The 2H(d,p)3H Reaction At Astrophysical Energies Studied Via The Trojan Horse Method And Pole Approximation Validity Test

Details The 2H(d,p)3H Reaction At Astrophysical Energies Studied Via The Trojan Horse Method And Pole Approximation Validity Test The 2H(d,p)3H Reaction At Astrophysical Energies Studied Via The Trojan Horse Method And Pole Approximation Validity Test

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1213..242s&link_type=abstract

FIFTH EUROPEAN SUMMER SCHOOL ON EXPERIMENTAL NUCLEAR ASTROPHYSICS. AIP Conference Proceedings, Volume 1213, pp. 242-245 (2010).

Astronomy and Astrophysics

Astrophysics

Nucleosynthesis, Fusion Reactors, Telescopes, Coulomb Blockade, Big Bang Nucleosynthesis, Components And Instrumentation, Ground-Based Ultraviolet, Optical And Infrared Telescopes, Coulomb Energies

Scientific paper

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 this S-factor is interesting also to plan reactions for fusion reactors to produce energy. 2H(d,p)3H has been studied through the Trojan Horse Method applied to the three-body reaction 2H(3He,pt)H, at a beam energy of 17 MeV. Once protons and tritons are detected in coincidence and the quasi-free events are selected, the obtained S-factor has been compared with direct reactions results. Such data are in agreement with the direct ones, and a pole invariance test has been obtained comparing the present result with another 2H(d,p)3H THM one, performed with a different spectator particle (see fig. 1).

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