1999/02/12 by G. Gerbier, J. Mallet, Gerbier, G. +5
Engineering · Physics and Astronomy · #Astrophysics (astro-ph) #CCD and CMOS Imaging Sensors #Dark Matter and Cosmic Phenomena #FOS: Physical sciences #Radioactive Decay and Measurement Techniques #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9902194
LaTex, 3 pages, 2 figures
arxiv created 1999/02/12 · openalex publication_date 1999/02/12 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
This note, with its five questions, is intended to contribute to a clarification about a claimed "evidence" by the DAMA group of an annual modulation of the counting rate of a Dark Matter NaI(Tl) detector as due to a neutralino (SUSY-LSP) Dark Matter candidate.