The absolute cross section for the reaction, He^3(α,γ) Be^7, has been measured over the range of energies 181 ≤ E_(cm) ≤ 2493 keV, using a gas target behind a thin nickel entrance foil. Calibrated NaI(Tl) crystals were used to detect the prompt capture radiation. Over the entire energy region the measured total cross section and branching ratio confirm theoretical predictions based on calculations neglecting the contributions to the matrix elements from the region inside the nuclear radius. These cross-section measurements have been used to obtain a new value for the low-energy cross-section factor, S_o, for this reaction (S_o = 0.47 ± .07 keY barns), and this value has been used to reevaluate the importance of the He^3(α,γ) Be^7 ...
The 3He(α,γ)7Be reaction presently represents the largest nuclear uncertainty in the predicted solar...
Improved absolute cross section and angular distribution measurements have been made for the direct...
This research was sponsored by the National Science Foundation Grant NSF PHY 87-1440
Cross sections for the 3He(α,γ)7Be reaction have been measured at several energies from Ecm = 165 to...
We derive simple expressions for the low-energy behavior of direct radiative capture cross sections,...
3 pags., 1 tab. -- Nuclear Physics in Astrophysics V 3–8 April 2011, Eilat, IsraelThe astrophysical ...
Background: The 3He(α, γ )7Be reaction is a widely studied nuclear reaction; however, it is still no...
The proton-proton chains (p-p chains), a series of nuclear reactions were proposed several decades a...
Differential cross sections for $^3$He-$\alpha$ scattering were measured in the energy range up to 3...
The astrophysical S-factor for the reaction Be-7(p, gamma)B-8 up to an energy of 2 MeV (c.m.) and th...
Reactions produced by the He3 bombardment of the He3 have been investigated for bombarding energies ...
Precise measurements of the total reaction cross section for 3He(3He,2p)4He He have been made in t...
The reaction rate of the 3He(α,γ)7 Be reaction is important both in the Big Bang Nucleosynthesis (BB...
Measurements of (He3,d) reactions can provide information on the proton widths of states that play a...
Die Arbeit beschreibt die Durchführung einer Messung des absoluten Wirkungsquerschnitts der Reaktion...
The 3He(α,γ)7Be reaction presently represents the largest nuclear uncertainty in the predicted solar...
Improved absolute cross section and angular distribution measurements have been made for the direct...
This research was sponsored by the National Science Foundation Grant NSF PHY 87-1440
Cross sections for the 3He(α,γ)7Be reaction have been measured at several energies from Ecm = 165 to...
We derive simple expressions for the low-energy behavior of direct radiative capture cross sections,...
3 pags., 1 tab. -- Nuclear Physics in Astrophysics V 3–8 April 2011, Eilat, IsraelThe astrophysical ...
Background: The 3He(α, γ )7Be reaction is a widely studied nuclear reaction; however, it is still no...
The proton-proton chains (p-p chains), a series of nuclear reactions were proposed several decades a...
Differential cross sections for $^3$He-$\alpha$ scattering were measured in the energy range up to 3...
The astrophysical S-factor for the reaction Be-7(p, gamma)B-8 up to an energy of 2 MeV (c.m.) and th...
Reactions produced by the He3 bombardment of the He3 have been investigated for bombarding energies ...
Precise measurements of the total reaction cross section for 3He(3He,2p)4He He have been made in t...
The reaction rate of the 3He(α,γ)7 Be reaction is important both in the Big Bang Nucleosynthesis (BB...
Measurements of (He3,d) reactions can provide information on the proton widths of states that play a...
Die Arbeit beschreibt die Durchführung einer Messung des absoluten Wirkungsquerschnitts der Reaktion...
The 3He(α,γ)7Be reaction presently represents the largest nuclear uncertainty in the predicted solar...
Improved absolute cross section and angular distribution measurements have been made for the direct...
This research was sponsored by the National Science Foundation Grant NSF PHY 87-1440