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相关论文: Space-Like Motions of Quantum Zero Mass Neutrinos

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Recently the OPERA collaboration {\cite{opera}} has reported the observation of superluminal neutrinos traveling a distance of 730 km from Grand Sasso Laboratory to CERN.These results contradict the basic tenet of the Theory of Special…

高能物理 - 唯象学 · 物理学 2011-12-13 Jorge Alfaro

The difference in light's travel time from CERN to GPS to Gran Sasso, on the one hand, and light going the direct route in vacuum (mimicked by neutrinos), on the other hand, is analyzed with a modified Robertson test theory of the Lorentz…

综合物理 · 物理学 2011-11-11 Jose G. Vargas

In this paper, we consider the apparent superluminal speed of neutrinos in their travel from CERN to Gran Susso, as measured by the OPERA experiment, within the framework of the Extended Lorentz Transformation Model. The model is based on a…

综合物理 · 物理学 2012-02-28 S. Hamieh

The OPERA experiment reported recently a puzzling result. The time of flight of a neutrino beam between the CERN and the Gran Sasso Laboratory has been measured to be slightly shorter than expected. More precisely, an early arrival time of…

综合物理 · 物理学 2011-10-18 Dominique Monderen

We show that the more energetic superluminal neutrinos with quadratically dispersed superluminalities \delta=\beta^2-1, for \beta=v/c where v is the neutrino velocity, also lose significant energy to radiation to the \nu+e^-+e^+ final state…

高能物理 - 唯象学 · 物理学 2015-06-03 B. F. L. Ward

Based on experimental discovery that the mass-square of neutrino is negative, a quantum equation for superluminal neutrino is proposed in comparison with Dirac equation and Dirac equation with imaginary mass. A virtual particle may also be…

高能物理 - 理论 · 物理学 2007-05-23 Guang-jiong Ni

The OPERA collaboration has claimed that muon neutrinos with mean energy of 17.5 GeV travel 730 km from CERN to the Gran Sasso at a speed exceeding that of light by about 7.5 km/s or 25 ppm. However, we show that such superluminal neutrinos…

高能物理 - 唯象学 · 物理学 2013-05-29 Andrew G. Cohen , Sheldon L. Glashow

During the years 2009 to 2011, neutrino beams were fired repeatedly from CERN towards a detector in Italy's Gran Sasso tunnel, some 4 deg south and 7 deg east of CERN, at a distance of 730.5 km, in the shape of short bunches of particles.…

综合物理 · 物理学 2011-11-17 Wolfgang Kundt

From a mathematical point of view velocities can be larger than c. It has been shown that Lorentz transformations are easily extended in Minkowski space to address velocities beyond the speed of light. Energy and momentum conservation fixes…

高能物理 - 唯象学 · 物理学 2007-05-23 S. Giani

Recently a series of analyses on the flight time of cosmic photons and neutrinos suggests that the speed of light \emph{in vacuo} takes the energy-dependent form $v(E)\simeq 1-E/E_{\text{LIV}}^{\gamma }$ with $E_{\text{LIV}}^{\gamma…

高能物理 - 唯象学 · 物理学 2022-12-14 Hao Li , Bo-Qiang Ma

The LVD time stability allows to establish a time-shift in the OPERA experiment, thus providing the first proof against Superluminal neutrinos, using the horizontal muons of the "Teramo Anomaly". This proof is particularly interesting since…

高能物理 - 实验 · 物理学 2015-06-05 Antonino Zichichi

From the data release of OPERA - CNGS experiment, and publicly announced on 23 September 2011, we cast a phenomenological model based on a Majorana neutrino state carrying a fictitious imaginary mass term, already discussed by Majorana in…

高能物理 - 唯象学 · 物理学 2015-05-30 F. Tamburini , M. Laveder

Neutrinos can gain mass from coupling to an ultralight field in slow roll. When such a field is displaced from its minimum, its vev acts just like the Higgs vev in spontaneous symmetry breaking. Although these masses may eventually vanish,…

高能物理 - 唯象学 · 物理学 2019-09-04 Guido D'Amico , Teresa Hamill , Nemanja Kaloper

The Cosmic Neutrinos Background (\textbf{CNB}) are Primordial Neutrinos decoupled when the Universe was very young. Its detection is complicated, especially if we take into account neutrino mass and a possible breaking of Lorentz Invariance…

天体物理学 · 物理学 2009-02-11 Jorge Alfaro , Pablo González

We review the peculiarities that make neutrino a very special cosmic messenger in high-energy astrophysics, and, in particular, to provide possible indications of deviations from special relativity, as it is suggested theoretically by…

高能物理 - 唯象学 · 物理学 2022-07-01 J. M. Carmona , J. L. Cortes , J. J. Relancio , M. A. Reyes

The OPERA collaboration has claimed the discovery of supeluminal neutrino propagation. However the superluminal interpretation of the OPERA result was refuted by Cohen and Glashow because it was shown that such superluminal neutrinos would…

高能物理 - 唯象学 · 物理学 2011-10-12 Irina Ya. Aref'eva , Igor V. Volovich

Recent experiments by OPERA with high energy neutrinos, as well as astrophysics observation data, may possibly prove violations of underlying principles of special relativity theory. This paper attempts to present an elementary modification…

综合物理 · 物理学 2012-01-30 Yu. I. Bogdanov , A. Yu. Bogdanov

Modified neutrino dispersion relations, which still obey the relativity principle, can have both a superluminal (muon-type) neutrino and a luminal (electron-type) neutrino, as long as neutrino-mass effects can be neglected. The idea is to…

高能物理 - 唯象学 · 物理学 2012-01-24 F. R. Klinkhamer

Within a covariant perturbative field-theoretical approach, the wave-packet modified neutrino propagator is expressed as an asymptotic expansion in powers of dimensionless Lorentz- and rotation-invariant variables. The expansion is valid at…

高能物理 - 唯象学 · 物理学 2022-09-02 Vadim A. Naumov , Dmitry S. Shkirmanov

We pinpoint how a subatomic particle with non-zero mass may attain, in principle, velocities faster-than-light by travelling in helical motion in the limit of very large momentum. This is an educated guess by virtue of the MINOS and OPERA…

综合物理 · 物理学 2011-10-06 E. Canessa
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