An ultralow background spectrometer is used as a detector of cold dark matter candidates from the halo of our galaxy. Using a realistic model for the galactic halo, large regions of the mass-cross section space are excluded for important halo component particles. In particular, a halo dominated by heavy standard Dirac neutrinos (taken as an example of particles with spin-independent Z0 exchange interactions) with masses between 20 GeV and 1 TeV is excluded. The local density of heavy standard Dirac neutrinos is <0.4 GeV/cm3 for masses between 17.5 GeV and 2.5 TeV, at the 68% confidence level.
|Original language||English (US)|
|Number of pages||6|
|Journal||Physics Letters B|
|State||Published - Sep 17 1987|
All Science Journal Classification (ASJC) codes
- Nuclear and High Energy Physics