Implications of fission mass distributions for the astrophysical r-process

The role of nuclear fission in the astrophysical r-process is examined, and calculated fission fragment mass distributions are utilized to interpret observed elemental abundance data. A number of features of the solar system abundance curve are accounted for. An extension of the r-process to neutron...

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Veröffentlicht in:	Astrophys. J.; (United States) 1978-08, Vol.223, p.1000
Hauptverfasser:	Steinberg, E. P., Wilkins, B. D.
Format:	Artikel
Sprache:	eng
Schlagworte:	ABUNDANCE BARYON REACTIONS BARYONS BASIC INTERACTIONS BETA DECAY CAPTURE CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS DECAY DISTRIBUTION ELEMENTARY PARTICLES ELEMENTS FERMIONS FISSION FISSION FRAGMENTS HADRON REACTIONS HADRONS INTERACTIONS LEPTONIC DECAY LIQUID DROP MODEL MASS MATHEMATICAL MODELS METALS NEUTRON REACTIONS NEUTRONS NUCLEAR FRAGMENTS NUCLEAR MODELS NUCLEAR REACTIONS NUCLEON REACTIONS NUCLEONS NUCLEOSYNTHESIS PARTICLE DECAY R PROCESS RARE EARTHS SOLAR SYSTEM STAR EVOLUTION WEAK INTERACTIONS WEAK PARTICLE DECAY 640102 > Astrophysics & Cosmology-- Stars & Quasi-Stellar, Radio & X-Ray Sources XENON ISOTOPES
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