Unique Signature of Dark Matter in Ancient Mica

Daniel P. Snowden-Ifft and Andrew J. Westphal
Phys. Rev. Lett. 78, 1628 – Published 3 March 1997
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Abstract

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.

  • Received 18 March 1996

DOI:https://doi.org/10.1103/PhysRevLett.78.1628

©1997 American Physical Society

Authors & Affiliations

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

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Vol. 78, Iss. 9 — 3 March 1997

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