Gaseous dark matter detectors

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 tha...

Full description

Bibliographic Details
Main Authors: Martoff, C. J., Sciolla, Gabriella
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:en_US
Published: Institute of Physics Publishing 2012
Online Access:http://hdl.handle.net/1721.1/70532
_version_ 1826211792634773504
author Martoff, C. J.
Sciolla, Gabriella
author2 Massachusetts Institute of Technology. Department of Physics
author_facet Massachusetts Institute of Technology. Department of Physics
Martoff, C. J.
Sciolla, Gabriella
author_sort Martoff, C. J.
collection MIT
description 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.
first_indexed 2024-09-23T15:11:28Z
format Article
id mit-1721.1/70532
institution Massachusetts Institute of Technology
language en_US
last_indexed 2024-09-23T15:11:28Z
publishDate 2012
publisher Institute of Physics Publishing
record_format dspace
spelling mit-1721.1/705322022-09-29T13:15:32Z Gaseous dark matter detectors Martoff, C. J. Sciolla, Gabriella Massachusetts Institute of Technology. Department of Physics Sciolla, Gabriella Sciolla, Gabriella 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. Massachusetts Institute of Technology. Dept. of Physics United States. Dept. of Energy (contract number DE-FG02-05ER41360) United States. Dept. of Energy (Fermilab) 2012-05-07T19:37:21Z 2012-05-07T19:37:21Z 2009-10 2009-05 Article http://purl.org/eprint/type/JournalArticle 1367-2630 http://hdl.handle.net/1721.1/70532 Sciolla, G, and C J Martoff. “Gaseous Dark Matter Detectors.” New Journal of Physics 11.10 (2009): 105018. Web. en_US http://dx.doi.org/10.1088/1367-2630/11/10/105018 New Journal of Physics Creative Commons Attribution 3.0 http://creativecommons.org/licenses/by/3.0/ application/pdf Institute of Physics Publishing New Journal of Physics
spellingShingle Martoff, C. J.
Sciolla, Gabriella
Gaseous dark matter detectors
title Gaseous dark matter detectors
title_full Gaseous dark matter detectors
title_fullStr Gaseous dark matter detectors
title_full_unstemmed Gaseous dark matter detectors
title_short Gaseous dark matter detectors
title_sort gaseous dark matter detectors
url http://hdl.handle.net/1721.1/70532
work_keys_str_mv AT martoffcj gaseousdarkmatterdetectors
AT sciollagabriella gaseousdarkmatterdetectors