The cross section for the F-18(p,alpha) O-15 reaction has been obtained in reverse kinematics (F-18 beam on CH2 target) between 550 and 740 keV above threshold, i.e. in a region of astrophysical interest. The reaction yield is dominated by a wide resonant state whose spin, parity, total width and partial widths were deduced from the analysis of the alpha-particle and elastic proton data
Proton and alpha widths for a 3/2+ ( l p = 0) state in 19Ne at Ex-7.1 MeV have been extracted using ...
An experimental measurement of the absolute cross section for the O^(17)(p, α)N^(14) reaction has b...
States in the astrophysically important Ne-19 nucleus have been populated directly using the O-15(al...
The cross section for the 18F(p,α) 15O reaction has been obtained in reverse kinematics (18F beam on...
F-18 radioactive beams were used to measure the F-18(p,alpha) reaction in the c.m. energy ranges of ...
The cross section for the {sup 18}F(p,{alpha}) reaction at energies below 1 MeV/u, of interest to th...
An excitation function for the 18F~p,a!15O reaction has been measured in the energy range Ec.m.5600–...
The 18O(p, α)15N reaction is of primary importance to pin down the uncertainties, due to nuclear phy...
The F-18, produced during nova explosions, is the main responsible for the 511 keV gamma-ray emitted...
Proton and alpha widths for a 3/2{sup +} ({ell}{sub p} = 0) state in {sup 19}Ne at E{sub x} = 7.1 Me...
The inelastic component of the key astrophysical resonance (1(-), E-x=6.15 MeV) in the O-14(alpha,p)...
The O-18(p, alpha)N-15 reaction rate has been deduced by means of the Trojan horse method. For the f...
The proton resonant properties in Ne-18, which determine the reaction rate of the key stellar O-14(a...
The inelastic component of the key astrophysical resonance (1(-), E-x=6.15 MeV) in the O-14(alpha,p)...
International audienceThe 18F nucleus is one of the radioactive isotopes produced during nova explos...
Proton and alpha widths for a 3/2+ ( l p = 0) state in 19Ne at Ex-7.1 MeV have been extracted using ...
An experimental measurement of the absolute cross section for the O^(17)(p, α)N^(14) reaction has b...
States in the astrophysically important Ne-19 nucleus have been populated directly using the O-15(al...
The cross section for the 18F(p,α) 15O reaction has been obtained in reverse kinematics (18F beam on...
F-18 radioactive beams were used to measure the F-18(p,alpha) reaction in the c.m. energy ranges of ...
The cross section for the {sup 18}F(p,{alpha}) reaction at energies below 1 MeV/u, of interest to th...
An excitation function for the 18F~p,a!15O reaction has been measured in the energy range Ec.m.5600–...
The 18O(p, α)15N reaction is of primary importance to pin down the uncertainties, due to nuclear phy...
The F-18, produced during nova explosions, is the main responsible for the 511 keV gamma-ray emitted...
Proton and alpha widths for a 3/2{sup +} ({ell}{sub p} = 0) state in {sup 19}Ne at E{sub x} = 7.1 Me...
The inelastic component of the key astrophysical resonance (1(-), E-x=6.15 MeV) in the O-14(alpha,p)...
The O-18(p, alpha)N-15 reaction rate has been deduced by means of the Trojan horse method. For the f...
The proton resonant properties in Ne-18, which determine the reaction rate of the key stellar O-14(a...
The inelastic component of the key astrophysical resonance (1(-), E-x=6.15 MeV) in the O-14(alpha,p)...
International audienceThe 18F nucleus is one of the radioactive isotopes produced during nova explos...
Proton and alpha widths for a 3/2+ ( l p = 0) state in 19Ne at Ex-7.1 MeV have been extracted using ...
An experimental measurement of the absolute cross section for the O^(17)(p, α)N^(14) reaction has b...
States in the astrophysically important Ne-19 nucleus have been populated directly using the O-15(al...