Published November 24, 2010 | Version v1
Journal article

Indirect Approach To The 2H(d,p)3H Reaction Study

  • 1. Dipartimento di Metodologie Fis. e Chim. per I'Ingegneria-Universita di Catania, Catania (Italy)
  • 2. INFN Laboratori Nazionali del Sud, Catania (Italy)
  • 3. School of Physics and Astronomy, University of Edinburgh (United Kingdom)
  • 4. Cyclotron Institute, ASCR, Rez (Czech Republic)
  • 5. Atomki, Debrecen (Hungary)
  • 6. Cyclotron Institute, Texas A and M University, College Station (United States)

Description

In order to understand primordial and stellar nucleosynthesis, we have studied 2H(d,p)3H reaction at 0.4 MeV down to astrophysical energies. Knowledge of its S-factor is interesting also to plan reactions for fusion reactors to produce energy. The 2H(d,p)H reaction has been studied through the Trojan Horse Method applied to the three-body reaction 2H(He,pt)H, at beam energy of 17 MeV. Once selection of protons and tritons detected in coincidence and the selection of quasi-free events, the obtained S-factor is compared with direct measurements. Such data are in agreement with the direct ones and a pole invariance test has been obtained comparing the present results with another 2H(d,p)3H THM measurements, where a different spectator particle was employed.

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
1304
Journal Issue
1
Journal Page Range
p. 420-424
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
From nuclei to stars
Acronym
Carpathian summer school of physics - Exotic nuclei and nuclear/particle astrophysics (III)
Dates
20 Jun - 3 Jul 2010
Place
Sinaia (Romania)

Optional Information

Notes
(c) 2010 American Institute of Physics