Munich cryogenic detector development for direct Dark Matter search

A. Nucciotti; P. Colling; S. Cooper; D. Dummer; F. v. Feilitzsch; P. Ferger; G. Forster; Matthias Frank; H. J. Gebauer; K. Hallatschek; E. Kellner; U. Nagel; F. Pröbst; A. Rulofs; W. Seidel; L. Stodolsky

doi:10.1016/0920-5632(94)90241-0

Munich cryogenic detector development for direct Dark Matter search

A. Nucciotti, P. Colling, S. Cooper, D. Dummer, F. v. Feilitzsch, P. Ferger, G. Forster, Matthias Frank, H. J. Gebauer, K. Hallatschek, E. Kellner, U. Nagel, F. Pröbst, A. Rulofs, W. Seidel, L. Stodolsky

Research output: Contribution to journal › Article › peer-review

3 Scopus citations

Abstract

We are developing massive cryogenic detectors with low energy thresholds and high resolution for use in a direct Dark Matter search experiment. Our detector consists of a superconducting phase transition thermometer evaporated onto the surface of an absorber crystal. An energy resolution of 220 eV FWHM (for 6 keV X-rays) has been reached with a 31 g sapphire crystal using a proximity-effect thermometer. The latest results for sapphire detectors using tungsten superconducting phase transition thermometers, whose development is just beginning, are also presented. The planned further development and use of such detectors in a search for Dark Matter particles (WIMPs) is discussed, showing their advantages for low WIMP masses.

Original language	English (US)
Pages (from-to)	172-174
Number of pages	3
Journal	Nuclear Physics B (Proceedings Supplements)
Volume	35
Issue number	C
DOIs	https://doi.org/10.1016/0920-5632(94)90241-0
State	Published - Jan 1 1994
Externally published	Yes

ASJC Scopus subject areas

Atomic and Molecular Physics, and Optics
Nuclear and High Energy Physics

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Nucciotti, A., Colling, P., Cooper, S., Dummer, D., Feilitzsch, F. V., Ferger, P., Forster, G., Frank, M., Gebauer, H. J., Hallatschek, K., Kellner, E., Nagel, U., Pröbst, F., Rulofs, A., Seidel, W., & Stodolsky, L. (1994). Munich cryogenic detector development for direct Dark Matter search. Nuclear Physics B (Proceedings Supplements), 35(C), 172-174. https://doi.org/10.1016/0920-5632(94)90241-0

Munich cryogenic detector development for direct Dark Matter search. / Nucciotti, A.; Colling, P.; Cooper, S.; Dummer, D.; Feilitzsch, F. v.; Ferger, P.; Forster, G.; Frank, Matthias; Gebauer, H. J.; Hallatschek, K.; Kellner, E.; Nagel, U.; Pröbst, F.; Rulofs, A.; Seidel, W.; Stodolsky, L.

In: Nuclear Physics B (Proceedings Supplements), Vol. 35, No. C, 01.01.1994, p. 172-174.

Research output: Contribution to journal › Article › peer-review

Nucciotti, A, Colling, P, Cooper, S, Dummer, D, Feilitzsch, FV, Ferger, P, Forster, G, Frank, M, Gebauer, HJ, Hallatschek, K, Kellner, E, Nagel, U, Pröbst, F, Rulofs, A, Seidel, W & Stodolsky, L 1994, 'Munich cryogenic detector development for direct Dark Matter search', Nuclear Physics B (Proceedings Supplements), vol. 35, no. C, pp. 172-174. https://doi.org/10.1016/0920-5632(94)90241-0

Nucciotti, A. ; Colling, P. ; Cooper, S. ; Dummer, D. ; Feilitzsch, F. v. ; Ferger, P. ; Forster, G. ; Frank, Matthias ; Gebauer, H. J. ; Hallatschek, K. ; Kellner, E. ; Nagel, U. ; Pröbst, F. ; Rulofs, A. ; Seidel, W. ; Stodolsky, L. / Munich cryogenic detector development for direct Dark Matter search. In: Nuclear Physics B (Proceedings Supplements). 1994 ; Vol. 35, No. C. pp. 172-174.

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AU - Forster, G.

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AU - Nagel, U.

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AB - We are developing massive cryogenic detectors with low energy thresholds and high resolution for use in a direct Dark Matter search experiment. Our detector consists of a superconducting phase transition thermometer evaporated onto the surface of an absorber crystal. An energy resolution of 220 eV FWHM (for 6 keV X-rays) has been reached with a 31 g sapphire crystal using a proximity-effect thermometer. The latest results for sapphire detectors using tungsten superconducting phase transition thermometers, whose development is just beginning, are also presented. The planned further development and use of such detectors in a search for Dark Matter particles (WIMPs) is discussed, showing their advantages for low WIMP masses.

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Munich cryogenic detector development for direct Dark Matter search

Abstract

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