Results 141 to 150 of about 241,450 (255)
, 2003 The general status of neutrino physics are given. The history of the neutrino, starting from Pauli and Fermi, is presented. The phenomenological V-A theory of the weak interaction and the unified theory of the weak and electromagnetic interactions, the so-called Standard Model, are discussed.
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Solar Neutrino Cross Sections and Nuclear Beta Decay [PDF]
, 1964 John N. Bahcall
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Neutrino amplitude decomposition, S matrix rephasing invariance, and reparametrization symmetry
Journal of High Energy PhysicsThe S matrix rephasing invariance is one of the fundamental principles of quantum mechanics that originates in its probabilistic interpretation. For a given S matrix which describes neutrino oscillation, one can define the two different rephased ...
Hisakazu Minakata
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On the angular distribution of the brookhaven 1962 neutrino experiment [PDF]
, 1963 J. Løvseth
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Neutrino at Different Epochs of the Friedmann Universe
UniverseAt least two relics of the Big Bang have survived: the cosmological microwave background (CMB) and the cosmological neutrino background (CνB). Being the second most abundant particle in the universe, the neutrino has a significant impact on its evolution
Alexandre V. Ivanchik +2 more
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Effect of a Degenerate Neutrino Sea on Electromagnetism [PDF]
, 1968 Jeffrey Paul Royer
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Non-localité et dissymétrie de l'interaction électron-neutrino dans le mode Ke3 [PDF]
, 1963 Charles Chahine, B. Jouvet
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Supernova Neutrino Neutrino Astronomy
, 2018 Modern neutrino facilities will be able to detect a large number of neutrinos from the next Galactic supernova. We investigate the viability of the triangulation method to locate a core-collapse supernova by employing the neutrino arrival time differences at various detectors.
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