T Itahashi et al 2004 J. Phys.: Conf. Ser. 2 75 doi:10.1088/1742-6596/2/1/010
T Itahashi1, N Kudomi1, Y Sakemi1, T Shima1, S Yoshida1, T Sakamoto1, E D Donets2 and E E Donets2
Show affiliationsThe laboratory condition where charged particle fusion reactions have been done is not exactly the same as that of stellar condition. To probe details of reaction and to test the prediction of standard solar model we need more precise data for charged particle fusion experiments in the laboratories. We propose several experimental approaches to reduce the ambiguity of the estimation of screening potential value which is crucial for obtaining the astrophysical S-factor. Experiment with bare target and bare beam interaction will be done by using proposed Electron Beam Ion Trap apparatus (NARITA).
29.25.-t Particle sources and targets
97.10.Cv Stellar structure, interiors, evolution, nucleosynthesis, ages
Accelerators, beams and electromagnetism
Instrumentation and measurement
Issue 1 (2004)
T Itahashi et al 2004 J. Phys.: Conf. Ser. 2 75
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