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A novel method to produce neutrino beams has recently been proposed : the beta-beams. This method consists in using the beta-decay of boosted radioactive nuclei to obtain an intense, collimated and pure neutrino beam. Here we propose to…

High Energy Physics - Phenomenology · Physics 2009-11-10 Cristina Volpe

The NOvA long-baseline neutrino experiment uses a pair of large, segmented, liquid-scintillator calorimeters to study neutrino oscillations, using GeV-scale neutrinos from the Fermilab NuMI beam. These detectors are also sensitive to the…

Instrumentation and Detectors · Physics 2023-02-18 NOvA Collaboration , M. A. Acero , P. Adamson , G. Agam , L. Aliaga , T. Alion , V. Allakhverdian , N. Anfimov , A. Antoshkin , E. Arrieta-Diaz , L. Asquith , A. Aurisano , A. Back , C. Backhouse , M. Baird , N. Balashov , P. Baldi , B. A. Bambah , S. Bashar , K. Bays , S. Bending , R. Bernstein , V. Bhatnagar , B. Bhuyan , J. Bian , J. Blair , A. C. Booth , P. Bour , R. Bowles , C. Bromberg , N. Buchanan , A. Butkevich , V. Bychkov , S. Calvez , T. J. Carroll , E. Catano-Mur , S. Childress , B. C. Choudhary , T. E. Coan , M. Colo , L. Corwin , L. Cremonesi , G. S. Davies , P. F. Derwent , P. Ding , Z. Djurcic , M. Dolce , D. Doyle , D. Dueñas Tonguino , E. C. Dukes , P. Dung , H. Duyang , S. Edayath , R. Ehrlich , M. Elkins , G. J. Feldman , P. Filip , W. Flanagan , J. Franc , M. J. Frank , H. R. Gallagher , R. Gandrajula , F. Gao , S. Germani , A. Giri , R. A. Gomes , M. C. Goodman , V. Grichine , M. Groh , R. Group , B. Guo , A. Habig , F. Hakl , A. Hall , J. Hartnell , R. Hatcher , A. Hatzikoutelis , K. Heller , V Hewes , A. Himmel , A. Holin , B. Howard , J. Huang , J. Hylen , F. Jediny , C. Johnson , M. Judah , I. Kakorin , D. Kalra , D. M. Kaplan , R. Keloth , O. Klimov , L. W. Koerner , L. Kolupaeva , S. Kotelnikov , M. Kubu , Ch. Kullenberg , A. Kumar , C. D. Kuruppu , V. Kus , T. Lackey , K. Lang , L. Li , S. Lin , A. Lister , M. Lokajicek , S. Luchuk , S. Magill , W. A. Mann , M. L. Marshak , M. Martinez-Casales , V. Matveev , B. Mayes , D. P. Méndez , M. D. Messier , H. Meyer , T. Miao , W. H. Miller , S. R. Mishra , A. Mislivec , R. Mohanta , A. Moren , A. Morozova , L. Mualem , M. Muether , S. Mufson , K. Mulder , R. Murphy , J. Musser , D. Naples , N. Nayak , J. K. Nelson , R. Nichol , G. Nikseresht , E. Niner , A. Norman , A. Norrick , T. Nosek , A. Olshevskiy , T. Olson , J. Paley , R. B. Patterson , G. Pawloski , O. Petrova , R. Petti , R. K. Plunkett , F. Psihas , A. Rafique , V. Raj , B. Ramson , B. Rebel , P. Rojas , V. Ryabov , O. Samoylov , M. C. Sanchez , S. Sánchez Falero , I. S. Seong , P. Shanahan , A. Sheshukov , P. Singh , V. Singh , E. Smith , J. Smolik , P. Snopok , N. Solomey , A. Sousa , K. Soustruznik , M. Strait , L. Suter , A. Sutton , C. Sweeney , R. L. Talaga , B. Tapia Oregui , P. Tas , R. B. Thayyullathil , J. Thomas , E. Tiras , D. Torbunov , J. Tripathi , A. Tsaris , Y. Torun , J. Urheim , P. Vahle , Z. Vallari , J. Vasel , P. Vokac , T. Vrba , M. Wallbank , T. K. Warburton , M. Wetstein , D. Whittington , D. A. Wickremasinghe , S. G. Wojcicki , J. Wolcott , A. Yallappa Dombara , K. Yonehara , S. Yu , Y. Yu , S. Zadorozhnyy , J. Zalesak , Y. Zhang , R. Zwaska

The IceCube Neutrino Observatory has detected high-energy astrophysical neutrinos in the TeV-PeV range. These neutrinos have an isotropic distribution on the sky, and therefore, likely originate from extragalactic sources. Active Galactic…

High Energy Astrophysical Phenomena · Physics 2021-10-27 Sreetama Goswami , George C. Privon , Marcos Santander

It is shown that explanations of atmospheric neutrino anomaly other than $\nu_\mu - \nu_\tau oscillations (e.g. decay, decoherence and $\nu_\mu - \nu_\tau - \nu_{KK}$ mixing) can be tested at future facilities. Stringent tests of CPT…

High Energy Physics - Phenomenology · Physics 2011-08-04 S. Pakvasa

The recent observation of Coherent Elastic Neutrino Nucleus Scattering (CE{\nu}NS) with neutrinos from pion decay at rest ({\pi}-DAR) sources by the COHERENT Collaboration has raised interest in this process in the search for new physics.…

High Energy Physics - Phenomenology · Physics 2023-11-30 R. R. Rossi , G. Sanchez Garcia , M. Tórtola

The IceCube Neutrino Detector observes tens of thousands of atmospheric neutrinos every year with its low energy extension DeepCore, covering the neutrino energy range from GeV to TeV. These neutrinos can be used to study particle…

High Energy Astrophysical Phenomena · Physics 2019-09-25 Anatoli Fedynitch , Juan-Pablo Yáñez

We discuss a specific population of galactic PeVatrons which may be the main source of the galactic cosmic-ray (CR) component well above PeV energies. Supernovae in compact clusters of massive stars are proposed as powerful sources of CRs,…

High Energy Astrophysical Phenomena · Physics 2018-10-31 A. M. Bykov , D. C. Ellison , P. E. Gladilin , S. M. Osipov

Sensitive tests of Lorentz invariance can emerge from the study of neutrino oscillations, particularly for atmospheric neutrinos where the effect is conveniently near-maximal and has been observed over a wide range of energies. We assume…

High Energy Physics - Phenomenology · Physics 2007-05-23 Sheldon Lee Glashow

The article describes the research program pursued by the TEXONO Collaboration towards an experiment to observe coherent scattering between neutrinos and the nucleus at the power reactor. The motivations of studying this process are…

High Energy Physics - Experiment · Physics 2009-11-11 Henry T. Wong

Neutrons play an important role in the dynamics of gamma-ray bursts. The presence of neutrons in the baryon-loaded fireball is expected. If the neutrons abundance is comparable to that of protons, important features may be observed such as…

High Energy Astrophysical Phenomena · Physics 2015-06-18 Nissim Fraija

The NOvA experiment's most recent search for eV-scale sterile neutrinos under a 3+1 model simultaneously analyses muon neutrino and neutral current datasets from the NuMI beam at its Near ($\sim$\qty{1}{km} baseline) and Far (\qty{810}{km}…

High Energy Physics - Experiment · Physics 2026-02-13 Adam Lister

Existing and planned observatories for cosmic neutrinos open up a huge window in energy from 10^7 to 10^17 GeV. Here, we discuss in particular the possibilities to use extremely energetic cosmic neutrinos as a diagnostic of astrophysical…

High Energy Physics - Phenomenology · Physics 2010-11-05 Andreas Ringwald

The recent discovery that neutrinos have mass opens a wide new field of experimentation. Accelerator-made neutrinos are essential. Ideas for future facilities include superbeams beta-beams and neutrino factories, each associated with one or…

High Energy Physics - Phenomenology · Physics 2008-11-26 Alain Blondel

We revisit the signatures from collisions of cosmic-rays on sub-GeV dark matter (DM) in the Milky Way. In addition to the upscattered DM component that can be probed by existing DM and neutrino experiments widely discussed, we examine the…

High Energy Astrophysical Phenomena · Physics 2020-11-09 Gang Guo , Yue-Lin Sming Tsai , Meng-Ru Wu , Qiang Yuan

The observed very high energy spectra of distant blazars are well described by secondary gamma rays produced in line-of-sight interactions of cosmic rays with background photons. In the absence of the cosmic-ray contribution, one would not…

High Energy Astrophysical Phenomena · Physics 2013-07-29 Oleg E. Kalashev , Alexander Kusenko , Warren Essey

We consider two-family neutrino oscillations in a medium of continuously-varying density as a limit of the process in a series of constant-density layers. We construct analytic expressions for the conversion amplitude at high energies…

High Energy Physics - Phenomenology · Physics 2008-11-26 Paul M. Fishbane , Peter Kaus

Coherent elastic neutrino-nucleus scattering (CE$\nu$NS) and other rare-event physics searches, like dark matter detection, have been especially furthered by increasing sensitivity to low-energy particle interactions. Experiments using…

Instrumentation and Detectors · Physics 2023-10-09 Charles Mark Lewis

The use of radioactive beams opens a new frontier for fusion studies. The coupling to the continuum can be explored with very loosely bound nuclei. Experiments were performed with beams of nuclei at or near the proton and neutron drip-lines…

Nuclear Experiment · Physics 2009-11-11 J. F. Liang , C. Signorini

The detection of an astrophysical flux of neutrinos in the TeV-PeV energy range by the IceCube observatory has opened new possibilities for the study of extreme cosmic accelerators. The apparent isotropy of the neutrino arrival directions…

High Energy Astrophysical Phenomena · Physics 2022-09-29 Naoko Kurahashi , Kohta Murase , Marcos Santander

We summarize the determination of some neutrino properties from the global analysis of solar, atmospheric, reactor, and accelerator neutrino data in the framework of three-neutrino mixing as well as in some extended scenarios such as the…

High Energy Physics - Phenomenology · Physics 2016-06-22 M. C. Gonzalez-Garcia , Michele Maltoni , Thomas Schwetz
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