Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
1998-10-29
Phys.Rev.Lett. 82 (1999) 3016-3019
Physics
High Energy Physics
High Energy Physics - Phenomenology
10 pages, 1 figure
Scientific paper
10.1103/PhysRevLett.82.3016
The origin of dark matter in the universe may be scalar particles produced by amplification of quantum fluctuations during a period of dilaton-driven inflation. We show, for the first time, that a single species of particles, depending on its mass and interactions, can be a source of both cold and hot dark matter simultaneously. Detection of such weakly interacting particles with masses below a fraction of an eV presents a new challenge for dark matter searches.
Brustein Ram
Hadad Merav
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