Results 101 to 110 of about 302 (148)

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

Open Res Eur
Castel Pablo JF, Cebrián Guajardo S, Dafni T, Díez Ibáñez D, Galán Lacarra J, García Pascual JA, Ezquerro Sastre Á, García Irastorza I, Luzón Marco G, Margalejo Blasco C, Mirallas Sánchez H, Obis Aparicio L, Ortiz de Solórzano A, Pérez Lázaro Ó, Porrón Lafuente J, Jiménez Puyuelo M.   +15 more
europepmc   +1 more source

Mathematical Modeling of Physical Reality: From Numbers to Fractals, Quantum Mechanics and the Standard Model. [PDF]

Entropy (Basel)
Kupczynski M.
europepmc   +1 more source

Spectral synthesis techniques for supernovae and kilonovae. [PDF]

Living Rev Comput Astrophys
Jerkstrand A.
europepmc   +1 more source

The Solar Neutrino Problem [PDF]

Annual Review of Astronomy and Astrophysics, 1995
The solar neutrino problem has persisted for almost three decades. Recent results from Kamiokande, SAGE, and GALLEX indicate a pattern of neutrino fluxes that is very difficult to reconcile with plausible variations in standard solar models. This situation is reviewed, and suggested particle physics solutions are discussed.
W C Haxton
exaly   +3 more sources

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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

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, J C Evans
exaly   +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, Joshua R, Klein, David L, Wark   +2 more
openaire   +2 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   +2 more sources

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   +2 more sources