期刊
ANNUAL REVIEW OF NUCLEAR AND PARTICLE SCIENCE, VOL 71, 2021
卷 71, 期 -, 页码 345-376出版社
ANNUAL REVIEWS
DOI: 10.1146/annurev-nucl-102419-033642
关键词
nuclear astrophysics; indirect methods; direct reactions; nucleosynthesis
资金
- US Department of Energy [DE-FG02-08ER41533]
- U.S. Department of Energy (DOE) [DE-FG02-08ER41533] Funding Source: U.S. Department of Energy (DOE)
The Trojan Horse Method is an indirect approach to determine astrophysical S-factors for reactions among charged particles at astrophysical energies by measuring the quasi-free cross section of a suitable three-body process. It is also useful for studying neutron-induced reactions, particularly with radioactive ion beams. This method's practical use and recent applications demonstrate its effectiveness in impacting selected astrophysical scenarios.
The Trojan Horse Method (THM) represents an indirect path to determine the bare nucleus astrophysical S-factor for reactions among charged particles at astrophysical energies. This is achieved by measuring the quasi-free cross section of a suitable three-body process. The method is also suited to study neutron-induced reactions, especially in the case of radioactive ion beams. A comprehensive review of the theoretical as well as experimental features behind the THM is presented here. An overview is given of some recent applications to demonstrate the method's practical use for reactions that have a great impact on selected astrophysical scenarios.
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