Dark matter search with CRESST cryogenic detectors

Abstract Results of the CRESST experiment at Gran Sasso using 262-g sapphire calorimeters with tungsten phase transition thermometers are presented. Calibration and analysis methods are described. Data taken in 2000 have been used to place limits on WIMP dark matter particles in the Galactic halo. T...
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Autor*in:	Angloher, G. [verfasserIn] Altmann, M. Bruckmayer, M. Bucci, C. Cooper, S. Cozzini, C. Di Stefano, P. von Feilitzsch, F. Frank, T. Hauff, D. Jagemann, Th. Jochum, J. Keeling, R. Kraus, H. Macallister, J. Pröbst, F. Ramachers, Y. Schnagl, J. Seidel, W. Sergeyev, I. Stark, M. Stodolsky, L. Wulandari, H.

Format:	Artikel
Sprache:	Englisch

Erschienen:	2003

Schlagwörter:	Phase Transition Tungsten Elementary Particle Dark Matter Calorimeter

Anmerkung:	© MAIK "Nauka/Interperiodica" 2003

Übergeordnetes Werk:	Enthalten in: Physics of atomic nuclei - Nauka/Interperiodica, 1993, 66(2003), 3 vom: März, Seite 494-496
Übergeordnetes Werk:	volume:66 ; year:2003 ; number:3 ; month:03 ; pages:494-496

Links:	Volltext

DOI / URN:	10.1134/1.1563712

Katalog-ID:	OLC2049896085

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650		4	\|a Phase Transition
650		4	\|a Tungsten
650		4	\|a Elementary Particle
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700	1		\|a Altmann, M. \|4 aut
700	1		\|a Bruckmayer, M. \|4 aut
700	1		\|a Bucci, C. \|4 aut
700	1		\|a Cooper, S. \|4 aut
700	1		\|a Cozzini, C. \|4 aut
700	1		\|a Di Stefano, P. \|4 aut
700	1		\|a von Feilitzsch, F. \|4 aut
700	1		\|a Frank, T. \|4 aut
700	1		\|a Hauff, D. \|4 aut
700	1		\|a Jagemann, Th. \|4 aut
700	1		\|a Jochum, J. \|4 aut
700	1		\|a Keeling, R. \|4 aut
700	1		\|a Kraus, H. \|4 aut
700	1		\|a Macallister, J. \|4 aut
700	1		\|a Pröbst, F. \|4 aut
700	1		\|a Ramachers, Y. \|4 aut
700	1		\|a Schnagl, J. \|4 aut
700	1		\|a Seidel, W. \|4 aut
700	1		\|a Sergeyev, I. \|4 aut
700	1		\|a Stark, M. \|4 aut
700	1		\|a Stodolsky, L. \|4 aut
700	1		\|a Wulandari, H. \|4 aut
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allfields	10.1134/1.1563712 doi (DE-627)OLC2049896085 (DE-He213)1.1563712-p DE-627 ger DE-627 rakwb eng 530 VZ Angloher, G. verfasserin aut Dark matter search with CRESST cryogenic detectors 2003 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © MAIK "Nauka/Interperiodica" 2003 Abstract Results of the CRESST experiment at Gran Sasso using 262-g sapphire calorimeters with tungsten phase transition thermometers are presented. Calibration and analysis methods are described. Data taken in 2000 have been used to place limits on WIMP dark matter particles in the Galactic halo. The sapphire detectors are especially sensitive to low-mass WIMPs with spin-dependent interaction and improve on existing limits in this region. Phase Transition Tungsten Elementary Particle Dark Matter Calorimeter Altmann, M. aut Bruckmayer, M. aut Bucci, C. aut Cooper, S. aut Cozzini, C. aut Di Stefano, P. aut von Feilitzsch, F. aut Frank, T. aut Hauff, D. aut Jagemann, Th. aut Jochum, J. aut Keeling, R. aut Kraus, H. aut Macallister, J. aut Pröbst, F. aut Ramachers, Y. aut Schnagl, J. aut Seidel, W. aut Sergeyev, I. aut Stark, M. aut Stodolsky, L. aut Wulandari, H. aut Enthalten in Physics of atomic nuclei Nauka/Interperiodica, 1993 66(2003), 3 vom: März, Seite 494-496 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:66 year:2003 number:3 month:03 pages:494-496 https://doi.org/10.1134/1.1563712 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_40 GBV_ILN_70 GBV_ILN_2014 GBV_ILN_2279 AR 66 2003 3 03 494-496
spelling	10.1134/1.1563712 doi (DE-627)OLC2049896085 (DE-He213)1.1563712-p DE-627 ger DE-627 rakwb eng 530 VZ Angloher, G. verfasserin aut Dark matter search with CRESST cryogenic detectors 2003 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © MAIK "Nauka/Interperiodica" 2003 Abstract Results of the CRESST experiment at Gran Sasso using 262-g sapphire calorimeters with tungsten phase transition thermometers are presented. Calibration and analysis methods are described. Data taken in 2000 have been used to place limits on WIMP dark matter particles in the Galactic halo. The sapphire detectors are especially sensitive to low-mass WIMPs with spin-dependent interaction and improve on existing limits in this region. Phase Transition Tungsten Elementary Particle Dark Matter Calorimeter Altmann, M. aut Bruckmayer, M. aut Bucci, C. aut Cooper, S. aut Cozzini, C. aut Di Stefano, P. aut von Feilitzsch, F. aut Frank, T. aut Hauff, D. aut Jagemann, Th. aut Jochum, J. aut Keeling, R. aut Kraus, H. aut Macallister, J. aut Pröbst, F. aut Ramachers, Y. aut Schnagl, J. aut Seidel, W. aut Sergeyev, I. aut Stark, M. aut Stodolsky, L. aut Wulandari, H. aut Enthalten in Physics of atomic nuclei Nauka/Interperiodica, 1993 66(2003), 3 vom: März, Seite 494-496 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:66 year:2003 number:3 month:03 pages:494-496 https://doi.org/10.1134/1.1563712 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_40 GBV_ILN_70 GBV_ILN_2014 GBV_ILN_2279 AR 66 2003 3 03 494-496
allfields_unstemmed	10.1134/1.1563712 doi (DE-627)OLC2049896085 (DE-He213)1.1563712-p DE-627 ger DE-627 rakwb eng 530 VZ Angloher, G. verfasserin aut Dark matter search with CRESST cryogenic detectors 2003 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © MAIK "Nauka/Interperiodica" 2003 Abstract Results of the CRESST experiment at Gran Sasso using 262-g sapphire calorimeters with tungsten phase transition thermometers are presented. Calibration and analysis methods are described. Data taken in 2000 have been used to place limits on WIMP dark matter particles in the Galactic halo. The sapphire detectors are especially sensitive to low-mass WIMPs with spin-dependent interaction and improve on existing limits in this region. Phase Transition Tungsten Elementary Particle Dark Matter Calorimeter Altmann, M. aut Bruckmayer, M. aut Bucci, C. aut Cooper, S. aut Cozzini, C. aut Di Stefano, P. aut von Feilitzsch, F. aut Frank, T. aut Hauff, D. aut Jagemann, Th. aut Jochum, J. aut Keeling, R. aut Kraus, H. aut Macallister, J. aut Pröbst, F. aut Ramachers, Y. aut Schnagl, J. aut Seidel, W. aut Sergeyev, I. aut Stark, M. aut Stodolsky, L. aut Wulandari, H. aut Enthalten in Physics of atomic nuclei Nauka/Interperiodica, 1993 66(2003), 3 vom: März, Seite 494-496 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:66 year:2003 number:3 month:03 pages:494-496 https://doi.org/10.1134/1.1563712 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_40 GBV_ILN_70 GBV_ILN_2014 GBV_ILN_2279 AR 66 2003 3 03 494-496
allfieldsGer	10.1134/1.1563712 doi (DE-627)OLC2049896085 (DE-He213)1.1563712-p DE-627 ger DE-627 rakwb eng 530 VZ Angloher, G. verfasserin aut Dark matter search with CRESST cryogenic detectors 2003 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © MAIK "Nauka/Interperiodica" 2003 Abstract Results of the CRESST experiment at Gran Sasso using 262-g sapphire calorimeters with tungsten phase transition thermometers are presented. Calibration and analysis methods are described. Data taken in 2000 have been used to place limits on WIMP dark matter particles in the Galactic halo. The sapphire detectors are especially sensitive to low-mass WIMPs with spin-dependent interaction and improve on existing limits in this region. Phase Transition Tungsten Elementary Particle Dark Matter Calorimeter Altmann, M. aut Bruckmayer, M. aut Bucci, C. aut Cooper, S. aut Cozzini, C. aut Di Stefano, P. aut von Feilitzsch, F. aut Frank, T. aut Hauff, D. aut Jagemann, Th. aut Jochum, J. aut Keeling, R. aut Kraus, H. aut Macallister, J. aut Pröbst, F. aut Ramachers, Y. aut Schnagl, J. aut Seidel, W. aut Sergeyev, I. aut Stark, M. aut Stodolsky, L. aut Wulandari, H. aut Enthalten in Physics of atomic nuclei Nauka/Interperiodica, 1993 66(2003), 3 vom: März, Seite 494-496 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:66 year:2003 number:3 month:03 pages:494-496 https://doi.org/10.1134/1.1563712 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_40 GBV_ILN_70 GBV_ILN_2014 GBV_ILN_2279 AR 66 2003 3 03 494-496
allfieldsSound	10.1134/1.1563712 doi (DE-627)OLC2049896085 (DE-He213)1.1563712-p DE-627 ger DE-627 rakwb eng 530 VZ Angloher, G. verfasserin aut Dark matter search with CRESST cryogenic detectors 2003 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © MAIK "Nauka/Interperiodica" 2003 Abstract Results of the CRESST experiment at Gran Sasso using 262-g sapphire calorimeters with tungsten phase transition thermometers are presented. Calibration and analysis methods are described. Data taken in 2000 have been used to place limits on WIMP dark matter particles in the Galactic halo. The sapphire detectors are especially sensitive to low-mass WIMPs with spin-dependent interaction and improve on existing limits in this region. Phase Transition Tungsten Elementary Particle Dark Matter Calorimeter Altmann, M. aut Bruckmayer, M. aut Bucci, C. aut Cooper, S. aut Cozzini, C. aut Di Stefano, P. aut von Feilitzsch, F. aut Frank, T. aut Hauff, D. aut Jagemann, Th. aut Jochum, J. aut Keeling, R. aut Kraus, H. aut Macallister, J. aut Pröbst, F. aut Ramachers, Y. aut Schnagl, J. aut Seidel, W. aut Sergeyev, I. aut Stark, M. aut Stodolsky, L. aut Wulandari, H. aut Enthalten in Physics of atomic nuclei Nauka/Interperiodica, 1993 66(2003), 3 vom: März, Seite 494-496 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:66 year:2003 number:3 month:03 pages:494-496 https://doi.org/10.1134/1.1563712 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_40 GBV_ILN_70 GBV_ILN_2014 GBV_ILN_2279 AR 66 2003 3 03 494-496
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title	Dark matter search with CRESST cryogenic detectors
ctrlnum	(DE-627)OLC2049896085 (DE-He213)1.1563712-p
title_full	Dark matter search with CRESST cryogenic detectors
author_sort	Angloher, G.
journal	Physics of atomic nuclei
journalStr	Physics of atomic nuclei
lang_code	eng
isOA_bool	false
dewey-hundreds	500 - Science
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publishDateSort	2003
contenttype_str_mv	txt
container_start_page	494
author_browse	Angloher, G. Altmann, M. Bruckmayer, M. Bucci, C. Cooper, S. Cozzini, C. Di Stefano, P. von Feilitzsch, F. Frank, T. Hauff, D. Jagemann, Th. Jochum, J. Keeling, R. Kraus, H. Macallister, J. Pröbst, F. Ramachers, Y. Schnagl, J. Seidel, W. Sergeyev, I. Stark, M. Stodolsky, L. Wulandari, H.
container_volume	66
class	530 VZ
format_se	Aufsätze
author-letter	Angloher, G.
doi_str_mv	10.1134/1.1563712
dewey-full	530
title_sort	dark matter search with cresst cryogenic detectors
title_auth	Dark matter search with CRESST cryogenic detectors
abstract	Abstract Results of the CRESST experiment at Gran Sasso using 262-g sapphire calorimeters with tungsten phase transition thermometers are presented. Calibration and analysis methods are described. Data taken in 2000 have been used to place limits on WIMP dark matter particles in the Galactic halo. The sapphire detectors are especially sensitive to low-mass WIMPs with spin-dependent interaction and improve on existing limits in this region. © MAIK "Nauka/Interperiodica" 2003
abstractGer	Abstract Results of the CRESST experiment at Gran Sasso using 262-g sapphire calorimeters with tungsten phase transition thermometers are presented. Calibration and analysis methods are described. Data taken in 2000 have been used to place limits on WIMP dark matter particles in the Galactic halo. The sapphire detectors are especially sensitive to low-mass WIMPs with spin-dependent interaction and improve on existing limits in this region. © MAIK "Nauka/Interperiodica" 2003
abstract_unstemmed	Abstract Results of the CRESST experiment at Gran Sasso using 262-g sapphire calorimeters with tungsten phase transition thermometers are presented. Calibration and analysis methods are described. Data taken in 2000 have been used to place limits on WIMP dark matter particles in the Galactic halo. The sapphire detectors are especially sensitive to low-mass WIMPs with spin-dependent interaction and improve on existing limits in this region. © MAIK "Nauka/Interperiodica" 2003
collection_details	GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_40 GBV_ILN_70 GBV_ILN_2014 GBV_ILN_2279
container_issue	3
title_short	Dark matter search with CRESST cryogenic detectors
url	https://doi.org/10.1134/1.1563712
remote_bool	false
author2	Altmann, M. Bruckmayer, M. Bucci, C. Cooper, S. Cozzini, C. Di Stefano, P. von Feilitzsch, F. Frank, T. Hauff, D. Jagemann, Th Jochum, J. Keeling, R. Kraus, H. Macallister, J. Pröbst, F. Ramachers, Y. Schnagl, J. Seidel, W. Sergeyev, I. Stark, M. Stodolsky, L. Wulandari, H.
author2Str	Altmann, M. Bruckmayer, M. Bucci, C. Cooper, S. Cozzini, C. Di Stefano, P. von Feilitzsch, F. Frank, T. Hauff, D. Jagemann, Th Jochum, J. Keeling, R. Kraus, H. Macallister, J. Pröbst, F. Ramachers, Y. Schnagl, J. Seidel, W. Sergeyev, I. Stark, M. Stodolsky, L. Wulandari, H.
ppnlink	131188437
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hochschulschrift_bool	false
doi_str	10.1134/1.1563712
up_date	2024-07-04T00:25:47.069Z
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