The (8)B(alpha,p)(11)C reaction is part of the network that can bypass the triple a process leading to the production of (12)C. We have measured the astrophysical reaction rate for this reaction by studying the inverse (11)C(p,alpha)(8)B process. The radioactive (11)C beam was produced via the p((11)B,(11)C)n reaction using the in-flight facility at the ATLAS accelerator. The astrophysical reaction rate obtained from the excitation function measured in the energy range E(x)=8.8-10 MeV was found to be a factor of 10-50 higher than previous estimates.</p
bInstitute for Applied Physics, Goethe-University Frankfurt am Main The accuracy of predicted isotop...
Neutrons produced by the carbon fusion reaction (12)C((12)C,n)(23)Mg play an important role in stell...
The cross section of the [Formula Presented] reaction was determined by in-beam measurements at ener...
The (8)B(alpha,p)(11)C reaction is part of the network that can bypass the triple a process leading ...
The {sup 11}C(p,{gamma}){sup 12}N reaction is expected to be an important branch point in supermassi...
We have performed the first direct measurement of the ^{83}Rb(p,γ) radiative capture reaction cross ...
The reactions ^{10}B(p,\alpha)^{7}Be and ^{11}B(p,\alpha)^{8}Be are studied at thermonuclear energie...
The evolution of massive stars with very low-metallicities depends critically on the amount of CNO n...
The cross section of 8Li(alpha,n)11B is very important for the study of primordial nuclesynthesis mo...
Neutron capture of short-lived isotopes can be important within several astrophysical environments. ...
Because of interest in the 11,12B(n,γ) reaction in seeding r-process nucleosynthesis through light n...
L’étude des réaction (a,g) d’intérêt astrophysique est vaste. Ces réactions ont un rôle important da...
Reactions of interest to nuclear astrophysics have been studied with radioactive beams at the ATLAS ...
We study the astrophysical reaction rate for the formation of $^{9}$Be through the three body reacti...
The formation of nuclei in slightly proton-rich regions of the neutrino-driven wind of core-collapse...
bInstitute for Applied Physics, Goethe-University Frankfurt am Main The accuracy of predicted isotop...
Neutrons produced by the carbon fusion reaction (12)C((12)C,n)(23)Mg play an important role in stell...
The cross section of the [Formula Presented] reaction was determined by in-beam measurements at ener...
The (8)B(alpha,p)(11)C reaction is part of the network that can bypass the triple a process leading ...
The {sup 11}C(p,{gamma}){sup 12}N reaction is expected to be an important branch point in supermassi...
We have performed the first direct measurement of the ^{83}Rb(p,γ) radiative capture reaction cross ...
The reactions ^{10}B(p,\alpha)^{7}Be and ^{11}B(p,\alpha)^{8}Be are studied at thermonuclear energie...
The evolution of massive stars with very low-metallicities depends critically on the amount of CNO n...
The cross section of 8Li(alpha,n)11B is very important for the study of primordial nuclesynthesis mo...
Neutron capture of short-lived isotopes can be important within several astrophysical environments. ...
Because of interest in the 11,12B(n,γ) reaction in seeding r-process nucleosynthesis through light n...
L’étude des réaction (a,g) d’intérêt astrophysique est vaste. Ces réactions ont un rôle important da...
Reactions of interest to nuclear astrophysics have been studied with radioactive beams at the ATLAS ...
We study the astrophysical reaction rate for the formation of $^{9}$Be through the three body reacti...
The formation of nuclei in slightly proton-rich regions of the neutrino-driven wind of core-collapse...
bInstitute for Applied Physics, Goethe-University Frankfurt am Main The accuracy of predicted isotop...
Neutrons produced by the carbon fusion reaction (12)C((12)C,n)(23)Mg play an important role in stell...
The cross section of the [Formula Presented] reaction was determined by in-beam measurements at ener...