Virtual depth by active background suppression: revisiting the cosmic muon induced background of Gerda Phase II
Virtual depth by active background suppression: revisiting the cosmic muon induced background of Gerda Phase II
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DOI:
10.1140/epjc/s10052-018-6079-3
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发表时间:
2018-02
期刊:
影响因子:
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通讯作者:
C. Wiesinger;L. Pandola;S. Schönert
中科院分区:
文献类型:
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作者:
C. Wiesinger;L. Pandola;S. Schönert
In-situ production of radioisotopes by cosmic muon interactions may generate a non-negligible background for deep underground rare event searches. Previous Monte Carlo studies for theGerdaexperiment atLngsidentified the delayed decays ofGe and its metastable stateGe as dominant cosmogenic background in the search for neutrinoless double beta decay ofGe. This might limit the sensitivity of next generation experiments aiming for increasedGe mass at background-free conditions and thereby define a minimum depth requirement. A re-evaluation of theGe background for theGerdaexperiment has been carried out by a set of Monte Carlo simulations. The obtainedGe production rate is () nuclei/(kgyear). After application of state-of-the-art active background suppression techniques and simple delayed coincidence cuts this corresponds to a background contribution ofcts/(keVkgyear). The suppression achieved by this strategy equals an effective muon flux reduction of more than one order of magnitude. This virtual depth increase opens the way for next generation rare event searches.