence of coherent elastic neutrino-nucleus scattering (CE$\nu$NS) from $^{8}$B solar neutrinos with the LUX-ZEPLIN experiment. This analysis uses a 5.7…
High Energy Physics - Experiment · Physics
2025-12-24
D. S. Akerib , A. K. Al Musalhi , F. Alder , B. J. Almquist , C. S. Amarasinghe , A. Ames , T. J. Anderson , N. Angelides , H. M. Araújo , J. E. Armstrong , M. Arthurs , A. Baker , S. Balashov , J. Bang , J. W. Bargemann , E. E. Barillier , D. Bauer , K. Beattie , A. Bhatti , T. P. Biesiadzinski , H. J. Birch , E. Bishop , G. M. Blockinger , C. A. J. Brew , P. Brás , S. Burdin , M. C. Carmona-Benitez , M. Carter , A. Chawla , H. Chen , Y. T. Chin , N. I. Chott , S. Contreras , M. V. Converse , R. Coronel , A. Cottle , G. Cox , D. Curran , C. E. Dahl , I. Darlington , S. Dave , A. David , J. Delgaudio , S. Dey , L. de Viveiros , L. Di Felice , C. Ding , J. E. Y. Dobson , E. Druszkiewicz , S. Dubey , C. L. Dunbar , S. R. Eriksen , S. Fayer , N. M. Fearon , N. Fieldhouse , S. Fiorucci , H. Flaecher , E. D. Fraser , T. M. A. Fruth , P. W. Gaemers , R. J. Gaitskell , A. Geffre , J. Genovesi , C. Ghag , J. Ghamsari , A. Ghosh , S. Ghosh , R. Gibbons , S. Gokhale , J. Green , M. G. D. van der Grinten , J. J. Haiston , C. R. Hall , T. Hall , R. H Hampp , S. J. Haselschwardt , M. A. Hernandez , S. A. Hertel , G. J. Homenides , M. Horn , D. Q. Huang , D. Hunt , E. Jacquet , R. S. James , K. Jenkins , A. C. Kaboth , A. C. Kamaha , M. K. Kannichankandy , D. Khaitan , A. Khazov , J. Kim , Y. D. Kim , D. Kodroff , E. V. Korolkova , H. Kraus , S. Kravitz , L. Kreczko , V. A. Kudryavtsev , C. Lawes , D. S. Leonard , K. T. Lesko , C. Levy , J. Lin , A. Lindote , W. H. Lippincott , J. Long , M. I. Lopes , W. Lorenzon , C. Lu , S. Luitz , W. Ma , V. Mahajan , P. A. Majewski , A. Manalaysay , R. L. Mannino , R. J. Matheson , C. Maupin , M. E. McCarthy , D. N. McKinsey , J. McLaughlin , J. B. McLaughlin , R. McMonigle , B. Mitra , E. Mizrachi , M. E. Monzani , K. Morå , E. Morrison , B. J. Mount , M. Murdy , A. St. J. Murphy , H. N. Nelson , F. Neves , A. Nguyen , C. L. O'Brien , F. H. O'Shea , I. Olcina , K. C. Oliver-Mallory , J. Orpwood , K. Y Oyulmaz , K. J. Palladino , N. J. Pannifer , N. Parveen , S. J. Patton , B. Penning , G. Pereira , E. Perry , T. Pershing , A. Piepke , S. S. Poudel , Y. Qie , J. Reichenbacher , C. A. Rhyne , G. R. C. Rischbieter , E. Ritchey , H. S. Riyat , R. Rosero , N. J. Rowe , T. Rushton , D. Rynders , S. Saltão , D. Santone , I. Sargeant , A. B. M. R. Sazzad , R. W. Schnee , G. Sehr , B. Shafer , S. Shaw , W. Sherman , K. Shi , T. Shutt , C. Silva , G. Sinev , J. Siniscalco , A. M. Slivar , R. Smith , V. N. Solovov , P. Sorensen , J. Soria , T. J. Sumner , A. Swain , M. Szydagis , D. R. Tiedt , M. Timalsina , D. R. Tovey , J. Tranter , M. Trask , K. Trengove , M. Tripathi , A. Usón , A. C. Vaitkus , O. Valentino , V. Velan , A. Wang , J. J. Wang , Y. Wang , L. Weeldreyer , T. J. Whitis , K. Wild , M. Williams , J. Winnicki , L. Wolf , F. L. H. Wolfs , S. Woodford , D. Woodward , C. J. Wright , Q. Xia , J. Xu , Y. Xu , M. Yeh , D. Yeum , J. Young , W. Zha , H. Zhang , T. Zhang , Y. Zhou
The next galactic core-collapse supernova will deliver a wealth of neutrinos which for the first time we are well-situated to measure. These explosions produce neutrinos with energies between 10 and 100 MeV over a period of tens of seconds.…
Instrumentation and Methods for Astrophysics · Physics
2017-10-03
Justin A. Vasel , Andrey Sheshukov , Alec Habig
We have simulated the response of a high energy neutrino telescope to the stream of low energy neutrinos produced by a supernova. The nominal threshold of such detectors is in the GeV energy range. The passage of a large flux of MeV…