HackerPapers

arXiv:astro-ph/9701215astro-ph

Unique Signature of Dark Matter in Ancient Mica

Daniel P. Snowden-Ifft, Andrew J. Westphal

Early discovery. Linked by one identifiable commenter. This paper is outside the main ranking; a mention is not an endorsement.

Abstract

Mica can store (for >1 Gy) etchable tracks caused by atoms recoiling from 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.

arXiv comments
5 pages, LaTeX, 2 figures. Accepted for publication at Phys. Rev. Lett
Journal reference
Phys.Rev.Lett. 78 (1997) 1628-1631
DOI
doi:10.1103/PhysRevLett.78.1628
Subjects
astro-phAstrophysics

On Hacker News

Linked by 1 identifiable commenter in 1 comment across 1 thread, from May 2017 to May 2017.

Comments linking this paper, per year.

Discussed in comments1 thread

    • Folks interested in this unusual combination may also be interested in the use of particle tracks to date geological samples > "Techniques for geological dating of minerals by chemical etching of fission fragment tracks" >…

      jessriedelView on HNParent context

Submitted to Hacker News

Connected through shared HN threads, not inferred similarity or a recommendation.