The R-process: The Astrophysical Origin of the Heavy Elements and Related Rare Isotope Accelerator Physics : Proceedings of the First Argonne/MSU/JINA/INT RIA Workshop : National Institute for Nuclear Theory, University of Washington, USA, 8-10 January 2004

Предна корица
World Scientific, 2004 - 260 страници
The r-process is a major mechanism for producing elements heavier than Fe. In this book, a summary of recent developments in theoretical, experimental and observational studies of the r-process are presented in 25 contributions. The collected papers are up to date, comprehensive and yet concise. The topics covered include experiments on nuclei far from stability, nuclear theory input for the r-process, observational and theoretical studies on abundances of heavy nuclei, and astrophysical models of the r-process. The proceedings have been selected for coverage in: OCo Index to Scientific & Technical Proceedings- (ISTP- / ISI Proceedings) OCo Index to Scientific & Technical Proceedings (ISTP CDROM version / ISI Proceedings) OCo CC Proceedings OCo Engineering & Physical Sciences. Contents: The r -Process in Supernovae (F-K Thielemann et al.); Weak Strength for Astrophysics (S M Austin & R Zegers); Neutron Captures and the r -Process (T Tauscher); Equation of State and Neutrino Opacity of Dense Steller Matter (S Reddy); An Overview of Observations of Neutron-Capture Elements in Metal-Poor Stars (J A Johnson); Nuclear Reaction Rates and the Production of Light p -Process Isotopes in Fast Expansions of Proton-Rich Matter (G C Jordan et al.); General Relativity and Neutrino-Driven Supernova Winds (C Y Cardall); Ejecta from Parametrized Prompt Explosion (S Wanajo et al.); Neutrino Transport in Core Collapse Supernovae (M LiebendArfer); and other papers. Readership: Graduate students and researchers in nuclear physics, astrophysics and accelerator physics."
 

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Съдържание

The rProcess in Supernovae
1
Precise Mass Measurements of Nuclides Approaching the rProcess
11
Recent Experimental Achievements and Future Possibilities
20
BDecay Studies of Neutron Rich Nickel Isotopes
30
Weak Strength for Astrophysics
34
Nuclear Masses and Fission Barriers
43
Understanding Beta Decay for the r Process
53
Neutron Captures and the rProcess
63
Origin of Heavy Elements Inferred from Galactic Chemical Evolution
138
Current Understanding and Future Tests
147
Nuclear Reaction Rates and the Production of Light pProcess Isotopes in Fast Expansions of ProtonRich Matter ...
157
rProcess Nucleosynthesis in ProtoMagnetar Winds
167
Treatment of the Injection Region and Requirements on Neutrino Emission ...
176
General Relativity and NeutrinoDriven Supernova Winds
186
An Update on the Hot Supernova Bubble rProcess
196
Ejecta from Parametrized Prompt Explosion
204

Supernova NeutrinoNucleus Physics and the rProcess
73
Equation of State and Neutrino Opacity of Dense Stellar Matter
89
An Overview of Observations of NeutronCapture Elements in MetalPoor Stars
99
Efficient Searches for rProcessEnhanced MetalPoor Stars
109
The rProcess Record in Meteorites
120
Inhomogenous Chemical Evolution and the Source of rProcess Elements
129
Are Collapsars Responsible for Some rProcess Elements? How Could We Tell?
214
Neutrino Transport in Core Collapse Supernovae
224
MultiDimensional and Fallback Effects
234
List of Participants
245
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