29 June 2018 to 4 July 2018
IBS HQ, Daejeon, Korea
Asia/Seoul timezone
There will be Welcome Reception at 18:00 on June 28, 2018

Ultra-light dark matter search with the spherical detector

3 Jul 2018, 16:30
30m
Room B (IBS HQ, Daejeon, Korea)

Room B

IBS HQ, Daejeon, Korea

Speaker

Dr giomataris ioannis (cea)

Description

The Spherical Proportional Detector is a new type of radiation detector based on a spherical geometry. It consists of a large spherical gas volume with a central electrode forming a radial electric field. A small spherical sensor located at the center is acting as a proportional amplification structure. Combination of sub-keV energy threshold and versatility of the target (Ne, He, H) opens the way to search for ultra light dark matter WIMPs down to 100 MeV. Recent results obtained with a low radioactivity detector, 60 cm in diameter operated at LSM underground laboratory will be presented. First results with Ne as target nuclei, exclude above 4.4・10-37 cm2 for a 0.5 GeV/c2 WIMP. The next project, under development, is a larger detector that consists of a selected pure copper sphere with a diameter of 1.4m to be installed at SNOLAB. This will allow benefiting from a 40 times larger volume, relative to the current detector and a much lower background level to reach unprecedented sensitivity in the range 100MeV to 1GeV. Other potential applications for low energy neutrino physics will be also discussed.

Primary author

Dr giomataris ioannis (cea)

Presentation materials