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In the energy range of 10-100 keV, the 2H(d,γ)4He reaction is of fundamental importance for the determination of deuteron burning and the 4He abundance in astronuclear processes. The observation of
The energy range of 10-100 keV, the 2H (d, γ) 4He reaction is of fundamental importance for the determination of deuteron burning and the abundance in astronuclear processes.