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- W105829458 abstract "Isospin-violating dark matter (IVDM) provides a possible mechanism to ameliorate the tension among recent direct detection experiments. For IVDM, we demonstrate that the results of direct detection experiments based on neutron-rich target nuclei may depend strongly on the density dependence of the symmetry energy which is presently largely unknown and controls the neutron skin thickness that reflects the relative difference of neutron and proton distributions in the neutron-rich nuclei. In particular, using the neutron and proton distributions obtained from Skyrme-Hartree-Fock calculations with the symmetry energy constrained by the latest model-independent measurement of the neutron skin thickness of $^{208}$Pb from PREX experiment at JLab, we find that for the xenophobic IVDM in the mass region constrained by CMDS-II(Si), the symmetry energy effect may enhance the sensitivity of Xe-based detectors (e.g., XENON100 and LUX) to the DM-proton cross section by a factor of $3$, compared with the results using the empirical Helm charge distributions. This symmetry energy effect can even enhance the sensitivity by more than an order of magnitude for the xenophobic IVDM with mass larger than $80$ GeV." @default.
- W105829458 created "2016-06-24" @default.
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- W105829458 date "2014-03-20" @default.
- W105829458 modified "2023-09-27" @default.
- W105829458 title "Symmetry Energy Effects in the Direct Detection of Isospin-Violating Dark Matter" @default.
- W105829458 hasPublicationYear "2014" @default.
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