Related papers: Mimicking diffuse supernova antineutrinos with the…

The Diffuse Supernova Neutrino Background

The Diffuse Supernova Neutrino Background (DSNB) is the weak glow of MeV neutrinos and antineutrinos from distant core-collapse supernovae. The DSNB has not been detected yet, but the Super-Kamiokande (SK) 2003 upper limit on the electron…

High Energy Astrophysical Phenomena · Physics 2011-02-18 John F. Beacom

The diffuse supernova neutrino background as a probe of late-time neutrino mass generation

The relic neutrinos from old supernova explosions are among the most ancient neutrino fluxes within experimental reach. Thus, the diffuse supernova neutrino background (DSNB) could teach us if neutrino masses were different in the past…

High Energy Physics - Phenomenology · Physics 2022-12-07 André de Gouvêa , Ivan Martinez-Soler , Yuber F. Perez-Gonzalez , Manibrata Sen

A Search for Neutrinos from the Solar hep Reaction and the Diffuse Supernova Neutrino Background with the Sudbury Neutrino Observatory

A search has been made for neutrinos from the hep reaction in the Sun and from the diffuse supernova neutrino background (DSNB) using data collected during the first operational phase of the Sudbury Neutrino Observatory, with an exposure of…

High Energy Physics - Experiment · Physics 2012-08-27 The SNO Collaboration

The Unknowns of the Diffuse Supernova Neutrino Background Hinder New Physics Searches

Neutrinos traveling over cosmic distances are ideal probes of new physics. We leverage on the approaching detection of the diffuse supernova neutrino background (DSNB) to explore whether, if the DSNB showed departures from theoretical…

High Energy Astrophysical Phenomena · Physics 2025-01-03 Miller MacDonald , Pablo Martínez-Miravé , Irene Tamborra

The Diffuse Supernova Neutrino Background

The Diffuse Supernova Neutrino Background (DSNB) in the MeV regime represents the cumulative cosmic neutrino emission, predominantly due to core collapse supernovae. We estimate the DSNB flux for different Star Formation Rate Density (SFRD)…

High Energy Astrophysical Phenomena · Physics 2020-01-22 Samalka Anandagoda , Dieter H. Hartmann , Marco Ajello , Abhishek Desai

Diffuse neutrinos from luminous and dark supernovae: prospects for upcoming detectors at the O(10) kt scale

We estimate the Diffuse Supernova Neutrino Background (DSNB) using the simulation results for neutron star-forming and black hole-forming stellar collapses from the Garching group. Scenarios with different distributions of black-hole…

High Energy Astrophysical Phenomena · Physics 2017-11-27 Alankrita Priya , Cecilia Lunardini

Detecting the Diffuse Supernova Neutrino Background with LENA

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

Diffuse supernova neutrinos at underground laboratories

I review the physics of the Diffuse Supernova Neutrino flux (or Background, DSNB), in the context of future searches at the next generation of neutrino observatories. The theory of the DSNB is discussed in its fundamental elements, namely…

Cosmology and Nongalactic Astrophysics · Physics 2016-05-24 Cecilia Lunardini

Neutrino nonradiative decay and the diffuse supernova neutrino background

The diffuse supernova neutrino background (DSNB) is the constant flux of neutrinos and antineutrinos emitted by all past core collapses in the observable Universe. We study the potential to extract information on the neutrino lifetime from…

High Energy Physics - Phenomenology · Physics 2024-01-29 Pilar Iváñez-Ballesteros , M. Cristina Volpe

Diffuse supernova neutrino background with up-to-date star formation rate measurements and long-term multidimensional supernova simulations

The sensitivity of current and future neutrino detectors like Super-Kamiokande (SK), JUNO, Hyper-Kamiokande (HK), and DUNE is expected to allow for the detection of the diffuse supernova neutrino background (DSNB). However, the DSNB model…

High Energy Astrophysical Phenomena · Physics 2024-11-15 Nick Ekanger , Shunsaku Horiuchi , Hiroki Nagakura , Samantha Reitz

Search for $hep$ solar neutrinos and the diffuse supernova neutrino background using all three phases of the Sudbury Neutrino Observatory

A search has been performed for neutrinos from two sources, the $hep$ reaction in the solar $pp$ fusion chain and the $\nu_e$ component of the diffuse supernova neutrino background (DSNB), using the full dataset of the Sudbury Neutrino…

High Energy Physics - Experiment · Physics 2020-11-16 B. Aharmim , S. N. Ahmed , A. E. Anthony , N. Barros , E. W. Beier , A. Bellerive , B. Beltran , M. Bergevin , S. D. Biller , E. Blucher , R. Bonventre , K. Boudjemline , M. G. Boulay , B. Cai , E. J. Callaghan , J. Caravaca , Y. D. Chan , D. Chauhan , M. Chen , B. T. Cleveland , G. A. Cox , X. Dai , H. Deng , F. B. Descamps , J. A. Detwiler , P. J. Doe , G. Doucas , P. -L. Drouin , M. Dunford , S. R. Elliott , H. C. Evans , G. T. Ewan , J. Farine , H. Fergani , F. Fleurot , R. J. Ford , J. A. Formaggio , N. Gagnon , K. Gilje , J. TM. Goon , K. Graham , E. Guillian , S. Habib , R. L. Hahn , A. L. Hallin , E. D. Hallman , P. J. Harvey , R. Hazama , W. J. Heintzelman , J. Heise , R. L. Helmer , A. Hime , C. Howard , M. Huang , P. Jagam , B. Jamieson , N. A. Jelley , M. Jerkins , K. J. Keeter , J. R. Klein , L. L. Kormos , M. Kos , C. Kraus , C. B. Krauss , A. Krüger , T. Kutter , C. C. M. Kyba , K. Labe , B. J. Land , R. Lange , A. LaTorre , J. Law , I. T. Lawson , K. T. Lesko , J. R. Leslie , I. Levine , J. C. Loach , R. MacLellan , S. Majerus , H. B. Mak , J. Maneira , R. D. Martin , A. Mastbaum , N. McCauley , A. B. McDonald , S. R. McGee , M. L. Miller , B. Monreal , J. Monroe , B. G. Nickel , A. J. Noble , H. M. O'Keeffe , N. S. Oblath , C. E. Okada , R. W. Ollerhead , G. D. Orebi Gann , S. M. Oser , R. A. Ott , S. J. M. Peeters , A. W. P. Poon , G. Prior , S. D. Reitzner , K. Rielage , B. C. Robertson , R. G. H. Robertson , M. H. Schwendener , J. A. Secrest , S. R. Seibert , O. Simard , D. Sinclair , P. Skensved , T. J. Sonley , L. C. Stonehill , G. Tešić , N. Tolich , T. Tsui , R. Van Berg , B. A. VanDevender , C. J. Virtue , B. L. Wall , D. Waller , H. Wan Chan Tseung , D. L. Wark , J. Wendland , N. West , J. F. Wilkerson , J. R. Wilson , T. Winchester , A. Wright , M. Yeh , F. Zhang , K. Zuber

Prospects for Detecting the Diffuse Supernova Neutrino Background with JUNO

We present the detection potential for the diffuse supernova neutrino background (DSNB) at the Jiangmen Underground Neutrino Observatory (JUNO), using the inverse-beta-decay (IBD) detection channel on free protons. We employ the latest…

High Energy Physics - Experiment · Physics 2022-10-14 JUNO Collaboration , Angel Abusleme , Thomas Adam , Shakeel Ahmad , Rizwan Ahmed , Sebastiano Aiello , Muhammad Akram , Fengpeng An , Qi An , Giuseppe Andronico , Nikolay Anfimov , Vito Antonelli , Tatiana Antoshkina , Burin Asavapibhop , João Pedro Athayde Marcondes de André , Didier Auguste , Nikita Balashov , Wander Baldini , Andrea Barresi , Davide Basilico , Eric Baussan , Marco Bellato , Antonio Bergnoli , Thilo Birkenfeld , Sylvie Blin , David Blum , Simon Blyth , Anastasia Bolshakova , Mathieu Bongrand , Clément Bordereau , Dominique Breton , Augusto Brigatti , Riccardo Brugnera , Riccardo Bruno , Antonio Budano , Mario Buscemi , Jose Busto , Ilya Butorov , Anatael Cabrera , Barbara Caccianiga , Hao Cai , Xiao Cai , Yanke Cai , Zhiyan Cai , Riccardo Callegari , Antonio Cammi , Agustin Campeny , Chuanya Cao , Guofu Cao , Jun Cao , Rossella Caruso , Cédric Cerna , Jinfan Chang , Yun Chang , Pingping Chen , Po-An Chen , Shaomin Chen , Xurong Chen , Yi-Wen Chen , Yixue Chen , Yu Chen , Zhang Chen , Jie Cheng , Yaping Cheng , Alexey Chetverikov , Davide Chiesa , Pietro Chimenti , Artem Chukanov , Gérard Claverie , Catia Clementi , Barbara Clerbaux , Selma Conforti Di Lorenzo , Daniele Corti , Flavio Dal Corso , Olivia Dalager , Christophe De La Taille , Zhi Deng , Ziyan Deng , Wilfried Depnering , Marco Diaz , Xuefeng Ding , Yayun Ding , Bayu Dirgantara , Sergey Dmitrievsky , Tadeas Dohnal , Dmitry Dolzhikov , Georgy Donchenko , Jianmeng Dong , Evgeny Doroshkevich , Marcos Dracos , Frédéric Druillole , Ran Du , Shuxian Du , Stefano Dusini , Martin Dvorak , Timo Enqvist , Heike Enzmann , Andrea Fabbri , Donghua Fan , Lei Fan , Jian Fang , Wenxing Fang , Marco Fargetta , Dmitry Fedoseev , Li-Cheng Feng , Qichun Feng , Richard Ford , Amélie Fournier , Haonan Gan , Feng Gao , Alberto Garfagnini , Arsenii Gavrikov , Marco Giammarchi , Agnese Giaz , Nunzio Giudice , Maxim Gonchar , Guanghua Gong , Hui Gong , Yuri Gornushkin , Alexandre Göttel , Marco Grassi , Vasily Gromov , Minghao Gu , Xiaofei Gu , Yu Gu , Mengyun Guan , Nunzio Guardone , Maria Gul , Cong Guo , Jingyuan Guo , Wanlei Guo , Xinheng Guo , Yuhang Guo , Paul Hackspacher , Caren Hagner , Ran Han , Yang Han , Muhammad Sohaib Hassan , Miao He , Wei He , Tobias Heinz , Patrick Hellmuth , Yuekun Heng , Rafael Herrera , YuenKeung Hor , Shaojing Hou , Yee Hsiung , Bei-Zhen Hu , Hang Hu , Jianrun Hu , Jun Hu , Shouyang Hu , Tao Hu , Zhuojun Hu , Chunhao Huang , Guihong Huang , Hanxiong Huang , Wenhao Huang , Xin Huang , Xingtao Huang , Yongbo Huang , Jiaqi Hui , Lei Huo , Wenju Huo , Cédric Huss , Safeer Hussain , Ara Ioannisian , Roberto Isocrate , Beatrice Jelmini , Kuo-Lun Jen , Ignacio Jeria , Xiaolu Ji , Xingzhao Ji , Huihui Jia , Junji Jia , Siyu Jian , Di Jiang , Wei Jiang , Xiaoshan Jiang , Ruyi Jin , Xiaoping Jing , Cécile Jollet , Jari Joutsenvaara , Sirichok Jungthawan , Leonidas Kalousis , Philipp Kampmann , Li Kang , Rebin Karaparambil , Narine Kazarian , Amina Khatun , Khanchai Khosonthongkee , Denis Korablev , Konstantin Kouzakov , Alexey Krasnoperov , Nikolay Kutovskiy , Pasi Kuusiniemi , Tobias Lachenmaier , Cecilia Landini , Sébastien Leblanc , Victor Lebrin , Frederic Lefevre , Ruiting Lei , Rupert Leitner , Jason Leung , Demin Li , Fei Li , Fule Li , Gaosong Li , Haitao Li , Huiling Li , Jiaqi Li , Mengzhao Li , Min Li , Nan Li , Nan Li , Qingjiang Li , Ruhui Li , Shanfeng Li , Tao Li , Weidong Li , Weiguo Li , Xiaomei Li , Xiaonan Li , Xinglong Li , Yi Li , Yufeng Li , Zepeng Li , Zhaohan Li , Zhibing Li , Ziyuan Li , Hao Liang , Hao Liang , Jiajun Liao , Ayut Limphirat , Sukit Limpijumnong , Guey-Lin Lin , Shengxin Lin , Tao Lin , Jiajie Ling , Ivano Lippi , Fang Liu , Haidong Liu , Hongbang Liu , Hongjuan Liu , Hongtao Liu , Hui Liu , Jianglai Liu , Jinchang Liu , Min Liu , Qian Liu , Qin Liu , Runxuan Liu , Shuangyu Liu , Shubin Liu , Shulin Liu , Xiaowei Liu , Xiwen Liu , Yan Liu , Yunzhe Liu , Alexey Lokhov , Paolo Lombardi , Claudio Lombardo , Kai Loo , Chuan Lu , Haoqi Lu , Jingbin Lu , Junguang Lu , Shuxiang Lu , Xiaoxu Lu , Bayarto Lubsandorzhiev , Sultim Lubsandorzhiev , Livia Ludhova , Arslan Lukanov , Fengjiao Luo , Guang Luo , Pengwei Luo , Shu Luo , Wuming Luo , Xiaojie Luo , Vladimir Lyashuk , Bangzheng Ma , Qiumei Ma , Si Ma , Xiaoyan Ma , Xubo Ma , Jihane Maalmi , Yury Malyshkin , Roberto Carlos Mandujano , Fabio Mantovani , Francesco Manzali , Xin Mao , Yajun Mao , Stefano M. Mari , Filippo Marini , Sadia Marium , Cristina Martellini , Gisele Martin-Chassard , Agnese Martini , Matthias Mayer , Davit Mayilyan , Ints Mednieks , Yue Meng , Anselmo Meregaglia , Emanuela Meroni , David Meyhöfer , Mauro Mezzetto , Jonathan Miller , Lino Miramonti , Paolo Montini , Michele Montuschi , Axel Müller , Massimiliano Nastasi , Dmitry V. Naumov , Elena Naumova , Diana Navas-Nicolas , Igor Nemchenok , Minh Thuan Nguyen Thi , Feipeng Ning , Zhe Ning , Hiroshi Nunokawa , Lothar Oberauer , Juan Pedro Ochoa-Ricoux , Alexander Olshevskiy , Domizia Orestano , Fausto Ortica , Rainer Othegraven , Alessandro Paoloni , Sergio Parmeggiano , Yatian Pei , Nicomede Pelliccia , Anguo Peng , Haiping Peng , Frédéric Perrot , Pierre-Alexandre Petitjean , Fabrizio Petrucci , Oliver Pilarczyk , Luis Felipe Piñeres Rico , Artyom Popov , Pascal Poussot , Wathan Pratumwan , Ezio Previtali , Fazhi Qi , Ming Qi , Sen Qian , Xiaohui Qian , Zhen Qian , Hao Qiao , Zhonghua Qin , Shoukang Qiu , Muhammad Usman Rajput , Gioacchino Ranucci , Neill Raper , Alessandra Re , Henning Rebber , Abdel Rebii , Bin Ren , Jie Ren , Barbara Ricci , Mariam Rifai , Mathieu Roche , Narongkiat Rodphai , Aldo Romani , Bedřich Roskovec , Xiangdong Ruan , Xichao Ruan , Saroj Rujirawat , Arseniy Rybnikov , Andrey Sadovsky , Paolo Saggese , Simone Sanfilippo , Anut Sangka , Nuanwan Sanguansak , Utane Sawangwit , Julia Sawatzki , Fatma Sawy , Michaela Schever , Cédric Schwab , Konstantin Schweizer , Alexandr Selyunin , Andrea Serafini , Giulio Settanta , Mariangela Settimo , Zhuang Shao , Vladislav Sharov , Arina Shaydurova , Jingyan Shi , Yanan Shi , Vitaly Shutov , Andrey Sidorenkov , Fedor Šimkovic , Chiara Sirignano , Jaruchit Siripak , Monica Sisti , Maciej Slupecki , Mikhail Smirnov , Oleg Smirnov , Thiago Sogo-Bezerra , Sergey Sokolov , Julanan Songwadhana , Boonrucksar Soonthornthum , Albert Sotnikov , Ondřej Šrámek , Warintorn Sreethawong , Achim Stahl , Luca Stanco , Konstantin Stankevich , Dušan Štefánik , Hans Steiger , Hans Steiger , Jochen Steinmann , Tobias Sterr , Matthias Raphael Stock , Virginia Strati , Alexander Studenikin , Shifeng Sun , Xilei Sun , Yongjie Sun , Yongzhao Sun , Narumon Suwonjandee , Michal Szelezniak , Jian Tang , Qiang Tang , Quan Tang , Xiao Tang , Alexander Tietzsch , Igor Tkachev , Tomas Tmej , Marco Danilo Claudio Torri , Konstantin Treskov , Andrea Triossi , Giancarlo Troni , Wladyslaw Trzaska , Cristina Tuve , Nikita Ushakov , Guillaume Vanroyen , Vadim Vedin , Giuseppe Verde , Maxim Vialkov , Benoit Viaud , Cornelius Moritz Vollbrecht , Cristina Volpe , Vit Vorobel , Dmitriy Voronin , Lucia Votano , Pablo Walker , Caishen Wang , Chung-Hsiang Wang , En Wang , Guoli Wang , Jian Wang , Jun Wang , Kunyu Wang , Lu Wang , Meifen Wang , Meng Wang , Meng Wang , Ruiguang Wang , Siguang Wang , Wei Wang , Wei Wang , Wenshuai Wang , Xi Wang , Xiangyue Wang , Yangfu Wang , Yaoguang Wang , Yi Wang , Yi Wang , Yifang Wang , Yuanqing Wang , Yuman Wang , Zhe Wang , Zheng Wang , Zhimin Wang , Zongyi Wang , Muhammad Waqas , Apimook Watcharangkool , Lianghong Wei , Wei Wei , Wenlu Wei , Yadong Wei , Kaile Wen , Liangjian Wen , Christopher Wiebusch , Steven Chan-Fai Wong , Bjoern Wonsak , Diru Wu , Qun Wu , Zhi Wu , Michael Wurm , Jacques Wurtz , Christian Wysotzki , Yufei Xi , Dongmei Xia , Xiang Xiao , Xiaochuan Xie , Yuguang Xie , Zhangquan Xie , Zhizhong Xing , Benda Xu , Cheng Xu , Donglian Xu , Fanrong Xu , Hangkun Xu , Jilei Xu , Jing Xu , Meihang Xu , Yin Xu , Yu Xu , Baojun Yan , Taylor Yan , Wenqi Yan , Xiongbo Yan , Yupeng Yan , Anbo Yang , Changgen Yang , Chengfeng Yang , Huan Yang , Jie Yang , Lei Yang , Xiaoyu Yang , Yifan Yang , Yifan Yang , Haifeng Yao , Zafar Yasin , Jiaxuan Ye , Mei Ye , Ziping Ye , Frédéric Yermia , Peihuai Yi , Na Yin , Xiangwei Yin , Zhengyun You , Boxiang Yu , Chiye Yu , Chunxu Yu , Hongzhao Yu , Miao Yu , Xianghui Yu , Zeyuan Yu , Zezhong Yu , Chengzhuo Yuan , Ying Yuan , Zhenxiong Yuan , Baobiao Yue , Noman Zafar , Vitalii Zavadskyi , Shan Zeng , Tingxuan Zeng , Yuda Zeng , Liang Zhan , Aiqiang Zhang , Feiyang Zhang , Guoqing Zhang , Haiqiong Zhang , Honghao Zhang , Jialiang Zhang , Jiawen Zhang , Jie Zhang , Jin Zhang , Jingbo Zhang , Jinnan Zhang , Peng Zhang , Qingmin Zhang , Shiqi Zhang , Shu Zhang , Tao Zhang , Xiaomei Zhang , Xin Zhang , Xuantong Zhang , Xueyao Zhang , Yan Zhang , Yinhong Zhang , Yiyu Zhang , Yongpeng Zhang , Yu Zhang , Yuanyuan Zhang , Yumei Zhang , Zhenyu Zhang , Zhijian Zhang , Fengyi Zhao , Jie Zhao , Rong Zhao , Shujun Zhao , Tianchi Zhao , Dongqin Zheng , Hua Zheng , Yangheng Zheng , Weirong Zhong , Jing Zhou , Li Zhou , Nan Zhou , Shun Zhou , Tong Zhou , Xiang Zhou , Jiang Zhu , Kangfu Zhu , Kejun Zhu , Zhihang Zhu , Bo Zhuang , Honglin Zhuang , Liang Zong , Jiaheng Zou

Fundamental physics with the diffuse supernova background neutrinos

The Universe is awash with tens-of-MeV neutrinos of all species coming from all past core-collapse supernovae. These have never been observed, but this state of affairs will change in the near future. In the less than ten years, the…

High Energy Physics - Phenomenology · Physics 2021-01-04 André de Gouvêa , Ivan Martinez-Soler , Yuber F. Perez-Gonzalez , Manibrata Sen

First Detailed Calculation of Atmospheric Neutrino Foregrounds to the Diffuse Supernova Neutrino Background in Super-Kamiokande

The Diffuse Supernova Neutrino Background (DSNB) -- a probe of the core-collapse mechanism and the cosmic star-formation history -- has not been detected, but its discovery may be imminent. A significant obstacle for DSNB detection in…

High Energy Physics - Phenomenology · Physics 2024-05-07 Bei Zhou , John F. Beacom

The Diffuse Supernova Neutrino Background is detectable in Super-Kamiokande

The Diffuse Supernova Neutrino Background (DSNB) provides an immediate opportunity to study the emission of MeV thermal neutrinos from core-collapse supernovae. The DSNB is a powerful probe of stellar and neutrino physics, provided that the…

Astrophysics · Physics 2009-05-01 Shunsaku Horiuchi , John F. Beacom , Eli Dwek

Synoptic Sky Surveys and the Diffuse Supernova Neutrino Background: Removing Astrophysical Uncertainties and Revealing Invisible Supernovae

The cumulative (anti)neutrino production from all core-collapse supernovae within our cosmic horizon gives rise to the diffuse supernova neutrino background (DSNB), which is on the verge of detectability. The observed flux depends on…

Cosmology and Nongalactic Astrophysics · Physics 2010-11-26 Amy Lien , Brian D. Fields , John F. Beacom

Diffuse neutrino background from past core-collapse supernovae

Core-collapse supernovae are among the most powerful explosions in the universe, emitting thermal neutrinos that carry away the majority of the gravitational binding energy released. These neutrinos create a diffuse supernova neutrino…

High Energy Astrophysical Phenomena · Physics 2025-10-09 Shin'ichiro Ando , Nick Ekanger , Shunsaku Horiuchi , Yusuke Koshio

The diffuse neutrino flux from supernovae: upper limit on the electron neutrino component from the non-observation of antineutrinos at SuperKamiokande

I derive an upper bound on the electron neutrino component of the diffuse supernova neutrino flux from the constraint on the antineutrino component at SuperKamiokande. The connection between antineutrino and neutrino channels is due to the…

High Energy Physics - Phenomenology · Physics 2009-11-11 Cecilia Lunardini

Diffuse Supernova Neutrino Background Search at Super-Kamiokande

A new search for the diffuse supernova neutrino background (DSNB) flux has been conducted at Super-Kamiokande (SK), with a $22.5\times2970$-kton$\cdot$day exposure from its fourth operational phase IV. The new analysis improves on the…

High Energy Astrophysical Phenomena · Physics 2021-12-20 Kamiokande Collaboration , K. Abe , C. Bronner , Y. Hayato , K. Hiraide , M. Ikeda , S. Imaizumi , J. Kameda , Y. Kanemura , Y. Kataoka , S. Miki , M. Miura , S. Moriyama , Y. Nagao , M. Nakahata , S. Nakayama , T. Okada , K. Okamoto , A. Orii , G. Pronost , H. Sekiya , M. Shiozawa , Y. Sonoda , Y. Suzuki , A. Takeda , Y. Takemoto , A. Takenaka , H. Tanaka , S. Watanabe , T. Yano , S. Han , T. Kajita , K. Okumura , T. Tashiro , J. Xia , G. D. Megias , D. Bravo-Bergu , L. Labarga , Ll. Marti , B. Zaldivar , B. W. Pointon , F. d. M. Blaszczyk , E. Kearns , J. L. Raaf , J. L. Stone , L. Wan , T. Wester , J. Bian , N. J. Griskevich , W. R. Kropp , S. Locke , S. Mine , M. B. Smy , H. W. Sobel , V. Takhistov , J. Hill , J. Y. Kim , I. T. Lim , R. G. Park , B. Bodur , K. Scholberg , C. W. Walter , S. Cao , L. Bernard , A. Coffani , O. Drapier , S. El Hedri , A. Giampaolo , M. Gonin , Th. A. Mueller , P. Paganini , B. Quilain , T. Ishizuka , T. Nakamura , J. S. Jang , J. G. Learned , L. H. V. Anthony , D. Martin , M. Scott , A. A. Sztuc , Y. Uchida , V. Berardi , M. G. Catanesi , E. Radicioni , N. F. Calabria , L. N. Machado , G. De Rosa , G. Collazuol , F. Iacob , M. Lamoureux , M. Mattiazzi , N. Ospina , L. Ludovici , Y. Maekawa , Y. Nishimura , M. Friend , T. Hasegawa , T. Ishida , T. Kobayashi , M. Jakkapu , T. Matsubara , T. Nakadaira , K. Nakamura , Y. Oyama , K. Sakashita , T. Sekiguchi , T. Tsukamoto , Y. Kotsar , Y. Nakano , H. Ozaki , T. Shiozawa , A. T. Suzuki , Y. Takeuchi , S. Yamamoto , A. Ali , Y. Ashida , J. Feng , S. Hirota , T. Kikawa , M. Mori , T. Nakaya , R. A. Wendell , K. Yasutome , P. Fernandez , N. McCauley , P. Mehta , K. M. Tsui , Y. Fukuda , Y. Itow , H. Menjo , T. Niwa , K. Sato , M. Tsukada , J. Lagoda , S. M. Lakshmi , P. Mijakowski , J. Zalipska , J. Jiang , C. K. Jung , C. Vilela , M. J. Wilking , C. Yanagisawa , K. Hagiwara , M. Harada , T. Horai , H. Ishino , S. Ito , H. Kitagawa , Y. Koshio , W. Ma , N. Piplani , S. Sakai , G. Barr , D. Barrow , L. Cook , A. Goldsack , S. Samani , D. Wark , F. Nova , T. Boschi , F. Di Lodovico , J. Gao , J. Migenda , M. Taani , S. Zsoldos , J. Y. Yang , S. J. Jenkins , M. Malek , J. M. McElwee , O. Stone , M. D. Thiesse , L. F. Thompson , H. Okazawa , S. B. Kim , J. W. Seo , I. Yu , K. Nishijima , M. Koshiba , K. Iwamoto , K. Nakagiri , Y. Nakajima , N. Ogawa , M. Yokoyama , K. Martens , M. R. Vagins , M. Kuze , S. Izumiyama , T. Yoshida , M. Inomoto , M. Ishitsuka , H. Ito , T. Kinoshita , R. Matsumoto , K. Ohta , M. Shinoki , T. Suganuma , A. K. Ichikawa , K. Nakamura , J. F. Martin , H. A. Tanaka , T. Towstego , R. Akutsu , V. Gousy-Leblanc , M. Hartz , A. Konaka , P. de Perio , N. W. Prouse , S. Chen , B. D. Xu , Y. Zhang , M. Posiadala-Zezula , D. Hadley , M. O'Flaherty , B. Richards , B. Jamieson , J. Walker , A. Minamino , K. Okamoto , G. Pintaudi , S. Sano , R. Sasaki

The Dark Matter Diffused Supernova Neutrino Background

We consider neutrinos scattering off Milky Way dark matter and the impact of this scattering on supernovae neutrinos. This can take the form of attenuation on the initial flux of neutrinos and a time-delayed flux of scattered neutrinos.…

High Energy Physics - Phenomenology · Physics 2026-01-08 Garv Chauhan , R. Andrew Gustafson , Gonzalo Herrera , Taj Johnson , Ian Shoemaker