Three-Body Treatment of the pep Reaction in the Sun

Three-Body Treatment of the pep Reaction in the Sun

The experimental result of the neutrino flux produced by the p  +  p  +  e → d  +  ν e reaction ( pep ) in the Sun at 1 AU was announced for the first time in 2012 by the Borexino collaboration. We use the three-body model for the proton–proton–electron system in the initial state for the calculatio...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Few-body systems 2014-08, Vol.55 (8-10), p.783-786, Article 783
Hauptverfasser: Irgaziev, B. F., Belyaev, V. B.
Format: Artikel
Sprache:eng
Schlagworte:
Atomic
Chemical reactions
Flux
Hadrons
Heavy Ions
Mathematical models
Molecular
Neutrinos
Nuclear Physics
Optical and Plasma Physics
Particle and Nuclear Physics
Physics
Physics and Astronomy
Sun
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
Beschreibung
Zusammenfassung:The experimental result of the neutrino flux produced by the p  +  p  +  e → d  +  ν e reaction ( pep ) in the Sun at 1 AU was announced for the first time in 2012 by the Borexino collaboration. We use the three-body model for the proton–proton–electron system in the initial state for the calculation of the rate of the pep reaction with various types of nucleon–nucleon potentials.
ISSN:0177-7963
1432-5411
DOI:10.1007/s00601-013-0748-4