Internet Archive Scholar

Gaseous dark matter detectors

(:Unkn) Unknown, University, My
2021

Preserved Fulltext

fulltext thumbnail
Web Archive Capture PDF (815.5 kB)
https://web.archive.org/web/20210226015326/https://scholarshare.temple.edu/bitstream/handle/20.500.12613/6065/Sciolla_2009_New_J._Phys._11_105018.pdf;jsessionid=AC4F043524878B08899CE3824D612AEA?sequence=2

A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2021; you can also visit the original URL. The file type is application/pdf.

Dark matter (DM) detectors with directional sensitivity have the potential of yielding an unambiguous positive observation of WIMPs as well as discriminating between galactic DM halo models. In this paper, we introduce the motivation for directional detectors, discuss the experimental techniques that make directional detection possible, and review the status of the experimental effort in this field. © IOP Publishing Ltd and Deutsche Physikalische Gesellschaft.
doi:10.34944/dspace/6047 fatcat:764h6ryrt5ffxpulalnyvmh72y
Citation

(:Unkn) Unknown, University, My. "Gaseous dark matter detectors." (2021)