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We reexamine the interpretation of the annual modulation signal observed by the DAMA experiment as due to WIMPs with a spin-dependent coupling mostly to protons.
1910
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1915
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1931
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1971
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1989
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F. Iachello, L. M. Krauss and G. Maino, Spin Dependent Scattering of Weakly Interacting Massive Particles in Heavy Nuclei,
1991
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1992
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M. T. Ressell, M. B. Aufderheide, S. D. Bloom, K. Griest, G. J. Mathews and D. A. Resler, Nuclear shell model calculations of neutralino - nucleus cross-sections for Si-29 and Ge-73,
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1998
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2001
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P. Ullio, M. Kamionkowski and P. Vogel, Spin dependent WIMPs in DAMA?,
2001
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2002
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2005
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D. P. Finkbeiner and N. Weiner, Exciting Dark Matter and the INTEGRAL/SPI 511 keV signal,
2007
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2008
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2009
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2009
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2009
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S. Chang, N. Weiner and I. Yavin, Magnetic Inelastic Dark Matter,
2010
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P. W. Graham, R. Harnik, S. Rajendran and P. Saraswat, Exothermic Dark Matter,
2010
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2010
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2010
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R. Schoenrich, J. Binney and W. Dehnen, Local Kinematics and the Local Standard of Rest,
2013
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2013
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2013
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2013
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2010
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S. K. Kim et al
2010
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2011
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C. McCabe, DAMA and CoGeNT without astrophysical uncertainties,
2011
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2012
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2012
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2012
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2012
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2013
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2014
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P. J. Fox, Y. Kahn and M. McCullough, Taking Halo-Independent Dark Matter Methods Out of the Bin,
2014
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2014
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2014
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