Results 41 to 50 of about 241,450 (255)
Neutrino mixing and neutrino telescopes [PDF]
Measuring flux ratios of ultra-high energy neutrinos is an alternative method to determine the neutrino mixing angles and the CP phase delta. We conduct a systematic analysis of the neutrino mixing probabilities and of various flux ratios measurable at neutrino telescopes.
openaire +2 more sources
Stodolsky's Theorem and Neutrino Oscillation Phases -- for pedestrians [PDF]
Neutrino oscillations are experimentally observable only as a result of interference between neutrino states with different masses and THE SAME ENERGY.
Lipkin, Harry J.
core +6 more sources
Neutrinos are difficult to detect because they weakly interact with matter, making their properties least known. The response of the neutrino detector depends on the optical properties of the liquid scintillator (LS).
Na-Ri Kim, Kyung-Kwang Joo, Hyun-Gi Lee
doaj +1 more source
Decay rate changes in radioactive gamma emission as affected by 18 MeV proton cyclotron [PDF]
Previous efforts to investigate changes in the decay constants of radioactive nuclides discovered that solar flares can temporarily alter radioactive decay rates.
Walg Jonathan, Feldman Jon, Orion Itzhak
doaj +1 more source
$\nu - K^0$ Analogy, Dirac-Majorana Neutrino Duality and the Neutrino Oscillations
The intent of this paper is to convey a new primary physical idea of a Dirac-Majorana neutrino duality in relation to the topical problem of neutrino oscillations.
Bahcall J. N.+7 more
core +2 more sources
Charmonium production at neutrino factories [PDF]
At existing and planned neutrino factories (high energy and high intensity neutrino beam facilities) precision studies of QCD in neutrino-nucleon interactions are a realistic opportunity.
A.D. Martin+17 more
core +2 more sources
Progress in neutrino oscillation searches and their implications
Neutrino Oscillation, in which a given flavour of neutrino transforms into another is a powerful tool for probing small neutrino masses. The intrinsic neutrino properties involved are neutrino mass squared difference $\Delta m^2$ and the mixing angle in ...
A Bandyopadhyay+41 more
core +1 more source
Unification of Neutrino-Neutrino and Neutrino-Antineutrino Oscillations
24pages.
Kimura, Keiichi, Takamura, Akira
openaire +2 more sources
Neutrino and anti-neutrino transport in accretion disks
We numerically solve the one dimensional Boltzmann equation of the neutrino and anti-neutrino transport in accretion disks and obtain the fully energy dependent and direction dependent neutrino and anti-neutrino emitting spectra, under condition that the
M. Ruffert, Ye-Fei Yuan, Zhen Pan
core +1 more source
Sterile Neutrinos in a Grand Unified Model
The recent experimental results indicating the neutrino oscillations may strongly suggest that at least one more light neutrino species is required in order to reconcile the existing data.
Bando, Masako, Yoshioka, Koichi
core +1 more source