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P. J. Fox, G. D. Kribs, and T. M. Tait, Interpreting Dark Matter Direct Detection Independently of the Local Velocity and Density Distribution
Original
1910
Earlier work this paper cites.
P. J. Fox, J. Liu, and N. Weiner, Integrating Out Astrophysical Uncertainties
Original
1915
Earlier work this paper cites.
S. Sarkar, Nonbaryonic dark matter , in NATO ASI Proc. 348: “Observational tests of cosmological inflation” , Durham, 1990, pp. 91-102
1990
Earlier work this paper cites.
R. J. Barlow, Extended maximum likelihood
1990
Earlier work this paper cites.
J. D. Lewin and P. F. Smith, Review of mathematics, numerical factors, and corrections for dark matter experiments based on elastic nuclear recoil
1996
Earlier work this paper cites.
G. J. Feldman and R. D. Cousins, A Unified approach to the classical statistical analysis of small signals
1998
Earlier work this paper cites.
G. Gelmini and P. Gondolo, WIMP annual modulation with opposite phase in Late-Infall halo models
2001
Earlier work this paper cites.
D. Tucker-Smith and N. Weiner, Inelastic dark matter
2001
Earlier work this paper cites.
S. Yellin, Finding an upper limit in the presence of an unknown background
2002
Earlier work this paper cites.
A. M. Green, Calculating exclusion limits for weakly interacting massive particle direct detection experiments without background subtraction
2002
Earlier work this paper cites.
A. Kurylov and M. Kamionkowski, Generalized analysis of weakly-interacting massive particle searches
2004
Earlier work this paper cites.
F. Giuliani, Are direct search experiments sensitive to all spin-independent WIMP candidates?
2005
Earlier work this paper cites.
C. Savage, G. Gelmini, P. Gondolo, and K. Freese, Compatibility of DAMA/LIBRA dark matter detection with other searches
Original
2009
Earlier work this paper cites.
C. McCabe, The Astrophysical Uncertainties Of Dark Matter Direct Detection Experiments
Original
2010
Earlier work this paper cites.

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2012
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2013

The unbearable lightness of being: CDMS versus XENON

Frandsen, Mads T., Kahlhoefer, Felix, McCabe, Christopher et al.

Understand

The CDMS-II collaboration has reported 3 events in a Si detector, which are consistent with being nuclear recoils due to scattering of Galactic dark matter particles with a mass of about 8.6 GeV and a cross-section on neutrons of about 2 x 10^-41 cm^2.

While a previous result from the XENON10 experiment has supposedly ruled out such particles as dark matter, we find by reanalysing the XENON10 data that this is not the case.
Some tension remains however with the upper limit placed by the XENON100 experiment, independently of astrophysical uncertainties concerning the Galactic dark matter distribution.
We explore possible ways of ameliorating this tension by altering the properties of dark matter interactions.