Indirect Detection of Dark Matter WIMPs in a Liquid Argon TPC
arXiv:hep-ph/0410206 · doi:10.1088/1475-7516/2005/01/001
Abstract
We assess the prospects for indirect detection of Weakly Interacting Massive Particles using a large Liquid Argon TPC detector. Signal events will consist of energetic electron (anti)neutrinos coming from the decay of leptons and quarks produced in WIMP annihilation in the core of the Sun. Background contamination from atmospheric neutrinos is expected to be low, thanks to the superb angular resolution and particle identification capabilities provided by the considered experimental set-up. We evaluate the event rates predicted for an annihilating WIMP as a function of its elastic scattering cross section with nucleons. This technique is particularly useful for WIMPs lighter than GeV
16 pages, 8 figures
References in corpus (36)
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
- Particle Dark Matter: Evidence, Candidates and Constraints
- Bounds on Universal Extra Dimensions
- DarkSUSY: Computing Supersymmetric Dark Matter Properties Numerically
- Inelastic Dark Matter
- Is the Lightest Kaluza-Klein Particle a Viable Dark Matter Candidate?
- Kaluza-Klein Dark Matter
- Search for Dark Matter WIMPs using Upward Through-going Muons in Super-Kamiokande
- Dark Matter Detection in the Light of Recent Experimental Results
- First Results from the Cryogenic Dark Matter Search in the Soudan Underground Lab
- Heavy Sneutrinos as Dark Matter
- Measuring and Understanding the Universe
- Prospects for Indirect Detection of Neutralino Dark Matter
- Indirect Detection of Dark Matter in km-size Neutrino Telescopes
- New Results from the Cryogenic Dark Matter Search Experiment
- The FLUKA atmospheric neutrino flux calculation
- Indirect Search for Neutralino Dark Matter with High Energy Neutrinos
- Probing Kaluza-Klein Dark Matter with Neutrino Telescopes
- WIMP diffusion in the solar system including solar depletion and its effect on Earth capture rates
- Oscillation effects on supernova neutrino rates and spectra and detection of the shock breakout in a liquid Argon TPC
- Neutrinos From Particle Decay in the Sun and Earth
- Limits on dark matter WIMPs using upward-going muons in the MACRO detector
- Physics potential at a neutrino factory: can we benefit from more than just detecting muons?
- Measurement of the muon decay spectrum with the ICARUS liquid Argon TPC
- Results from the Antarctic Muon and Neutrino Detector Array (AMANDA)
- The NAIAD experiment for WIMP searches at Boulby mine and recent results
- Neutrino Indirect Detection of Neutralino Dark Matter in the CMSSM
- High Energy Neutrinos From Superheavy Dark Matter Annihilation
- On the energy and baseline optimization to study effects related to the -phase (CP-/T-violation) in neutrino oscillations at a Neutrino Factory
- Decoupling supernova and neutrino oscillation physics with LAr TPC detectors
- High-energy neutrino fluxes from supermassive dark matter
- Ideas for future liquid Argon detectors
- Indirect Detection of Dark Matter WIMPs in a Liquid Argon TPC
- Particle Production in the Interstellar Medium
- GeV to TeV astrophysical tau neutrinos
- The AMANDA Neutrino Telescope and the Indirect Search for Dark Matter
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- Neutrino flavor ratios as diagnostic of solar WIMP annihilation
- Reconstructing WIMP properties with neutrino detectors
- aro: a tool for neutrino flux generation from WIMPs
- Warped Kaluza-Klein Dark Matter
- Neutrino Probes of the Nature of Light Dark Matter
- Indirect Detection of Dark Matter WIMPs in a Liquid Argon TPC
- Probing the Dark Matter mass and nature with neutrinos