Gast ::
| Hauptseite > Publikationsdatenbank > Borexino Sensitivity Studies towards Detection of Solar Neutrinos from the CNO Fusion Cycle > print |
| Hauptseite > Publikationsdatenbank > Borexino Sensitivity Studies towards Detection of Solar Neutrinos from the CNO Fusion Cycle > print |
| 001 | 890009 | ||
| 005 | 20210127115424.0 | ||
| 024 | 7 | _ | |a 10.5281/ZENODO.4401808 |2 doi |
| 024 | 7 | _ | |a 2128/27066 |2 Handle |
| 037 | _ | _ | |a FZJ-2021-00603 |
| 100 | 1 | _ | |a Penek, Ömer |0 P:(DE-Juel1)171602 |b 0 |e Corresponding author |u fzj |
| 111 | 2 | _ | |a The XXIX International Conference on Neutrino Physics and Astrophysics |c Chicago |d 2020-06-22 - 2020-07-02 |w USA |
| 245 | _ | _ | |a Borexino Sensitivity Studies towards Detection of Solar Neutrinos from the CNO Fusion Cycle |
| 260 | _ | _ | |c 2020 |
| 336 | 7 | _ | |a Conference Paper |0 33 |2 EndNote |
| 336 | 7 | _ | |a INPROCEEDINGS |2 BibTeX |
| 336 | 7 | _ | |a conferenceObject |2 DRIVER |
| 336 | 7 | _ | |a CONFERENCE_POSTER |2 ORCID |
| 336 | 7 | _ | |a Output Types/Conference Poster |2 DataCite |
| 336 | 7 | _ | |a Poster |b poster |m poster |0 PUB:(DE-HGF)24 |s 1611670200_21288 |2 PUB:(DE-HGF) |x Other |
| 502 | _ | _ | |c RWTH Aachen |
| 520 | _ | _ | |a The 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. |
| 536 | _ | _ | |a 612 - Cosmic Matter in the Laboratory (POF3-612) |0 G:(DE-HGF)POF3-612 |c POF3-612 |f POF III |x 0 |
| 588 | _ | _ | |a Dataset connected to DataCite |
| 700 | 1 | _ | |a et al. Borexino Collaboration |0 P:(DE-HGF)0 |b 1 |
| 773 | _ | _ | |a 10.5281/ZENODO.4401808 |
| 856 | 4 | _ | |u https://juser.fz-juelich.de/record/890009/files/Penek_Neutrino_2020_Poster_Final.pdf |y OpenAccess |
| 909 | C | O | |o oai:juser.fz-juelich.de:890009 |p openaire |p open_access |p VDB |p driver |
| 910 | 1 | _ | |a Forschungszentrum Jülich |0 I:(DE-588b)5008462-8 |k FZJ |b 0 |6 P:(DE-Juel1)171602 |
| 913 | 1 | _ | |a DE-HGF |b Forschungsbereich Materie |l Materie und Universum |1 G:(DE-HGF)POF3-610 |0 G:(DE-HGF)POF3-612 |3 G:(DE-HGF)POF3 |2 G:(DE-HGF)POF3-600 |4 G:(DE-HGF)POF |v Cosmic Matter in the Laboratory |x 0 |
| 914 | 1 | _ | |y 2020 |
| 915 | _ | _ | |a OpenAccess |0 StatID:(DE-HGF)0510 |2 StatID |
| 920 | 1 | _ | |0 I:(DE-Juel1)IKP-2-20111104 |k IKP-2 |l Experimentelle Hadrondynamik |x 0 |
| 980 | _ | _ | |a poster |
| 980 | _ | _ | |a VDB |
| 980 | _ | _ | |a UNRESTRICTED |
| 980 | _ | _ | |a I:(DE-Juel1)IKP-2-20111104 |
| 980 | 1 | _ | |a FullTexts |
| Library | Collection | CLSMajor | CLSMinor | Language | Author |
|---|