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Simulation of the Directional Dark Matter Detector (D3) and Directional Neutron Observer (DiNO)

Published online by Cambridge University Press:  15 February 2012

F. Mayet ,
D. Santos ,
I. Jaegle ,
H. Feng ,
S. Ross ,
J. Yamaoka  and
S.E. Vahsen
I. Jaegle
Affiliation:
Department of Physics and Astronomy, University of Hawaii, 2505 Correa Rd., Honolulu, HI 96822, USA. e-mail: [email protected] ;
H. Feng
Affiliation:
Department of Physics and Astronomy, University of Hawaii, 2505 Correa Rd., Honolulu, HI 96822, USA. e-mail: [email protected] ;
S. Ross
Affiliation:
Department of Physics and Astronomy, University of Hawaii, 2505 Correa Rd., Honolulu, HI 96822, USA. e-mail: [email protected] ;
J. Yamaoka
Affiliation:
Department of Physics and Astronomy, University of Hawaii, 2505 Correa Rd., Honolulu, HI 96822, USA. e-mail: [email protected] ;
S.E. Vahsen
Affiliation:
Department of Physics and Astronomy, University of Hawaii, 2505 Correa Rd., Honolulu, HI 96822, USA. e-mail: [email protected] ;
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Abstract

Preliminary simulation and optimization studies of the Directional Dark Matter Detector and the Directional Neutron Observer are presented. These studies show that the neutron interaction with the gas-target in these detectors is treated correctly by GEANT4 and that by lowering the pressure, the sensitivity to low-mass WIMP candidates is increased. The use of negative ion drift might allow us to search the WIMP mass region suggested by the results of the non-directional experiments DAMA/LIBRA, CoGeNT and CRESST-II.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 53: CYGNUS 2011: Third International Conference on Directional Detection of Dark Matter , 2012 , pp. 111 - 118
Copyright
© EAS, EDP Sciences 2012

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References

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