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We suggest to use a polarized electron target for improving the sensitivity of the search for the neutrino magnetic moment to the level $\sim 3\cdot10^{-13}\mu_B$ in the processes of neutrino (antineutrino) -- electron scattering. It is…

High Energy Physics - Phenomenology · Physics 2009-10-31 T. I. Rashba , V. B. Semikoz

In the recent years important discoveries in the field of low energy neutrino physics (E$_\nu$ in the $\approx$ MeV range) have been achieved. Results of the solar neutrino experiment SNO show clearly flavor transitions from $\nu_e$ to…

High Energy Physics - Phenomenology · Physics 2009-11-10 Lothar Oberauer

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 detection of solar-neutrinos of different origin via induced beta beta process of Mo100 is investigated. The particular counting rates and energy distributions of emitted electrons are presented. A discussion in respect to…

High Energy Physics - Phenomenology · Physics 2009-11-07 P. Domin , F. Simkovic , S. V. Semenov , Yu. V. Gaponov

Development of large mass detectors for low-energy neutrinos and dark matter may allow supernova detection via neutrino-nucleus elastic scattering. An elastic-scattering detector could observe a few, or more, events per ton for a galactic…

Astrophysics · Physics 2009-11-07 C. J. Horowitz , K. J. Coakley , D. N. McKinsey

A thorough understanding of neutrino-nucleus scattering physics is crucial for the successful execution of the entire US neutrino physics program. Neutrino-nucleus interaction constitutes one of the biggest systematic uncertainties in…

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

We present searches for light dark matter (DM) with masses 3-9 GeV/$c^2$ in the presence of coherent elastic neutrino-nucleus scattering (CE$\nu$NS) from $^{8}$B solar neutrinos with the LUX-ZEPLIN experiment. This analysis uses a 5.7…

High Energy Physics - Experiment · Physics 2025-12-24 D. S. Akerib , A. K. Al Musalhi , F. Alder , B. J. Almquist , C. S. Amarasinghe , A. Ames , T. J. Anderson , N. Angelides , H. M. Araújo , J. E. Armstrong , M. Arthurs , A. Baker , S. Balashov , J. Bang , J. W. Bargemann , E. E. Barillier , D. Bauer , K. Beattie , A. Bhatti , T. P. Biesiadzinski , H. J. Birch , E. Bishop , G. M. Blockinger , C. A. J. Brew , P. Brás , S. Burdin , M. C. Carmona-Benitez , M. Carter , A. Chawla , H. Chen , Y. T. Chin , N. I. Chott , S. Contreras , M. V. Converse , R. Coronel , A. Cottle , G. Cox , D. Curran , C. E. Dahl , I. Darlington , S. Dave , A. David , J. Delgaudio , S. Dey , L. de Viveiros , L. Di Felice , C. Ding , J. E. Y. Dobson , E. Druszkiewicz , S. Dubey , C. L. Dunbar , S. R. Eriksen , S. Fayer , N. M. Fearon , N. Fieldhouse , S. Fiorucci , H. Flaecher , E. D. Fraser , T. M. A. Fruth , P. W. Gaemers , R. J. Gaitskell , A. Geffre , J. Genovesi , C. Ghag , J. Ghamsari , A. Ghosh , S. Ghosh , R. Gibbons , S. Gokhale , J. Green , M. G. D. van der Grinten , J. J. Haiston , C. R. Hall , T. Hall , R. H Hampp , S. J. Haselschwardt , M. A. Hernandez , S. A. Hertel , G. J. Homenides , M. Horn , D. Q. Huang , D. Hunt , E. Jacquet , R. S. James , K. Jenkins , A. C. Kaboth , A. C. Kamaha , M. K. Kannichankandy , D. Khaitan , A. Khazov , J. Kim , Y. D. Kim , D. Kodroff , E. V. Korolkova , H. Kraus , S. Kravitz , L. Kreczko , V. A. Kudryavtsev , C. Lawes , D. S. Leonard , K. T. Lesko , C. Levy , J. Lin , A. Lindote , W. H. Lippincott , J. Long , M. I. Lopes , W. Lorenzon , C. Lu , S. Luitz , W. Ma , V. Mahajan , P. A. Majewski , A. Manalaysay , R. L. Mannino , R. J. Matheson , C. Maupin , M. E. McCarthy , D. N. McKinsey , J. McLaughlin , J. B. McLaughlin , R. McMonigle , B. Mitra , E. Mizrachi , M. E. Monzani , K. Morå , E. Morrison , B. J. Mount , M. Murdy , A. St. J. Murphy , H. N. Nelson , F. Neves , A. Nguyen , C. L. O'Brien , F. H. O'Shea , I. Olcina , K. C. Oliver-Mallory , J. Orpwood , K. Y Oyulmaz , K. J. Palladino , N. J. Pannifer , N. Parveen , S. J. Patton , B. Penning , G. Pereira , E. Perry , T. Pershing , A. Piepke , S. S. Poudel , Y. Qie , J. Reichenbacher , C. A. Rhyne , G. R. C. Rischbieter , E. Ritchey , H. S. Riyat , R. Rosero , N. J. Rowe , T. Rushton , D. Rynders , S. Saltão , D. Santone , I. Sargeant , A. B. M. R. Sazzad , R. W. Schnee , G. Sehr , B. Shafer , S. Shaw , W. Sherman , K. Shi , T. Shutt , C. Silva , G. Sinev , J. Siniscalco , A. M. Slivar , R. Smith , V. N. Solovov , P. Sorensen , J. Soria , T. J. Sumner , A. Swain , M. Szydagis , D. R. Tiedt , M. Timalsina , D. R. Tovey , J. Tranter , M. Trask , K. Trengove , M. Tripathi , A. Usón , A. C. Vaitkus , O. Valentino , V. Velan , A. Wang , J. J. Wang , Y. Wang , L. Weeldreyer , T. J. Whitis , K. Wild , M. Williams , J. Winnicki , L. Wolf , F. L. H. Wolfs , S. Woodford , D. Woodward , C. J. Wright , Q. Xia , J. Xu , Y. Xu , M. Yeh , D. Yeum , J. Young , W. Zha , H. Zhang , T. Zhang , Y. Zhou

Several next-generation experiments aim to make the first measurement of the neutrino flux from the Carbon-Nitrogen-Oxygen (CNO) solar fusion cycle. We calculate how much time these experiments will need to run for in order to measure this…

High Energy Physics - Phenomenology · Physics 2018-04-11 David G. Cerdeno , Jonathan H. Davis , Malcolm Fairbairn , Aaron C. Vincent

We demonstrate the prompt-delayed signals induced by knockout neutrons from the quasi-elastic scattering in neutrino experiments provides a new avenue for detecting light dark matter. As an illustration, we consider the detection of…

High Energy Physics - Phenomenology · Physics 2026-03-25 Yuanlin Gong , Feiran Lin , Ning Liu , Liangliang Su , Lei Wu

The coupling of the baryonic current to new neutrino states \nu_b with strength in excess of the weak interactions is a viable extension of the Standard Model. We analyze the signature of \nu_b appearance in the solar neutrino flux that…

High Energy Physics - Phenomenology · Physics 2013-08-19 Maxim Pospelov , Josef Pradler

Despite being neutral particles, neutrinos can acquire non-zero electromagnetic properties from radiative corrections that can be induced by the presence of new physics. Electromagnetic neutrino processes induce spectral distortions in…

High Energy Physics - Phenomenology · Physics 2024-12-20 Valentina De Romeri , Dimitrios K. Papoulias , Gonzalo Sanchez Garcia , Christoph A. Ternes , Mariam Tórtola

There are compelling evidences for the existence of a fourth degree of freedom of neutrinos i.e. sterile neutrino. In the recent studies the role of sterile component of neutrinos has been found to be crucial, not only in particle physics,…

High Energy Physics - Phenomenology · Physics 2019-04-12 Ankush , Rishu Verma , Gazal Sharma , B. C. Chauhan

We examine scenarios in which a dark sector (dark matter, dark radiation, or dark energy) couples to the active neutrinos. For light and weakly-coupled exotic sectors we find that scalar, vector, or tensor dark backgrounds may appreciably…

High Energy Physics - Phenomenology · Physics 2018-07-18 Francesco Capozzi , Ian M. Shoemaker , Luca Vecchi

The purpose of the present paper is to study the 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 summarized as…

High Energy Physics - Experiment · Physics 2009-11-10 Y. Giomataris , J. D. Vergados

The presence of dark matter has been ascertained through a wealth of astrophysical and cosmological phenomena and its nature is a central puzzle in modern science. Elementary particles stand as the most compelling explanation. They have…

High Energy Physics - Phenomenology · Physics 2019-10-02 Daniel A. Camargo , Farinaldo S. Queiroz , Riccardo Sturani

Radiative corrections to the electron recoil-energy spectra and to total cross sections are computed for neutrino-electron scattering by solar neutrinos. Radiative corrections change monotonically the electron recoil spectrum for incident…

Astrophysics · Physics 2016-08-30 John N. Bahcall , Marc Kamionkowski , Alberto Sirlin

The JUNO liquid scintillator-based experiment, construction of which is on-going in Jiangmen (China), will start operations in 2020 and will detect anti-neutrinos from nearby reactors; but also solar neutrinos via elastic scattering on…

Instrumentation and Detectors · Physics 2020-01-08 Giuseppe Salamanna

Low-energy high-resolution neutrino-electron scattering experiments may play an important role in testing the gauge structure of the electroweak interaction. We discuss the use of strong radioactive neutrino sources (e.g. $^{51}$Cr) in…

High Energy Physics - Phenomenology · Physics 2007-05-23 O. G. Miranda , V. B. Semikoz , J. W. F. Valle

We consider different methods and observables which can be obtained by the measurement of neutrino scattering off nucleons and nuclei with the purpose of finding evidence for the strange form factors of the nucleon, which enter into…

High Energy Physics - Phenomenology · Physics 2007-05-23 W. M. Alberico