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Dark Matter Sensitivity of the CYGNO Detector with HFO-1234ze Enhanced Gas Mixtures
arXiv Physics
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이 매체는 공공·자유 라이선스로 본문을 직접 표시합니다.Abstract
The CYGNO collaboration introduces an innovative approach to direct dark matter detection, proposing a high-resolution optical Time Projection Chamber.
It operates at atmospheric pressure with a He:CF4 (60:40) gas mixture and uses a triple Gas Electron Multiplier stage for signal amplification.
A key feature is its optical readout system, which captures the scintillation light produced during the electron avalanche.
This setup allows 3D event reconstruction by combining the time profile of the light detected by photomultiplier tubes with high-granularity, pixelated X-Y tracking recorded by a scientific camera.
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