Detection of galactic 'dark matter' consisting of neutral weakly interacting particles with masses of 1-10 GeV/sq S

Details Detection of galactic 'dark matter' consisting of neutral weakly interacting particles with masses of 1-10 GeV/sq S Detection of galactic 'dark matter' consisting of neutral weakly interacting particles with masses of 1-10 GeV/sq S

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pzetf..49..314b&link_type=abstract

Pis'ma v Zhurnal Eksperimental'noi i Teoreticheskoi Fiziki (ISSN 0370-274X), vol. 49, March 25, 1989, p. 314-317. In Russian.

Physics

Dark Matter, Galactic Structure, Milky Way Galaxy, Neutral Particles, Weak Interactions (Field Theory), Elastic Scattering, Particle Mass, Radiation Measuring Instruments

Scientific paper

The currently existing means of detecting weakly interacting massive particles (WIMP) are briefly reviewed. A method for detecting particles of galactic cold dark matter is then proposed which employs an emission detector using a liquid saturated hydrocarbon as the working medium. The WIMP detector proposed here is capable of detecting particles with a mass as low as 0.7 GeV/sq s.

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