Published August 2014
| Version v1
Journal article
Three-Body Treatment of the pep Reaction in the Sun
Creators
- 1. Institute of Applied Physics of National University of Uzbekistan, Tashkent (Uzbekistan)
- 2. BLTP, Joint Institute of Nuclear Research, Dubna (Russian Federation)
Description
The experimental result of the neutrino flux produced by the p + p + e → d + νe 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. (author)
Additional details
Identifiers
Publishing Information
- Journal Title
- Few-Body Systems
- Journal Volume
- 55
- Journal Issue
- 8-10
- Journal Page Range
- p. 783-786
- ISSN
- 0177-7963
- CODEN
- FBSYEQ
Conference
- Title
- 22. European Conference on Few-Body Problems in Physics
- Dates
- 9-13 Sep 2013
- Place
- Krakow (Poland)
INIS
- Country of Publication
- Austria
- Country of Input or Organization
- Austria
- INIS RN
- 46017653
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ELECTRON-PROTON INTERACTIONS; ELECTRONS; NEUTRINOS; NUCLEON-NUCLEON POTENTIAL; PROTON-PROTON INTERACTIONS; PROTONS; SUN; THREE-BODY PROBLEM
- Descriptors DEC
- BARYON-BARYON INTERACTIONS; BARYONS; ELECTRON-NUCLEON INTERACTIONS; ELEMENTARY PARTICLES; FERMIONS; HADRON-HADRON INTERACTIONS; HADRONS; INTERACTIONS; LEPTON-BARYON INTERACTIONS; LEPTON-HADRON INTERACTIONS; LEPTON-NUCLEON INTERACTIONS; LEPTONS; MAIN SEQUENCE STARS; MANY-BODY PROBLEM; MASSLESS PARTICLES; NUCLEON-NUCLEON INTERACTIONS; NUCLEONS; PARTICLE INTERACTIONS; POTENTIALS; PROTON-NUCLEON INTERACTIONS; STARS