Nuclear Astrophysics Studied by Neutrons
Yasuki Nagai
Abstract
Open-access reader
Yasuki Nagai
Abstract
Open-access reader
Heavier elements than iron are synthesized by neutron capture reactions in stars, either by the slow neutron capture process or the rapid neutron capture process. Due to the recent observational and theoretical progress in the study of stellar nucleosynthesis and Big-Bang nulceosynthesis, much interest has arisen regarding experimental study of the neutron capture reaction of a nucleus. This report briefly describes the recent progress mentioned above, the experimental study aimed at measuring the neutron capture cross sections of a nucleus, and future plans to further extend the activity of nuclear astrophysics using neutrons.
OpenAlex reports 1 citations for this work. Citation counts describe recorded attention and do not establish research quality.
A contribution statement is not available in the OpenAlex record.
Method details are not available in the OpenAlex metadata.
Findings are not separately available in the OpenAlex metadata.
Limitations are not available in the OpenAlex metadata.
Application details are not available in the OpenAlex metadata.
Heavier elements than iron are synthesized by neutron capture reactions in stars, either by the slow neutron capture process or the rapid neutron capture process. Due to the recent observational and theoretical progress in the study of stellar nucleosynthesis and Big-Bang nulceosynthesis, much interest has arisen regarding experimental study of the neutron capture reaction of a nucleus. This report briefly describes the recent progress mentioned above, the experimental study aimed at measuring the neutron capture cross sections of a nucleus, and future plans to further extend the activity of nuclear astrophysics using neutrons.
Key concepts: Nucleosynthesis, Nuclear astrophysics, r-process, Physics, Neutron capture, s-process, Nuclear physics, Neutron