The study of solar neutrinos and of non-standard neutrino interactions with Borexino
Clicks: 250
ID: 272897
2020
Article Quality & Performance Metrics
Overall Quality
Not rated
Combines reader engagement with the AI quality analysis. This
article has not been analysed, so there is no overall score —
reader engagement is measured and shown alongside.
Reader Engagement
Emerging Content
30.0
/100
250 views
40 readers
AI Quality Assessment
Not analyzed
Readership in this journal
EmergingRanked #284 of 935 articles by views in journal of physics: conference series
Most read
Least read
Bar heights use a square-root scale. Only the 120 most-read articles are drawn; the journal has 935 in total.
Mint this article as an NFT
Not yet mintedCreate a permanent, verifiable on-chain record of this article on the Scimatic Network. The NFT is held in your Journament account, and you can withdraw it to your own wallet at any time.
5
SUSD
one-off · no wallet required
Abstract
The Borexino liquid scintillator neutrino observatory has a unique capability to perform high-precision solar neutrino observations thanks to its exceptional radiopurity and good energy resolution (5% at 1 MeV). A comprehensive study of the pp-chain neutrinos was presented that includes the direct measurements of 7Be, pp and pep neutrino fluxes with the highest precision ever achieved (down to 2.8% in the 7Be component), the 8B with the lowest energy threshold, the best limit on CNO neutrinos and the first Borexino limit on hep neutrinos. These results are important to validate the MSW-LMA oscillation paradigm across the full solar energy range and to exclude possible Non-Standard neutrino Interactions (NSIs). In particular the effects of neutrino-flavor-diagonal Neutral-Current (NC) interactions that modify the vee and vτe couplings while preserving their chiral and flavor structures, have been investigated. At detection, the shape of the electron-recoil spectrum is affected by changes in the vee and vτe couplings, quantified by the parameters and . New bounds to all four parameters were obtained, quite stringent compared to the global ones. In particular, the best constraint to-date on was achieved. A comprehensive summary of all the recent results on solar neutrinos from Borexino is reported in the present paper.
| Reference Key |
zuzel2020journalthe
Use this key to autocite in the manuscript while using
SciMatic Manuscript Manager or Thesis Manager
|
|---|---|
| Authors | Sandra Zavatarelli,Matteo Agostini,K. Altenmüller,S. Appel,V. Atroshchenko,Z. Bagdasarian,D. Basilico,G. Bellini,J. Benziger,D. Bick,G. Bonfini,D. Bravo,B. Caccianiga,F. Calaprice,A. Caminata,L. Cappelli,P. Cavalcante,F. Cavanna,A. Chepurnov,K. Choi,D. D’Angelo,S. Davini,A. Derbin,A. Di Giacinto,V. Di Marcello,X.F. Ding,A. Di Lüdovico,L. Di Noto,I. Drachnev,A. Formozov,Davide Franco,F. Gabriele,C. Galbiati,M. Gschwender,C. Ghiano,M. Giammarchi,A. Goretti,M. Gromov,D. Güffanti,C. Hagner,E. Hungerford,Aldo Ianni,Andrea Ianni,A. Jany,D. Jeschke,S. Kumaran,V. Kobychev,G. Korga,T. Lachenmaier,M. Laubenstein,E. Litvinovich,P. Lombardi,Irina Lomskaya,L. Ludhova,G. Lukyanchenko,I. Machulin,G. Manuzio,S. Marcocci,J. Maricic,J. Martyn,E. Meroni,M. Meyer,L. Miramonti,M. Misiaszek,V. Muratova,B. Neumair,M. Nieslony,L. Oberauer,V. Orekhov,F. Ortica,M. Pallavicini,L. Papp,O. Penek,L. Pietrofaccia,N. Pilipenko,A. Pocar,G. Raikov,M.T. Ranalli,G. Ranucci,A. Razeto,A. Re,M. Redchuk,A. Romani,N. Rossi,S. Rottenanger,S. Schönert,D. Semenov,M. Skorokhvatov,O. Smirnov,Albert Sotnikov,Y. Suvorov,R. Tartaglia,G. Testera,J. Thurn,E. Unzhakov,A. Vishneva,R.B. Vogelaar,F. von Feilitzsch,M. Wojcik,M. Wurm,O. Zaimidoroga,K. Zuber,G. Zuzel;Sandra Zavatarelli;Matteo Agostini;K. Altenmüller;S. Appel;V. Atroshchenko;Z. Bagdasarian;D. Basilico;G. Bellini;J. Benziger;D. Bick;G. Bonfini;D. Bravo;B. Caccianiga;F. Calaprice;A. Caminata;L. Cappelli;P. Cavalcante;F. Cavanna;A. Chepurnov;K. Choi;D. D’Angelo;S. Davini;A. Derbin;A. Di Giacinto;V. Di Marcello;X.F. Ding;A. Di Lüdovico;L. Di Noto;I. Drachnev;A. Formozov;Davide Franco;F. Gabriele;C. Galbiati;M. Gschwender;C. Ghiano;M. Giammarchi;A. Goretti;M. Gromov;D. Güffanti;C. Hagner;E. Hungerford;Aldo Ianni;Andrea Ianni;A. Jany;D. Jeschke;S. Kumaran;V. Kobychev;G. Korga;T. Lachenmaier;M. Laubenstein;E. Litvinovich;P. Lombardi;Irina Lomskaya;L. Ludhova;G. Lukyanchenko;I. Machulin;G. Manuzio;S. Marcocci;J. Maricic;J. Martyn;E. Meroni;M. Meyer;L. Miramonti;M. Misiaszek;V. Muratova;B. Neumair;M. Nieslony;L. Oberauer;V. Orekhov;F. Ortica;M. Pallavicini;L. Papp;O. Penek;L. Pietrofaccia;N. Pilipenko;A. Pocar;G. Raikov;M.T. Ranalli;G. Ranucci;A. Razeto;A. Re;M. Redchuk;A. Romani;N. Rossi;S. Rottenanger;S. Schönert;D. Semenov;M. Skorokhvatov;O. Smirnov;Albert Sotnikov;Y. Suvorov;R. Tartaglia;G. Testera;J. Thurn;E. Unzhakov;A. Vishneva;R.B. Vogelaar;F. von Feilitzsch;M. Wojcik;M. Wurm;O. Zaimidoroga;K. Zuber;G. Zuzel; |
| Journal | journal of physics: conference series |
| Year | 2020 |
| DOI |
10.1088/1742-6596/1468/1/012192
|
| URL | |
| Keywords |
Citations
No citations found. To add a citation, contact the admin at info@scimatic.org
Comments
No comments yet. Be the first to comment on this article.