Results 1 to 10 of about 1,007 (87)
Nuclear Physics A, 2003 10 pages, 2 figures. Invited talk at 18th International Conference on Particles and Nuclei (PANIC 08), Eilat, Israel, 9-14 Nov ...
Bellotti, E. +3 more
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Neutrino interaction physics in neutrino telescopes [PDF]
The European Physical Journal Special Topics, 2021 AbstractNeutrino telescopes can observe neutrino interactions starting at GeV energies by sampling a small fraction of the Cherenkov radiation produced by charged secondary particles. These experiments instrument volumes massive enough to collect substantial samples of neutrinos up to the TeV scale as well as small samples at the PeV scale. This unique
Teppei Katori +2 more
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AIP Conference Proceedings, 1999 These lectures describe some aspects of the physics of massive neutrinos. After a brief introduction of neutrinos in the Standard Model, I discuss possible patterns for their masses. In particular, I show how the presence of a large Majorana mass term for the right-handed neutrinos can engender tiny neutrino masses for the observed neutrinos.
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American Journal of Physics, 2000 The basic concepts of neutrino physics are presented at a level appropriate for integration into elementary courses on quantum mechanics and/or modern physics.
Haxton, WC, Holstein, BR
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Physics with reactor neutrinos [PDF]
Reports on Progress in Physics, 2019 Neutrinos produced by nuclear reactors have played a major role in advancing our knowledge of the properties of neutrinos. The first direct detection of the neutrino, confirming its existence, was performed using reactor neutrinos. More recent experiments utilizing reactor neutrinos have also found clear evidence for neutrino oscillation, providing ...
Xin Qian, Jen-Chieh Peng
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Journal of Physics: Conference Series, 2005 Lectures presented by Paul Langacker at the 11th Mexican School of Particles and Fields, Xalapa, Ver., Mexico, August 2004 (33 pages)
Langacker, Paul +2 more
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Solar neutrinos: Solar physics and neutrino physics [PDF]
Nuclear Physics B - Proceedings Supplements, 1994 Abstract It is shown that the current solar neutrino situation, with results from the Homestake experiment, the Kamiokande experiment, GALLEX and SAGE is unfortunately still ambiguous. The differences between observations and the standard solar theory may still be due to either astrophysical inputs or new neutrino physics.
D.N. Schramm, X. Shi
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EXPERIMENTAL NEUTRINO PHYSICS [PDF]
International Journal of Modern Physics A, 2005 The current experimental status of neutrino physics is reviewed. It contains the evidences for a non-vanishing neutrino rest mass from neutrino oscillation searches. In addition an outlook is given on determining the various mixing matrix elements and mass differences more precisely with new experiments.
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NEUTRINO PHYSICS (THEORY) [PDF]
High Energy Physics, 2005 Nonzero neutrino masses are the first definitive need to extend the standard model. After reviewing the basic framework, I describe the status of some of the major issues, including tests of the basic framework of neutrino masses and mixings; the question of Majorana vs.
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Nuclear Physics B - Proceedings Supplements, 1994 Present limits on neutrino masses are briefly reviewed, along with cosmological and astrophysical hints from dark matter, solar and atmospheric neutrino observations that suggest neutrino masses. These would imply many possible new phenomena such as neutrinoless $ $ decay, lepton flavour violating processes such as neutrino oscillations, $ \ra e $
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