4.7 Article

Xenophobic dark matter

Journal

PHYSICAL REVIEW D
Volume 88, Issue 1, Pages -

Publisher

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.88.015021

Keywords

-

Funding

  1. NSF [PHY-0970173]
  2. Simons Foundation Fellowship
  3. U.S. Department of Energy [DE-FG02-04ER41291, DE-FG02-92ER40701]
  4. Gordon and Betty Moore Foundation [776]
  5. Caltech Moore Center for Theoretical Cosmology and Physics
  6. Direct For Mathematical & Physical Scien
  7. Division Of Physics [1316792, 970173] Funding Source: National Science Foundation

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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) approximate to -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.

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