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It was recently shown that standard sub-GeV dark matter candidates can be effectively probed by large neutrino observatories via annual modulation of the total photomultiplier hit rate. That work focused on the production of light by the…

High Energy Physics - Phenomenology · Physics 2025-12-17 Lillian Santos-Olmsted , Rebecca K. Leane , Carlos Blanco , John F. Beacom

We investigate the sensitivity of some of the proposed next-generation neutrino experiments to a galactic supernova. In particular, we study how well the supernova parameters (the average energies and luminosities) can be separated from the…

High Energy Physics - Phenomenology · Physics 2010-10-27 Solveig Skadhauge , Renata Zukanovich Funchal

Observation of supernovae (SN) through their neutrino emission is a fundamental point to understand both SN dynamics and neutrino physical properties. JUNO is a 20kton liquid scintillator detector, under construction in Jiangmen, China. The…

High Energy Astrophysical Phenomena · Physics 2019-10-09 C. Martellini , S. M. Mari , P. Montini , G. Settanta

Environmental radioactivity is a dominant background for rare decay search experiments, and it is difficult to completely remove such an impurity from detector vessels. We propose a scintillation balloon as the active vessel of a liquid…

Instrumentation and Detectors · Physics 2019-11-18 S. Obara , Y. Gando , K. Ishidoshiro

The multi-ton-scale liquid xenon detectors, with an excellent energy resolution of a few keV, will be constructed to probe the dark-matter particles. In this paper, we show that precision measurements of the low-energy solar neutrinos via…

High Energy Physics - Phenomenology · Physics 2019-02-15 Guo-yuan Huang , Shun Zhou

Neutrino-antineutrino conversion is an important new physics process. The observation of this phenomenon could indicate total lepton number violation and potential CPT-violation. Searching for the appearance of electron antineutrinos from…

High Energy Physics - Phenomenology · Physics 2019-06-26 S. J. Li , J. J. Ling , N. Raper , M. V. Smirnov

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

Large liquid argon (LAr) detectors, up to 100 kton scale, are presently being considered for proton decay searches and neutrino astrophysics as well as far detectors for the next generation of long baseline neutrino oscillation experiments,…

Instrumentation and Detectors · Physics 2009-12-23 A. Marchionni

The MeV region of antineutrino energy is of special interest for physics research and for monitoring nuclear nonproliferation. Whereas liquid scintillation detectors are typically used to detect the Inverse Beta Decay (IBD), it has recently…

Instrumentation and Detectors · Physics 2023-07-19 Thomas Radermacher , Johannes Bosse , Sarah Friedrich , Malte Göttsche , Stefan Roth , Georg Schwefer

We discuss here new, enabling technologies for future photon-based neutrino detectors. These technologies touch nearly every aspect of such detectors: new scintillating materials, new methods of loading isotopes, new photon sensors and…

Dark matter direct detection experiments have become excellent low-energy neutrino detectors. We present a few novel ideas to probe Beyond the Standard Model physics from neutrinos at these experiments. First, we discuss signatures arising…

High Energy Physics - Phenomenology · Physics 2025-01-22 Gonzalo Herrera

The Jiangmen Underground Neutrino Observatory (JUNO), a 20 kton multi-purpose underground liquid scintillator detector, was proposed with the determination of the neutrino mass hierarchy as a primary physics goal. It is also capable of…

Instrumentation and Detectors · Physics 2016-02-02 Fengpeng An , Guangpeng An , Qi An , Vito Antonelli , Eric Baussan , John Beacom , Leonid Bezrukov , Simon Blyth , Riccardo Brugnera , Margherita Buizza Avanzini , Jose Busto , Anatael Cabrera , Hao Cai , Xiao Cai , Antonio Cammi , Guofu Cao , Jun Cao , Yun Chang , Shaomin Chen , Shenjian Chen , Yixue Chen , Davide Chiesa , Massimiliano Clemenza , Barbara Clerbaux , Janet Conrad , Davide D'Angelo , Herve De Kerret , Zhi Deng , Ziyan Deng , Yayun Ding , Zelimir Djurcic , Damien Dornic , Marcos Dracos , Olivier Drapier , Stefano Dusini , Stephen Dye , Timo Enqvist , Donghua Fan , Jian Fang , Laurent Favart , Richard Ford , Marianne Goger-Neff , Haonan Gan , Alberto Garfagnini , Marco Giammarchi , Maxim Gonchar , Guanghua Gong , Hui Gong , Michel Gonin , Marco Grassi , Christian Grewing , Mengyun Guan , Vic Guarino , Gang Guo , Wanlei Guo , Xin-Heng Guo , Caren Hagner , Ran Han , Miao He , Yuekun Heng , Yee Hsiung , Jun Hu , Shouyang Hu , Tao Hu , Hanxiong Huang , Xingtao Huang , Lei Huo , Ara Ioannisian , Manfred Jeitler , Xiangdong Ji , Xiaoshan Jiang , Cecile Jollet , Li Kang , Michael Karagounis , Narine Kazarian , Zinovy Krumshteyn , Andre Kruth , Pasi Kuusiniemi , Tobias Lachenmaier , Rupert Leitner , Chao Li , Jiaxing Li , Weidong Li , Weiguo Li , Xiaomei Li , Xiaonan Li , Yi Li , Yufeng Li , Zhi-Bing Li , Hao Liang , Guey-Lin Lin , Tao Lin , Yen-Hsun Lin , Jiajie Ling , Ivano Lippi , Dawei Liu , Hongbang Liu , Hu Liu , Jianglai Liu , Jianli Liu , Jinchang Liu , Qian Liu , Shubin Liu , Shulin Liu , Paolo Lombardi , Yongbing Long , Haoqi Lu , Jiashu Lu , Jingbin Lu , Junguang Lu , Bayarto Lubsandorzhiev , Livia Ludhova , Shu Luo , Vladimir Lyashuk , Randolph Mollenberg , Xubo Ma , Fabio Mantovani , Yajun Mao , Stefano M. Mari , William F. McDonough , Guang Meng , Anselmo Meregaglia , Emanuela Meroni , Mauro Mezzetto , Lino Miramonti , Thomas Mueller , Dmitry Naumov , Lothar Oberauer , Juan Pedro Ochoa-Ricoux , Alexander Olshevskiy , Fausto Ortica , Alessandro Paoloni , Haiping Peng , Jen-Chieh Peng , Ezio Previtali , Ming Qi , Sen Qian , Xin Qian , Yongzhong Qian , Zhonghua Qin , Georg Raffelt , Gioacchino Ranucci , Barbara Ricci , Markus Robens , Aldo Romani , Xiangdong Ruan , Xichao Ruan , Giuseppe Salamanna , Mike Shaevitz , Valery Sinev , Chiara Sirignano , Monica Sisti , Oleg Smirnov , Michael Soiron , Achim Stahl , Luca Stanco , Jochen Steinmann , Xilei Sun , Yongjie Sun , Dmitriy Taichenachev , Jian Tang , Igor Tkachev , Wladyslaw Trzaska , Stefan van Waasen , Cristina Volpe , Vit Vorobel , Lucia Votano , Chung-Hsiang Wang , Guoli Wang , Hao Wang , Meng Wang , Ruiguang Wang , Siguang Wang , Wei Wang , Yi Wang , Yi Wang , Yifang Wang , Zhe Wang , Zheng Wang , Zhigang Wang , Zhimin Wang , Wei Wei , Liangjian Wen , Christopher Wiebusch , Bjorn Wonsak , Qun Wu , Claudia-Elisabeth Wulz , Michael Wurm , Yufei Xi , Dongmei Xia , Yuguang Xie , Zhi-zhong Xing , Jilei Xu , Baojun Yan , Changgen Yang , Chaowen Yang , Guang Yang , Lei Yang , Yifan Yang , Yu Yao , Ugur Yegin , Frederic Yermia , Zhengyun You , Boxiang Yu , Chunxu Yu , Zeyuan Yu , Sandra Zavatarelli , Liang Zhan , Chao Zhang , Hong-Hao Zhang , Jiawen Zhang , Jingbo Zhang , Qingmin Zhang , Yu-Mei Zhang , Zhenyu Zhang , Zhenghua Zhao , Yangheng Zheng , Weili Zhong , Guorong Zhou , Jing Zhou , Li Zhou , Rong Zhou , Shun Zhou , Wenxiong Zhou , Xiang Zhou , Yeling Zhou , Yufeng Zhou , Jiaheng Zou

Neutrino astrophysics offers new perspectives on the Universe investigation: high energy neutrinos, produced by the most energetic phenomena in our Galaxy and in the Universe, carry complementary (if not exclusive) information about the…

High Energy Astrophysical Phenomena · Physics 2010-02-11 T. Chiarusi , M. Spurio

In the late stages of nuclear burning for massive stars ($M>8~M_{\sun}$), the production of neutrino-antineutrino pairs through various processes becomes the dominant stellar cooling mechanism. As the star evolves, the energy of these…

Detecting the extremely low-energy neutrinos that form the Cosmic Neutrino Background (CNB) presents many experimental challenges, but pursuing this elusive goal is still worthwhile because these weakly-interacting particles could provide a…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-16 M. M. Hedman

We examine the prospects for using lead as a supernova-neutrino detector by considering the spectrum of electrons produced, and the number of one- and two-neutron events. We show that the electron energy spectrum from charged-current…

High Energy Physics - Phenomenology · Physics 2014-11-17 J. Engel , G. C. McLaughlin , C. Volpe

The SNO+ experiment is the follow up of the SNO experiment, replacing the heavy water volume with about 780 tons of liquid scintillator (LAB) in order to shift the sensitive threshold to lower energy range. The 6000 m.w.e. natural rock…

High Energy Physics - Experiment · Physics 2019-08-14 V. Lozza

We find that it is possible to increase sensitivity to low energy physics in a third or fourth DUNE-like module with careful controls over radiopurity and some modifications to a detector similar to the DUNE Far Detector design. In…

The Deep Underground Neutrino Experiment (DUNE) is a leading-edge experiment designed to perform neutrino science and proton decay searches. In particular, the far detector will consist of four 10-kton Liquid Argon (LAr) Time Projection…

Instrumentation and Detectors · Physics 2020-08-26 Chiara Lastoria

The strange quark contribution to proton's spin ($\Delta s$) is a fundamental quantity that is poorly determined from current experiments. Neutrino-proton elastic scattering (pES) is a promising channel to measure this quantity, and…

High Energy Physics - Phenomenology · Physics 2022-11-17 Bhavesh Chauhan