WIMP identification through a combined measurement of axial and scalar couplings
arXiv:0705.2502 · doi:10.1103/PhysRevLett.99.151301
Abstract
We study the prospects for detecting Weakly Interacting Massive Particles (WIMPs), in a number of phenomenological scenarios, with a detector composed of a target simultaneously sensitive to both spin-dependent and spin-independent couplings, as is the case of COUPP (Chicagoland Observatory for Underground Particle Physics). First, we show that sensitivity to both couplings optimizes chances of initial WIMP detection. Second, we demonstrate that in case of detection, comparison of the signal on two complementary targets, such as in COUPP CF3I and C4F10 bubble chambers, allows a significantly more precise determination of the dark matter axial and scalar couplings. This strategy would provide crucial information on the nature of the WIMPs, and possibly allow discrimination between neutralino and Kaluza-Klein dark matter.
arXiv comment4 pages 2 figures, uses revtex. References added and Fig.2 improved. To appear in PRL
References in corpus (24)
- Particle Dark Matter: Evidence, Candidates and Constraints
- Supersymmetric Dark Matter
- Bounds on Universal Extra Dimensions
- Non-Baryonic Dark Matter - Observational Evidence and Detection Methods
- Is the Lightest Kaluza-Klein Particle a Viable Dark Matter Candidate?
- Kaluza-Klein Dark Matter
- Radiative Corrections to Kaluza-Klein Masses
- Re-Evaluation of the Elastic Scattering of Supersymmetric Dark Matter
- Dark Matter Detection in the Light of Recent Experimental Results
- Precise Calculation of the Relic Density of Kaluza-Klein Dark Matter in Universal Extra Dimensions
- The Abundance of Kaluza-Klein Dark Matter with Coannihilation
- Limits on direct detection of neutralino dark matter from b -> s gamma decays
- Precision electroweak constraints on Universal Extra Dimensions revisited
- Exploration of Elastic Scattering Rates for Supersymmetric Dark Matter
- Neutralino dark matter in supergravity theories with non-universal scalar and gaugino masses
- Relic abundance of dark matter in the minimal universal extra dimension model
- Significant effects of second KK particles on LKP dark matter physics
- Pinning down neutralino properties from a possible modulation signal in WIMP direct search
- Update of the direct detection of dark matter and the role of the nuclear spin
- Improved Bounds on Universal Extra Dimensions and Consequences for LKP Dark Matter
- Development of Bubble Chambers With Enhanced Stability and Sensitivity to Low-Energy Nuclear Recoils
- Direct detection of neutralino dark matter in supergravity
- Efficient Coannihilation Process through Strong Higgs Self-Coupling in LKP Dark Matter Annihilation
- Distinguishing Supersymmetry From Universal Extra Dimensions or Little Higgs Models With Dark Matter Experiments
Cited by in corpus (39)
- Hadronic Uncertainties in the Elastic Scattering of Supersymmetric Dark Matter
- Final Analysis and Results of the Phase II SIMPLE Dark Matter Search
- Deducing the nature of dark matter from direct and indirect detection experiments in the absence of collider signatures of new physics
- A Next-Generation Liquid Xenon Observatory for Dark Matter and Neutrino Physics
- Improved Spin-Dependent WIMP Limits from a Bubble Chamber
- The moment of truth for WIMP Dark Matter
- On dark matter models with uniquely spin-dependent detection possibilities
- Complementarity of Dark Matter Direct Detection Targets
- Right-handed sneutrino dark matter in the NMSSM
- Identification of Dark Matter particles with LHC and direct detection data
- Dark matter effective field theory scattering in direct detection experiments
- Spin Dependence of Dark Matter Scattering
- Collider signals and neutralino dark matter detection in relic-density-consistent models without universality
- Identifying WIMP dark matter from particle and astroparticle data
- Taming astrophysical bias in direct dark matter searches
- Annihilation vs. Decay: Constraining dark matter properties from a gamma-ray detection
- Discriminating dark matter candidates using direct detection
- On the Correlation Between the Spin-Independent and Spin-Dependent Direct Detection of Dark Matter
- Complementarity of direct and indirect Dark Matter detection experiments
- Global fits of the Minimal Universal Extra Dimensions scenario
- Complementarity of dark matter direct detection: the role of bolometric targets
- Complementarity of Indirect and Accelerator Dark Matter Searches
- Directional detection of Dark Matter
- Astrophysical limitations to the identification of dark matter: indirect neutrino signals vis-a-vis direct detection recoil rates
- Fermion WIMPless Dark Matter at DeepCore and IceCube
- On the spin-dependent sensitivity of XENON100
- Multi-Dimensional Effective Field Theory Analysis for Direct Detection of Dark Matter
- Constraining Dark Matter Properties with Gamma-Rays from the Galactic Center with Fermi-LAT
- Enhanced Line Signals from Annihilating Kaluza-Klein Dark Matter
- Determining Ratios of WIMP-Nucleon Cross Sections from Direct Dark Matter Detection Data
- Opening the energy window on direct dark matter detection
- Surrogate Models for Direct Dark Matter Detection
- Constraining the Milky Way Dark Matter Density Profile with Gamma-Rays with Fermi-LAT
- A scheme for the extraction of WIMP-nucleon scattering cross sections from total event rates
- Fabrication and Response of High Concentration SIMPLE Superheated Droplet Detectors with Different Liquids
- On the importance of direct detection combined limits for spin independent and spin dependent dark matter interactions
- Modelling the transient processes produced under heavy particle irradiation
- Scintillating bolometers: a key for determining WIMP parameters
- Effects of Residue Background Events in Direct Dark Matter Detection Experiments on the Determinations of Ratios of WIMP-Nucleon Cross Sections