TES-Based Light Detectors for the CRESST Direct Dark Matter Search

J. Rothe; G. Angloher; P. Bauer; A. Bento; C. Bucci; L. Canonica; A. D’Addabbo; 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; K. Schäffner; J. Schieck; V. Schipperges; S. Schönert; W. Seidel; M. Stahlberg; L. Stodolsky; C. Strandhagen; R. Strauss; A. Tanzke; H. H. Trinh Thi; C. Türkoğlu; A. Ulrich; I. Usherov; S. Wawoczny; M. Willers; M. Wüstrich

doi:10.1007/s10909-018-1944-x

TES-Based Light Detectors for the CRESST Direct Dark Matter Search

J. Rothe, G. Angloher, P. Bauer, A. Bento, C. Bucci, L. Canonica, A. D’Addabbo, 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. LangenkämperJ. Loebell, M. Mancuso, E. Mondragon, A. Münster, C. Pagliarone, F. Petricca, W. Potzel, F. Pröbst, R. Puig, F. Reindl, K. Schäffner, J. Schieck, V. Schipperges, S. Schönert, W. Seidel, M. Stahlberg, L. Stodolsky, C. Strandhagen, R. Strauss, A. Tanzke, H. H. Trinh Thi, C. Türkoğlu, A. Ulrich, I. Usherov, S. Wawoczny, M. Willers, M. Wüstrich

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Abstract

The CRESST experiment uses cryogenic detectors based on transition-edge sensors to search for dark matter interactions. Each detector module consists of a scintillating CaWO₄ crystal and a silicon-on-sapphire (SOS) light detector which operate in coincidence (phonon-light technique). The 40-mm-diameter SOS disks (2 g mass) used in the data taking campaign of CRESST-II Phase 2 (2014–2016) reached absolute baseline resolutions of σ= 4–7 eV. This is the best performance reported for cryogenic light detectors of this size. Newly developed silicon beaker light detectors (4 cm height, 4 cm diameter, 6 g mass), which cover a large fraction of the target crystal surface, have achieved a baseline resolution of σ=5.8eV. First results of further improved light detectors developed for the ongoing low-threshold CRESST-III experiment are presented.

Original language	English
Pages (from-to)	1160-1166
Number of pages	7
Journal	Journal of Low Temperature Physics
Volume	193
Issue number	5-6
DOIs	https://doi.org/10.1007/s10909-018-1944-x
State	Published - 1 Dec 2018

Keywords

Cryogenic light detector
Direct dark matter search
Transition-edge sensor

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10.1007/s10909-018-1944-x

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Rothe, J., Angloher, G., Bauer, P., Bento, A., Bucci, C., Canonica, L., D’Addabbo, A., Defay, X., Erb, A., Feilitzsch, F. V., Ferreiro Iachellini, N., Gorla, P., Gütlein, A., Hauff, D., Jochum, J., Kiefer, M., Kluck, H., Kraus, H., Lanfranchi, J. C., ... Wüstrich, M. (2018). TES-Based Light Detectors for the CRESST Direct Dark Matter Search. Journal of Low Temperature Physics, 193(5-6), 1160-1166. https://doi.org/10.1007/s10909-018-1944-x

@article{56a687a5e34d4a0f9e6923a5fe77c453,

title = "TES-Based Light Detectors for the CRESST Direct Dark Matter Search",

abstract = "The CRESST experiment uses cryogenic detectors based on transition-edge sensors to search for dark matter interactions. Each detector module consists of a scintillating CaWO4 crystal and a silicon-on-sapphire (SOS) light detector which operate in coincidence (phonon-light technique). The 40-mm-diameter SOS disks (2 g mass) used in the data taking campaign of CRESST-II Phase 2 (2014–2016) reached absolute baseline resolutions of σ= 4–7 eV. This is the best performance reported for cryogenic light detectors of this size. Newly developed silicon beaker light detectors (4 cm height, 4 cm diameter, 6 g mass), which cover a large fraction of the target crystal surface, have achieved a baseline resolution of σ=5.8eV. First results of further improved light detectors developed for the ongoing low-threshold CRESST-III experiment are presented.",

keywords = "Cryogenic light detector, Direct dark matter search, Transition-edge sensor",

author = "J. Rothe and G. Angloher and P. Bauer and A. Bento and C. Bucci and L. Canonica and A. D{\textquoteright}Addabbo and X. Defay and A. Erb and Feilitzsch, {F. v.} and {Ferreiro Iachellini}, N. and P. Gorla and A. G{\"u}tlein and D. Hauff and J. Jochum and M. Kiefer and H. Kluck and H. Kraus and Lanfranchi, {J. C.} and A. Langenk{\"a}mper and J. Loebell and M. Mancuso and E. Mondragon and A. M{\"u}nster and C. Pagliarone and F. Petricca and W. Potzel and F. Pr{\"o}bst and R. Puig and F. Reindl and K. Sch{\"a}ffner and J. Schieck and V. Schipperges and S. Sch{\"o}nert and W. Seidel and M. Stahlberg and L. Stodolsky and C. Strandhagen and R. Strauss and A. Tanzke and {Trinh Thi}, {H. H.} and C. T{\"u}rkoğlu and A. Ulrich and I. Usherov and S. Wawoczny and M. Willers and M. W{\"u}strich",

note = "Publisher Copyright: {\textcopyright} 2018, The Author(s).",

year = "2018",

month = dec,

day = "1",

doi = "10.1007/s10909-018-1944-x",

language = "English",

volume = "193",

pages = "1160--1166",

journal = "Journal of Low Temperature Physics",

issn = "0022-2291",

publisher = "Springer New York",

number = "5-6",

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Rothe, J, Angloher, G, Bauer, P, Bento, A, Bucci, C, Canonica, L, D’Addabbo, A, Defay, X, Erb, A, Feilitzsch, FV, Ferreiro Iachellini, N, Gorla, P, Gütlein, A, Hauff, D, Jochum, J, Kiefer, M, Kluck, H, Kraus, H, Lanfranchi, JC, Langenkämper, A, Loebell, J, Mancuso, M, Mondragon, E, Münster, A, Pagliarone, C, Petricca, F, Potzel, W, Pröbst, F, Puig, R, Reindl, F, Schäffner, K, Schieck, J, Schipperges, V, Schönert, S, Seidel, W, Stahlberg, M, Stodolsky, L, Strandhagen, C, Strauss, R, Tanzke, A, Trinh Thi, HH, Türkoğlu, C, Ulrich, A, Usherov, I, Wawoczny, S, Willers, M & Wüstrich, M 2018, 'TES-Based Light Detectors for the CRESST Direct Dark Matter Search', Journal of Low Temperature Physics, vol. 193, no. 5-6, pp. 1160-1166. https://doi.org/10.1007/s10909-018-1944-x

TY - JOUR

T1 - TES-Based Light Detectors for the CRESST Direct Dark Matter Search

AU - Rothe, J.

AU - Angloher, G.

AU - Bauer, P.

AU - Bento, A.

AU - Bucci, C.

AU - Canonica, L.

AU - D’Addabbo, A.

AU - Defay, X.

AU - Erb, A.

AU - Feilitzsch, F. v.

AU - Ferreiro Iachellini, N.

AU - Gorla, P.

AU - Gütlein, A.

AU - Hauff, D.

AU - Jochum, J.

AU - Kiefer, M.

AU - Kluck, H.

AU - Kraus, H.

AU - Lanfranchi, J. C.

AU - Langenkämper, A.

AU - Loebell, J.

AU - Mancuso, M.

AU - Mondragon, E.

AU - Münster, A.

AU - Pagliarone, C.

AU - Petricca, F.

AU - Potzel, W.

AU - Pröbst, F.

AU - Puig, R.

AU - Reindl, F.

AU - Schäffner, K.

AU - Schieck, J.

AU - Schipperges, V.

AU - Schönert, S.

AU - Seidel, W.

AU - Stahlberg, M.

AU - Stodolsky, L.

AU - Strandhagen, C.

AU - Strauss, R.

AU - Tanzke, A.

AU - Trinh Thi, H. H.

AU - Türkoğlu, C.

AU - Ulrich, A.

AU - Usherov, I.

AU - Wawoczny, S.

AU - Willers, M.

AU - Wüstrich, M.

PY - 2018/12/1

Y1 - 2018/12/1

N2 - The CRESST experiment uses cryogenic detectors based on transition-edge sensors to search for dark matter interactions. Each detector module consists of a scintillating CaWO4 crystal and a silicon-on-sapphire (SOS) light detector which operate in coincidence (phonon-light technique). The 40-mm-diameter SOS disks (2 g mass) used in the data taking campaign of CRESST-II Phase 2 (2014–2016) reached absolute baseline resolutions of σ= 4–7 eV. This is the best performance reported for cryogenic light detectors of this size. Newly developed silicon beaker light detectors (4 cm height, 4 cm diameter, 6 g mass), which cover a large fraction of the target crystal surface, have achieved a baseline resolution of σ=5.8eV. First results of further improved light detectors developed for the ongoing low-threshold CRESST-III experiment are presented.

AB - The CRESST experiment uses cryogenic detectors based on transition-edge sensors to search for dark matter interactions. Each detector module consists of a scintillating CaWO4 crystal and a silicon-on-sapphire (SOS) light detector which operate in coincidence (phonon-light technique). The 40-mm-diameter SOS disks (2 g mass) used in the data taking campaign of CRESST-II Phase 2 (2014–2016) reached absolute baseline resolutions of σ= 4–7 eV. This is the best performance reported for cryogenic light detectors of this size. Newly developed silicon beaker light detectors (4 cm height, 4 cm diameter, 6 g mass), which cover a large fraction of the target crystal surface, have achieved a baseline resolution of σ=5.8eV. First results of further improved light detectors developed for the ongoing low-threshold CRESST-III experiment are presented.

KW - Cryogenic light detector

KW - Direct dark matter search

KW - Transition-edge sensor

UR - http://www.scopus.com/inward/record.url?scp=85046772190&partnerID=8YFLogxK

U2 - 10.1007/s10909-018-1944-x

DO - 10.1007/s10909-018-1944-x

M3 - Article

AN - SCOPUS:85046772190

SN - 0022-2291

VL - 193

SP - 1160

EP - 1166

JO - Journal of Low Temperature Physics

JF - Journal of Low Temperature Physics

IS - 5-6

ER -

TES-Based Light Detectors for the CRESST Direct Dark Matter Search

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Keywords

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