التفاصيل البيبلوغرافية
| العنوان: |
Flux Modulations seen by the Muon Veto of the GERDA Experiment |
| المؤلفون: |
Agostini, M., Allardt, M., Bakalyarov, A., Balata, M., Barabanov, I., Barros, N., Baudis, L., Bauer, C., Becerici-Schmidt, N., Bellotti, E., Belogurov, S., Belyaev, S., Benato, G., Bettini, A., Bezrukov, L., Bode, T., Borowicz, D., Brudanin, V., Brugnera, R., Caldwell, A., Cattadori, C., Chernogorov, A., D'Andrea, V., Demidova, E., di Vacri, A., Domula, A., Doroshkevich, E., Egorov, V., Falkenstein, R., Fedorova, O., Freund, K., Frodyma, N., Gangapshev, A., Garfagnini, A., Grabmayr, P., Gurentsov, V., Gusev, K., Hegai, A., Heisel, M., Hemmer, S., Hofmann, W., Hult, M., Inzhechik, L., Ioannucci, L., Csáthy, J., Jochum, J., Junker, M., Kazalov, V., Kihm, T., Kirpichnikov, I., Kirsch, A., Klimenko, A., Knapp, M., Knöpfle, K., Kochetov, O., Kornoukhov, V., Kuzminov, V., Laubenstein, M., Lazzaro, A., Lebedev, V., Lehnert, B., Liao, H., Lindner, M., Lippi, I., Lubashevskiy, A., Lubsandorzhiev, B., Lutter, G., Macolino, C., Majorovits, B., Maneschg, W., Medinaceli, E., Misiaszek, M., Moseev, P., Nemchenok, I., Palioselitis, D., Panas, K., Pandola, L., Pelczar, K., Pullia, A., Riboldi, S., Ritter, F., Rumyantseva, N., Sada, C., Salathe, M., Schmitt, C., Schneider, B., Schönert, S., Schreiner, J., Schütz, A., Schulz, O., Schwingenheuer, B., Selivanenko, O., Shevchik, E., Shirchenko, M., Simgen, H., Smolnikov, A., Stanco, L., Stepaniuk, M., Strecker, H., Vanhoefer, L., Vasenko, A., Veresnikova, A., vonSturm, K., Wagner, V., Walter, M., Wegmann, A., Wester, T., Wilsenach, H., Wojcik, M., Yanovich, E., Zhitnikov, I., Zhukov, S., Zinatulina, D., Zuber, K., Zuzel, G. |
| المصدر: |
Astroparticle Physics |
| سنة النشر: |
2016 |
| المجموعة: |
Max Planck Society: MPG.PuRe |
| مصطلحات موضوعية: |
GERDA - Abteilung Hofmann |
| الوصف: |
The GERDA experiment at LNGS of INFN is equipped with an active muon veto. The main part of the system is a water Cherenkov veto with 66~PMTs in the water tank surrounding the GERDA cryostat. The muon flux recorded by this veto shows a seasonal modulation. Two effects have been identified which are caused by secondary muons from the CNGS neutrino beam (2.2 %) and a temperature modulation of the atmosphere (1.4 %). A mean cosmic muon rate of $I^0_{\mu} = (3.477 \pm 0.002_{\textrm{stat}} \pm 0.067_{\textrm{sys}}) \times 10^{-4}$/(s$\cdot$m$^2$) was found in good agreement with other experiments at LNGS at a depth of 3500~meter water equivalent. |
| نوع الوثيقة: |
article in journal/newspaper |
| وصف الملف: |
application/pdf |
| اللغة: |
unknown |
| العلاقة: |
info:eu-repo/semantics/altIdentifier/arxiv/1601.06007; http://hdl.handle.net/11858/00-001M-0000-002B-B3BF-7Test; http://hdl.handle.net/11858/00-001M-0000-002B-B3C1-0Test |
| الإتاحة: |
https://doi.org/10.1016/j.astropartphys.2016.08.002Test
http://hdl.handle.net/11858/00-001M-0000-002B-B3BF-7Test
http://hdl.handle.net/11858/00-001M-0000-002B-B3C1-0Test |
| حقوق: |
info:eu-repo/semantics/openAccess ; http://arxiv.org/help/licenseTest |
| رقم الانضمام: |
edsbas.F33A2E89 |
| قاعدة البيانات: |
BASE |
