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200 papers

The origin of Petaelectronvolt (PeV) astrophysical neutrinos is fundamental to our understanding of the high-energy Universe. Apart from the technical challenges of operating detectors deep below ice, oceans, and lakes, the phenomenological…

High Energy Astrophysical Phenomena · Physics 2022-10-05 I. Liodakis , T. Hovatta , V. Pavlidou , A. C. S. Readhead , R. D. Blandford , S. Kiehlmann , E. Lindfors , W. Max-Moerbeck , T. J. Pearson , M. Petropoulou

The quest to understand the nature dark matter is one of the most relevant ones in Particle Physics nowadays, since it constitutes most of the matter of the Universe and it is still unknown what it is made of. In order to answer to this…

High Energy Astrophysical Phenomena · Physics 2016-10-04 J. D. Zornoza

The ANTARES detector is the most sensitive neutrino telescope observing the southern sky and the world's first particle detector operating in the deep sea. It is installed in the Mediterranean Sea at a depth of 2475 m. As an example of…

High Energy Astrophysical Phenomena · Physics 2019-08-14 Th. Eberl

Neutrinos are fundamental particles ubiquitous in the Universe. Their properties remain elusive despite more than 50 years of intense research activity. In this review we remind the reader of the noticeable properties of these particles and…

Solar and Stellar Astrophysics · Physics 2015-05-19 S. Turck-Chieze , S. Couvidat

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

Neutrinos are a very promising messenger at tens of EeV and above. They can be produced by several channels, namely as by products of hadronic interactions at the sources, as the main products of the decay of super massive particles and, in…

High Energy Astrophysical Phenomena · Physics 2019-08-14 A. D. Supanitsky , G. Medina-Tanco , K. Asano , D. Cline , T. Ebisuzaki , S. Inoue , P. Lipari , A. Santangelo , K. Shinozaki , G. Sigl , Y. Takahashi , M. Teshima

Neutrons serve as unique probes for exploring the microscopic structure of matter, with the performance of a neutron source fundamentally governing the depth of scientific exploration and the breadth of industrial applicability. To address…

Neutral currents induced matter oscillations of electroweak-active (anti-)neutrinos to sterile neutrinos can explain the observed motion of pulsars. In contrast to a recently proposed explanation of the pulsar birth velocities based on the…

High Energy Physics - Phenomenology · Physics 2014-11-17 Alexander Kusenko , Gino Segre

The upcoming European Spallation Source (ESS) will soon provide the most intense neutrino source in the world. We propose the Search for Hidden Neutrinos at the ESS (SHiNESS) experiment, highlighting its unique opportunities to search for…

High Energy Physics - Experiment · Physics 2025-05-28 Stefano Roberto Soleti , Pilar Coloma , Juan Jose Gómez Cadenas , Anatael Cabrera

Even the elusive neutrinos are trapped in matter, albeit transiently, in several astrophysical circumstances. Their interactions with the ambient matter not only reveal the properties of such exotic matter itself, but also shed light on the…

Astrophysics · Physics 2009-11-06 M. Prakash , J. M. Lattimer , R. F. Sawyer , R. R. Volkas

The ANTARES Collaboration is aiming at the construction and the operation of a large undersea neutrino telescope for neutrino astronomy, neutrino oscillation and indirect dark matter searches. Started 3 years ago an intensive R&D program…

Astrophysics · Physics 2009-10-31 F. Montanet

The role of neutrinos in stars is introduced for students with little prior astrophysical exposure. We begin with neutrinos as an energy-loss channel in ordinary stars and conversely, how stars provide information on neutrinos and possible…

Solar and Stellar Astrophysics · Physics 2012-05-22 Georg Raffelt

Many galactic and extragalactic astrophysical sources are currently considered promising candidates as high energy neutrino emitters. Astrophysical neutrinos can be detected as upward-going muons produced in charged-current interactions…

Astrophysics · Physics 2012-08-27 The MACRO Collaboration

Our present knowledge of neutrinos can be summarized in terms of the "standard neutrino scenario". Phenomenology of this scenario as well as attempts to uncover physics behind neutrino mass and mixing are described. Goals of future studies…

High Energy Physics - Phenomenology · Physics 2008-12-18 Alexei Yu. Smirnov

Neutrinos from a future Galactic supernova will be detected by several large underground detectors, in particular by SuperKamiokande (SK) and the Sudbury Neutrino Observatory (SNO). If, as expected, the $\nu_{\mu}$ and $\nu_{\tau}$…

Astrophysics · Physics 2007-05-23 Petr Vogel

In the present paper we study some neutrino properties as they may appear in the low energy neutrinos emitted in triton decay with maximum neutrino energy of 18.6 keV. The technical challenges to this end can be achieved by building a very…

High Energy Physics - Phenomenology · Physics 2015-06-25 Giomataris , J. D. Vergados

Recent data lead us to a simple and intriguing form of the neutrino mass matrix. In particular, we find solar neutrino oscillations to be nearly maximal (and rule out the small-angle MSW explanation of solar neutrino observations) if relic…

High Energy Physics - Phenomenology · Physics 2009-09-11 Howard Georgi , S. L. Glashow

Neutrino telescopes provide a unique observational gateway to the high-energy universe, enabling the study of cosmic accelerators and extreme environments that remain inaccessible to the other high-energy messengers. Although they share…

High Energy Astrophysical Phenomena · Physics 2026-03-24 Aya Ishihara

We provide elements for a discussion of the expected neutrino signal from Supernova Remnants (SNR) in the Milky Way. After recalling why SNR are interesting and certain remarkable achievements of H.E.S.S., we describe a simple and…

Astrophysics · Physics 2007-05-23 Francesco Vissani

The ANTARES project aims at the construction of a neutrino telescope 2500 m below the surface of the Mediterranean sea, close to the southern French coast. The apparatus will consist of a 3D array of photomultiplier tubes, which detects the…

Astrophysics · Physics 2019-08-14 G. F. Burgio