Paper
3 March 1995 Neutron capture origin for the heavy elements
Kohji Takahashi
Author Affiliations +
Proceedings Volume 2339, International Conference on Neutrons and Their Applications; (1995) https://doi.org/10.1117/12.204152
Event: 4th International Conference on Applications of Nuclear Techniques: Neutrons and their Applications, 1994, Crete, Greece
Abstract
Most naturally occurring elements were evidently synthesized in the interiors of stars, and, in particular, most of the heavy ones via neutron capture processes. We present here an introductory review on the stellar alchemy by neutrons. In due course, we attempt to cover the very basics through the latest developments of theoretical studies of the rapid (r-) process.
© (1995) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Kohji Takahashi "Neutron capture origin for the heavy elements", Proc. SPIE 2339, International Conference on Neutrons and Their Applications, (3 March 1995); https://doi.org/10.1117/12.204152
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KEYWORDS
Stars

Chemical elements

Iron

Data modeling

Solar system

Combustion

Information operations

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