Results 1 to 10 of about 266 (80)

Measurement of sound speed vs. depth in South Pole ice for neutrino astronomy [PDF]

open access: yesAstroparticle Physics, 2010
14 pages, 7 ...
Abbasi, R.   +207 more
openaire   +10 more sources

Measurement of CNGS muon neutrino speed with Borexino [PDF]

open access: yesPhysics Letters B, 2012
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.
Alvarez Sanchez, P.   +105 more
openaire   +9 more sources

Neutrino interactions in the late universe

open access: yesJournal of High Energy Physics, 2021
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]

open access: yesPhysical Review D, 2014
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

open access: yesPhysical Review D, 2015
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

open access: yesRevista Facultad de Ingeniería Universidad de Antioquia, 2012
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

Luminescence of water or ice as a new detection method for magnetic monopoles

open access: yesEPJ Web of Conferences, 2017
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

Whipped and Mixed Warm Clouds in the Deep Sea

open access: yesGeophysical Research Letters, Volume 53, Issue 2, 28 January 2026.
Abstract Turbulence is indispensable to redistribute nutrients for all life forms larger than microbial, on land and in the ocean. Yet, the development of deep‐sea turbulence was not studied in three dimensions to date. As a disproportionate laboratory, an array of nearly 3,000 high‐resolution temperature sensors had been installed for three years on ...
Hans van Haren, KM3NeT collaboration
wiley   +1 more source

Quantum GraviElectro Dynamics

open access: yesAnnalen der Physik, Volume 538, Issue 1, January 2026.
The BRST invariant Lagrangian of the gravitationally interacting U(1)$U(1)$ gauge theory, namely the Quantum GraviElectro Dynamics (QGED). The Yan–Mills theory with the Hilbert–Einstein gravitational Lagrangian, namely the Yang–Mills–Utiyama (YMU) theory, is defined and quantised using the standard procedure. The theory is perturbatively renormalisable,
Yoshimasa Kurihara
wiley   +1 more source

Testing the Weak Cosmic Censorship Conjecture via Test Particle–Induced Overcharging/Overspinning of Kerr–Newman–Modified Gravity Black Hole

open access: yesAdvances in Astronomy, Volume 2026, Issue 1, 2026.
We examine the weak cosmic censorship conjecture (WCCC) violation by throwing a charged and rotating test particle into a Kerr–Newman–modified gravity black hole (KN–MOG BH). The result depends on several factors, such as the relative sign of the particle’s charge and its direction of rotation with respect to black hole (BH).
Waqar Ahmad   +2 more
wiley   +1 more source

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