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For over 20 years NASA has struggled to find an explanation to the Pioneer anomaly. Now it becomes clear the solution to the riddle is that they have uncovered evidence that c, the speed of light, is not quite a universal constant. Using J.…

General Physics · Physics 2007-05-23 E. D. Greaves

Assuming that neutrinos are spacelike (tachyonic) fermions, we calculate width for the kinematically allowed, lepton number conserving, three-body decay $\nu_{\alpha}\rightarrow \nu_{\alpha} \; \nu_{\beta} \bar{\nu}_{\beta}$ in the Standard…

High Energy Physics - Phenomenology · Physics 2023-10-05 Jakub Rembielinski , Jacek Ciborowski

Gamma-ray bursts (GRBs) are expected to provide a source of ultra high energy cosmic rays, accompanied with potentially detectable neutrinos at neutrino telescopes. Recently, IceCube has set an upper bound on this neutrino flux well below…

High Energy Physics - Phenomenology · Physics 2013-11-21 L. Dorame , O. G. Miranda , J. W. F. Valle

Cosmologically motivated theories that explain small acceleration rate of the Universe via modification of gravity at very large, horizon or super-horizon distances, can be tested by precision gravitational measurements at much shorter…

High Energy Physics - Phenomenology · Physics 2009-11-07 Gia Dvali , Andrei Gruzinov , Matias Zaldarriaga

A review of supersymmetric dark matter in minimal supergravity unification with R-parity invariance and with radiative breaking of the electro-weak symmetry is given. The analysis shows the lightest neutralino is the LSP over most of the…

High Energy Physics - Phenomenology · Physics 2007-05-23 Pran Nath , R. Arnowitt

In this work it is shown, that for short 3ns neutrino pulses reported by OPERA, a relativistic shape deforming effect of the neutrino distribution function due to spontaneous emission, produces an earlier arrival of 65.8ns in agreement with…

High Energy Physics - Phenomenology · Physics 2011-12-06 Rafael Torrealba

One of the cornerstones of special relativity is the postulate that all observers measure exactly the same photon speeds independently on the photon energies. However, a hypothesized structure of spacetime may alter this conclusion at…

High Energy Physics - Phenomenology · Physics 2019-08-14 Vlasios Vasileiou

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

Lorentz invariance is a fundamental symmetry of spacetime and serves as the cornerstone of modern physics, supporting the constancy of the speed of light. A crucial implication of this principle is that no particle can propagate faster than…

High Energy Physics - Phenomenology · Physics 2025-06-26 Yu-Ming Yang , Xing-Jian Lv , Xiao-Jun Bi , Peng-Fei Yin

Electron accelerations of the order of $10^{21} g$ obtained by laser fields open up the possibility of experimentally testing one of the cornerstones of general relativity, the weak equivalence principle, which states that the local effects…

General Relativity and Quantum Cosmology · Physics 2015-06-05 L. Á. Gergely , T. Harko

It continues to be alleged that superluminal influences of any sort would be inconsistent with special relativity for the following three reasons: (i) they would imply the existence of a distinguished' frame; (ii) they would allow the…

History and Philosophy of Physics · Physics 2013-05-22 Kent A. Peacock

Various experiments have shown superluminal group and signal velocities recently. Experiments were essentials carried out with microwave tunnelling, with frustrated total internal reflection, and with gain-assisted anomalous dispersion.…

Classical Physics · Physics 2009-11-06 G. Nimtz , A. A. Stahlhofen , A. Haibel

We revisit the model building challenges that one faces when trying to reconcile the OPERA claim of neutrino superluminality with other observational constraints. The severity of the supernova bound and of the kinematical constraints of…

High Energy Physics - Phenomenology · Physics 2015-06-03 Arthur Hebecker , Alexander Knochel

In quantum tunnelling, what appears an infinitely fast barrier traversal can be explained in terms of an Aharonov-like weak measurement of the tunnelling time, in which the role of the pointer is played by the particle's own coordinate. A…

Quantum Physics · Physics 2007-05-23 D. Sokolovski

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…

High Energy Physics - Phenomenology · Physics 2015-06-03 B. F. L. Ward

The existence of a cosmic neutrino background has been inferred indirectly from cosmological surveys through its effect on the linear-theory evolution of primordial density perturbations, as well as from measurements of the primordial…

Cosmology and Nongalactic Astrophysics · Physics 2024-04-17 Selim C. Hotinli , Nashwan Sabti , Jaxon North , Marc Kamionkowski

We describe an experimental installation for a new test of the weak equivalence principle for neutron. The device is a sensitive gravitational spectrometer for ultra-cold neutrons allowing to precisely compare the gain in kinetic energy of…

Instrumentation and Detectors · Physics 2015-12-09 G. V. Kulin , A. I. Frank , S. V. Goryunov , D. V. Kustov , P. Geltenbort , M. Jentschel , A. N. Strepetov , V. A. Bushuev

This talk reports the latest indications of an anomaly in the measurements of atmospheric neutrinos. New results from Soudan-2 and Super-Kamiokande provide evidence that the ratio of nu_mu to nu_e interactions is not as expected. High…

High Energy Physics - Experiment · Physics 2009-10-31 Edward Kearns

If Lorentz invariance is only an approximate property of equations describing a sector of matter above some critical distance scale, the speed of light c will not necessarily be the only critical speed in vacuum. Superluminal sectors of…

High Energy Physics - Phenomenology · Physics 2008-02-03 Luis Gonzalez-Mestres

On-going projects to discover Type Ia supernovae at redshifts z = 0.3 - 1, coupled with improved techniques to narrow the dispersion in SN Ia peak magnitudes, have renewed the prospects for determining the cosmic deceleration parameter q_0.…

Astrophysics · Physics 2007-05-23 Joshua A. Frieman
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