Coulomb dissociation, a tool for nuclear astrophysics
arXiv:0705.3307 · doi:10.1088/0954-3899/35/1/014003 10.1088/0954-3899/35/1/014028
Abstract
A short status report on Coulomb dissociation, an indirect method for nuclear astrophysics is given. An analytically solvable approach to study electromagnetic excitation in ^{11}Be, the archetype of a halo nucleus, is proposed.
6 pages, contribution to Nuclear Physics in Astrophysics III, 26-31 March 2007, Dresden, Germany, typos corrected, accepted for publication in J.Phys. G
References in corpus (13)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Updated Big Bang Nucleosynthesis confronted to WMAP observations and to the Abundance of Light Elements
- What do we (not) know theoretically about solar neutrino fluxes?
- Surprising Sun
- A Measurement of the Coulomb Dissociation of 8B at 254 MeV/nucleon and the 8B Solar Neutrino Flux
- Precise measurement of the ^7Be(p,gamma)^8B S-factor
- New measurement and analysis of the 7Be(p,gamma)8B cross section
- 7Be(p,gamma)8B astrophysical S-factor from precision cross section measurements
- Coulomb dissociation of 8B and the low-energy cross section of the 7Be(p,gamma)8B solar fusion reaction
- Electromagnetic Dissociation of 8B and the Rate of the 7Be(p,gamma)8B Reaction in the Sun
- Low energy measurement of the 7Be(p,gamma)8B cross section
- A New Measurement of the Proton Capture Rate on 7Be and the S17(0) Factor
- Low-energy cross section of the 7Be(p,g)8B solar fusion reaction from Coulomb dissociation of 8B