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A search for light dark matter in XENON10 data

J. Angle, E. Aprile, F. Arneodo, L. Baudis, A. Bernstein, A. Bolozdynya, P. Brusov, L. C. C. Coelho, C. E. Dahl, L. DeViveiros, A. D. Ferella, L. M. P. Fernandes, S. Fiorucci, R. J. Gaitskell, K. L. Giboni, R. Gomez, R. Hasty, L. Kastens, J. Kwong, J. A. M. Lopes, N. Madden, A. Manalaysay, A. Manzur, D. N. McKinsey, M. E. Monzani, K. Ni, U. Oberlack, J. Orboeck, G. Plante, R. Santorelli, J. M. F. dos Santos, P. Shagin, T. Shutt, P. Sorensen, S. Schulte, C. Winant, M. Yamashita

TL;DR

The data strongly constrain recent elastic dark matter interpretations of excess low-energy events observed by CoGeNT and CRESST-II, as well as the DAMA annual modulation signal.

Abstract

We report results of a search for light (<10 GeV) particle dark matter with the XENON10 detector. The event trigger was sensitive to a single electron, with the analysis threshold of 5 electrons corresponding to 1.4 keV nuclear recoil energy. Considering spin-independent dark matter-nucleon scattering, we exclude cross sections σ_n>3.5x10^{-42} cm^2, for a dark matter particle mass m_χ=8 GeV. We find that our data strongly constrain recent elastic dark matter interpretations of excess low-energy events observed by CoGeNT and CRESST-II, as well as the DAMA annual modulation signal.

A search for light dark matter in XENON10 data

TL;DR

The data strongly constrain recent elastic dark matter interpretations of excess low-energy events observed by CoGeNT and CRESST-II, as well as the DAMA annual modulation signal.

Abstract

We report results of a search for light (<10 GeV) particle dark matter with the XENON10 detector. The event trigger was sensitive to a single electron, with the analysis threshold of 5 electrons corresponding to 1.4 keV nuclear recoil energy. Considering spin-independent dark matter-nucleon scattering, we exclude cross sections σ_n>3.5x10^{-42} cm^2, for a dark matter particle mass m_χ=8 GeV. We find that our data strongly constrain recent elastic dark matter interpretations of excess low-energy events observed by CoGeNT and CRESST-II, as well as the DAMA annual modulation signal.

Paper Structure

This paper contains 1 equation, 3 figures, 1 table.

Figures (3)

  • Figure 1: The electron yield $\mathcal{Q}_y$ of liquid xenon for nuclear recoils. Theoretical curves (solid and dashed) were calculated from Eq. \ref{['eq1']}, as described in the text. Also shown are measurements from 2010manzur ($\bigstar$), 2010sorensen_idm (dash-dot curve, with $\pm1\sigma$ contours) and 2006aprile ($\fullmoon$ and $\blacksquare$, uncertainty omitted for clarity).
  • Figure 2: (left) All candidate dark matter events remaining ($\times$ and $\fullmoon$) after the cuts listed in Table \ref{['table1']}. Events in which an S1 was found are shown as $\fullmoon$. The number of electrons in the S2 signal is indicated by the inset scale. (top) Distribution of candidate events with $\leq4$ electrons ($+$), and distribution of background single electrons ($\triangle$) as described in the text. (right) S2 pulse width distributions for single scatter nuclear recoils in the top, middle and bottom third of the detector.
  • Figure 3: Curves indicate 90% C.L. exclusion limits on spin-independent $\sigma_n$ for elastic dark matter scattering, obtained by CDMS (dotted 2010akerib, and dashed 2010ahmed) and XENON100 (dash-dot 2010aprile100). The region consistent with assumption of a positive detection by CoGeNT is shown (hatched) 2010aalseth, and (shaded) 2010chang3; the latter assumes a 30% exponential background. Also shown is the $3\sigma$ allowed region for the DAMA annual modulation signal (solid contour) 2011savage.