The Trojan Horse Method in nuclear astrophysics

M Aliotta, M Lattuada, M G Pellegriti, R G Pizzone, C Spitaleri, D Miljanic, C Rolfs, S Typel, H H Wolter

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

Because of the Coulomb barrier, reaction cross sections in astrophysics cannot be accessed directly at the relevant Gamow energies, unless very favourable conditions are met (e.g. LUNA - underground experiments). Theoretical extrapolations of available data are then needed to derive the astrophysical S(0)-factor. Various indirect processes have been used in order to obtain additional information on the parameters entering these extrapolations.

The Trojan Horse Method is an indirect method which might help to bypass some of the problems typically encountered in direct measurements, namely the presence of the Coulomb barrier and the effect of the electron screening. However, a comparison with direct data in an appropriate energy region (e.g. around the Coulomb barrier) is crucial before extending the method to the relevant Gamow energy. Additionally, experimental and theoretical tests are needed to validate the assumptions underlying the method.

The application of the Trojan Horse Method to some cases of interest is discussed.

Original languageEnglish
Title of host publication4TH SYMPOSIUM ON NUCLEAR PHYSICS
EditorsM Arnould, M Lewitowicz, YT Oganessian, H Akimune, M Ohta, H Utsunomiya, T Wada, T Yamagata
Place of PublicationMELVILLE
PublisherAmerican Institute of Physics
Pages116-126
Number of pages11
ISBN (Print)1-56396-996-3
Publication statusPublished - 2001
Event4th Symposium on Nuclear Physics - TOURS
Duration: 4 Sep 20007 Sep 2000

Conference

Conference4th Symposium on Nuclear Physics
CityTOURS
Period4/09/007/09/00

Keywords

  • ENERGIES
  • SCATTERING
  • RELEVANT

Fingerprint

Dive into the research topics of 'The Trojan Horse Method in nuclear astrophysics'. Together they form a unique fingerprint.

Cite this