4.7 Article

Enriched TeO2 bolometers with active particle discrimination: Towards the CUPID experiment

Journal

PHYSICS LETTERS B
Volume 767, Issue -, Pages 321-329

Publisher

ELSEVIER
DOI: 10.1016/j.physletb.2017.02.011

Keywords

Double beta decay; Bolometers; Isotope enrichment; Cherenkov emission; Neganov-Luke effect

Funding

  1. LUCIFER experiment - European Research Council under the Seventh Framework Programme (FP7) ERC Grant [247115]
  2. Italian Ministry of Research [PRIN 2010ZXAZK9]
  3. US National Science Foundation [0605119, 1307204]
  4. National Natural Science Foundation of China [51302287, 61405229]
  5. US Department of Energy National Nuclear Security Administration [DE-NA0000979]
  6. US Department of Energy by LLNL [DE-AC52-07NA27344]
  7. LUMINEU program from the Agence Nationale de la Recherche (France)
  8. Direct For Mathematical & Physical Scien
  9. Division Of Physics [1307204, 0605119] Funding Source: National Science Foundation
  10. Direct For Mathematical & Physical Scien
  11. Division Of Physics [1614611] Funding Source: National Science Foundation

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We present the performances of two 92% enriched (TeO2)-Te-130 crystals operated as thermal bolometers in view of a next generation experiment to search for neutrinoless double beta decay of Te-130. The crystals, 435 g each, show an energy resolution, evaluated at the 2615keV gamma-line of Tl-208, of 6.5 and 4.3keV FWHM. The only observable internal radioactive contamination arises from U-238 (15 and 8 mu Bq/kg, respectively). The internal activity of the most problematic nuclei for neutrinoless double beta decay, Ra-226 and Th-228, are both evaluated as < 3.1 mu Bq/kg for one crystal and < 2.3 mu Bq/kg for the second. Thanks to the readout of the weak Cherenkov light emitted by beta/gamma particles by means of Neganov-Luke bolometric light detectors we were able to perform an event-by-event identification of beta/gamma events with a 95% acceptance level, while establishing a rejection factor of 98.21% and 99.99% for alpha particles. (C) 2017 The Authors. Published by Elsevier B.V.

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