Secondary scintillation yield from gaseous micropattern electron multipliers in direct Dark Matter detection
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Secondary scintillation yield from gaseous micropattern electron multipliers in direct Dark Matter detection

C.M.B. Monteiro,A.S. Conceição,F.D. Amaro,J.M. Maia,A.C.S.S.M. Bento,L.F.R. Ferreira,J.F.C.A. Veloso,J.M.F. dos Santos,A. Breskin,R. Chechik;C.M.B. Monteiro;A.S. Conceição;F.D. Amaro;J.M. Maia;A.C.S.S.M. Bento;L.F.R. Ferreira;J.F.C.A. Veloso;J.M.F. dos Santos;A. Breskin;R. Chechik;
physics letters b 2009 Vol. 677 pp. 133-138
125
chechik2009physicssecondary

Keywords

dark matter gem xenon scintillation dual-phase detectors mhsp avalanche photodiodes

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DOI:
10.1016/j.physletb.2009.05.020
URL:
https://sciprofiles.com/publication/view/b0caa7882...

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ID: 273452
Ref Key: chechik2009physicssecondary
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