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
1988 ◽  
Vol 205 (4) ◽  
pp. 553-558 ◽  
Author(s):  
Keith A. Olive ◽  
Mark Srednicki

1991 ◽  
Vol 368 ◽  
pp. 626 ◽  
Author(s):  
David Dearborn ◽  
Kim Griest ◽  
Georg Raffelt

1990 ◽  
Vol 339 (2) ◽  
pp. 407-416 ◽  
Author(s):  
James G. Bartlett ◽  
Marcelo Gleiser ◽  
Joseph Silk

1990 ◽  
Vol 05 (20) ◽  
pp. 1543-1553 ◽  
Author(s):  
DAVID O. CALDWELL

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.


1988 ◽  
Author(s):  
A. K. Drukier ◽  
Katherine Freese ◽  
Joshua Frieman

Sign in / Sign up

Export Citation Format

Share Document