Track length measurement of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e248" altimg="si3.svg"><mml:mrow><mml:msup><mml:mrow /><mml:mrow><mml:mn>19</mml:mn></mml:mrow></mml:msup><mml:msup><mml:mrow><mml:mi mathvariant="normal">F</mml:mi></mml:mrow><mml:mrow><mml:mo>+</mml:mo></mml:mrow></mml:msup></mml:mrow></mml:math> ions with the MIMAC directional Dark Matter detector prototype
نویسندگان
چکیده
Weakly Interacting Massive Particles (WIMPs) are one of the most preferred candidate for Dark Matter. WIMPs should interact with nuclei detectors. If a robust signal is eventually observed in direct detection experiments, best signature to confirm its Galactic origin would be nuclear recoil track direction. The MIMAC collaboration has developed low pressure gas detector providing both kinetic energy and three-dimensional reconstruction recoils. In this paper we report first ever observations $^{19}$F tracks $5$ cm drift prototype detector, range ($6$-$26$ keV), using specially ion beam facilities. We have measured lengths found significant differences between our measurements standard simulations. order understand these differences, performed series complementary experiments simulations study impact diffusion eventual systematics. show an unexpected dependence number read-out corresponding on electric field applied $512\ \mathrm{\mu m}$ gap Micromegas detector. introduced, based flash-ADC observable, corrections reconstruct physical 3D length primary electron clouds proposing physics behind corrections. that space charge effects need taken into account explain These may shed new light high-gain TPC ionization signals general particularly at energy.
منابع مشابه
A prototype of a directional detector for non-baryonic dark matter search: MIMAC
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ژورنال
عنوان ژورنال: Nuclear Instruments and Methods in Physics Research
سال: 2021
ISSN: ['1872-9576', '0168-9002']
DOI: https://doi.org/10.1016/j.nima.2020.164569