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Related papers: Loop-induced Neutrino Non-Standard Interactions

200 papers

We analyze the possibility of probing non-standard neutrino interactions (NSI, for short) through the detection of neutrinos produced in a future galactic supernova (SN).We consider the effect of NSI on the neutrino propagation through the…

High Energy Physics - Phenomenology · Physics 2008-11-26 A. Esteban-Pretel , R. Tomàs , J. W. F. Valle

The neutrino oscillation experiments are setting increasingly strong upper bounds on the vector Non-Standard neutrino Interactions (NSI) with matter fields. However, the bounds on the axial NSI are more relaxed, raising the hope that…

High Energy Physics - Phenomenology · Physics 2025-08-12 S. Abbaslu , Yasaman Farzan

We consider the decoupling of neutrinos in the early Universe in presence of non-standard neutral current neutrino-electron interactions (NSI). We first discuss a semi-analytical approach to solve the relevant kinetic equations and then…

High Energy Physics - Phenomenology · Physics 2009-11-11 Gianpiero Mangano , Gennaro Miele , Sergio Pastor , Teguayco Pinto , Ofelia Pisanti , Pasquale D. Serpico

Neutrino nonstandard interactions (NSI) were investigated earlier in the solar case and were shown to reduce the tensions between the data and the large mixing angle solution predictions. We extend the previous framework to the supernova…

High Energy Physics - Phenomenology · Physics 2013-05-29 C. R. Das , Joao Pulido

We investigate non-standard neutrino interactions (NSIs) in the Zee--Babu model. The size of NSIs predicted by this model is obtained from a full scan over the parameter space, taking into account constraints from low-energy experiments…

High Energy Physics - Phenomenology · Physics 2009-11-18 Tommy Ohlsson , Thomas Schwetz , He Zhang

We explore the effects of non-standard neutrino interactions (NSI) and how they modify neutrino propagation in the Deep Underground Neutrino Experiment (DUNE). We find that NSI can significantly modify the data to be collected by the DUNE…

High Energy Physics - Phenomenology · Physics 2016-06-22 André de Gouvêa , Kevin J. Kelly

In the traditional neutrinophilic two-Higgs doublet model ($\nu$2HDM), there is no non-standard neutrino interaction (NSI) as the interactions between the Standard Model fermions with neutrinos are negligibly small due to the tiny mixing of…

High Energy Physics - Phenomenology · Physics 2018-09-07 Ujjal Kumar Dey , Newton Nath , Soumya Sadhukhan

We report new constraints on flavor-changing non-standard neutrino interactions (NSI) using data from the MINOS experiment. We analyzed a combined set of beam neutrino and antineutrino data, and found no evidence for deviations from…

We present a detailed analysis on nonstandard neutrino interactions (NSI) with electrons including all muon and electron (anti)-neutrino data from existing accelerators and reactors, in conjunction with the ``neutrino counting'' data (e- e+…

High Energy Physics - Phenomenology · Physics 2008-11-26 J. Barranco , O. G. Miranda , C. A. Moura , J. W. F. Valle

We calculated the size and sign of interference (I) in elastic {\nu}_{e}e-scattering process in the presence of nonstandard neutrino interactions (NSI). The size of interference predicted by standard model (SM) is -1.09, while that measured…

High Energy Physics - Phenomenology · Physics 2011-09-27 Amir Nawaz Khan , Farida Tahir

We introduce a model for Non-Standard neutral current Interaction (NSI) between neutrinos and the matter fields, with an arbitrary coupling to the up and down quarks. The model is based on a new $U(1)$ gauge symmetry with a light gauge…

High Energy Physics - Phenomenology · Physics 2023-02-22 Nicolás Bernal , Yasaman Farzan

Current neutrino experiments measure the neutrino mixing parameters with an unprecedented accuracy. The upcoming generation of experiments will be sensitive to subdominant effects that can give information on the unknown neutrino…

High Energy Physics - Phenomenology · Physics 2018-01-30 Y. Farzan , M. Tortola

We consider Non-Standard neutrino Interactions (NSI), described by four-fermion operators of the form $(\bar{\nu}_{\alpha} \gamma {\nu}_{\beta}) (\bar{f} \gamma f)$, where $f$ is an electron or first generation quark. We assume these…

High Energy Physics - Phenomenology · Physics 2010-04-06 S. Davidson , C. Pena-Garay , N. Rius , A. Santamaria

Theories beyond the Standard Model must respect its gauge symmetry. This implies strict constraints on the possible models of Non-Standard Neutrino Interactions (NSIs). We review here the present status of NSIs from the point of view of…

High Energy Physics - Phenomenology · Physics 2009-11-26 D. Hernandez

We discuss reactor antineutrino oscillations with non-standard interactions (NSIs) at the neutrino production and detection processes. The neutrino oscillation probability is calculated with a parametrization of the NSI parameters by…

High Energy Physics - Phenomenology · Physics 2015-03-23 Yu-Feng Li , Ye-Ling Zhou

The possible non-standard interactions (NSIs) of neutrinos with matter plays important role in the global determination of neutrino properties. In our study we select various data sets from LHC measurements at 13 TeV with integrated…

High Energy Physics - Phenomenology · Physics 2021-02-24 DianYu Liu , ChuanLe Sun , Jun Gao

We derive model-independent bounds on production and detection non-standard neutrino interactions (NSI). We find that the constraints for NSI parameters are around O(10^{-2}) to O(10^{-1}). Furthermore, we review and update the constraints…

High Energy Physics - Phenomenology · Physics 2009-09-28 Carla Biggio , Mattias Blennow , Enrique Fernandez-Martinez

Searching for non-standard neutrino interactions, as a means for discovering physics beyond the Standard Model, has one of the key goals of dedicated neutrino experiments, current and future. We demonstrate here that much of the parameter…

High Energy Physics - Phenomenology · Physics 2020-07-06 Debajyoti Choudhury , Kirtiman Ghosh , Saurabh Niyogi

The discovery of neutrino oscillations implies that neutrinos are massive and mixed, necessitating an extension of the Standard Model, which may require the introduction of non-standard neutrino interactions (NSI). We investigate the…

High Energy Physics - Phenomenology · Physics 2023-08-16 Sudip Jana , Sophie Klett

Non-Standard Interactions (NSI) between neutrinos and matter affect the neutrino flavor oscillations. Due to the high matter density in the core of the Sun, solar neutrinos are suited to probe these interactions. Using the $277$ kton-yr…

High Energy Physics - Experiment · Physics 2022-03-23 Kamiokande Collaboration , P. Weatherly , K. Abe , C. Bronner , Y. Hayato , K. Hiraide , M. Ikeda , K. Iyogi , J. Kameda , Y. Kanemura , Y. Kataoka , Y. Kato , Y. Kishimoto , S. Miki , M. Miura , S. Moriyama , T. Mochizuki , M. Nakahata , Y. Nakano , S. Nakayama , T. Okada , K. Okamoto , A. Orii , G. Pronost , K. Sato , H. Sekiya , M. Shiozawa , Y. Sonoda , Y. Suzuki , A. Takeda , Y. Takemoto , A. Takenaka , H. Tanaka , S. Tasaka , X. Wang , S. Watanabe , T. Yano , S. Han , T. Kajita , K. Kaneyuki , K. Okumura , T. Tashiro , R. Wang , J. Xia , G. D. Megias , L. Labarga , B. Zaldivar , B. W. Pointon , F. d. M. Blaszczyk , C. Kachulis , E. Kearns , J. L. Raaf , J. L. Stone , L. R. Sulak , S. Sussman , L. Wan , T. Wester , S. Berkman , S. Tobayama , J. Bian , M. Elnimr , N. J. Griskevich , W. R. Kropp , S. Locke , S. Mine , M. B. Smy , H. W. Sobel , V. Takhistov , A. Yankelevich , K. S. Ganezer , J. Hill , J. Y. Kim , I. T. Lim , R. G. Park , B. Bodur , Z. Li , K. Scholberg , C. W. Walter , L. Bernard , A. Coffani , O. Drapier , A. Giampaolo , S. El Hedri , J. Imber , Th. A. Mueller , P. Paganini , B. Quilain , A. D. Santos , T. Ishizuka , T. Nakamura , J. S. Jang , J. G. Learned , S. Matsuno , S. Cao , J. Amey , L. H. V. Anthony , R. P. Litchfield , W. Y. Ma , D. Martin , M. Scott , A. A. Sztuc , Y. Uchida , M. O. Wascko , V. Berardi , M. G. Catanesi , R. A. Intonti , E. Radicioni , N. F. Calabria , L. N. Machado , G. De Rosa , G. Collazuol , F. Iacob , M. Lamoureux , M. Mattiazzi , N. Ospina , L. Ludovici , M. Gonin , Y. Maekawa , Y. Nishimura , M. Friend , T. Hasegawa , T. Ishida , M. Jakkapu , T. Kobayashi , T. Matsubara , T. Nakadaira , K. Nakamura , Y. Oyama , K. Sakashita , T. Sekiguchi , T. Tsukamoto , T. Boschi , F. Di Lodovico , J. Gao , T. Katori , J. Migenda , M. Taani , S. Zsoldos , KE. Abe , M. Hasegawa , Y. Isobe , Y. Kotsar , H. Miyabe , H. Ozaki , T. Sugimoto , A. T. Suzuki , Y. Takeuchi , S. Yamamoto , Y. Ashida , J. Feng , T. Hayashino , S. Hirota , M. Jiang , T. Kikawa , M. Mori , T. Nakaya , R. A. Wendell , K. Yasutome , P. Fernandez , N. McCauley , P. Mehta , A. Pritchard , K. M. Tsui , Y. Fukuda , Y. Itow , H. Menjo , M. Murase , K. Frankiewicz , J. Lagoda , S. M. Lakshmi , M. Mandal , P. Mijakowski , Y. S. Prabhu , J. Zalipska , M. Jia , J. Jiang , C. K. Jung , X. Li , J. L. Palomino , G. Santucci , C. Vilela , M. J. Wilking , C. Yanagisawa , D. Fukuda , K. Hagiwara , M. Harada , H. Ishino , S. Ito , H. Kitagawa , Y. Koshio , W. Ma , S. Sakai , M. Sakuda , Y. Takahira , C. Xu , Y. Kuno , G. Barr , D. Barrow , L. Cook , A. Goldsack , S. Samani , C. Simpson , D. Wark , S. Molina Sedgwick , R. Tacik , F. Nova , J. Y. Yang , S. J. Jenkins , M. Malek , J. M. McElwee , O. Stone , M. D. Thiesse , L. F. Thompson , H. Okazawa , Y. Choi , S. B. Kim , J. W. Seo , I. Yu , A. Ichikawa , K. D. Nakamura , K. Nishijima , M. Koshiba , K. Iwamoto , K. Nakagiri , Y. Nakajima , Y. Suda , N. Taniuchi , M. Yokoyama , K. Martens , M. Murdoch , M. R. Vagins , D. Hamabe , S. Izumiyama , M. Kuze , Y. Okajima , T. Yoshida , M. Inomoto , M. Ishitsuka , H. Ito , T. Kinoshita , R. Matsumoto , M. Shinoki , T. Suganuma , M. Yonenaga , J. F. Martin , C. M. Nantais , H. A. Tanaka , T. Towstego , R. Akutsu , P. de Perio , V. Gousy-Leblanc , M. Hartz , A. Konaka , P. de Perio , N. W. Prouse , S. Chen , B. D. Xu , B. Zhang , M. Posiadala-Zezula , D. Hadley , M. Nicholson , M. O'Flaherty , B. Richards , A. Ali , B. Jamieson , P. Giorgio , Ll. Marti , A. Minamino , G. Pintaudi , S. Sano , R. Sasaki , K. Wada