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000890009 005__ 20210127115424.0
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000890009 037__ $$aFZJ-2021-00603
000890009 1001_ $$0P:(DE-Juel1)171602$$aPenek, Ömer$$b0$$eCorresponding author$$ufzj
000890009 1112_ $$aThe XXIX International Conference on Neutrino Physics and Astrophysics$$cChicago$$d2020-06-22 - 2020-07-02$$wUSA
000890009 245__ $$aBorexino Sensitivity Studies towards Detection of Solar Neutrinos from the CNO Fusion Cycle
000890009 260__ $$c2020
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000890009 502__ $$cRWTH Aachen
000890009 520__ $$aThe Borexino detector, located at the Laboratori Nazionali del Gran Sasso in Italy, is a liquid scintillator detector with a primary goal to measure solar neutrinos. The *pp* fusion chain has been measured in Borexino with an outstanding precision through the detection of *pp*, *pep*, $^{7}$Be, and $^{8}$B neutrinos. It is well motivated by standard solar models that around 1 per cent of the solar energy is fueled by the so-called Carbon-Nitrogen-Oxygen (CNO) cycle. A direct measurement of the CNO cycle is difficult due to the high spectral correlation with the background isotope $^{210}$Bi and *pep* neutrinos. The sensitivity to CNO neutrinos was evaluated through a likelihood-ratio test, based on thousands of pseudo-experiments analyzed with a counting analysis as well as spectral fit. This poster presents the resulting discovery potential of Borexino towards the CNO cycle in the Sun.
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000890009 7001_ $$0P:(DE-HGF)0$$aet al. Borexino Collaboration$$b1
000890009 773__ $$a10.5281/ZENODO.4401808
000890009 8564_ $$uhttps://juser.fz-juelich.de/record/890009/files/Penek_Neutrino_2020_Poster_Final.pdf$$yOpenAccess
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000890009 9141_ $$y2020
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000890009 9201_ $$0I:(DE-Juel1)IKP-2-20111104$$kIKP-2$$lExperimentelle Hadrondynamik$$x0
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