The (3)He((4)He, gamma)(7)Be reaction is the key process for the production of (7)Be and (8)B neutrinos in the Sun. We have designed a new experimental setup to study this reaction with high accuracy at low energies using two different experimental techniques. The first method consists in measuring the prompt capture gamma-ray transitions with an ultra-low background germanium detector heavily shielded and placed at close distance from a (3)He windowless gas target. With another fully shielded large-volume germanium detector we will also measure the beta-decay of the (7)Be residual nuclei. The aim of the experiment is to reduce the error on the astrophysical factor S(3,4) to 4%
The 3He(α, γ)7Be reaction plays an important role in the interpretation of the results of the solar ...
The nuclear physics input from the 3He(alpha,gamma)7Be cross section is a major uncertainty in the f...
The 3He(alpha,gamma)7Be reaction presently represents the largest nuclear uncertainty in the predict...
The (3)He((4)He, gamma)(7)Be reaction is the key process for the production of (7)Be and (8)B neutri...
The 3He(4He,γ)7Be reaction is the key process for the production of 7Be and 8B neutrinos in the Sun....
The 3He(4He,γ)7Be reaction is the key process for the production of 7Be and 8B neutrinos in the Sun....
The (3)He((4)He, gamma)(7)Be reaction is the key process for the production of (7)Be and (8)B neutri...
Solar neutrino fluxes depend both on astrophysical and on nuclear physics inputs, namely on the cros...
Solar neutrino fluxes depend both on astrophysical and on nuclear physics inputs, namely on the cros...
The nuclear physics input from the 3He(a,g)7Be cross section is a major uncertainty in the fluxes of...
The He-3(alpha, gamma)Be-7 process is a key reaction in both Big-Bang nucleosynthesis and p-p chain ...
Recently, the LUNA collaboration has carried out a high precision measurement on the (3)He(alpha,gam...
The flux of Be-7 and B-8 neutrinos from the Sun and the production of Li-7 via primordial nucleosynt...
The 3He(α, γ)7Be reaction plays an important role in the interpretation of the results of the solar ...
The nuclear physics input from the 3He(alpha,gamma)7Be cross section is a major uncertainty in the f...
The 3He(alpha,gamma)7Be reaction presently represents the largest nuclear uncertainty in the predict...
The (3)He((4)He, gamma)(7)Be reaction is the key process for the production of (7)Be and (8)B neutri...
The 3He(4He,γ)7Be reaction is the key process for the production of 7Be and 8B neutrinos in the Sun....
The 3He(4He,γ)7Be reaction is the key process for the production of 7Be and 8B neutrinos in the Sun....
The (3)He((4)He, gamma)(7)Be reaction is the key process for the production of (7)Be and (8)B neutri...
Solar neutrino fluxes depend both on astrophysical and on nuclear physics inputs, namely on the cros...
Solar neutrino fluxes depend both on astrophysical and on nuclear physics inputs, namely on the cros...
The nuclear physics input from the 3He(a,g)7Be cross section is a major uncertainty in the fluxes of...
The He-3(alpha, gamma)Be-7 process is a key reaction in both Big-Bang nucleosynthesis and p-p chain ...
Recently, the LUNA collaboration has carried out a high precision measurement on the (3)He(alpha,gam...
The flux of Be-7 and B-8 neutrinos from the Sun and the production of Li-7 via primordial nucleosynt...
The 3He(α, γ)7Be reaction plays an important role in the interpretation of the results of the solar ...
The nuclear physics input from the 3He(alpha,gamma)7Be cross section is a major uncertainty in the f...
The 3He(alpha,gamma)7Be reaction presently represents the largest nuclear uncertainty in the predict...