Built on

P. J. Fox, J. Liu and N. Weiner, Integrating Out Astrophysical Uncertainties,
Original
1915
Earlier work this paper cites.
R. H. Helm, Inelastic and Elastic Scattering of 187-Mev Electrons from Selected Even-Even Nuclei,
Original
1956
Earlier work this paper cites.
G. Angloher et al
Original
1971
Earlier work this paper cites.
D. Tucker-Smith and N. Weiner, “Inelastic dark matter,” Phys. Rev. D 64
2001
Earlier work this paper cites.
R. Bernabei et al
2003
Earlier work this paper cites.
A. Kurylov and M. Kamionkowski, Generalized analysis of weakly interacting massive particle searches,
2004
Earlier work this paper cites.
G. Gelmini and P. Gondolo, DAMA dark matter detection compatible with other searches,
2005
Earlier work this paper cites.
D. P. Finkbeiner and N. Weiner, Exciting Dark Matter and the INTEGRAL/SPI 511 keV signal,
2007
Earlier work this paper cites.
M. C. Smith et al
2007
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R. Bernabei et al
Original
2008
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.

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2014

Direct Detection of Light "Ge-phobic" Exothermic Dark Matter

Gelmini, Graciela B., Georgescu, Andreea, Huh, Ji-Haeng

Understand

We present comparisons of direct dark matter (DM) detection data for light WIMPs with exothermic scattering with nuclei (exoDM), both assuming the Standard Halo Model (SHM) and in a halo model - independent manner.

Exothermic interactions favor light targets, thus reducing the importance of upper limits derived from xenon targets, the most restrictive of which is at present the LUX limit.
In our SHM analysis the CDMS-II-Si and CoGeNT regions become allowed by these bounds, however the recent SuperCDMS limit rejects both regions for exoDM with isospin-conserving couplings.
An isospin-violating coupling of the exoDM, in particular one with a neutron to proton coupling ratio of $-0.8$ (which we call "Ge-phobic"), maximally reduces the DM coupling to germanium and allows the CDMS-II-Si region to become compatible with all bounds.

Built on

P. J. Fox, J. Liu and N. Weiner, Integrating Out Astrophysical Uncertainties,
Original
1915
Earlier work this paper cites.
R. H. Helm, Inelastic and Elastic Scattering of 187-Mev Electrons from Selected Even-Even Nuclei,
Original
1956
Earlier work this paper cites.
G. Angloher et al
Original
1971
Earlier work this paper cites.
D. Tucker-Smith and N. Weiner, “Inelastic dark matter,” Phys. Rev. D 64
2001
Earlier work this paper cites.
R. Bernabei et al
2003
Earlier work this paper cites.
A. Kurylov and M. Kamionkowski, Generalized analysis of weakly interacting massive particle searches,
2004
Earlier work this paper cites.
G. Gelmini and P. Gondolo, DAMA dark matter detection compatible with other searches,
2005
Earlier work this paper cites.
D. P. Finkbeiner and N. Weiner, Exciting Dark Matter and the INTEGRAL/SPI 511 keV signal,
2007
Earlier work this paper cites.
M. C. Smith et al
2007
Earlier work this paper cites.
R. Bernabei et al
Original
2008
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.