Experimental challenge to nuclear physics problems in the {nu}p-process
- Center for Nuclear Study, University of Tokyo (CNS), Wako Branch, 2-1 Hirosawa, Wako, Saitama, 351-0198 (Japan)
Astrophysical stellar reactions at extremely high temperatures involve a variety of problems both in nuclear reactions and nuclear structures. Specifically, the problems in the {nu}pprocess were discussed in this talk based on our recent experimental results with low-energy RI beams and a simulation study. The {nu}p-process is one of the key processes for investigating the mechanism of type II supernovae, and the process could be possibly responsible for 'the excess production' of p-nuclei around mass 90-100. Alpha cluster resonances have been discovered experimentally to play a crucial role for the stellar ({alpha}, p) reactions just above the alpha threshold. Neutron induced reactions in the proton-rich nuclear regions in the {nu}p-process are also suggested to play an important role, which involve nuclear structures of high level density at high excitation energies, probably giant resonances. The discussion also covered the p-nuclei production through the {nu}p-process at around mass 100.
- OSTI ID:
- 22075743
- Journal Information:
- AIP Conference Proceedings, Vol. 1484, Issue 1; Conference: Conference on origin of matter and evolution of galaxies 2011, Wako (Japan), 14-17 Nov 2011; Other Information: (c) 2012 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
- Country of Publication:
- United States
- Language:
- English
Similar Records
TYPE Ia SUPERNOVAE AS SITES OF THE p-PROCESS: TWO-DIMENSIONAL MODELS COUPLED TO NUCLEOSYNTHESIS
Stellar Nuclear Structure
Related Subjects
79 ASTROPHYSICS
COSMOLOGY AND ASTRONOMY
ALPHA PARTICLES
ASTROPHYSICS
CLUSTER MODEL
ENERGY LEVELS
ENERGY-LEVEL DENSITY
EXCITATION
GIANT RESONANCE
NEUTRINO-PROTON INTERACTIONS
NEUTRONS
NUCLEAR REACTIONS
NUCLEAR STRUCTURE
NUCLEOSYNTHESIS
PROTONS
RADIOACTIVE ION BEAMS
STAR EVOLUTION
SUPERNOVAE