New signatures and sources for the detection of WIMP dark matter in the solar system1

Lawrence M. Krauss

doi:10.1016/S0370-1573(98)00066-0

New signatures and sources for the detection of WIMP dark matter in the solar system¹

Lawrence M. Krauss

Arizona State University

Research output: Contribution to journal › Article › peer-review

Abstract

I first outline new results on the angular modulation of WIMP dark matter scattering on targets in terrestrial laboratories, based on our uncertainties of the WIMP halo distribution, I then outline an exciting new result which indicates that for the high end of allowed SUSY WIMP scattering cross sections there exists a new distribution of WIMP dark matter in our solar system which could produce a dramatically different signal from halo WIMP dark matter in terrestrial detectors.

Original language	English (US)
Pages (from-to)	235-241
Number of pages	7
Journal	Physics Report
Volume	307
Issue number	1-4
DOIs	https://doi.org/10.1016/S0370-1573(98)00066-0
State	Published - Dec 1 1998

Keywords

95.35.+d

ASJC Scopus subject areas

General Physics and Astronomy

Access to Document

10.1016/S0370-1573(98)00066-0

Cite this

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title = "New signatures and sources for the detection of WIMP dark matter in the solar system1",

abstract = "I first outline new results on the angular modulation of WIMP dark matter scattering on targets in terrestrial laboratories, based on our uncertainties of the WIMP halo distribution, I then outline an exciting new result which indicates that for the high end of allowed SUSY WIMP scattering cross sections there exists a new distribution of WIMP dark matter in our solar system which could produce a dramatically different signal from halo WIMP dark matter in terrestrial detectors.",

keywords = "95.35.+d",

author = "Krauss, {Lawrence M.}",

note = "Funding Information: Research supported in part by DOE. ",

year = "1998",

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AB - I first outline new results on the angular modulation of WIMP dark matter scattering on targets in terrestrial laboratories, based on our uncertainties of the WIMP halo distribution, I then outline an exciting new result which indicates that for the high end of allowed SUSY WIMP scattering cross sections there exists a new distribution of WIMP dark matter in our solar system which could produce a dramatically different signal from halo WIMP dark matter in terrestrial detectors.

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