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Phys. Rev. Lett. 78, 1628–1631 (1997)

Unique Signature of Dark Matter in Ancient Mica

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Daniel P. Snowden-Ifft
Department of Physics, Amherst College, Amherst, Massachusetts 01002

Andrew J. Westphal
Department of Physics, University of California at Berkeley, Berkeley, California 94720

Received 18 March 1996; revised 21 November 1996; published in the issue dated 3 March 1997

Mica can store (for >1Gyr) etchable tracks caused by atoms recoiling from weakly interacting massive particles (WIMPs). Because a background from fission neutrons will eventually limit this technique, a unique signature for WIMPs in ancient mica is needed. Our motion around the center of the Galaxy causes WIMPs, unlike neutrons, to enter the mica from a preferred direction on the sky. Mica is a directional detector and despite the complex rotations that natural mica crystals make with respect to this WIMP “wind,” there is a substantial dependence of etch pit density on present day mica orientation.

© 1997 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.78.1628
DOI:
10.1103/PhysRevLett.78.1628
PACS:
95.35.+d, 07.77.-n, 14.80.Ly, 91.25.Ng