Laboratory Limits on Galactic Cold Dark Matter

D. O. Caldwell, R. M. Eisberg, D. M. Grumm, M. S. Witherell, B. Sadoulet, F. S. Goulding, and A. R. Smith
Phys. Rev. Lett. 61, 510 – Published 1 August 1988
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Abstract

Interesting limits are set on candidates for cold-dark-matter particles in the halo of our Galaxy from their interaction with a very-low-background Ge detector used to search for double-β decay. Dirac neutrinos constituting all of dark matter are excluded for masses between 12 GeV/c2 and 1.4 TeV/c2. There are slightly better limits on magninos and cosmions, proposed massive particles which also explain the solar-neutrino problem but which interact more strongly with Ge. In addition, millicharged shadow matter is ruled out as the main form of dark matter.

  • Received 13 November 1987

DOI:https://doi.org/10.1103/PhysRevLett.61.510

©1988 American Physical Society

Authors & Affiliations

D. O. Caldwell, R. M. Eisberg, D. M. Grumm, and M. S. Witherell

  • Department of Physics, University of California, Santa Barbara, California 93106

B. Sadoulet

  • Physics Department, University of California, Berkeley, California 94720

F. S. Goulding and A. R. Smith

  • Lawrence Berkeley Laboratory, Berkeley, California 94720

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Vol. 61, Iss. 5 — 1 August 1988

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