Results from 730 kg days of the CRESST-II Dark Matter Search

Abstract

The CRESST-II cryogenic Dark Matter search, aiming at detection of WIMPs via elastic scattering off nuclei in CaWO${}_4$ crystals, completed 730 kg days of data taking in 2011. We present the data collected with eight detector modules, each with a two-channel readout; one for a phonon signal and the other for coincidently produced scintillation light. The former provides a precise measure of the energy deposited by an interaction, and the ratio of scintillation light to deposited energy can be used to discriminate different types of interacting particles and thus to distinguish possible signal events from the dominant backgrounds. Sixty-seven events are found in the acceptance region where a WIMP signal in the form of low energy nuclear recoils would be expected. We estimate background contributions to this observation from four sources: 1) "leakage" from the e/γ-band 2) "leakage" from the α-particle band 3) neutrons and 4) Pb-206 recoils from Po-210 decay. Using a maximum likelihood analysis, we find, at a high statistical significance, that these sources alone are not sufficient to explain the data. The addition of a signal due to scattering of relatively light WIMPs could account for this discrepancy, and we determine the associated WIMP parameters.

17 pages, 13 figures

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• Results from a Low-Energy Analysis of the CDMS II Germanium Data
• Commissioning Run of the CRESST-II Dark Matter Search

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• Gamma-ray lines constraints in the NMSSM
• Right-handed sneutrinos as asymmetric DM and neutrino masses from neutrinophilic Higgs bosons
• Calculated WIMP signals at the ANDES laboratory: comparison with northern and southern located dark matter detectors
• Contamination of Dark Matter Experiments from Atmospheric Magnetic Dipoles
• Electroweak scale invariant models with small cosmological constant
• A simulation-based study of the neutron backgrounds for NaI dark matter experiments
• Experimental status of particle and astroparticle searches for supersymmetry
• Production and suppression of delayed light in NaI
• Dark Matter phenomenology : from simplified WIMP models to refined alternative solutions
• Are superheavy stable quark clusters viable candidates for the dark matter?
• Probing light WIMPs with directional detection experiments
• Effective scalar four-fermion interaction for Ge-phobic exothermic dark matter and the CDMS-II Silicon excess
• Directional Dark Matter Searches with Carbon Nanotubes
• Dark Matters in Gauged B-3L_i Model
• Isospin-Violating Dark Matter in the $U(1{)}^{\prime }$ Model with $E_6$ Origin
• Constraints on millicharged particles by neutron stars
• Bayesian analysis of multiple direct detection experiments
• Dark Matter Balls Help Supernovae to Explode
• Isospin-Violating Dark Matter Benchmarks for Snowmass 2013
• Bounds from multi-messenger astronomy on the Super Heavy Dark Matter
• Composite dark matter and direct-search experiments
• Dark matter from unification
• Indirect Dark Matter Searches and Models
• Exothermic Dark Matter with Light Mediator after LUX and PandaX-II in 2016
• Model-Independent Identification of Inelastic WIMPs from Direct Dark Matter Detection Experiments
• Observation of Time-Dependent Internal Charge Amplification in a Planar Germanium Detector at Cryogenic Temperature
• Bottom quark contribution to spin-dependent dark matter detection
• $\mathcal{O}$(1) GeV dark matter in SUSY and a very light pseudoscalar at the LHC
• DUNE potential for sub-GeV dark matter in proton beam dump mode
• Constraining dark matter in the LRTH model with latest LHC, XENON100 and LUX data
• The Lightest Massive Invisible Particles at the LHC
• Application of Time Projection Chambers with GEMs and Pixels to WIMP Searches and Fast Neutron Detection
• Supersymmetry - When Theory Inspires Experimental Searches
• Constraints on Dark Matter annihilation and Its Equation of State after Planck Data
• Higher-Order QCD prediction for dark matter pair associated with a b-jet production at the LHC
• Complementarity of direct and indirect searches in the pMSSM
• Higgs, supersymmetry and dark matter after Run I of the LHC
• A likelihood framework for cryogenic scintillating calorimeters used in the CRESST dark matter search
• Low Energy Investigations at Kamioka Observatory
• Have we found conclusive evidence for dark matter through direct detection experiments?
• New Directions in Direct Dark Matter Searches
• Searching for MeV-mass neutrinophilic Dark Matter with Large Scale Dark Matter Detectors
• New Dark Matter Detector using Nanoscale Explosives
• Measuring the Mass of Dark Matter at the LHC
• Cosmological implications of electromagnetically interacting dark matter: milli-charged particles and atoms with singly and doubly charged dark matter
• Differentiating hidden sector dark matter from light WIMPs with Germanium detectors
• Study of light detection and sensitivity for a ton-scale liquid xenon dark matter detector
• Performance of a CRESST-II Detector Module with True $4\pi$-veto
• Probing Isospin-Violating Dark Matter
• Fits to Light WIMPs
• Constraining Fermionic Dark Matter with Galactic Neutron Stars
• Online triggers for supernova and pre-supernova neutrino detection with cryogenic detectors
• Dark matter heating of Planet 9, and its observational implications
• GUT and Supersymmetry at the LHC and in dark matter