2000
DOI: 10.1016/s0168-9002(99)01378-9
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First tests on phonon threshold spectroscopy

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Cited by 9 publications
(17 citation statements)
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“…Due to the long recombination time of quasiparticles at temperature well below the transition temperature of the superconductor, a significant fraction of the particle energy will be trapped in the superconductive layer in form of quasiparticles for a time that can extend up to the millisecond range in ultrapure aluminum. The subsequent recombination of quasiparticles to ∼ 1.2 K phonons will add a delayed component to the phonon signal read by the sensor on the crystal [54], less important in bulk events. Therefore, just by studying the signal shape and in particular the rise-time, it will be possible to discriminate bulk versus surface events, as the latter should be slower with a rise-time difference in the millisecond range.…”
Section: Discrimination Of Surface Radioactivity In Crossmentioning
confidence: 99%
“…Due to the long recombination time of quasiparticles at temperature well below the transition temperature of the superconductor, a significant fraction of the particle energy will be trapped in the superconductive layer in form of quasiparticles for a time that can extend up to the millisecond range in ultrapure aluminum. The subsequent recombination of quasiparticles to ∼ 1.2 K phonons will add a delayed component to the phonon signal read by the sensor on the crystal [54], less important in bulk events. Therefore, just by studying the signal shape and in particular the rise-time, it will be possible to discriminate bulk versus surface events, as the latter should be slower with a rise-time difference in the millisecond range.…”
Section: Discrimination Of Surface Radioactivity In Crossmentioning
confidence: 99%
“…Finally, it is important to develop procedures to avoid surface contamination during the construction and storage of the detector components and the detector assembling. In particular, any exposure to air may lead to dangerous 222 Rn-induced pollution. 126 To prevent that, the detector assembly has to be carried out at least in a clean room and/or in glove boxes under a nitrogen atmosphere, as e.g.…”
Section: 2017 1:18 Wspc/instruction File Lrt˙bolometers˙v04amentioning
confidence: 99%
“…In particular, in spite of a twice lower light yield, an efficient α rejection has been recently demonstrated with Li 2 100 MoO 4 scintillating bolometers operated without a reflecting film. 41 developed for dark mater search detectors, 222 in which only one superconducting thermometer is used, while the rest of the surface is covered by an additional superconducting film. The working principle is the following: athermal phonons released by a particle interaction within a few mm from the surface (i.e.…”
Section: Surface α and β Backgroundmentioning
confidence: 99%
“…Rare α decay Ce, Nd, Sm, Eu, Gd, Dy, 144 Nd, 147,148,149 Sm, 151 Eu, [29] Ho, Er, Tm, Yb, Lu, Hf, 152 Gd, 174,176 Hf, 180 W, Ta, W, Re, Os, Ir, Pt, Au, 184,186,187 Os, 190 Pt, 209 Bi Hg, Tl, Pb, Bi, Th, U Rare β decay K, Ca, V, Rb, Zr, Cd, In, 50 V, 113 Cd, 115 In [29][30][31][32] Te, La, Lu, Ta, Re (4-fold-forbidden β decay) Double-β decay Ar, Ca, Cr, Fe, Ni, Zn, Ge, 48 Ca, 76 Ge, 82 Se, 96 Zr, [33][34][35][36][37] Se, Kr, Sr, Zr, Mo, Ru, Pd, 100 Mo, 110 Pd, 116 Cd, 124 Sn, Cd, Sn, Te, Xe, Ba, Ce, Nd, 130 Te, 136 Xe, 150 Nd Sm, Gd, Dy, Er, Yb, Hf, W, Os, Pt, Hg, Th, U Dark matter (WIMP a ) low/high atomic mass 7 Li, 11 B, 19 F, 23 Na, 27 Al, 73 Ge, [38][39][40]…”
Section: Applicationmentioning
confidence: 99%