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Directional Detection Rates of Dark Matter (WIMPs)

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Presentation on theme: "Directional Detection Rates of Dark Matter (WIMPs)"— Presentation transcript:

1 Directional Detection Rates of Dark Matter (WIMPs)
Debasish Majumdar‏ Saha Institute of Nuclear Physics Kolkata

2 Rotation of galactic disc through the halo of Dark Matter causes the earth to experience an apparent wind of Dark Matter

3 Because of the earth’s annual revolution around the sun the WIMP flux encountered by the earth continually changes over the period of the year.

4 Variation due to diurnal rotation of earth

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17 Detectors Chosen CF4 Detector NEWAGE at Kamioka Micro-TPC
CS2 Detector DRIFT Detector at Boulby mine Time Projection Chamber Able to reconstruct 3D track (Directionality of the track) 54 deg 33 min North 0 deg 49 min west CF4 Detector NEWAGE at Kamioka Micro-TPC CF4 with 152 Torr. 36 deg 25 min North 137 deg 18 min East

18 Daily (and annual) variations of rates

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24 Ratio of rates in two directions

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27 Thank you

28 Back ups

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