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The combined requirements, of (i) a natural solution to the fermion mass hierarchy problem and (ii) an explanation of both the atmospheric and solar neutrino problems, lead to an essentially unique picture of neutrino masses and mixing…

High Energy Physics - Phenomenology · Physics 2009-10-30 C. D. Froggatt , M. Gibson , H. B. Nielsen

Next-generation xenon detectors with multi-ton-year exposure are powerful direct probes of dark matter candidates, in particular the favorite weakly-interacting massive particles. Coupled with the features of low thresholds and backgrounds,…

High Energy Physics - Phenomenology · Physics 2019-10-09 Chung-Chun Hsieh , Lakhwinder Singh , Chih-Pan Wu , Jiunn-Wei Chen , Hsin-Chang Chi , C. -P. Liu , Mukesh K. Pandey , Henry T. Wong

The neutrino mass hierarchy is one of the neutrino fundamental properties yet to be determined. We introduce a method to determine neutrino mass hierarchy by comparing the interaction rate of neutral current (NC) interactions,…

High Energy Physics - Phenomenology · Physics 2016-07-27 Kwang-Chang Lai , Fei-Fan Lee , Feng-Shiuh Lee , Guey-Lin Lin , Tsung-Che Liu , Yi Yang

The {\sc Majorana} collaboration is searching for neutrinoless double beta decay using $^{76}$Ge, which has been shown to have a number of advantages in terms of sensitivities and backgrounds. The observation of neutrinoless double-beta…

There is recent evidence that some SiC X grains from the Murchison meteorite may contain supernova-produced {\nu}-process 11B and or 7Li encapsulated in the grains. The synthesis of 11B and 7Li via neutrino-induced nucleon emission (the…

High Energy Astrophysical Phenomena · Physics 2014-05-06 G. J. Mathews , T. Kajino , W. Aoki , W. Fujiya , J. B. Pitts

We consider searches for dark matter annihilation to monoenergetic neutrinos in the core of the Sun. We find that liquid scintillation neutrino detectors have enhanced sensitivity to this class of dark matter models, due to the energy and…

High Energy Physics - Phenomenology · Physics 2015-07-14 Jason Kumar , Pearl Sandick

Neutrinos and dark matter (DM) are two of the least understood components of the Universe, yet both play crucial roles in cosmic evolution. Clues about their fundamental properties may emerge from discrepancies in cosmological measurements…

Cosmology and Nongalactic Astrophysics · Physics 2026-01-12 Lei Zu , William Giarè , Chi Zhang , Eleonora Di Valentino , Yue-Lin Sming Tsai , Sebastian Trojanowski

The flux of low energy neutrinos (<E_nu>~ 4 GeV) has been studied with the MACRO detector at Gran Sasso via the detection of muon neutrinos interactions inside the apparatus, and of upward-going stopping muons. Data collected in ~3 y with…

High Energy Physics - Experiment · Physics 2019-08-14 M. Spurio

The ANTARES Collaboration proposes to construct a large area water Cherenkov detector in the deep Mediterranean Sea, optimised for the detection of muons from high-energy astrophysical neutrinos. This paper presents the scientific…

Astrophysics · Physics 2012-08-27 ANTARES Collaboration

We revisit the sensitivity to non-resonant, heavy Majorana neutrinos $N$ in same-sign $W^\pm W^\pm$ scattering at the $\sqrt{s}=13$ TeV LHC and its high-luminosity upgrade. As a benchmark scenario, we work in the context of the…

High Energy Physics - Phenomenology · Physics 2021-03-11 Benjamin Fuks , Jonas Neundorf , Krisztian Peters , Richard Ruiz , Matthias Saimpert

We present a search for non-zero theta_{13} and deviations of sin^2 theta_{23} from 0.5 in the oscillations of atmospheric neutrino data from Super-Kamiokande -I, -II, and -III. No distortions of the neutrino flux consistent with non-zero…

High Energy Physics - Experiment · Physics 2012-08-27 Kamiokande Collaboration , R. Wendell , C. Ishihara , K. Abe , Y. Hayato , T. Iida , M. Ikeda , K. Iyogi , J. Kameda , K. Kobayashi , Y. Koshio , Y. Kozuma , M. Miura , S. Moriyama , M. Nakahata , S. Nakayama , Y. Obayashi , H. Ogawa , H. Sekiya , M. Shiozawa , Y. Suzuki , A. Takeda , Y. Takenaga , Y. Takeuchi , K. Ueno , K. Ueshima , H. Watanabe , S. Yamada , T. Yokozawa , S. Hazama , H. Kaji , T. Kajita , K. Kaneyuki , T. McLachlan , K. Okumura , Y. Shimizu , N. Tanimoto , M. R. Vagins , F. Dufour , E. Kearns , M. Litos , J. L. Raaf , J. L. Stone , L. R. Sulak , W. Wang , M. Goldhaber , K. Bays , D. Casper , J. P. Cravens , W. R. Kropp , S. Mine , C. Regis , M. B. Smy , H. W. Sobel , K. S. Ganezer , J. Hill , W. E. Keig , J. S. Jang , J. Y. Kim , I. T. Lim , J. Albert , M. Fechner , K. Scholberg , C. W. Walter , S. Tasaka , J. G. Learned , S. Matsuno , Y. Watanabe , T. Hasegawa , T. Ishida , T. Ishii , T. Kobayashi , T. Nakadaira , K. Nakamura , K. Nishikawa , H. Nishino , Y. Oyama , K. Sakashita , T. Sekiguchi , T. Tsukamoto , A. T. Suzuki , A. Minamino , T. Nakaya , Y. Fukuda , Y. Itow , G. Mitsuka , T. Tanaka , C. K. Jung , G. Lopez , C. McGrew , C. Yanagisawa , N. Tamura , H. Ishino , A. Kibayashi , S. Mino , T. Mori , M. Sakuda , H. Toyota , Y. Kuno , M. Yoshida , S. B. Kim , B. S. Yang , T. Ishizuka , H. Okazawa , Y. Choi , K. Nishijima , Y. Yokosawa , M. Koshiba , M. Yokoyama , Y. Totsuka , S. Chen , Y. Heng , Z. Yang , H. Zhang , D. Kielczewska , P. Mijakowski , K. Connolly , M. Dziomba , E. Thrane , R. J. Wilkes

We study the precision to which the sign of \delta m_{32}^2 can be determined at a neutrino factory, as a function of stored energies and baselines. This is done by simultaneously fitting the channels \nu_\mu \to \nu_\mu$, \bar\nu_e \to…

High Energy Physics - Phenomenology · Physics 2009-09-15 V. Barger , S. Geer , R. Raja , K. Whisnant

The Dirac leptonic CP phase {\delta}_CP is one of the crucial unknown parameters in neutrino oscillation physics. In this paper we explore the possibility of using low energy atmospheric neutrino events to probe {\delta}_CP . We show that…

High Energy Physics - Phenomenology · Physics 2019-12-25 D Indumathi , M V N Murthy , Lakshmi S. Mohan

We examine the prospects for supersymmetry discovery in the minimal supergravity (mSUGRA) model via indirect detection of neutralino dark matter. We investigate rates for muon detection in neutrino telescopes, and detection of photons,…

High Energy Physics - Phenomenology · Physics 2011-07-19 Howard Baer , Alexander Belyaev , Tadas Krupovnickas , Jorge O'Farrill

Measuring the neutrino mixing parameter \ensuremath{\sin^2\theta_{13}} to the sub-percent precision level could be necessary in the next ten years for the precision unitary test of the PMNS matrix. In this work, we discuss the possibility…

High Energy Physics - Experiment · Physics 2023-03-17 Jinnan Zhang , Jun Cao

Searches for mass-3 component in the electron neutrino flavor state $\sin{\theta}_{13}$ and for sterile neutrinos can be carried out in the same small mixing angle antineutrino oscillation experiment at a reactor. As an example we consider…

High Energy Physics - Phenomenology · Physics 2007-05-23 V. Kopeikin , L. Mikaelyan , V. Sinev

Cosmology is making impressive progress and it is producing stringent bounds on the sum of the neutrino masses {\Sigma}, a parameter of great importance for the current laboratory experiments. In this letter, we exploit the potential…

High Energy Physics - Phenomenology · Physics 2015-12-15 Stefano Dell'Oro , Simone Marcocci , Matteo Viel , Francesco Vissani

Many experiments are being planned to measure the neutrino mixing parameter $\theta_{13}$ using reactor as well as accelerator neutrino beams. In this note, the theoretical significance of a high precision measurement of this parameter is…

High Energy Physics - Phenomenology · Physics 2008-11-26 R. N. Mohapatra

A search for heavy right-handed Majorana neutrinos is performed with the ATLAS detector at the CERN Large Hadron Collider, using the 140 $\mathrm{fb}^{-1}$ of proton-proton collision data at $\sqrt{s}$ = 13 TeV collected during Run 2. This…

High Energy Physics - Experiment · Physics 2024-12-05 ATLAS Collaboration

The possibilities of detecting high energy neutrinos through inclined showers produced in the atmosphere are addressed with an emphasis on the detection of air showers by arrays of particle detectors. Rates of inclined showers produced by…

Astrophysics · Physics 2011-05-12 Enrique Zas
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