Measurement of CNGS muon neutrino speed with Borexino [PDF]
We have measured the speed of muon neutrinos with the Borexino detector using short-bunch CNGS beams. The final result for the difference in time-of-flight between a =17 GeV muon neutrino and a particle moving at the speed of light in vacuum is t = 0.8 \pm 0.7stat \pm 2.9sys ns, well consistent with zero.
Johann Martyn +2 more
exaly +15 more sources
Measurement of sound speed vs. depth in South Pole ice for neutrino astronomy [PDF]
14 pages, 7 ...
Subir Sarkar, James Beatty
exaly +11 more sources
Neutrino interactions in the late universe
The cosmic neutrino background is both a dramatic prediction of the hot Big Bang and a compelling target for current and future observations. The impact of relativistic neutrinos in the early universe has been observed at high significance in a number of
Daniel Green +2 more
doaj +1 more source
Measuring speed of gravitational waves by observations of photons and neutrinos from compact binary mergers and supernovae [PDF]
Detection of gravitational waves (GW) provides us an opportunity to test general relativity in strong and dynamical regimes of gravity. One of the tests is checking whether GW propagates with the speed of light or not. This test is crucial because the velocity of GW has not ever been directly measured.
Nishizawa, Atsushi, Nakamura, Takashi
openaire +3 more sources
Precision measurement of the speed of propagation of neutrinos using the MINOS detectors
10 pages, six figures, after refereeing re-submitted to ...
Adamson, P +122 more
openaire +5 more sources
Description of execution time dynamics for a set of concurrent real-time tasks
A Real-time System (RTS) implemented in a digital computer interacts with the physical world through knowledge variables (sensors, actuators, Analogical - Digital, and Digital-Analogical convertors) processing its requirements through real-time tasks ...
Pedro Guevara López +2 more
doaj +1 more source
Consequences of Neutrino Lorentz Violation For Leptonic Meson Decays [PDF]
If the observation by OPERA of apparently superluminal neutrinos is correct, the Lagrangian for second-generation leptons must break Lorentz invariance. We calculate the effects of an energy-independent change in the neutrino speed on another observable,
Altschul, Brett
core +3 more sources
Observationally Determining the Properties of Dark Matter [PDF]
Determining the properties of the dark components of the universe remains one of the outstanding challenges in cosmology. We explore how upcoming CMB anisotropy measurements, galaxy power spectrum data, and supernova (SN) distance measurements can ...
A. G. Riess +39 more
core +2 more sources
Luminescence of water or ice as a new detection method for magnetic monopoles
Cosmic ray detectors use air as a radiator for luminescence. In water and ice, Cherenkov light is the dominant light producing mechanism when the particle’s velocity exceeds the Cherenkov threshold, approximately three quarters of the speed of light in ...
Pollmann Anna Obertacke
doaj +1 more source
Birth Kick Distributions and the Spin-Kick Correlation of Young Pulsars [PDF]
Evidence from pulsar wind nebula symmetry axes and radio polarization observations suggests that pulsar motions correlate with the spin directions.
Blaauw A. +6 more
core +2 more sources

