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IDM2008 - Identification of Dark Matter 2008
IDM2008 - Identification of Dark Matter 2008
18-22 August 2008 AlbaNova
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Directional Dark Matter Search with Nuclear Emulsion (15'+5')
Directional detection of WIMP is very important, because direction of WIMP 
wind might have daily modulation.  So this way can be confirmed WIMP signal 
high reliabirity  than using annual modulation by the detector having 
derectional sensitivity. 
 We will experiment dark matter serch with Nuclear Emulsion. Nuclear Emulsion
has high density and high resolution. So, It is possible to be large mass 
detector and to search of WIMP by direction of nuclear recoil track . This  
detector is very unique and strong for dark matter search.
 Now, we are doing R&D of detector to detect the WIMP. We developed very 
high resolution nuclear emulsion for dark matter search, and comfirmed it have 
ability to detect the WIMP signal. In this talk, I will talk about status R&D result  
the method of readout track and background rejection,  future plan and 
Id: 378
Place: AlbaNova
Room: Oskar Klein auditorium
Starting date:
20-Aug-2008   08:50
Duration: 20'
Contribution type: Talk
Primary Authors: Mr. NAKA, Tatsuhiro (Nagoya University , Japan)
Co-Authors: Mr. NAKAMURA, Mitsuhiro (Nagoya University , Japan)
Mr. SATO, Osamu (Nagoya University , Japan)
Mr. NAKANO, Toshiyuki (Nagoya University , Japan)
Mr. NIWA, Kimio (Nagoya University , Japan)
Presenters: Mr. NAKA, Tatsuhiro
Material: slide Slides
Included in session: Direct detection - experiments
Included in track: Direct detection - experiments

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