A model of superluminal neutrinos

被引：9

作者：

Marfatia, D. ^{[1
]}

Paes, H. ^{[2
]}

Pakvasa, S. ^{[3
]}

Weiler, T. J. ^{[4
]}

机构：

[1] Univ Kansas, Dept Phys & Astron, Lawrence, KS 66045 USA

[2] Tech Univ Dortmund, Fak Phys, D-44221 Dortmund, Germany

[3] Univ Hawaii, Dept Phys & Astron, Honolulu, HI 96822 USA

[4] Vanderbilt Univ, Dept Phys & Astron, Nashville, TN 37235 USA

来源：

PHYSICS LETTERS B | 2012年 / 707卷 / 05期

关键词：

D O I：

10.1016/j.physletb.2012.01.028

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Motivated by the tentative observation of superluminal neutrinos by the OPERA experiment, we present a model of active-sterile neutrino oscillations in which sterile neutrinos are superluminal and active neutrinos appear superluminal by virtue of neutrino mixing. The model demonstrates some interesting possibilities and challenges that apply to a large class of models aiming to explain the OPERA result. (C) 2012 Elsevier B.V. All rights reserved.

引用

页码：553 / 557

页数：5

共 50 条

[31] The superluminal model of pulsars
Ardavan, H
PULSAR ASTRONOMY - 2000 AND BEYOND: IAU COLLOQUIUM 177, 2000, 202 : 365 - 366
[32] Superluminal neutrinos from Lorentz-violating dimension-5 operators
C. A. G. Almeida
M. A. Anacleto
F. A. Brito
E. Passos
The European Physical Journal C, 2012, 72
[33] Superluminal neutrinos from Lorentz-violating dimension-5 operators
Almeida, C. A. G.
Anacleto, M. A.
Brito, F. A.
Passos, E.
EUROPEAN PHYSICAL JOURNAL C, 2012, 72 (01):
[34] A search for the analogue to Cherenkov radiation by high energy neutrinos at superluminal speeds in ICARUS
Antonello, M.
Aprili, P.
Baibussinov, B.
Ceolin, M. Baldo
Benetti, P.
Calligarich, E.
Canci, N.
Carbonara, F.
Centro, S.
Cesana, A.
Cieslik, K.
Cline, D. B.
Cocco, A. G.
Dabrowska, A.
Dequal, D.
Dermenev, A.
Dolfini, R.
Farnese, C.
Fava, A.
Ferrari, A.
Fiorillo, G.
Gibin, D.
Berzolari, A. Gigli
Gninenko, S.
Guglielmi, A.
Haranczyk, M.
Holeczek, J.
Ivashkin, A.
Kisiel, J.
Kochanek, I.
Lagoda, J.
Mania, S.
Mannocchi, G.
Menegolli, A.
Meng, G.
Montanari, C.
Otwinowski, S.
Periale, L.
Piazzoli, A.
Picchi, P.
Pietropaolo, F.
Plonski, P.
Rappoldi, A.
Raselli, G. L.
Rossella, M.
Rubbia, C.
Sala, P. R.
Scantamburlo, E.
Scaramelli, A.
Segreto, E.
PHYSICS LETTERS B, 2012, 711 (3-4) : 270 - 275
[35] Problems with the superluminal pulsar model
Hewish, A
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1996, 280 (03) : L27 - L30
[36] THE PITOWSKY MODEL AND SUPERLUMINAL SIGNALS
JOZSA, R
FOUNDATIONS OF PHYSICS, 1989, 19 (11) : 1327 - 1335
[37] A Model for Neutrinos
Sidharth, B. G.
INTERNATIONAL JOURNAL OF THEORETICAL PHYSICS, 2013, 52 (12) : 4412 - 4415
[38] A Model for Neutrinos
B. G. Sidharth
International Journal of Theoretical Physics, 2013, 52 : 4412 - 4415
[39] SUPERLUMINAL NEUTRINOS Loose Cable May Unravel Faster-Than-Light Result
Cartlidge, Edwin
SCIENCE, 2012, 335 (6072) : 1027 - 1027
[40] Evidence for two neutrino mass eigenstates from SN 1987A and the possibility of superluminal neutrinos
Ehrlich, Robert
ASTROPARTICLE PHYSICS, 2012, 35 (10) : 625 - 628

← 1 2 3 4 5 →