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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…

General Physics · Physics 2011-10-18 Dominique Monderen

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

The OPERA collaboration reported [1] an anomaly in the ratio of the speed of neutrinos to the speed of light of (v-c)/c =(2.48\pm0.28 (stat.) \pm 0.30 (sys.))\times10-5. I identify sources of systematic uncertainty that were not considered…

High Energy Physics - Experiment · Physics 2011-10-12 Juergen Knobloch

Based on the principle of relativity and the postulate of invariant speed and length, we propose the theory of special relativity with cosmological constant ${\cal SR}_{c,R}$ if the invariant length whose square is the inverse of the…

High Energy Physics - Theory · Physics 2009-11-10 Han-Ying Guo , Chao-Guang Huang , Zhan Xu , Bin Zhou

The de Sitter invariant special relativity is a natural extension of the usual Einstein special relativity. Within this framework a generalization of special relativity (SR) for the de Sitter space-time introduces a new length scale $R$,…

High Energy Physics - Phenomenology · Physics 2016-10-28 Daria A. Tretyakova

Deformed Special Relativity (DSR) is a generalization of Special Relativity based on a deformed Minkowski space, i.e. a four-dimensional space-time with metric coefficients depending on the energy. We show that, in the DSR framework, it is…

High Energy Physics - Theory · Physics 2007-05-23 Fabio Cardone , Alessio Marrani , Roberto Mignani

First, we extend the special relativity into the superluminal case and put forward a superluminal theory of kinematics, in which we show that the temporal coordinate need exchanging with one of the spatial coordinates in a superluminal…

General Physics · Physics 2009-07-22 Z. C. Tu , Z. Y. Wan

Doubly special relativity (DSR) is an effective model for encoding quantum gravity in flat spacetime. As a result of the nonlinearity of the Lorentz transformation, the energy-momentum dispersion relation is modified. One simple way to…

General Relativity and Quantum Cosmology · Physics 2015-12-02 Benrong Mu , Peng Wang , Haitang Yang

In the context of theories where particles can have different limiting velocities, we review the running of particle speeds towards a common limiting velocity at low energy. Motivated by the recent OPERA experimental results, we describe a…

High Energy Physics - Phenomenology · Physics 2015-03-19 Mohamed M. Anber , John F. Donoghue

This paper explores whether quantum field theory allows the events of emission and absorption of a single particle to be separated by a space-like interval without violating Lorentz symmetries and causality. Although the answer is indeed…

High Energy Physics - Phenomenology · Physics 2012-04-03 S. P. Horvath , D. Schritt , D. V. Ahluwalia

As 2011 ended, two results stood out which seemed to go against twentieth century ideas. The first was the OPERA superluminal neutrino observation contradicting Special Relativity. The second was lack of a definitive appearance of the Higgs…

General Physics · Physics 2015-02-24 Burra G. Sidharth

Recent results from the SNO, Super-Kamiokande and Borexino experiments do not show the expected upturn of the energy spectrum of events (the ratio $R \equiv N_{obs}/N_{SSM}$) at low energies. At the same time, cosmological observations…

High Energy Physics - Phenomenology · Physics 2015-03-17 P. C. de Holanda , A. Yu. Smirnov

The set of kinetic equations describing the process of conversion of a beam of protons into mesons and then to neutrinos is solved. The asymptotic evolution of the density profile of neutrinos is essentially the same as that obtained in the…

Data Analysis, Statistics and Probability · Physics 2011-10-18 Robert Alicki

We propose that supernova relic neutrino (SRN) observation can be used to set constraints on the neutrino decay models. Because of the long distance scale from cosmological supernovae to the Earth, SRN have possibility to provide much…

High Energy Physics - Phenomenology · Physics 2009-11-10 Shin'ichiro Ando

With the latest astronomical data including Cosmic Microwave Background (WMAP three year, CBI, ACBAR, VSA), Type Ia Supernova ("gold sample"), Galaxy Clustering (SDSS 3-D matter power, Lyman-$\alpha$ forest and Baryon Acoustic Oscillating…

Astrophysics · Physics 2010-10-27 Gong-Bo Zhao , Jun-Qing Xia , Xinmin Zhang

Quantum coherence can significantly increase the strength of the forward scattering of neutrinos propagating through the Earth and interacting with matter. The index of refraction of the neutrinos propagating in a medium and hence their…

High Energy Physics - Phenomenology · Physics 2015-05-30 Ram Brustein , Dmitri Semikoz

To explain both the OPERA experiment and all the known phenomenological constraints/observations on Lorentz violation, the Background Dependent Lorentz Violation (BDLV) has been proposed. We study the BDLV in a model independent way, and…

High Energy Physics - Phenomenology · Physics 2015-05-30 Tianjun Li , Dimitri V. Nanopoulos

Some experiments, performed at Berkeley, Cologne, Florence, Vienna, Orsay, Rennes, etc., led to the claim that something seems to travel with a group velocity larger than the speed c of light in vacuum. Various other experimental results…

Classical Physics · Physics 2016-12-28 Erasmo Recami , Flavio Fontana , Roberto Garavaglia

Scientists from the OPERA experiment have measured neutrinos supposedly travelling at a velocity faster than light contrary to the theory of relativity. Even when the measurements are precise, the interpretation of this problem is being…

General Physics · Physics 2011-10-27 J. Manuel Garcia-Islas

The OPERA neutrino experiment at the underground Gran Sasso Laboratory has measured the velocity of neutrinos from the CERN CNGS beam over a baseline of about 730 km. The measurement is based on data taken by OPERA in the years 2009, 2010…

High Energy Physics - Experiment · Physics 2015-05-30 The OPERA Collaboration , T. Adam , N. Agafonova , A. Aleksandrov , O. Altinok , P. Alvarez Sanchez , A. Anokhina , S. Aoki , A. Ariga , T. Ariga , D. Autiero , A. Badertscher , A. Ben Dhahbi , A. Bertolin , C. Bozza , T. Brugiere , R. Brugnera , F. Brunet , G. Brunetti , S. Buontempo , B. Carlus , F. Cavanna , A. Cazes , L. Chaussard , M. Chernyavsky , V. Chiarella , A. Chukanov , G. Colosimo , M. Crespi , N. D'Ambrosio , G. De Lellis , M. De Serio , Y. Declais , P. del Amo Sanchez , F. Di Capua , A. Di Crescenzo , D. Di Ferdinando , N. Di Marco , S. Dmitrievsky , M. Dracos , D. Duchesneau , S. Dusini , T. Dzhatdoev , J. Ebert , I. Efthymiopoulos , O. Egorov , A. Ereditato , L. S. Esposito , J. Favier , T. Ferber , R. A. Fini , T. Fukuda , A. Garfagnini , G. Giacomelli , M. Giorgini , M. Giovannozzi , C. Girerd , J. Goldberg , C. Gollnitz , D. Golubkov , L. Goncharova , Y. Gornushkin , G. Grella , F. Grianti , E. Gschwendtner , C. Guerin , A. M. Guler , C. Gustavino , C. Hagner , K. Hamada , T. Hara , R. Enikeev , M. Hierholzer , A. Hollnagel , M. Ieva , H. Ishida , K. Ishiguro , K. Jakovcic , C. Jollet , M. Jones , F. Juget , M. Kamiscioglu , J. Kawada , S. H. Kim , M. Kimura , E. Kiritsis , N. Kitagawa , B. Klicek , J. Knuesel , K. Kodama , M. Komatsu , U. Kose , I. Kreslo , C. Lazzaro , J. Lenkeit , A. Ljubicic , A. Longhin , A. Malgin , G. Mandrioli , J. Marteau , T. Matsuo , V. Matveev , N. Mauri , A. Mazzoni , E. Medinaceli , F. Meisel , A. Meregaglia , P. Migliozzi , S. Mikado , D. Missiaen , P. Monacelli , K. Morishima , U. Moser , M. T. Muciaccia , N. Naganawa , T. Naka , M. Nakamura , T. Nakano , Y. Nakatsuka , D. Naumov , V. Nikitina , F. Nitti , S. Ogawa , N. Okateva , A. Olchevsky , O. Palamara , A. Paoloni , B. D. Park , I. G. Park , A. Pastore , L. Patrizii , E. Pennacchio , H. Pessard , C. Pistillo , N. Polukhina , M. Pozzato , K. Pretzl , F. Pupilli , R. Rescigno , F. Riguzzi , T. Roganova , H. Rokujo , G. Rosa , I. Rostovtseva , A. Rubbia , A. Russo , V. Ryasny , O. Ryazhskaya , O. Sato , Y. Sato , Z. Sahnoun , A. Schembri , J. Schuler , L. Scotto Lavina , J. Serrano , I. Shakiryanova , A. Sheshukov , H. Shibuya , G. Shoziyoev , S. Simone , M. Sioli , C. Sirignano , G. Sirri , J. S. Song , M. Spinetti , L. Stanco , N. Starkov , S. Stellacci , M. Stipcevic , T. Strauss , S. Takahashi , M. Tenti , F. Terranova , I. Tezuka , V. Tioukov , P. Tolun , N. T. Tran , S. Tufanli , P. Vilain , M. Vladimirov , L. Votano , J. -L. Vuilleumier , G. Wilquet , B. Wonsak , J. Wurtz , V. Yakushev , C. S. Yoon , J. Yoshida , Y. Zaitsev , S. Zemskova , A. Zghiche