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Non-standard neutrino-nucleon interaction is formulated and explored within the energy range of quasi-elastic scattering. In particular, the study focuses on the neutral-current elastic (anti)neutrino scattering off nucleons described by…

High Energy Physics - Phenomenology · Physics 2016-12-28 D. K. Papoulias , T. S. Kosmas

The sensitivity of the atmospheric neutrino experiments to the non-standard flavor-dependent interaction in neutrino propagation is studied under the assumption that the only nonvanishing components of the non-standard matter effect are the…

High Energy Physics - Phenomenology · Physics 2016-06-22 Osamu Yasuda

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

Non-standard neutrino interactions (NSI) affect both their propagation through matter and their detection, with bounds on NSI parameters coming from various astrophysical and terrestrial neutrino experiments. In this paper, we show that NSI…

High Energy Physics - Phenomenology · Physics 2017-08-31 Bhaskar Dutta , Shu Liao , Louis E. Strigari , Joel W. Walker

We study the modification of the detected flavor content of ultra high-energy astrophysical neutrinos in the presence of non-standard interactions of neutrinos with the Earth matter. Unlike the case of new physics affecting the propagation…

High Energy Physics - Phenomenology · Physics 2017-02-28 M. C. Gonzalez-Garcia , Michele Maltoni , Ivan Martinez-Soler , Ningqiang Song

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

We quantify our present knowledge of the size and flavor structure of non-standard neutrino interactions which affect the matter background in the evolution of solar, atmospheric, reactor and long-baseline accelerator neutrinos as…

High Energy Physics - Phenomenology · Physics 2020-10-05 Ivan Esteban , M. C. Gonzalez-Garcia , Michele Maltoni , Ivan Martinez-Soler , Jordi Salvado

Imposing non-Abelian discrete flavour symmetries to neutrino non-standard interactions (NSIs) is discussed for the first time. For definiteness, we choose $A_4$ as the flavour symmetry, which is subsequently broken to the residual symmetry…

High Energy Physics - Phenomenology · Physics 2019-03-08 TseChun Wang , Ye-Ling Zhou

We examine the potential to probe generalized neutrino interactions (GNI), exotic effective couplings due to new physics interactions beyond the Standard Model, in the coherent-elastic neutrino-nucleus scattering experiments in light of the…

High Energy Physics - Phenomenology · Physics 2022-03-16 L. J. Flores , Newton Nath , Eduardo Peinado

We consider the potential of a generic neutrino factory (NUFACT) in probing non-standard neutrino-matter interactions (NSI). We find that the sensitivity to flavour-changing (FC) NSI can be substantially improved with respect to present…

High Energy Physics - Phenomenology · Physics 2009-09-17 P. Huber , J. W. F. Valle

New physics beyond the Standard Model (SM) may appear in the form of non-standard neutrino interactions (NSI). We have studied neutral current (anti)neutrino-nucleon scattering in presence of NSI. We obtain that in this scenario, nucleon…

High Energy Physics - Phenomenology · Physics 2025-06-12 Ilma , M. Rafi Alam , L. Alvarez-Ruso , M. Benitez Galan , I. Ruiz Simo , S. K. Singh

Non-Standard neutrino Interactions (NSI) are vector contact interactions involving two neutrinos and two first generation fermions, which can affect neutrino propagation in matter. SU(2) gauge invariance suggests that NSI should be…

High Energy Physics - Phenomenology · Physics 2020-02-24 Sacha Davidson , Martin Gorbahn

We study the effects of non-standard interactions on the oscillation pattern of atmospheric neutrinos. We use neutrino oscillograms as our main tool to infer the role of non-standard interactions (NSI) parameters at the probability level in…

High Energy Physics - Phenomenology · Physics 2016-06-21 Animesh Chatterjee , Poonam Mehta , Debajyoti Choudhury , Raj Gandhi

Thanks to a number of neutrino oscillation and Coherent Elastic neutrino Nucleus Scattering (CE$\nu$NS) experiments, the vector Non-Standard Interactions (NSI) of neutrinos have been well studied and constrained. We show that the…

High Energy Physics - Phenomenology · Physics 2026-01-28 Yasaman Farzan , Saeed Abbaslu

We explore the possibility of probing the nonstandard interactions between the neutrino and a hypothetical massive scalar or pseudoscalar via neutrino flavor transformation in supernovae. We find that in the ultrarelativistic limit, the…

High Energy Astrophysical Phenomena · Physics 2018-06-06 Yue Yang , James P. Kneller

Neutrino non-standard interactions (NSI) with electrons are known to alter the picture of neutrino decoupling from the cosmic plasma. NSI modify both flavour oscillations through matter effects, and the annihilation and scattering between…

High Energy Physics - Phenomenology · Physics 2021-08-17 Pablo F. de Salas , Stefano Gariazzo , Pablo Martínez-Miravé , Sergio Pastor , Mariam Tórtola

Data from solar neutrino and KamLAND experiments have led to a discovery of nonzero neutrino masses. Here we investigate what these data can tell us about neutrino interactions with matter, including the poorly constrained flavor-changing…

High Energy Physics - Phenomenology · Physics 2008-11-26 Alexander Friedland , Cecilia Lunardini , Carlos Pena-Garay

Neutrino oscillation experiments provide a unique tool for probing neutrino-matter interactions, especially those involving the tau neutrino. We describe the sensitivity of the present atmospheric neutrino data to these interactions in the…

High Energy Physics - Phenomenology · Physics 2007-05-23 Alexander Friedland , Cecilia Lunardini , Michele Maltoni

We investigate the effects of a Non-Standard Interaction (NSI) extension of the standard model of particle physics on solar neutrino flavour oscillations. This NSI model introduces a $U_{Z^\prime}(1)$ gauge symmetry through a $Z^\prime$…

High Energy Physics - Phenomenology · Physics 2023-08-31 Ilídio Lopes

The neutral-current (NC) non-standard interactions (NSI) of neutrinos with fermions can modify the flavor oscillations of atmospheric neutrinos as they propagate through the Earth. We present constraints on the NC-NSI parameters…

High Energy Physics - Phenomenology · Physics 2025-12-30 J Krishnamoorthi , Anil Kumar , Sanjib Kumar Agarwalla