Tumino, Aurora ; Bertulani, Carlos A. ; La Cognata, Marco ; Lamia, Livio ; Pizzone, Rosario Gianluca ; Romano, Stefano ; Typel, Stefan (2021)
The Trojan Horse Method: A Nuclear Physics Tool for Astrophysics.
In: Annual Review of Nuclear and Particle Science, 71 (1)
doi: 10.1146/annurev-nucl-102419-033642
Article, Bibliographie
Abstract
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.
Item Type: | Article |
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Erschienen: | 2021 |
Creators: | Tumino, Aurora ; Bertulani, Carlos A. ; La Cognata, Marco ; Lamia, Livio ; Pizzone, Rosario Gianluca ; Romano, Stefano ; Typel, Stefan |
Type of entry: | Bibliographie |
Title: | The Trojan Horse Method: A Nuclear Physics Tool for Astrophysics |
Language: | English |
Date: | September 2021 |
Journal or Publication Title: | Annual Review of Nuclear and Particle Science |
Volume of the journal: | 71 |
Issue Number: | 1 |
DOI: | 10.1146/annurev-nucl-102419-033642 |
Abstract: | 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. |
Divisions: | 05 Department of Physics 05 Department of Physics > Institute of Nuclear Physics 05 Department of Physics > Institute of Nuclear Physics > Theoretische Kernphysik 05 Department of Physics > Institute of Nuclear Physics > Theoretische Kernphysik > Kernphysik und Nukleare Astrophysik 05 Department of Physics > Institute of Nuclear Physics > Theoretische Kernphysik > 05 Department of Physics > Institute of Nuclear Physics > Theoretische Kernphysik > Schwerionenphysik 05 Department of Physics > Institute of Nuclear Physics > Theoretische Kernphysik > Theoretical Nuclear Astrophysics Group |
Date Deposited: | 13 Jul 2022 07:05 |
Last Modified: | 06 Jan 2023 12:51 |
PPN: | 503405450 |
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