The Lisbon-Zaragoza-Paris dark matter search

Girard, T.A.; Morales, A.; Waysand, G.; Collar, J. I.; Bruere-Dawson, R.; Bonnierballe, P.; Dubos, H.; Garcı́a, E.; Gomes, M. L.; Jeudy, V.; Limagne, D.; Morales, J.; Perrier, Pierre; Puimedón, J.; Sáenz, C.; Salinas, A.; Sarsa, M.L.; Seco, Joao; Solórzano, A. Ortíz de; Villar, J. A.; Yong, Joshua J.H.

doi:10.1016/0920-5632(96)00213-7

Cited by 2 publications

(2 citation statements)

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“…Dark matter experiments with phonon-mediated detectors are planned by the CDMS collaboration (UC Berkeley and Stanford University) [Ake95], by the CRESST collaboration (TU Munich, MPI Munich and Oxford University) [Sei95] and by the EDELWEISS collaboration (CEA Saclay and CNRS Orsay, Paris and Lyon) [Cha95]. Two collaborations are intending to set up a dark matter search experiment by using superconducting superheated granules: the ORPHEUS collaboration (University of Bern, Paul Scherrer Institut and LAPP Annecy) [Sch95] and the Lisbon-Zaragoza-Paris Collaboration [Gir95].…”

Section: Detection Of Non-baryonic Dark Matter In Our Galactic Halomentioning

confidence: 99%

“…The major collaborations utilizing cryogenic particle detector concepts for cold dark matter search are: the CDMS collaboration using phonon-mediated and simultaneous ionization techniques [Ake95], the CRESST collaboration [Sei95] and the EDELWEISS collaboration [Cha95], both using phonon-mediated detectors, the ORPHEUS collaboration [Abp95c] and the Lisbon-Zaragoza-Paris Dark Matter Search [Gir95] with superconducting superheated granule detectors.…”

Section: Background-blind Bubble Chambersmentioning

confidence: 99%

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Cryogenic particle detectors

Twerenbold

1996

Rep. Prog. Phys.

112

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A review of cryogenic particle detectors is presented. A major motivation for developing this type of particle detector is their superior sensitivity to weakly ionizing particle interactions. This makes them suitable devices for detecting solar neutrinos via the coherent neutrino scattering off nuclei and for detecting non-baryonic dark matter candidates in our galactic halo. Cryogenic particle detectors have reached, and in some cases already surpassed, the high energy resolution of the best semiconducting detectors, and they have the potential of becoming the next generation of high-resolution detectors. The emphasis of this review is on the basic condensed matter physics of these low-temperature detectors and to present an overview of the present experimental status.

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