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Related papers: Subluminal OPERA Neutrinos

200 papers

The recent measurement of the neutrino velocity with the OPERA detector in the CNGS beam, on whose basis it was found that (v-c)/c = (2.48 \pm 0.28 (stat.) \pm 0.30 (sys.)) 10e-5, does not contain any significant violation of Local Lorentz…

General Physics · Physics 2012-03-05 F. Cardone , R. Mignani , A. Petrucci

We argue that with the current experimental setup of the OPERA neutrino experiment no `bit' of information faster than light was or could be sent, and therefore no violation of Lorentz symmetry and/or causality was observed.

High Energy Physics - Phenomenology · Physics 2011-10-19 F. Giacosa , P. Kovacs , S. Lottini

In this report are recalled in a simple form some of the main concepts about neutrinos, starting from their discovery and classifying them in the Standard Model of the Microcosm. Then are presented the main natural sources of neutrinos,…

Popular Physics · Physics 2013-04-15 Giorgio Giacomelli

We argue that the neutrino advance of time observed in MINOS and OPERA experiments can be explained in the framework of the standard relativistic quantum theory as a manifestation of the large effective transverse size of the eigenmass…

High Energy Physics - Phenomenology · Physics 2011-10-06 Dmitry V. Naumov , Vadim A. Naumov

A recent measurement of neutrino velocity by the OPERA experiment and prediction of energy loss of superluminal neutrino via the pair creation process $\nu\to \nu e^+e^-$ stimulated a search of isolated $e^+e^-$ pairs in detectors with good…

High Energy Physics - Phenomenology · Physics 2013-03-13 Paolo Walter Cattaneo

It has been recently suggested by Dvali and Vikman that the superluminal neutrino phenomenology of the OPERA experiment may be due to an environmental feature of the Earth, naturally yielding a long-range fifth force of gravitational origin…

General Relativity and Quantum Cosmology · Physics 2015-03-19 Lorenzo Iorio

We tried to fit in any way the recent Opera-Cern claims of a neutrino super-luminal speed with observed Supernova SN1987A neutrino burst and all (or most) neutrino flavor oscillation. We considered three main frame-works: (1) A tachyon…

High Energy Astrophysical Phenomena · Physics 2012-06-15 D. Fargion , D. D'Armiento

The effect of nonlinear self-interaction can be associated with superluminal velocity of neutrino. The power energy spectrum E=p+Cp^a is derived from the nonlinear Dirac equation when interaction term V=\lambda (\psi \gamma_\mu \psi \psi…

High Energy Physics - Phenomenology · Physics 2012-01-11 Ernst Trojan

We ask whether the recent OPERA results on neutrino superluminality could be an environmental effect characteristic of the local neighborhood of our planet, without the need of violation of the Poincar\'e-invariance at a fundamental level.…

High Energy Physics - Phenomenology · Physics 2012-03-05 Gia Dvali , Alexander Vikman

We analyze the possibility of superluminal neutrino propagation delta v = (v - c)/c > 0 as indicated by OPERA data, in view of previous phenomenological constraints from supernova SN1987a and gravitational Cerenkov radiation. We argue that…

High Energy Physics - Phenomenology · Physics 2015-05-30 Jean Alexandre , John Ellis , Nick E. Mavromatos

OPERA collaboration has reported evidence of superluminal phenomenon for neutrinos. One of the possible ways to explain the superluminality is to have Lorentz symmetry violated. It has been shown that dispersion relations put forwards has…

High Energy Physics - Phenomenology · Physics 2015-06-03 Gang Guo , Xiao-Gang He

We discuss the kinematic limits for the process \nu_\mu \rightarrow \nu_\mu + e^+ + e^- in the assumption that neutrinos are superluminal. We derive our results by assuming that: i) it exists one reference frame in which energy and momentum…

High Energy Physics - Phenomenology · Physics 2011-10-21 F. L. Villante , F. Vissani

The OPERA experiment is a long baseline neutrino oscillation experiment aimed at observing the $\nu_{\mu} \rightarrow \nu_{\tau} $ neutrino oscillation in the CERN neutrino to Gran Sasso beamline in the appearance mode by detecting the…

High Energy Physics - Experiment · Physics 2019-08-13 Thomas Strauss

In this paper, we consider the problem of quantum measurement of neutrino velocity. We show, that the well known neutrino flavor oscillations are always accompanied by the oscillations of neutrino velocity. In particular, the velocity of a…

High Energy Physics - Phenomenology · Physics 2015-04-02 Branislav Sazdović , Milovan Vasilić

We revisit the bremsstrahlung process of a superluminal neutrino motivated by OPERA results. From a careful analysis of the plane wave solutions of the superluminal neutrino, we find that the squared matrix elements contain additional terms…

High Energy Physics - Phenomenology · Physics 2015-06-03 Fedor Bezrukov , Hyun Min Lee

If the observation by OPERA of apparently superluminal neutrinos is correct, the Lagrangian for second-generation leptons must break Lorentz invariance. We calculate the effects of an energy-independent change in the neutrino speed on…

High Energy Physics - Phenomenology · Physics 2011-11-15 Brett Altschul

While the OPERA experimental scrutiny is ongoing in the community, in the present article we construct a toy model of {\it extended Lorentz code} (ELC) of the uniform motion, which will be a well established consistent and unique…

General Physics · Physics 2013-03-07 G. Ter-Kazarian

In the context of the sensational results concerning superluminal velocities, announced recently by the OPERA Collaboration, we have proposed a classical model yielding a statistically calculated measured velocity of a beam, higher than the…

Data Analysis, Statistics and Probability · Physics 2015-03-13 Bogusław Broda

The neutrino speed measurement experiments are the continuations of the classic light speed measurement experiments have been done in range of the solar planet system (Ole Roemer, 1676), in star system (James Braidely, 1728) and, at last,…

High Energy Physics - Phenomenology · Physics 2013-02-06 D. S. Baranov , G. G. Volkov
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