Have we found conclusive evidence for dark matter through direct detection experiments?
Abstract
We employ a SUSY-model-independent method to examine the remaining evidence for the low mass dark matter. Using the XENON100's recent result of 224.6 live days × 34kg exposure and PICASSO's result published in 2009, we have obtained a constrain of couplings, \| an \| < 0.6 and \| ap \| < 1.0, corresponding to the spin-dependent cross section of σn < 5.6 × 10- 38cm2 and σp < 1.6 × 10- 37cm2. Spin-independent isospin violating dark matter model also failed to reconcile the recent result from XENON100 with the positive results from DAMA and CoGeNT.
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