Considering the importance of the 26Al nuclei in Astrophysics, in this work, preliminary results regarding a campaign of measurements related with this radioisotope production, are presented. We have taken advantage of two different facilities: first, the radio-nucleus is produced by means of irradiation of targets selected in correlation with particular reactions; once the enrichment with 26Al was made, the targets are analyzed in an AMS machine to obtain the concentration of 26Al produced during the irradiation. With this off-line method, it is possible to measure acceptable small cross sections of a selected low energy reaction. In this work, our preliminary results for three different energies of 28Si(d,α)26Al reaction cross s...
The observation of 26Al gives us the proof of active nucleosynthesis in the Milky Way. However the i...
International audienceAl-26 was the first cosmic radioactivity ever detected in the galaxy as well a...
The 26Al(3He,d)27Si reaction was measured from 0°≤θc.m.≤35° at E(3He)=20 MeV using a quadrupole-dipo...
Considering the importance of the 26Al nuclei in Astrophysics, in this work, preliminary results reg...
Considering the importance of the 26Al nuclei in Astrophysics, in this work, preliminary results reg...
For charged-particle induced reactions occurring in astrophysical scenarios, projectile energies are...
The origin of 26Al in the universe is one of mysteries of astrophysics. It was proposed that the rea...
Accelerator Mass Spectrometry is a technique commonly used to approach low concentrations of certain...
The nucleosynthetic origin of 26Al (t1/2=0.72 Myr) in the early solar system is still an open questi...
The detection of the 1809 keV emission line associated with the decay of 26Al in the interstellar me...
26Al was the first cosmic radioactivity ever detected in the galaxy as well as one of the first exti...
The 26mAl(p,γ)27Si reaction is thought have a significant impact of the nucleosynthesis of both 26Mg...
The cosmic 1.809 MeV γ-ray emitted by the radioactive nucleus 26Al in the Galaxy is one of the key o...
The observation of 26Al gives us the proof of active nucleosynthesis in the Milky Way. However the i...
The measurements described in the preceding paper (I) are used to obtain the position, spin and isob...
The observation of 26Al gives us the proof of active nucleosynthesis in the Milky Way. However the i...
International audienceAl-26 was the first cosmic radioactivity ever detected in the galaxy as well a...
The 26Al(3He,d)27Si reaction was measured from 0°≤θc.m.≤35° at E(3He)=20 MeV using a quadrupole-dipo...
Considering the importance of the 26Al nuclei in Astrophysics, in this work, preliminary results reg...
Considering the importance of the 26Al nuclei in Astrophysics, in this work, preliminary results reg...
For charged-particle induced reactions occurring in astrophysical scenarios, projectile energies are...
The origin of 26Al in the universe is one of mysteries of astrophysics. It was proposed that the rea...
Accelerator Mass Spectrometry is a technique commonly used to approach low concentrations of certain...
The nucleosynthetic origin of 26Al (t1/2=0.72 Myr) in the early solar system is still an open questi...
The detection of the 1809 keV emission line associated with the decay of 26Al in the interstellar me...
26Al was the first cosmic radioactivity ever detected in the galaxy as well as one of the first exti...
The 26mAl(p,γ)27Si reaction is thought have a significant impact of the nucleosynthesis of both 26Mg...
The cosmic 1.809 MeV γ-ray emitted by the radioactive nucleus 26Al in the Galaxy is one of the key o...
The observation of 26Al gives us the proof of active nucleosynthesis in the Milky Way. However the i...
The measurements described in the preceding paper (I) are used to obtain the position, spin and isob...
The observation of 26Al gives us the proof of active nucleosynthesis in the Milky Way. However the i...
International audienceAl-26 was the first cosmic radioactivity ever detected in the galaxy as well a...
The 26Al(3He,d)27Si reaction was measured from 0°≤θc.m.≤35° at E(3He)=20 MeV using a quadrupole-dipo...