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Violation of Lorentz invariance (VLI) has been suggested as an explanation of the superluminal velocities of muon neutrinos reported by OPERA. In this note we show that the amount of VLI required to explain this result poses severe…

High Energy Physics - Phenomenology · Physics 2011-12-21 R. Cowsik , S. Nussinov , U. Sarkar

The hypothesis of Lorentz violation in the neutrino sector has intrigued scientists for the last two to three decades. A number of theoretical arguments support the emergence of such violations first and foremost for neutrinos, which…

High Energy Physics - Phenomenology · Physics 2020-10-06 Ulrich D. Jentschura

We use previous work on the Hilbert space for mixed fields to derive deformed dispersion relations for neutrino flavor states. We then discuss how these dispersion relations may be incorporated into frameworks encoding the breakdown of…

High Energy Physics - Phenomenology · Physics 2009-11-10 Massimo Blasone , Joao Magueijo , Paulo Pires-Pacheco

Modern experiments on neutron and allowed nuclear $\beta$ decay search for new semileptonic interactions, beyond the ``left-handed'' electroweak force. We show that ongoing and planned $\beta$-decay experiments, with isotopes at rest and in…

High Energy Physics - Phenomenology · Physics 2015-11-30 K. K. Vos , H. W. Wilschut , R. G. E. Timmermans

High-energy neutrino flares are interesting prospective counterparts to photon flares, as their detection would guarantee the presence of accelerated hadrons within a source, provide precious information about cosmic-ray acceleration and…

High Energy Astrophysical Phenomena · Physics 2020-09-02 Claire Guépin

We perform a covariant wave-packet analysis of neutrino oscillations taking into account the lifetime of the neutrino production process . We find that flavor oscillations in space are washed out when the neutrinos are produced from long…

High Energy Physics - Phenomenology · Physics 2016-09-06 Subhendra Mohanty

Lorentz invariance is a well known fundamental concept of special relativity but its violation is predicted by some variations of quantum gravity, string theory, and some alternatives to general relativity. We study neutrino oscillation at…

High Energy Physics - Phenomenology · Physics 2016-12-30 S. A. Alavi , M. Dehghani Madise

When neutrinos are produced from long lived particles the life-time of the source particle affects the flavour conversion probability formula. Due to this source dependence experiments (like LSND) which use muon decay neutrinos are two…

High Energy Physics - Phenomenology · Physics 2007-05-23 Subhendra Mohanty

The effective-Lagrangian description of Lorentz-invariance violation provided by the so-called Standard-Model Extension covers all the sectors of the Standard Model, allowing for model-independent studies of high-energy phenomena that might…

High Energy Physics - Phenomenology · Physics 2021-03-10 J. Alfonso Ahuatzi-Avendaño , Javier Montaño , Héctor Novales-Sánchez , Mónica Salinas , J. Jesús Toscano

We present an updated and improved global fit analysis of current flavor and electroweak precision observables to derive bounds on unitarity deviations of the leptonic mixing matrix and on the mixing of heavy neutrinos with the active…

Neutrino flavour oscillation is one of the primary indication of the existence of new physics beyond standard model. The presence of small neutrino mass is indispensable to explicate the oscillation among different flavours of neutrino. By…

High Energy Physics - Phenomenology · Physics 2023-01-31 Trisha Sarkar

Astrophysical objects such as active-galactic nuclei (AGN) and gamma-ray bursts (GRBs) can be sources of high energy, astrophysical neutrinos. The decay of charged pions produces electron and muon-flavor neutrinos from the primary decay of…

High Energy Physics - Phenomenology · Physics 2013-01-23 D. Hollander

A search for neutrino oscillations induced by Lorentz violation has been performed using 4,438 live-days of Super-Kamiokande atmospheric neutrino data. The Lorentz violation is included in addition to standard three-flavor oscillations…

High Energy Physics - Experiment · Physics 2015-03-18 Kamiokande Collaboration , K. Abe , Y. Haga , Y. Hayato , M. Ikeda , K. Iyogi , J. Kameda , Y. Kishimoto , M. Miura , S. Moriyama , M. Nakahata , Y. Nakano , S. Nakayama , H. Sekiya , M. Shiozawa , Y. Suzuki , A. Takeda , H. Tanaka , T. Tomura , K. Ueno , R. A. Wendell , T. Yokozawa , T. Irvine , T. Kajita , I. Kametani , K. Kaneyuki , K. P. Lee , T. McLachlan , Y. Nishimura , E. Richard , K. Okumura , L. Labarga , P. Fernandez , J. Gustafson , E. Kearns , J. L. Raaf , S. Berkman , H. A. Tanaka , S. Tobayama , J. L. Stone , L. R. Sulak , M. Goldhaber , G. Carminati , W. R. Kropp , S. Mine , P. Weatherly , A. Renshaw , M. B. Smy , H. W. Sobel , V. Takhistov , K. S. Ganezer , B. L. Hartfiel , J. Hill , W. E. Keig , N. Hong , J. Y. Kim , I. T. Lim , T. Akiri , A. Himmel , K. Scholberg , C. W. Walter , T. Wongjirad , T. Ishizuka , S. Tasaka , J. S. Jang , J. G. Learned , S. Matsuno , S. N. Smith , T. Hasegawa , T. Ishida , T. Ishii , T. Kobayashi , T. Nakadaira , K. Nakamura , Y. Oyama , K. Sakashita , T. Sekiguchi , T. Tsukamoto , A. T. Suzuki , Y. Takeuchi , C. Bronner , S. Hirota , K. Huang , K. Ieki , T. Kikawa , A. Minamino , A. Murakami , T. Nakaya , K. Suzuki , S. Takahashi , K. Tateishi , Y. Fukuda , K. Choi , Y. Itow , G. Mitsuka , P. Mijakowski , J. Hignight , J. Imber , C. K. Jung , C. Yanagisawa , H. Ishino , A. Kibayashi , Y. Koshio , T. Mori , M. Sakuda , R. Yamaguchi , T. Yano , Y. Kuno , R. Tacik , S. B. Kim , H. Okazawa , Y. Choi , K. Nishijima , M. Koshiba , Y. Suda , Y. Totsuka , M. Yokoyama , K. Martens , Ll. Marti , M. R. Vagins , J. F. Martin , P. de Perio , A. Konaka , M. J. Wilking , S. Chen , Y. Zhang , K. Connolly , R. J. Wilkes

The three-flavor neutrino oscillation model describes the well-studied phenomenon of neutrinos produced in association with one charged lepton: electron, muon, or tau, and then later detected in association with a possibly different charged…

High Energy Physics - Phenomenology · Physics 2026-03-25 Peter B. Denton

We examine the parameter space region of the inverse seesaw model that is consistent with neutrino oscillation data. We focus on the correlation between the current limits from the search of the $\mu\to e\gamma$ lepton flavor violating…

High Energy Physics - Phenomenology · Physics 2023-08-28 J. C. Garnica , G. Hernández-Tomé , E. Peinado

Recent evidence appears to confirm that the ultra-high-energy primary cosmic ray spectrum consists mostly of protons. The fact that these protons can traverse large distances to reach Earth allows us to place bounds on Lorentz violations.…

High Energy Physics - Phenomenology · Physics 2008-11-26 Brett Altschul

It can be expected from the result for the atmospheric neutrino by the SUPERKAMIOKANDE and the CHOOZ result that the the lepton-flavor violating (LFV) interaction between the second and third generations exits at the high energy scale. This…

High Energy Physics - Phenomenology · Physics 2007-05-23 J. Hisano

The occurrence of neutrino oscillations demands the existence of flavour violation in charged lepton sector. The relation between the branching ratios of different charged lepton flavour violating (CLFV) decay modes depends on the details…

High Energy Physics - Phenomenology · Physics 2025-03-11 Pravesh Chndra Awasthi , Jai More , Akhila Kumar Pradhan , Kumar Rao , Purushottam Sahu , S. Uma Sankar

Neutrinos from the cosmos have proven to be ideal for probing the nature of space-time. Previous studies on high-energy events of IceCube suggested that some of these events might be gamma-ray burst neutrinos, with their speeds varying…

High Energy Physics - Theory · Physics 2024-05-29 Chengyi Li , Bo-Qiang Ma

When the standard model is extended with right-handed neutrinos the symmetries of the resulting Lagrangian are enlarged with a new global U(1)R Abelian factor. In the context of minimal seesaw models we analyze the implications of a…

High Energy Physics - Phenomenology · Physics 2015-06-11 D. Aristizabal Sierra
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