Consistent dark matter interpretation for CoGeNT and DAMA/LIBRA

被引:115
|
作者
Hooper, Dan [1 ,2 ]
Collar, J. I. [3 ,4 ]
Hall, Jeter [1 ]
McKinsey, Dan [5 ]
Kelso, Christopher M. [3 ]
机构
[1] Fermilab Natl Accelerator Lab, Ctr Particle Astrophys, Batavia, IL 60510 USA
[2] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA
[3] Univ Chicago, Dept Phys, Chicago, IL 60637 USA
[4] Univ Chicago, KICP, Enrico Fermi Inst, Chicago, IL 60637 USA
[5] Yale Univ, Dept Phys, New Haven, CT 06520 USA
来源
PHYSICAL REVIEW D | 2010年 / 82卷 / 12期
关键词
NUCLEAR RECOILS; CALIBRATION; NAI(TL); IONIZATION; CRYSTAL; SILICON; SEARCH;
D O I
10.1103/PhysRevD.82.123509
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper, we study the recent excess of low-energy events observed by the CoGeNT Collaboration and the annual modulation reported by the DAMA/LIBRA Collaboration, and discuss whether these signals could both be the result of the same elastically scattering dark matter particle. We find that, without channeling but when taking into account uncertainties in the relevant quenching factors, a dark matter candidate with a mass of approximately 7 GeV and a cross section with nucleons of sigma(DM-N) similar to 2 X 10(-4) pb (2 X 10(-40) cm(2)) could account for both of these observations. We also comment on the events recently observed in the oxygen band of the CRESST experiment and point out that these could potentially be explained by such a particle. Lastly, we compare the region of parameter space favored by DAMA/LIBRA and CoGeNT to the constraints from XENON10, XENON100, and CDMS (Si) and find that these experiments cannot at this time rule out a dark matter interpretation of these signals.
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页数:8
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