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MIMAC: MIcro-tpc MAtrix of Chambers for dark matter directional detection

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arxiv 1311.0616 v1 pith:7JGEKO6D submitted 2013-11-04 physics.ins-det astro-ph.CO

classification physics.ins-detastro-ph.CO
keywords darkdetectiondirectionalfirstmatterbackgroundchambersdeveloped
verification ladder T0 review T1 audit T2 compute T3 formal
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Directional detection of non-baryonic Dark Matter is a promising search strategy for discriminating WIMP events from neutrons, the ultimate background for dark matter direct detection. This strategy requires both a precise measurement of the energy down to a few keV and 3D reconstruction of tracks down to a few mm. The MIMAC (MIcro-tpc MAtrix of Chambers) collaboration has developed in the last years an original prototype detector based on the direct coupling of large pixelized micromegas with a special developed fast self-triggered electronics showing the feasibility of a new generation of directional detectors. The first bi-chamber prototype has been installed at Modane, underground laboratory in June 2012. The first undergournd background events, the gain stability and calibration are shown. The first spectrum of nuclear recoils showing 3D tracks coming from the radon progeny is presented.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Ubiquitous Corotation of Dark Matter Halos: Implications for Direct Detection

    hep-ph 2026-07 conditional novelty 6.0 of 10

    Dark matter in simulated Milky Way analogues preferentially corotates with the baryonic disk, suppressing predicted direct-detection rates for light WIMPs, reducing directional modulation, and producing a 21% astrophy...

  2. First Directional Dark Matter Limits from the MIMAC {\mu}-TPC Detector

    astro-ph.CO 2026-07 conditional novelty 6.0 of 10

    With ~0.02 kg·days of hydrogen and a data-driven ON/OFF galactic-map analysis, MIMAC finds no Cygnus-directed excess and sets σ_SD-p < 6.65×10^{-36} cm² (90% CL).

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