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Track reconstruction with MIMAC

Authors :
J. Billard
F. Mayet
Daniel Santos
Laboratoire de Physique Subatomique et de Cosmologie (LPSC)
Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)
MIMAC
Source :
EAS Publications Series, 3rd Workshop on Directional Detection of Dark Matter (CYGNUS 2011), 3rd Workshop on Directional Detection of Dark Matter (CYGNUS 2011), Jun 2011, Aussois, France. pp.137-145, ⟨10.1051/eas/1253017⟩
Publication Year :
2011
Publisher :
HAL CCSD, 2011.

Abstract

Directional detection of Dark Matter is a promising search strategy. However, to perform such kind of detection, the recoiling tracks have to be accurately reconstructed: direction, sense and position in the detector volume. In order to optimize the track reconstruction and to fully exploit the data from the MIMAC detector, we developed a likelihood method dedicated to the track reconstruction. This likelihood approach requires a full simulation of track measurements with MIMAC in order to compare real tracks to simulated ones. Finally, we found that the MIMAC detector should have the required performance to perform a competitive directional detection of Dark Matter.<br />Comment: 9 pages, 6 figures; Proceedings of the 3rd International conference on Directional Detection of Dark Matter (CYGNUS 2011), Aussois, France, 8-10 June 2011

Details

Language :
English
Database :
OpenAIRE
Journal :
EAS Publications Series, 3rd Workshop on Directional Detection of Dark Matter (CYGNUS 2011), 3rd Workshop on Directional Detection of Dark Matter (CYGNUS 2011), Jun 2011, Aussois, France. pp.137-145, ⟨10.1051/eas/1253017⟩
Accession number :
edsair.doi.dedup.....ee5e3593c6018ea7b8089fafe6d808cd
Full Text :
https://doi.org/10.1051/eas/1253017⟩