التفاصيل البيبلوغرافية
العنوان:
Long-term monitoring of the ANTARES optical module efficiencies using $$^{40}\mathrm{{K}}$$ 40 K decays in sea water
المؤلفون:
A. Albert , M. André , M. Anghinolfi , G. Anton , M. Ardid , J.-J. Aubert , J. Aublin , T. Avgitas , B. Baret , J. Barrios-Martí , S. Basa , B. Belhorma , V. Bertin , S. Biagi , R. Bormuth , J. Boumaaza , S. Bourret , M. C. Bouwhuis , H. Brânzaş , R. Bruijn , J. Brunner , J. Busto , A. Capone , L. Caramete , J. Carr , S. Celli , M. Chabab , R. Cherkaoui El Moursli , T. Chiarusi , M. Circella , J. A. B. Coelho , A. Coleiro , M. Colomer , R. Coniglione , H. Costantini , P. Coyle , A. Creusot , A. F. Díaz , A. Deschamps , C. Distefano , I. Di Palma , A. Domi , C. Donzaud , D. Dornic , D. Drouhin , T. Eberl , I. El Bojaddaini , N. El Khayati , D. Elsässer , A. Enzenhöfer , A. Ettahiri , F. Fassi , I. Felis , G. Ferrara , L. A. Fusco , P. Gay , H. Glotin , T. Grégoire , R. Gracia Ruiz , K. Graf , S. Hallmann , H. van Haren , A. J. Heijboer , Y. Hello , J. J. Hernández-Rey , J. Hößl , J. Hofestädt , G. Illuminati , C. W. James , M. de Jong , M. Jongen , M. Kadler , O. Kalekin , U. Katz , A. Kouchner , M. Kreter , I. Kreykenbohm , V. Kulikovskiy , C. Lachaud , R. Lahmann , D. Lefèvre , E. Leonora , G. Levi , M. Lotze , S. Loucatos , M. Marcelin , A. Margiotta , A. Marinelli , J. A. Martínez-Mora , R. Mele , K. Melis , P. Migliozzi , A. Moussa , S. Navas , E. Nezri , A. Nuñez , M. Organokov , G. E. Păvălaş , C. Pellegrino , P. Piattelli , V. Popa , T. Pradier , L. Quinn , C. Racca , N. Randazzo , G. Riccobene , A. Sánchez-Losa , M. Saldaña , I. Salvadori , D. F. E. Samtleben , M. Sanguineti , P. Sapienza , F. Schüssler , M. Spurio , Th. Stolarczyk , M. Taiuti , Y. Tayalati , A. Trovato , B. Vallage , V. Van Elewyck , F. Versari , D. Vivolo , J. Wilms , D. Zaborov , J. D. Zornoza , J. Zúñiga
المصدر:
The European Physical Journal C . 78
بيانات النشر:
Springer Science and Business Media LLC, 2018.
سنة النشر:
2018
مصطلحات موضوعية:
Physics , Physics and Astronomy (miscellaneous) , 010308 nuclear & particles physics , Astrophysics::High Energy Astrophysical Phenomena , Astrophysics::Instrumentation and Methods for Astrophysics , Time evolution , 01 natural sciences , Nuclear physics , Optical Module , 13. Climate action , Long term monitoring , 0103 physical sciences , Calibration , Seawater , 14. Life underwater , Neutrino , 010303 astronomy & astrophysics , Engineering (miscellaneous) , Cherenkov radiation , Radioactive decay
الوصف:
Cherenkov light induced by radioactive decay products is one of the major sources of background light for deep-sea neutrino telescopes such as ANTARES. These decays are at the same time a powerful calibration source. Using data collected by the ANTARES neutrino telescope from mid 2008 to 2017, the time evolution of the photon detection efficiency of optical modules is studied. A modest loss of only 20% in 9 years is observed. The relative time calibration between adjacent modules is derived as well.
تدمد:
1434-6052
الوصول الحر:
https://explore.openaire.eu/search/publication?articleId=doi_________::5f0ea697fd8bbc8864007910451156b1Test https://doi.org/10.1140/epjc/s10052-018-6132-2Test
حقوق:
OPEN
رقم الانضمام:
edsair.doi...........5f0ea697fd8bbc8864007910451156b1
قاعدة البيانات:
OpenAIRE
