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Publication
Featured researches published by C. Pagliarone.
arXiv: Cosmology and Nongalactic Astrophysics | 2016
F. Petricca; G. Angloher; A. Bento; C. Bucci; L. Canonica; X. Defay; A. Erb; F.v. Feilitzsch; N. Ferreiro Iachellini; P. Gorla; A. Gütlein; D. Hauff; J. Jochum; M. Kiefer; H. Kluck; H. Kraus; J.-C. Lanfranchi; J. Loebell; A. Münster; C. Pagliarone; W. Potzel; F. Pröbst; F. Reindl; K. Schäffner; Jochen Schieck; S. Schönert; W. Seidel; L. Stodolsky; C. Strandhagen; R. Strauss
The CRESST experiment, located at Laboratori Nazionali del Gran Sasso in Italy, searches for dark matter particles via their elastic scattering off nuclei in a target material. The CRESST target consists of scintillating CaWO
Journal of Physics: Conference Series | 2016
R. Strauss; G. Angloher; A. Bento; C. Bucci; L. Canonica; X. Defay; A. Erb; F. von Feilitzsch; N. Ferreiro Iachellini; P. Gorla; A. Gütlein; D. Hauff; J. Jochum; M. Kiefer; H. Kluck; H. Kraus; J.-C. Lanfranchi; J. Loebell; A. Münster; C. Pagliarone; F. Petricca; W. Potzel; F. Pröbst; F. Reindl; K. Schäffner; Jochen Schieck; S. Schönert; W. Seidel; L. Stodolsky; C. Strandhagen
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arXiv: Instrumentation and Detectors | 2016
F. Reindl; G. Angloher; A. Bento; C. Bucci; L. Canonica; X. Defay; A. Erb; F.v. Feilitzsch; N. Ferreiro Iachellini; P. Gorla; A. Gütlein; D. Hauff; J. Jochum; M. Kiefer; H. Kluck; H. Kraus; J.-C. Lanfranchi; J. Loebell; A. Münster; C. Pagliarone; F. Petricca; W. Potzel; F. Pröbst; K. Schäffner; Jochen Schieck; S. Schönert; W. Seidel; L. Stodolsky; C. Strandhagen; R. Strauss
crystals, which are operated as cryogenic calorimeters at millikelvin temperatures. Each interaction in the CaWO
Proceedings of The European Physical Society Conference on High Energy Physics — PoS(EPS-HEP2017) | 2017
C. Türkoğlu; G. Angloher; P. Bauer; A. Bento; C. Bucci; L. Canonica; X. Defay; A. Erb; F.v. Feilitzsch; N. Ferreiro Iachellini; P. Gorla; A. Gütlein; D. Hauff; J. Jochum; M. Kiefer; H. Kluck; H. Kraus; J.-C. Lanfranchi; A. Langenkämper; J. Loebell; M. Mancuso; E. Mondragon; A. Münster; C. Pagliarone; F. Petricca; W. Potzel; F. Pröbst; R. Puig; F. Reindl; J. Rothe
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27th International Conference on Neutrino Physics and Astrophysics (Neutrino 2016) | 2017
M. Willers; G. Angloher; A. Bento; C. Bucci; L. Canonica; X. Defay; A. Erb; F.v. Feilitzsch; N. Ferreiro Iachellini; A. Gütlein; P. Gorla; D. Hauff; J. Jochum; M. Kiefer; H. Kluck; H. Kraus; J-C Lanfranchi; J. Loebell; M. Mancuso; A. Münster; C. Pagliarone; F. Petricca; W. Potzel; F. Pröbst; R. Puig; F. Reindl; K. Schäffner; Jochen Schieck; S. Schönert; W. Seidel
target crystal produces a phonon signal and a light signal that is measured by a second cryogenic calorimeter. Since the CRESST-II result in 2015, the experiment is leading the field of direct dark matter search for dark matter masses below 1.7\,GeV/
European Physical Journal C | 2016
G. Angloher; A. Bento; C. Bucci; L. Canonica; X. Defay; A. Erb; F. von Feilitzsch; N. Ferreiro Iachellini; P. Gorla; A. Gütlein; D. Hauff; J. Jochum; M. Kiefer; H. Kluck; H. Kraus; J.-C. Lanfranchi; J. Loebell; A. Münster; C. Pagliarone; F. Petricca; W. Potzel; Frank J. Probst; F. Reindl; K. Schäffner; Jochen Schieck; S. Schönert; W. Seidel; L. Stodolsky; C. Strandhagen; R. Strauss
c^2
European Physical Journal C | 2017
G. Angloher; P. Bauer; A. Bento; C. Bucci; L. Canonica; X. Defay; A. Erb; F.v. Feilitzsch; N. Ferreiro Iachellini; P. Gorla; A. Gütlein; D. Hauff; J. Jochum; M. Kiefer; H. Kluck; H. Kraus; J.-C. Lanfranchi; A. Langenkämper; J. Loebell; M. Mancuso; E. Mondragon; A. Münster; L. Oberauer; C. Pagliarone; F. Petricca; W. Potzel; F. Pröbst; R. Puig; F. Reindl; J. Rothe
, extending the reach of direct searches to the sub-GeV/
European Physical Journal C | 2017
G. Angloher; P. Bauer; A. Bento; C. Bucci; L. Canonica; X. Defay; A. Erb; F.v. Feilitzsch; N. Ferreiro Iachellini; P. Gorla; A. Gütlein; D. Hauff; J. Jochum; M. Kiefer; H. Kluck; H. Kraus; J.-C. Lanfranchi; J. Loebell; M. Mancuso; A. Münster; C. Pagliarone; F. Petricca; W. Potzel; F. Pröbst; R. Puig; F. Reindl; K. Schäffner; Jochen Schieck; S. Schönert; W. Seidel
c^2
Journal of Low Temperature Physics | 2016
R. Strauss; G. Angloher; A. Bento; C. Bucci; L. Canonica; X. Defay; A. Erb; F.v. Feilitzsch; N. Ferreiro Iachellini; P. Gorla; A. Gütlein; D. Hauff; J. Jochum; M. Kiefer; H. Kluck; H. Kraus; J.-C. Lanfranchi; J. Loebell; A. Münster; C. Pagliarone; F. Petricca; W. Potzel; F. Pröbst; F. Reindl; K. Schäffner; Jochen Schieck; S. Schönert; W. Seidel; L. Stodolsky; C. Strandhagen
mass region. For CRESST-III, whose Phase 1 started in July 2016, detectors have been optimized to reach the performance required to further probe the low-mass region with unprecedented sensitivity. In this contribution the achievements of the CRESST-III detectors will be discussed together with preliminary results and perspectives of Phase 1.
arXiv: High Energy Physics - Phenomenology | 2018
G. Angloher; P. Bauer; A. Bento; E. Bertoldo; C. Bucci; L. Canonica; A. D'Addabbo; X. Defay; S. Di Lorenzo; A. Erb; F.v. Feilitzsch; N. Ferreiro Iachellini; P. Gorla; D. Hauff; J. Jochum; M. Kiefer; H. Kluck; H. Kraus; A. Langenkämper; M. Mancuso; V. Mokina; E. Mondragon; V. Morgalyuk; A. Münster; M. Olmi; C. Pagliarone; F. Petricca; W. Potzel; F. Pröbst; F. Reindl
The next generation direct dark matter experiment CRESST-III has a high potential to significantly increase the sensitivity to low-mass WIMPs (mx 10GeV/c2). We present the new CRESST detector module: it consists of a 24 g CaWO4 crystal operated as a phonon detector and a 20×20 mm2 silicon-on-sapphire light detector. The phonon energy threshold is lowered to ~100eV and a light detector resolution of typically 5eV is achieved. A fully-scintillating inner detector housing is realised which efficiently rejects events from surface-alpha decays. The CaWO4 sticks holding the target crystal are also operated as calorimeters to discriminate all possible artefacts related to the support structure. A projection for the sensitivity to spin-independent WIMP-nucleon scattering is given for the first phase of CRESST-III which will start beginning of 2016.