Results 191 to 200 of about 101,723 (259)

Training and onboarding initiatives in high energy physics experiments. [PDF]

open access: yesFront Big Data
Reinsvold Hall A   +18 more
europepmc   +1 more source

The waning of the WIMP: endgame? [PDF]

open access: yesEur Phys J C Part Fields
Arcadi G   +9 more
europepmc   +1 more source

A Bayesian analysis of the solar neutrino problem

open access: green, 1996
C.M. Bhat   +3 more
openalex   +1 more source

Solar-Neutrino Problem and Three-Neutrino Oscillations

Physical Review Letters, 1986
The phenomena of neutrinos changing flavor as they propagate through matter is examined with three neutrino species. The three-neutrino problem separates into two resonances when the mixing angles are small and/or when the mass scales are well separated.
, Kuo, , Pantaleone
openaire   +3 more sources

The solar neutrino problem

Nuclear Instruments and Methods, 1973
The observed capture rate for solar neutrinos in the 37Cl detector is lower than the predicted capture rate. This discrepancy between theory and observation is known as the ‘solar neutrino problem’. I review the basic elements in this problem: the detector efficiency, the theory of stellar (solar) evolution, the nuclear physics of energy generation ...
J. Bahcall
openaire   +2 more sources

Neutrino oscillations and the solar-neutrino problem

Physical Review D, 1987
The values of neutrino masses and mixing angles which are required by the Mikheyev-Smirnov-Wolfenstein (MSW) solution to the solar-neutrino problem are found from analytic solutions to the neutrino propagation equations in the Sun. They coincide with those obtained through extensive numerical computations by Rosen and Gelb.
, Dar, , Mann, , Melina, , Zajfman
openaire   +3 more sources

Solution of the solar-neutrino problem

Physical Review Letters, 1990
Comparison of the results from the Kamiokande neutrino-electron scattering experiment with those from the chlorine experiment and with solar models shows that the explanation of the solar-neutrino problem probably requires physics beyond the standard electroweak model with zero neutrino masses.
, Bahcall, , Bethe
openaire   +3 more sources

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