A search for strongly interacting dark matter

Physics

Scientific paper

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Scientific paper

A silicon semiconductor detector near the top of the atmosphere is used to search for strongly interacting particles in our galactic halo. The data exclude, as the dominant component of the halo, such particles with masses between ~ 2 GeV/c2 and 105 GeV/c2. Comparisons are made with a previously reported subterranean search for weakly interacting halo particles.

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