Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.281g&link_type=abstract
Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:
Astronomy and Astrophysics
Astrophysics
Scientific paper
Direct detection of WIMP dark matter cadidates requires an extremely high level of background rejection. The only way out is particle identification which, for experiments based on nucleus recoil, is most efficiently performed by simultaneously detecting ionization or light and phonons. We discuss and compare the different approaches, having in mind the potential need to build rather large detectors and the difficulties that this requirement may raise for some cryogenic devices. It is claimed that the luminescent bolometer red by arrays of superconducting tunnel junctions, as proposed by the author some years ago, ultimately provides the most appropriate WIMP detector.
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