English
Related papers

Related papers: Constraints on non-standard flavor-dependent inter…

200 papers

We investigate the effects of neutral current Non-Standard Interactions in propagation on atmospheric neutrino experiments such as Super-Kamiokande and Hyper-Kamiokande. With the ansatz where the parameters which have strong constraints…

High Energy Physics - Phenomenology · Physics 2014-05-20 Shinya Fukasawa

In this talk we discuss the possibility to test the hypothesis, which has been proposed to explain the tension between the mass-squared differences of the solar neutrino and KamLAND experiments by the non-standard flavor-dependent…

High Energy Physics - Phenomenology · Physics 2016-11-01 Osamu Yasuda

In this paper we study non-standard neutrino interactions as an example of physics beyond the standard model using atmospheric neutrino data collected during the Super-Kamiokande I(1996-2001) and II(2003-2005) periods. We focus on…

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 2015-03-30 Shinya Fukasawa , Osamu Yasuda

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 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

It was suggested that a tension between the mass-squared differences obtained from the solar neutrino and KamLAND experiments can be solved by introducing the non-standard flavor-dependent interaction in neutrino propagation. In this paper…

High Energy Physics - Phenomenology · Physics 2017-01-04 Shinya Fukasawa , Osamu Yasuda

The phenomenon of neutrino oscillations has been established as the leading mechanism behind neutrino flavor transitions, providing solid experimental evidence that neutrinos are massive and lepton flavors are mixed. Here we review…

High Energy Physics - Phenomenology · Physics 2013-03-21 Tommy Ohlsson

Many scenarios of new physics predict the existence of neutrino Non-Standard Interactions, new vector contact interactions between neutrinos and first generation fermions beyond the Standard Model. We obtain model-independent constraints on…

High Energy Physics - Phenomenology · Physics 2020-05-20 Jorge Terol-Calvo , Mariam Tórtola , Avelino Vicente

We present a new analysis of non-universal and flavor changing non-standard neutrino interactions (NSI) in \nu_e e or \bar{\nu}_e e scattering. Our global analysis of these process includes all relevant experiments, such as the most recent…

High Energy Physics - Phenomenology · Physics 2009-09-17 J. Barranco , O. G. Miranda , C. A. Moura , J. W. F. Valle

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

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

Theoretical models which present flavor changing neutrino interactions and simultaneously prevent this particle from acquiring any mass exist. We discuss some of them and their predictions for neutrino oscillations in matter which can…

High Energy Physics - Phenomenology · Physics 2007-05-23 M. M. Guzzo , H. Nunokawa , O. L. G. Peres , V. Pleitez , R. Zukanovich Funchal

We have reconsidered the atmospheric neutrino anomaly in light of the laetst data from Super-Kamiokande contained events and from Super-Kamiokande and MACRO up-going muons. We have reanalysed the proposed solution to the atmospheric…

High Energy Physics - Phenomenology · Physics 2010-05-28 N. Fornengo , M. Maltoni , R. Tomas , J. W. F. Valle

It is shown that the results of the Super-Kamiokande atmospheric neutrino experiment, interpreted in terms of nu_mu<--->nu_tau flavor transitions, can probe possible decoherence effects induced by new physics (e.g., by quantum gravity) with…

High Energy Physics - Phenomenology · Physics 2009-10-07 E. Lisi , A. Marrone , D. Montanino

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 review the status of the solutions to neutrino anomalies by flavor-changing as well as flavor-diagonal neutrino interactions. While it is difficult to explain the atmospheric neutrino data the solar neutrino data can be well accounted…

High Energy Physics - Phenomenology · Physics 2009-10-31 Hiroshi Nunokawa

New physics in neutrino sector can reveal itself via non-standard neutrino interactions which can result in modification of the standard picture of neutrino propagation in matter. Experiments with atmospheric neutrinos has been used to…

High Energy Physics - Phenomenology · Physics 2020-04-06 S. V. Demidov

Non-standard neutrino self interactions (NSSI) could be stronger than Fermi interactions. We investigate the ability to constrain these four-neutrino interactions by their effect on the flux of neutrinos originating from a galactic…

High Energy Physics - Phenomenology · Physics 2020-02-19 Minjie Lei , Noah Steinberg , James D. Wells

We study the effect of the non-resonant, vacuum oscillation-like neutrino flavor conversion induced by non-standard flavor changing and non-universal flavor diagonal neutrino interactions with electrons in the sun. We have found an…

High Energy Physics - Phenomenology · Physics 2009-10-31 M. M. Guzzo , H. Nunokawa , P. C. de Holanda , O. L. G. Peres
‹ Prev 1 2 3 10 Next ›