Physical Review Letters· 2012Q1
Dark Matter Results from 225 Live Days of XENON100 Data
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- 2012year
Short summary
The XENON100 experiment found no evidence for dark matter interactions after 224.6 live days of data collection, setting new limits on dark matter particle properties.
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Key points
- XENON100 collected 224.6 live days of data with a 34 kg exposure.
- No evidence for dark matter interactions was found; observed events matched background expectations.
- The experiment set the most stringent limit on spin-independent WIMP-nucleon scattering cross-section above 8 GeV/c².
- A minimum cross-section limit of 2 x 10⁻⁴⁵ cm² was achieved at 55 GeV/c² WIMP mass (90% CL).
AI-generated from the title and abstract; the full text is not read.
Abstract
We report on a search for particle dark matter with the XENON100 experiment, operated at the Laboratori Nazionali del Gran Sasso for 13 months during 2011 and 2012. XENON100 features an ultralow electromagnetic background of $(5.3\ifmmode\pm\else\textpm\fi{}0.6)\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}3}\text{ }\text{ }\mathrm{events}/({\mathrm{keV}}_{\mathrm{ee}}\ifmmode\times\else\texttimes\fi{}\mathrm{kg}\ifmmode\times\else\texttimes\fi{}\mathrm{day})$ in the energy region of interest. A blind analysis of $224.6\text{ }\mathrm{\text{live days}}\ifmmode\times\else\texttimes\fi{}34\text{ }\text{ }\mathrm{kg}$ exposure has yielded no evidence for dark matter interactions. The two candidate events observed in the predefined nuclear recoil energy range of $6.6--30.5\text{ }\text{ }{\mathrm{keV}}_{\mathrm{nr}}$ are consistent with the background expectation of ($1.0\ifmmode\pm\else\textpm\fi{}0.2$) events. A profile likelihood analysis using a $6.6--43.3\text{ }\text{ }{\mathrm{keV}}_{\mathrm{nr}}$ energy range sets the most stringent limit on the spin-independent elastic weakly interacting massive particle--nucleon scattering cross section for weakly interacting massive particle masses above $8\text{ }\text{ }\mathrm{GeV}/{c}^{2}$, with a minimum of $2\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}45}\text{ }\text{ }{\mathrm{cm}}^{2}$ at $55\text{ }\text{ }\mathrm{GeV}/{c}^{2}$ and 90% confidence level.
The authors' abstract, as published at the source. Physical Review Letters, 2012 · DOI ↗
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Field: Nuclear and High Energy Physics
Nuclear and High Energy PhysicsPhysics and Astronomy