Window for the dark matter solution to the solar neutrino problem

1991 ◽  
Vol 368 ◽  
pp. 626 ◽  
Author(s):  
David Dearborn ◽  
Kim Griest ◽  
Georg Raffelt
Keyword(s):  
Dark Matter ◽  
Solar Neutrino ◽  
Solar Neutrino Problem

Solitonic dark matter and the solar neutrino problem

1990 ◽  
Vol 339 (2) ◽  
pp. 407-416 ◽  
Author(s):  
James G. Bartlett ◽  
Marcelo Gleiser ◽  
Joseph Silk
Keyword(s):  
Dark Matter ◽  
Solar Neutrino ◽  
Solar Neutrino Problem

Cold dark matter candidates and the solar neutrino problem

1985 ◽  
Vol 299 ◽  
pp. 1001 ◽  
Author(s):  
L. M. Krauss ◽  
K. Freese ◽  
D. N. Spergel ◽  
W. H. Press
Keyword(s):  
Dark Matter ◽  
Solar Neutrino ◽  
Cold Dark Matter ◽  
Solar Neutrino Problem

THE SEARCH FOR DARK MATTER

1990 ◽  
Vol 05 (20) ◽  
pp. 1543-1553 ◽  
Author(s):  
DAVID O. CALDWELL
Keyword(s):  
Dark Matter ◽  
Standard Model ◽  
Solar Neutrino ◽  
Particle Physics ◽  
Solar Neutrino Problem ◽  
The Standard Model ◽  
The Universe

The particle constituting probably more than 90% of the mass of the universe is unknown in the Standard Model of particle physics. Non-accelerator experiments, particularly those using Ge and Si detectors, and accelerator experiments, especially at SLC and LEP, have eliminated as dark matter wide classes of candidate particles. Examples are weak isodoublet neutrinos of mass ≳30 eV/c 2, sneutrinos, technibaryons, microcharged shadow matter, and probably Cosmions, which could both be dark matter and solve the solar neutrino problem.

NEUTRINO OSCILLATION AND LEPTON MASS MATRIX

1994 ◽  
Vol 09 (01) ◽  
pp. 41-50 ◽  
Author(s):  
KEN-ITI MATUMOTO ◽  
DAIJIRO SUEMATSU
Keyword(s):  
Solar Neutrino ◽  
Phase Structure ◽  
Quark Mass ◽  
Mass Matrix ◽  
Lepton Sector ◽  
Solar Neutrino Problem ◽  
Quark Sector ◽  
Mass Matrices ◽  
Suppression Mechanism ◽  
The Right

We apply the empirical quark mass matrices to the lepton sector and study the solar neutrino problem and the atmospheric vμ deficit problem simultaneously. We show that their consistent explanation is possible on the basis of these matrices. The lepton sector mass matrices need the phase structure which is different from the ones of the quark sector. However, even if the phase structure of the mass matrices is identical in both sectors, an interesting suppression mechanism of sin 2 2θ12 which is related to the solar neutrino problem can be induced from the right-handed neutrino Majorana mass matrix. We discuss such a possibility through the concrete examples.

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