The Trojan Horse Method: A Nuclear Physics Tool for Astrophysics-Reference-Cited by-同舟云学术

The Trojan Horse Method: A Nuclear Physics Tool for Astrophysics

Published:2021-09-21 Issue:1 Volume:71 Page:345-376
ISSN:0163-8998
Container-title:Annual Review of Nuclear and Particle Science
language:en
Short-container-title:Annu. Rev. Nucl. Part. Sci.

Author:

Tumino Aurora¹²,Bertulani Carlos A.³,La Cognata Marco²,Lamia Livio²⁴⁵,Pizzone Rosario Gianluca²,Romano Stefano²⁴⁵,Typel Stefan⁶⁷

Affiliation:

1. Facoltà di Ingegneria e Architettura, Università degli Studi di Enna “Kore,” 94100 Enna, Italy

2. Laboratori Nazionali del Sud, INFN, 95123 Catania, Italy;

3. Department of Physics and Astronomy, Texas A&M University–Commerce, Commerce, Texas 75429, USA

4. Dipartimento di Fisica e Astronomia “E. Majorana,” Università degli Studi di Catania, 95131 Catania, Italy

5. Centro Siciliano di Fisica Nucleare e Struttura della Materia (CSFNSM), 95123 Catania, Italy

6. Fachbereich Physik, Institut für Kernphysik, Technische Universität Darmstadt, 64289 Darmstadt, Germany

7. GSI Helmholtzzentrum für Schwerionenforschung GmbH, 64291 Darmstadt, Germany

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.

Publisher

Annual Reviews

Subject

Nuclear and High Energy Physics

Link

https://www.annualreviews.org/doi/pdf/10.1146/annurev-nucl-102419-033642

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