Published November 12, 2012
| Version v1
Journal article
Proton-rich nucleosynthesis and nuclear physics
Creators
- 1. Dept. of Physics, NCSU, Raleigh, NC 27695 (United States)
- 2. Dept. of Physics, University of Basel, 4056 Basel (Switzerland)
Description
Although the detailed conditions for explosive nucleosynthesis are derived from astrophysical modeling, nuclear physics determines fundamental patterns in abundance yields, not only for equilibrium processes. Focussing on the νp- and the γ-process, general nucleosynthesis features within the range of astrophysical models, but (mostly) independent of details in the modelling, are presented. Remaining uncertainties due to uncertain Q-values and reaction rates are discussed.
Additional details
Identifiers
- DOI
- 10.1063/1.4763376;
- arXiv
- arXiv:1304.0929v1;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 1484
- Journal Issue
- 1
- Journal Page Range
- p. 73-78
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- Conference on origin of matter and evolution of galaxies 2011
- Dates
- 14-17 Nov 2011
- Place
- Wako (Japan)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 44034881
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ASTROPHYSICS; COMPUTERIZED SIMULATION; EQUILIBRIUM; NEUTRINO-PROTON INTERACTIONS; NUCLEAR REACTION KINETICS; NUCLEAR REACTION YIELD; NUCLEOSYNTHESIS; PROTONS; Q-VALUE
- Descriptors DEC
- BARYONS; ELEMENTARY PARTICLES; ENERGY; FERMIONS; HADRONS; INTERACTIONS; KINETICS; LEPTON-BARYON INTERACTIONS; LEPTON-HADRON INTERACTIONS; LEPTON-NUCLEON INTERACTIONS; NEUTRINO-NUCLEON INTERACTIONS; NUCLEONS; PARTICLE INTERACTIONS; PHYSICS; REACTION KINETICS; SIMULATION; SYNTHESIS; YIELDS
Optional Information
- Notes
- (c) 2012 American Institute of Physics