Light WIMP Searches: The Effect of the Uncertainty in Recoil Energy Scale and Quenching Factor
arXiv:1010.5187
Abstract
Taking liquid xenon detectors as a case study, the importance of a robust recoil energy calibration as a prerequisite to a search for light-mass Weakly Interacting Massive Particles (WIMPs) is emphasized. Important shortfalls in the analysis of existing measurements of the relative scintillation efficiency and ionization yield for nuclear recoils in liquid xenon are described, leading to the conclusion that recent attempts to extract light-WIMP sensitivity limits from the XENON10 and XENON100 detectors are premature and overly optimistic.
arXiv comment11 pages
Cited by in corpus (18)
- Mirror dark matter: Cosmology, galaxy structure and direct detection
- Toward A Consistent Picture For CRESST, CoGeNT and DAMA
- Halo independent comparison of direct dark matter detection data
- Coherent neutrino-nucleus scattering detection with a CsI[Na] scintillator at the SNS spallation source
- Phenomenology of Dark Matter from A4 Flavor Symmetry
- Implications of CoGeNT's New Results For Dark Matter
- Novel Higgs Decays and Dark Matter in the E(6)SSM
- Elastic scattering signals of solar neutrinos with enhanced baryonic currents
- CoGeNT, DAMA, and Light Neutralino Dark Matter
- Search for Low-Mass Dark Matter with CsI(Tl) Crystal Detectors
- Mirror dark matter interpretations of the DAMA, CoGeNT and CRESST-II data
- Implications of mirror dark matter kinetic mixing for CMB anisotropies
- A systematic halo-independent analysis of direct detection data within the framework of Inelastic Dark Matter
- Direct detection experiments explained with mirror dark matter
- Quenching factor measurements of sodium nuclear recoils in NaI:Tl determined by spectrum fitting
- Hidden sector dark matter explains the DAMA, CoGeNT, CRESST-II and CDMS/Si experiments
- Technical aspects in dark matter investigations
- Effective scalar four-fermion interaction for Ge-phobic exothermic dark matter and the CDMS-II Silicon excess