Auriga simulations show the LMC induces azimuthal anisotropies in directional DM recoils that enhance discovery prospects relative to the Standard Halo Model.
Vahsen et al.,Cygnus: Feasibility of a nuclear recoil observatory with directional sensitivity to dark matter and neutrinos,arXiv preprint arXiv:2008.12587(2020)
7 Pith papers cite this work. Polarity classification is still indexing.
7
Pith papers citing it
representative citing papers
Silver-zeolite outperforms activated charcoal by three orders of magnitude in radon capture at room temperature when tested in a spherical proportional counter for dark matter applications.
A 2HDM extended by two real scalar singlets is scanned with evolutionary strategies to locate regions satisfying vacuum, unitarity, oblique-parameter, collider and dark-matter constraints.
Simulations of solar CEvNS events produce annually varying ring-like 3D recoil distributions in directional detectors that lack target dependence and contrast with fixed WIMP signals.
Adding methane to He-40%CF4 improves TPC stability, scintillation yield, and directional sensitivity for low-mass dark matter in the CYGNO experiment compared to isobutane.
Upgraded T-DAQ enables continuous imaging with reduced dead time, extended PMT time-tagging, and synchronous operation of multiple cameras without a master unit.
Validation identifies Nylon-supported PET or Kapton sheet with copper strips as preferred low-radioactivity field cage configuration for the CYGNO-04 demonstrator.
citing papers explorer
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Directional dark matter signatures of the Large Magellanic Cloud
Auriga simulations show the LMC induces azimuthal anisotropies in directional DM recoils that enhance discovery prospects relative to the Standard Halo Model.
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Demonstration of Efficient Radon Removal by Silver-Zeolite in a Dark Matter Detector
Silver-zeolite outperforms activated charcoal by three orders of magnitude in radon capture at room temperature when tested in a spherical proportional counter for dark matter applications.
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Machine Learning in the 2HDM2S model for Dark Matter
A 2HDM extended by two real scalar singlets is scanned with evolutionary strategies to locate regions satisfying vacuum, unitarity, oblique-parameter, collider and dark-matter constraints.
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Simulations of 3-Dimensional Recoil Response to Coherent Elastic Neutrino-Nucleus Scattering Events in Directional Direct Dark Matter Detectors
Simulations of solar CEvNS events produce annually varying ring-like 3D recoil distributions in directional detectors that lack target dependence and contrast with fixed WIMP signals.
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He-CF4-CH4 ternary mixtures as target gas for the CYGNO directional dark matter experiment
Adding methane to He-40%CF4 improves TPC stability, scintillation yield, and directional sensitivity for low-mass dark matter in the CYGNO experiment compared to isobutane.
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Upgrade of the Trigger and Data Acquisition System for Continuous Imaging and Multi-Camera Operation in CYGNO
Upgraded T-DAQ enables continuous imaging with reduced dead time, extended PMT time-tagging, and synchronous operation of multiple cameras without a master unit.
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Characterization of field cage and cathode for low radioactivity operation with the CYGNO experiment
Validation identifies Nylon-supported PET or Kapton sheet with copper strips as preferred low-radioactivity field cage configuration for the CYGNO-04 demonstrator.