Xenophobic Dark Matter

TL;DR

This paper explores xenophobic dark matter models with isospin-violating interactions that reduce xenon detector sensitivity, aligning certain experimental signals and suggesting future tests via direct detection, collider, and indirect searches.

Contribution

It introduces and analyzes xenophobic dark matter models with specific isospin violation, showing their potential to reconcile experimental signals and be tested by upcoming experiments.

Findings

Xenophobic models can reconcile CoGeNT and CDMS-Si signals.

Xenophobia limits are set by xenon isotope natural abundance.

Future experiments at xenon detectors, LHC, and Fermi-LAT can test these models.

Abstract

We consider models of xenophobic dark matter, in which isospin-violating dark matter-nucleon interactions significantly degrade the response of xenon direct detection experiments. For models of near-maximal xenophobia, with neutron-to-proton coupling ratio $f_n / f_p \approx -0.64$, and dark matter mass near 8 GeV, the regions of interest for CoGeNT and CDMS-Si and the region of interest identified by Collar and Fields in CDMS-Ge data can be brought into agreement. This model may be tested in future direct, indirect, and collider searches. Interestingly, because the natural isotope abundance of xenon implies that xenophobia has its limits, we find that this xenophobic model may be probed in the near future by xenon experiments. Near-future data from the LHC and Fermi-LAT may also provide interesting alternative probes of xenophobic dark matter.