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Cold, ultralight ($\ll$ eV) bosonic dark matter with a misalignment abundance can induce temporal variation in the masses and couplings of Standard Model particles. We find that fast variations in neutrino oscillation parameters can lead to…

High Energy Physics - Phenomenology · Physics 2018-04-25 Gordan Krnjaic , Pedro A. N. Machado , Lina Necib

The discovery of the acceleration of the rate of expansion of the Universe fosters new explorations of the behavior of gravitation theories in the cosmological context. Either the GR framework is valid but a cosmic component with a negative…

General Relativity and Quantum Cosmology · Physics 2010-11-02 Pilar Ruiz-Lapuente

The search for neutrinos emitted in coincidence with Gamma-Bay Burst has been so far unsuccessfully. In this paper we show that the recent result reported by the OPERA Collaboration on an early arrival time of muon neutrinos with respect to…

High Energy Physics - Phenomenology · Physics 2015-05-30 D. Autiero , P. Migliozzi , A. Russo

Dark matter represents currently an outstanding problem in both cosmology and particle physics. In this review we discuss the possible explanations for dark matter and the experimental observables which can eventually lead to the discovery…

High Energy Physics - Phenomenology · Physics 2021-04-26 A. Arbey , F. Mahmoudi

In spring 2012 CERN provided two weeks of a short bunch proton beam dedicated to the neutrino velocity measurement over a distance of 730 km. The OPERA neutrino experiment at the underground Gran Sasso Laboratory used an upgraded setup…

High Energy Physics - Experiment · Physics 2015-06-12 The OPERA Collaboration , T. Adam , N. Agafonova , A. Aleksandrov , A. Anokhina , S. Aoki , A. Ariga , T. Ariga , D. Autiero , A. Badertscher , A. Ben Dhahbi , M. Beretta , A. Bertolin , C. Bozza , T. Brugière , R. Brugnera , F. Brunet , G. Brunetti , B. Buettner , S. Buontempo , B. Carlus , F. Cavanna , A. Cazes , L. Chaussard , M. Chernyavsky , V. Chiarella , A. Chukanov , N. D'Ambrosio , G. De Lellis , M. De Serio , P. del Amo Sanchez , A. Di Crescenzo , D. Di Ferdinando , N. Di Marco , S. Dmitrievsky , M. Dracos , D. Duchesneau , S. Dusini , T. Dzhatdoev , J. Ebert , A. Ereditato , L. S. Esposito , J. Favier , G. Felici , T. Ferber , R. A. Fini , T. Fukuda , A. Garfagnini , G. Giacomelli , C. Girerd , C. Goellnitz , J. Goldberg , D. Golubkov , Y. Gornushkin , G. Grella , F. Grianti , C. Guerin , A. M. Guler , C. Gustavino , C. Hagner , K. Hamada , T. Hara , M. Hierholzer , A. Hollnagel , H. Ishida , K. Ishiguro , K. Jakovcic , C. Jollet , C. Kamiscioglu , M. Kamiscioglu , J. Kawada , J. H. Kim , S. H. Kim , M. Kimura , N. Kitagawa , B. Klicek , K. Kodama , M. Komatsu , U. Kose , I. Kreslo , A. Lauria , C. Lazzaro , J. Lenkeit , A. Ljubicic , A. Longhin , C. Mancini-Terracciano , A. Malgin , G. Mandrioli , J. Marteau , T. Matsuo , V. Matveev , N. Mauri , E. Medinaceli , A. Meregaglia , P. Migliozzi , S. Mikado , P. Monacelli , M. C. Montesi , K. Morishima , U. Moser , M. T. Muciaccia , M. Nakamura , T. Nakano , Y. Nakatsuka , D. Naumov , V. Nikitina , S. Ogawa , A. Olchevsky , K. Ozaki , O. Palamara , A. Paoloni , B. D. Park , I. G. Park , A. Pastore , L. Patrizii , E. Pennacchio , H. Pessard , C. Pistillo , D. Podgrudkov , N. Polukhina , M. Pozzato , K. Pretzl , F. Pupilli , R. Rescigno , M. Roda , T. Roganova , H. Rokujo , G. Rosa , I. Rostovtseva , A. Rubbia , A. Russo , O. Ryazhskaya , O. Sato , Y. Sato , A. Schembri , W. Schmidt-Parzefall , J. Schuler , 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. M. Stellacci , M. Stipcevic , T. Strauss , S. Takahashi , M. Tenti , F. Terranova , V. Tioukov , P. Tolun , S. Tufanli , P. Vilain , M. Vladimirov , L. Votano , J. L. Vuilleumier , G. Wilquet , B. Wonsak , J. Wurtz , C. S. Yoon , J. Yoshida , Y. Zaitsev , S. Zemskova , A. Zghiche , R. Zimmermann

Sensitive dark matter (DM) experiments can be well exploited beyond their designated targets, allowing to explore a breadth of physics topics. As we discuss, future large direct DM detection experiments constitute impressive telescopes,…

High Energy Physics - Phenomenology · Physics 2022-03-02 Volodymyr Takhistov

It is shown that the recently detected acceleration of the universe can be understood by considering a modification of the teleparallel equivalent of General Relativity (TEGR), with no need of dark energy. The solution also exhibits phases…

Astrophysics · Physics 2009-07-30 Gabriel Bengochea , Rafael Ferraro

In this paper we review a part of the approaches that have been considered to explain the extraordinary discovery of the late time acceleration of the Universe. We discuss the arguments that have led physicists and astronomers to accept…

Cosmology and Nongalactic Astrophysics · Physics 2010-12-13 Domenico Sapone

Recently, Cohen and Glashow [A.G. Cohen, S.L. Glashow, Phys. Rev. Lett. {\bf 107}, 181803 (2011)] pointed out that the superluminal neutrinos reported by the OPERA would lose their energy rapidly via the Cherenkov-like process. The…

High Energy Physics - Phenomenology · Physics 2012-03-27 Zhe Chang , Xin Li , Sai Wang

Since some experiments have found superluminality, we assume that the particles in the universe are divided into three classes: the subluminal, luminal and superluminal particles by the speed of light, their energy-momenum relations are E2…

General Physics · Physics 2011-11-29 An Yong Li

In this paper I discuss whether superluminal particles exist in the general relativistic theory of gravity. It seems that the answer to this question is negative. In truth the result may only represent a difficulty to {\bf special} but not…

General Relativity and Quantum Cosmology · Physics 2013-06-18 Asher Yahalom

Velocity-dependent interactions in a fundamental-string dominated universe lead quite naturally, with reasonable assumptions on initial conditions, to an accelerating expanding universe without assuming the existence of a cosmological…

Astrophysics · Physics 2009-11-07 Ramzi R. Khuri

In the brane-world scenario, our universe is understood as a three dimensional hypersurface embedded in a higher dimensional space-time. The fluctuations of the brane along the extra dimensions are seen from the four-dimensional point of…

High Energy Physics - Phenomenology · Physics 2007-05-23 J. A. R. Cembranos , A. Dobado , A. L. Maroto

Experimental evidence and theoretical argument in favor the claim of neutrino being likely a superluminal particle, a tachyon, are discussed from six aspects with details.

High Energy Physics - Phenomenology · Physics 2007-05-23 Guang-Jiong Ni

Solitons in space-time capable of transporting time-like observers at superluminal speeds have long been tied to violations of the weak, strong, and dominant energy conditions of general relativity. This trend was recently broken by a new…

General Relativity and Quantum Cosmology · Physics 2022-01-04 Erik W. Lentz

A physical metric is introduced as one that directly gives experimental data without further coordinate transformation. It will be shown that the geodesic equation for the Schwartzschild metric does not give the correct expression for the…

General Physics · Physics 2011-11-29 Yukio Tomozawa

We consider the matter effects on neutrinos moving in background on the basis of the corresponding quantum wave equations. Both Dirac and Majorana neutrino cases are discussed. The effects for Dirac neutrino reflection and trapping as well…

High Energy Physics - Phenomenology · Physics 2008-11-26 Alexander Grigoriev , Alexander Studenikin , Alexei Ternov

We constrain Horava-Lifshitz gravity using the results of OPERA and ICARUS neutrino speed experiments, which show that neutrinos are luminal particles, examining the fermion propagation in the earth's gravitational field. In particular,…

General Relativity and Quantum Cosmology · Physics 2013-01-29 Emmanuel N. Saridakis

Several lines of evidence suggest that some of the dark matter may be non-baryonic: the non-detection of various plausible baryonic candidates for dark matter inferred, e.g., from galaxy rotation curves and from cluster of galaxy velocity…

Astrophysics · Physics 2007-05-23 David N. Spergel

Observations of an apparent acceleration in the expansion rate of the universe, derived from measurements of high-redshift supernovae, have been used to support the hypothesis that the universe is permeated by some form of dark energy. We…

General Relativity and Quantum Cosmology · Physics 2007-05-23 Robin Booth
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