Search for Dark Matter Axions with CAST-CAPP

Haloscopes aim at detecting axions by converting them into photons using high-quality resonant cavities, where the cavity resonance should be tuned with the unknown axion mass. Here, the authors improve exclusion limits using four phase-matched resonant cavities and a fast frequency scanning techniq...
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Autor*in:	C. M. Adair [verfasserIn] K. Altenmüller [verfasserIn] V. Anastassopoulos [verfasserIn] S. Arguedas Cuendis [verfasserIn] J. Baier [verfasserIn] K. Barth [verfasserIn] A. Belov [verfasserIn] D. Bozicevic [verfasserIn] H. Bräuninger [verfasserIn] G. Cantatore [verfasserIn] F. Caspers [verfasserIn] J. F. Castel [verfasserIn] S. A. Çetin [verfasserIn] W. Chung [verfasserIn] H. Choi [verfasserIn] J. Choi [verfasserIn] T. Dafni [verfasserIn] M. Davenport [verfasserIn] A. Dermenev [verfasserIn] K. Desch [verfasserIn] B. Döbrich [verfasserIn] H. Fischer [verfasserIn] W. Funk [verfasserIn] J. Galan [verfasserIn] A. Gardikiotis [verfasserIn] S. Gninenko [verfasserIn] J. Golm [verfasserIn] M. D. Hasinoff [verfasserIn] D. H. H. Hoffmann [verfasserIn] D. Díez Ibáñez [verfasserIn] I. G. Irastorza [verfasserIn] K. Jakovčić [verfasserIn] J. Kaminski [verfasserIn] M. Karuza [verfasserIn] C. Krieger [verfasserIn] Ç. Kutlu [verfasserIn] B. Lakić [verfasserIn] J. M. Laurent [verfasserIn] J. Lee [verfasserIn] S. Lee [verfasserIn] G. Luzón [verfasserIn] C. Malbrunot [verfasserIn] C. Margalejo [verfasserIn] M. Maroudas [verfasserIn] L. Miceli [verfasserIn] H. Mirallas [verfasserIn] L. Obis [verfasserIn] A. Özbey [verfasserIn] K. Özbozduman [verfasserIn] M. J. Pivovaroff [verfasserIn] M. Rosu [verfasserIn] J. Ruz [verfasserIn] E. Ruiz-Chóliz [verfasserIn] S. Schmidt [verfasserIn] M. Schumann [verfasserIn] Y. K. Semertzidis [verfasserIn] S. K. Solanki [verfasserIn] L. Stewart [verfasserIn] I. Tsagris [verfasserIn] T. Vafeiadis [verfasserIn] J. K. Vogel [verfasserIn] M. Vretenar [verfasserIn] S. Youn [verfasserIn] K. Zioutas [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2022

Übergeordnetes Werk:	In: Nature Communications - Nature Portfolio, 2016, 13(2022), 1, Seite 9
Übergeordnetes Werk:	volume:13 ; year:2022 ; number:1 ; pages:9

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.1038/s41467-022-33913-6

Katalog-ID:	DOAJ027870944

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allfields	10.1038/s41467-022-33913-6 doi (DE-627)DOAJ027870944 (DE-599)DOAJ2d52b11f8305495ea826ef6617840ebd DE-627 ger DE-627 rakwb eng C. M. Adair verfasserin aut Search for Dark Matter Axions with CAST-CAPP 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Haloscopes aim at detecting axions by converting them into photons using high-quality resonant cavities, where the cavity resonance should be tuned with the unknown axion mass. Here, the authors improve exclusion limits using four phase-matched resonant cavities and a fast frequency scanning technique. Science Q K. Altenmüller verfasserin aut V. Anastassopoulos verfasserin aut S. Arguedas Cuendis verfasserin aut J. Baier verfasserin aut K. Barth verfasserin aut A. Belov verfasserin aut D. Bozicevic verfasserin aut H. Bräuninger verfasserin aut G. Cantatore verfasserin aut F. Caspers verfasserin aut J. F. Castel verfasserin aut S. A. Çetin verfasserin aut W. Chung verfasserin aut H. Choi verfasserin aut J. Choi verfasserin aut T. Dafni verfasserin aut M. Davenport verfasserin aut A. Dermenev verfasserin aut K. Desch verfasserin aut B. Döbrich verfasserin aut H. Fischer verfasserin aut W. Funk verfasserin aut J. Galan verfasserin aut A. Gardikiotis verfasserin aut S. Gninenko verfasserin aut J. Golm verfasserin aut M. D. Hasinoff verfasserin aut D. H. H. Hoffmann verfasserin aut D. Díez Ibáñez verfasserin aut I. G. Irastorza verfasserin aut K. Jakovčić verfasserin aut J. Kaminski verfasserin aut M. Karuza verfasserin aut C. Krieger verfasserin aut Ç. Kutlu verfasserin aut B. Lakić verfasserin aut J. M. Laurent verfasserin aut J. Lee verfasserin aut S. Lee verfasserin aut G. Luzón verfasserin aut C. Malbrunot verfasserin aut C. Margalejo verfasserin aut M. Maroudas verfasserin aut L. Miceli verfasserin aut H. Mirallas verfasserin aut L. Obis verfasserin aut A. Özbey verfasserin aut K. Özbozduman verfasserin aut M. J. Pivovaroff verfasserin aut M. Rosu verfasserin aut J. Ruz verfasserin aut E. Ruiz-Chóliz verfasserin aut S. Schmidt verfasserin aut M. Schumann verfasserin aut Y. K. Semertzidis verfasserin aut S. K. Solanki verfasserin aut L. Stewart verfasserin aut I. Tsagris verfasserin aut T. Vafeiadis verfasserin aut J. K. Vogel verfasserin aut M. Vretenar verfasserin aut S. Youn verfasserin aut K. Zioutas verfasserin aut In Nature Communications Nature Portfolio, 2016 13(2022), 1, Seite 9 (DE-627)626457688 (DE-600)2553671-0 20411723 nnns volume:13 year:2022 number:1 pages:9 https://doi.org/10.1038/s41467-022-33913-6 kostenfrei https://doaj.org/article/2d52b11f8305495ea826ef6617840ebd kostenfrei https://doi.org/10.1038/s41467-022-33913-6 kostenfrei https://doaj.org/toc/2041-1723 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_211 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_2110 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 13 2022 1 9
spelling	10.1038/s41467-022-33913-6 doi (DE-627)DOAJ027870944 (DE-599)DOAJ2d52b11f8305495ea826ef6617840ebd DE-627 ger DE-627 rakwb eng C. M. Adair verfasserin aut Search for Dark Matter Axions with CAST-CAPP 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Haloscopes aim at detecting axions by converting them into photons using high-quality resonant cavities, where the cavity resonance should be tuned with the unknown axion mass. Here, the authors improve exclusion limits using four phase-matched resonant cavities and a fast frequency scanning technique. Science Q K. Altenmüller verfasserin aut V. Anastassopoulos verfasserin aut S. Arguedas Cuendis verfasserin aut J. Baier verfasserin aut K. Barth verfasserin aut A. Belov verfasserin aut D. Bozicevic verfasserin aut H. Bräuninger verfasserin aut G. Cantatore verfasserin aut F. Caspers verfasserin aut J. F. Castel verfasserin aut S. A. Çetin verfasserin aut W. Chung verfasserin aut H. Choi verfasserin aut J. Choi verfasserin aut T. Dafni verfasserin aut M. Davenport verfasserin aut A. Dermenev verfasserin aut K. Desch verfasserin aut B. Döbrich verfasserin aut H. Fischer verfasserin aut W. Funk verfasserin aut J. Galan verfasserin aut A. Gardikiotis verfasserin aut S. Gninenko verfasserin aut J. Golm verfasserin aut M. D. Hasinoff verfasserin aut D. H. H. Hoffmann verfasserin aut D. Díez Ibáñez verfasserin aut I. G. Irastorza verfasserin aut K. Jakovčić verfasserin aut J. Kaminski verfasserin aut M. Karuza verfasserin aut C. Krieger verfasserin aut Ç. Kutlu verfasserin aut B. Lakić verfasserin aut J. M. Laurent verfasserin aut J. Lee verfasserin aut S. Lee verfasserin aut G. Luzón verfasserin aut C. Malbrunot verfasserin aut C. Margalejo verfasserin aut M. Maroudas verfasserin aut L. Miceli verfasserin aut H. Mirallas verfasserin aut L. Obis verfasserin aut A. Özbey verfasserin aut K. Özbozduman verfasserin aut M. J. Pivovaroff verfasserin aut M. Rosu verfasserin aut J. Ruz verfasserin aut E. Ruiz-Chóliz verfasserin aut S. Schmidt verfasserin aut M. Schumann verfasserin aut Y. K. Semertzidis verfasserin aut S. K. Solanki verfasserin aut L. Stewart verfasserin aut I. Tsagris verfasserin aut T. Vafeiadis verfasserin aut J. K. Vogel verfasserin aut M. Vretenar verfasserin aut S. Youn verfasserin aut K. Zioutas verfasserin aut In Nature Communications Nature Portfolio, 2016 13(2022), 1, Seite 9 (DE-627)626457688 (DE-600)2553671-0 20411723 nnns volume:13 year:2022 number:1 pages:9 https://doi.org/10.1038/s41467-022-33913-6 kostenfrei https://doaj.org/article/2d52b11f8305495ea826ef6617840ebd kostenfrei https://doi.org/10.1038/s41467-022-33913-6 kostenfrei https://doaj.org/toc/2041-1723 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_211 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_2110 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 13 2022 1 9
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allfieldsGer	10.1038/s41467-022-33913-6 doi (DE-627)DOAJ027870944 (DE-599)DOAJ2d52b11f8305495ea826ef6617840ebd DE-627 ger DE-627 rakwb eng C. M. Adair verfasserin aut Search for Dark Matter Axions with CAST-CAPP 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Haloscopes aim at detecting axions by converting them into photons using high-quality resonant cavities, where the cavity resonance should be tuned with the unknown axion mass. Here, the authors improve exclusion limits using four phase-matched resonant cavities and a fast frequency scanning technique. Science Q K. Altenmüller verfasserin aut V. Anastassopoulos verfasserin aut S. Arguedas Cuendis verfasserin aut J. Baier verfasserin aut K. Barth verfasserin aut A. Belov verfasserin aut D. Bozicevic verfasserin aut H. Bräuninger verfasserin aut G. Cantatore verfasserin aut F. Caspers verfasserin aut J. F. Castel verfasserin aut S. A. Çetin verfasserin aut W. Chung verfasserin aut H. Choi verfasserin aut J. Choi verfasserin aut T. Dafni verfasserin aut M. Davenport verfasserin aut A. Dermenev verfasserin aut K. Desch verfasserin aut B. Döbrich verfasserin aut H. Fischer verfasserin aut W. Funk verfasserin aut J. Galan verfasserin aut A. Gardikiotis verfasserin aut S. Gninenko verfasserin aut J. Golm verfasserin aut M. D. Hasinoff verfasserin aut D. H. H. Hoffmann verfasserin aut D. Díez Ibáñez verfasserin aut I. G. Irastorza verfasserin aut K. Jakovčić verfasserin aut J. Kaminski verfasserin aut M. Karuza verfasserin aut C. Krieger verfasserin aut Ç. Kutlu verfasserin aut B. Lakić verfasserin aut J. M. Laurent verfasserin aut J. Lee verfasserin aut S. Lee verfasserin aut G. Luzón verfasserin aut C. Malbrunot verfasserin aut C. Margalejo verfasserin aut M. Maroudas verfasserin aut L. Miceli verfasserin aut H. Mirallas verfasserin aut L. Obis verfasserin aut A. Özbey verfasserin aut K. Özbozduman verfasserin aut M. J. Pivovaroff verfasserin aut M. Rosu verfasserin aut J. Ruz verfasserin aut E. Ruiz-Chóliz verfasserin aut S. Schmidt verfasserin aut M. Schumann verfasserin aut Y. K. Semertzidis verfasserin aut S. K. Solanki verfasserin aut L. Stewart verfasserin aut I. Tsagris verfasserin aut T. Vafeiadis verfasserin aut J. K. Vogel verfasserin aut M. Vretenar verfasserin aut S. Youn verfasserin aut K. Zioutas verfasserin aut In Nature Communications Nature Portfolio, 2016 13(2022), 1, Seite 9 (DE-627)626457688 (DE-600)2553671-0 20411723 nnns volume:13 year:2022 number:1 pages:9 https://doi.org/10.1038/s41467-022-33913-6 kostenfrei https://doaj.org/article/2d52b11f8305495ea826ef6617840ebd kostenfrei https://doi.org/10.1038/s41467-022-33913-6 kostenfrei https://doaj.org/toc/2041-1723 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_211 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_2110 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 13 2022 1 9
allfieldsSound	10.1038/s41467-022-33913-6 doi (DE-627)DOAJ027870944 (DE-599)DOAJ2d52b11f8305495ea826ef6617840ebd DE-627 ger DE-627 rakwb eng C. M. Adair verfasserin aut Search for Dark Matter Axions with CAST-CAPP 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Haloscopes aim at detecting axions by converting them into photons using high-quality resonant cavities, where the cavity resonance should be tuned with the unknown axion mass. Here, the authors improve exclusion limits using four phase-matched resonant cavities and a fast frequency scanning technique. Science Q K. Altenmüller verfasserin aut V. Anastassopoulos verfasserin aut S. Arguedas Cuendis verfasserin aut J. Baier verfasserin aut K. Barth verfasserin aut A. Belov verfasserin aut D. Bozicevic verfasserin aut H. Bräuninger verfasserin aut G. Cantatore verfasserin aut F. Caspers verfasserin aut J. F. Castel verfasserin aut S. A. Çetin verfasserin aut W. Chung verfasserin aut H. Choi verfasserin aut J. Choi verfasserin aut T. Dafni verfasserin aut M. Davenport verfasserin aut A. Dermenev verfasserin aut K. Desch verfasserin aut B. Döbrich verfasserin aut H. Fischer verfasserin aut W. Funk verfasserin aut J. Galan verfasserin aut A. Gardikiotis verfasserin aut S. Gninenko verfasserin aut J. Golm verfasserin aut M. D. Hasinoff verfasserin aut D. H. H. Hoffmann verfasserin aut D. Díez Ibáñez verfasserin aut I. G. Irastorza verfasserin aut K. Jakovčić verfasserin aut J. Kaminski verfasserin aut M. Karuza verfasserin aut C. Krieger verfasserin aut Ç. Kutlu verfasserin aut B. Lakić verfasserin aut J. M. Laurent verfasserin aut J. Lee verfasserin aut S. Lee verfasserin aut G. Luzón verfasserin aut C. Malbrunot verfasserin aut C. Margalejo verfasserin aut M. Maroudas verfasserin aut L. Miceli verfasserin aut H. Mirallas verfasserin aut L. Obis verfasserin aut A. Özbey verfasserin aut K. Özbozduman verfasserin aut M. J. Pivovaroff verfasserin aut M. Rosu verfasserin aut J. Ruz verfasserin aut E. Ruiz-Chóliz verfasserin aut S. Schmidt verfasserin aut M. Schumann verfasserin aut Y. K. Semertzidis verfasserin aut S. K. Solanki verfasserin aut L. Stewart verfasserin aut I. Tsagris verfasserin aut T. Vafeiadis verfasserin aut J. K. Vogel verfasserin aut M. Vretenar verfasserin aut S. Youn verfasserin aut K. Zioutas verfasserin aut In Nature Communications Nature Portfolio, 2016 13(2022), 1, Seite 9 (DE-627)626457688 (DE-600)2553671-0 20411723 nnns volume:13 year:2022 number:1 pages:9 https://doi.org/10.1038/s41467-022-33913-6 kostenfrei https://doaj.org/article/2d52b11f8305495ea826ef6617840ebd kostenfrei https://doi.org/10.1038/s41467-022-33913-6 kostenfrei https://doaj.org/toc/2041-1723 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_211 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_2110 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 13 2022 1 9
language	English
source	In Nature Communications 13(2022), 1, Seite 9 volume:13 year:2022 number:1 pages:9
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authorswithroles_txt_mv	C. M. Adair @@aut@@ K. Altenmüller @@aut@@ V. Anastassopoulos @@aut@@ S. Arguedas Cuendis @@aut@@ J. Baier @@aut@@ K. Barth @@aut@@ A. Belov @@aut@@ D. Bozicevic @@aut@@ H. Bräuninger @@aut@@ G. Cantatore @@aut@@ F. Caspers @@aut@@ J. F. Castel @@aut@@ S. A. Çetin @@aut@@ W. Chung @@aut@@ H. Choi @@aut@@ J. Choi @@aut@@ T. Dafni @@aut@@ M. Davenport @@aut@@ A. Dermenev @@aut@@ K. Desch @@aut@@ B. Döbrich @@aut@@ H. Fischer @@aut@@ W. Funk @@aut@@ J. Galan @@aut@@ A. Gardikiotis @@aut@@ S. Gninenko @@aut@@ J. Golm @@aut@@ M. D. Hasinoff @@aut@@ D. H. H. Hoffmann @@aut@@ D. Díez Ibáñez @@aut@@ I. G. Irastorza @@aut@@ K. Jakovčić @@aut@@ J. Kaminski @@aut@@ M. Karuza @@aut@@ C. Krieger @@aut@@ Ç. Kutlu @@aut@@ B. Lakić @@aut@@ J. M. Laurent @@aut@@ J. Lee @@aut@@ S. Lee @@aut@@ G. Luzón @@aut@@ C. Malbrunot @@aut@@ C. Margalejo @@aut@@ M. Maroudas @@aut@@ L. Miceli @@aut@@ H. Mirallas @@aut@@ L. Obis @@aut@@ A. Özbey @@aut@@ K. Özbozduman @@aut@@ M. J. Pivovaroff @@aut@@ M. Rosu @@aut@@ J. Ruz @@aut@@ E. Ruiz-Chóliz @@aut@@ S. Schmidt @@aut@@ M. Schumann @@aut@@ Y. K. Semertzidis @@aut@@ S. K. Solanki @@aut@@ L. Stewart @@aut@@ I. Tsagris @@aut@@ T. Vafeiadis @@aut@@ J. K. Vogel @@aut@@ M. Vretenar @@aut@@ S. Youn @@aut@@ K. Zioutas @@aut@@
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Adair</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Search for Dark Matter Axions with CAST-CAPP</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2022</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Haloscopes aim at detecting axions by converting them into photons using high-quality resonant cavities, where the cavity resonance should be tuned with the unknown axion mass. 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author	C. M. Adair
spellingShingle	C. M. Adair misc Science misc Q Search for Dark Matter Axions with CAST-CAPP
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topic_title	Search for Dark Matter Axions with CAST-CAPP
topic	misc Science misc Q
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format_facet	Elektronische Aufsätze Aufsätze Elektronische Ressource
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title	Search for Dark Matter Axions with CAST-CAPP
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title_full	Search for Dark Matter Axions with CAST-CAPP
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journal	Nature Communications
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author_browse	C. M. Adair K. Altenmüller V. Anastassopoulos S. Arguedas Cuendis J. Baier K. Barth A. Belov D. Bozicevic H. Bräuninger G. Cantatore F. Caspers J. F. Castel S. A. Çetin W. Chung H. Choi J. Choi T. Dafni M. Davenport A. Dermenev K. Desch B. Döbrich H. Fischer W. Funk J. Galan A. Gardikiotis S. Gninenko J. Golm M. D. Hasinoff D. H. H. Hoffmann D. Díez Ibáñez I. G. Irastorza K. Jakovčić J. Kaminski M. Karuza C. Krieger Ç. Kutlu B. Lakić J. M. Laurent J. Lee S. Lee G. Luzón C. Malbrunot C. Margalejo M. Maroudas L. Miceli H. Mirallas L. Obis A. Özbey K. Özbozduman M. J. Pivovaroff M. Rosu J. Ruz E. Ruiz-Chóliz S. Schmidt M. Schumann Y. K. Semertzidis S. K. Solanki L. Stewart I. Tsagris T. Vafeiadis J. K. Vogel M. Vretenar S. Youn K. Zioutas
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author-letter	C. M. Adair
doi_str_mv	10.1038/s41467-022-33913-6
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title_sort	search for dark matter axions with cast-capp
title_auth	Search for Dark Matter Axions with CAST-CAPP
abstract	Haloscopes aim at detecting axions by converting them into photons using high-quality resonant cavities, where the cavity resonance should be tuned with the unknown axion mass. Here, the authors improve exclusion limits using four phase-matched resonant cavities and a fast frequency scanning technique.
abstractGer	Haloscopes aim at detecting axions by converting them into photons using high-quality resonant cavities, where the cavity resonance should be tuned with the unknown axion mass. Here, the authors improve exclusion limits using four phase-matched resonant cavities and a fast frequency scanning technique.
abstract_unstemmed	Haloscopes aim at detecting axions by converting them into photons using high-quality resonant cavities, where the cavity resonance should be tuned with the unknown axion mass. Here, the authors improve exclusion limits using four phase-matched resonant cavities and a fast frequency scanning technique.
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title_short	Search for Dark Matter Axions with CAST-CAPP
url	https://doi.org/10.1038/s41467-022-33913-6 https://doaj.org/article/2d52b11f8305495ea826ef6617840ebd https://doaj.org/toc/2041-1723
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author2	K. Altenmüller V. Anastassopoulos S. Arguedas Cuendis J. Baier K. Barth A. Belov D. Bozicevic H. Bräuninger G. Cantatore F. Caspers J. F. Castel S. A. Çetin W. Chung H. Choi J. Choi T. Dafni M. Davenport A. Dermenev K. Desch B. Döbrich H. Fischer W. Funk J. Galan A. Gardikiotis S. Gninenko J. Golm M. D. Hasinoff D. H. H. Hoffmann D. Díez Ibáñez I. G. Irastorza K. Jakovčić J. Kaminski M. Karuza C. Krieger Ç. Kutlu B. Lakić J. M. Laurent J. Lee S. Lee G. Luzón C. Malbrunot C. Margalejo M. Maroudas L. Miceli H. Mirallas L. Obis A. Özbey K. Özbozduman M. J. Pivovaroff M. Rosu J. Ruz E. Ruiz-Chóliz S. Schmidt M. Schumann Y. K. Semertzidis S. K. Solanki L. Stewart I. Tsagris T. Vafeiadis J. K. Vogel M. Vretenar S. Youn K. Zioutas
author2Str	K. Altenmüller V. Anastassopoulos S. Arguedas Cuendis J. Baier K. Barth A. Belov D. Bozicevic H. Bräuninger G. Cantatore F. Caspers J. F. Castel S. A. Çetin W. Chung H. Choi J. Choi T. Dafni M. Davenport A. Dermenev K. Desch B. Döbrich H. Fischer W. Funk J. Galan A. Gardikiotis S. Gninenko J. Golm M. D. Hasinoff D. H. H. Hoffmann D. Díez Ibáñez I. G. Irastorza K. Jakovčić J. Kaminski M. Karuza C. Krieger Ç. Kutlu B. Lakić J. M. Laurent J. Lee S. Lee G. Luzón C. Malbrunot C. Margalejo M. Maroudas L. Miceli H. Mirallas L. Obis A. Özbey K. Özbozduman M. J. Pivovaroff M. Rosu J. Ruz E. Ruiz-Chóliz S. Schmidt M. Schumann Y. K. Semertzidis S. K. Solanki L. Stewart I. Tsagris T. Vafeiadis J. K. Vogel M. Vretenar S. Youn K. Zioutas
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doi_str	10.1038/s41467-022-33913-6
up_date	2024-07-03T14:29:12.830Z
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