Results 131 to 140 of about 24,404 (180)

Micromegas with GEM preamplification for enhanced energy threshold in low-background gaseous time projection chambers. [PDF]

open access: yesOpen Res Eur
Castel Pablo JF   +15 more
europepmc   +1 more source

The solar neutrino problem

AIP Conference Proceedings, 1979
A summary of the results of the Brookhaven solar neutrino experiment is given and discussed in relation to solar‐model calculations. A review is given of the merits of various new solar neutrino detectors that have been proposed.
B T Cleveland
exaly   +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   +2 more sources

Solving the Solar Neutrino Problem

Scientific American Sp, 2003
Building a detector the size of a 10-story building two kilometers underground is a strange way to study solar phenomena. Yet that has turned out to be the key to unlocking a decades-old puzzle about the physical processes occurring inside the sun. English physicist Arthur Eddington suggested as early as 1920 that nuclear fusion powered the sun, but ...
Arthur B, McDonald   +2 more
openaire   +2 more sources

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