The 14N(p, gamma )15O reaction has been investigated by the LUNA experiment at the National Laboratory of Gran Sasso (LNGS). This study has been performed with two different setups. The first one, suitable for the detection of gamma -rays produced by single transitions, has been based on an HPGe detector and a solid target. In a second phase, we used a BGO summing crystal as a detector and a windowless gas target. The BGO high detection efficiency and the target purity allowed us to measure the total S factor down to Ecm = 70 keV
I will describe the measurement of 14N(p,γ)15O done in the context of the LUNA experiment. The deter...
The rate of the carbon-nitrogen-oxygen (CNO) cycle of hydrogen burning is controlled by the 14N(p,γ ...
Deep underground in Gran Sasso National Laboratory (Italy), at the LUNA facility, the cross section ...
The 14N(p,gamma )15O reaction has been investigated by LUNA at the National Laboratory of Gran Sasso...
The N-14(p,gamma)O-15 reaction has been investigated by LUNA at the National Laboratory of Gran Sass...
The 14N(p,γ)15O reaction has been investigated by the LUNA experiment at the National Laboratory of ...
The 14N(p,\u3b3)15O reaction has been investigated by the LUNA experiment at the National Laboratory...
The 14N(p, γ)15O reaction has been investigated by the LUNA experiment at the National Laboratory of...
The rate of the carbon-nitrogen-oxygen (CNO) cycle of hydrogen burning is controlled by the 14N(p,\u...
In stars, four hydrogen nuclei are converted into a helium nucleus by two competing nuclear fusion p...
The astrophysical S-factor of 14N(p,gamma)15O has been measured for effective center-of-mass energie...
In stars, four hydrogen nuclei are converted into a helium nucleus by two competing nuclear fusion p...
We report on a new measurement of the 14N(p, \u3b3 )15O capture cross section at Ep = 140 to 400 keV...
Deep underground in Gran Sasso National Laboratory (Italy), at the LUNA facility, the cross section ...
Direct measurements of small nuclear reaction cross sections require a low background in the signal ...
I will describe the measurement of 14N(p,γ)15O done in the context of the LUNA experiment. The deter...
The rate of the carbon-nitrogen-oxygen (CNO) cycle of hydrogen burning is controlled by the 14N(p,γ ...
Deep underground in Gran Sasso National Laboratory (Italy), at the LUNA facility, the cross section ...
The 14N(p,gamma )15O reaction has been investigated by LUNA at the National Laboratory of Gran Sasso...
The N-14(p,gamma)O-15 reaction has been investigated by LUNA at the National Laboratory of Gran Sass...
The 14N(p,γ)15O reaction has been investigated by the LUNA experiment at the National Laboratory of ...
The 14N(p,\u3b3)15O reaction has been investigated by the LUNA experiment at the National Laboratory...
The 14N(p, γ)15O reaction has been investigated by the LUNA experiment at the National Laboratory of...
The rate of the carbon-nitrogen-oxygen (CNO) cycle of hydrogen burning is controlled by the 14N(p,\u...
In stars, four hydrogen nuclei are converted into a helium nucleus by two competing nuclear fusion p...
The astrophysical S-factor of 14N(p,gamma)15O has been measured for effective center-of-mass energie...
In stars, four hydrogen nuclei are converted into a helium nucleus by two competing nuclear fusion p...
We report on a new measurement of the 14N(p, \u3b3 )15O capture cross section at Ep = 140 to 400 keV...
Deep underground in Gran Sasso National Laboratory (Italy), at the LUNA facility, the cross section ...
Direct measurements of small nuclear reaction cross sections require a low background in the signal ...
I will describe the measurement of 14N(p,γ)15O done in the context of the LUNA experiment. The deter...
The rate of the carbon-nitrogen-oxygen (CNO) cycle of hydrogen burning is controlled by the 14N(p,γ ...
Deep underground in Gran Sasso National Laboratory (Italy), at the LUNA facility, the cross section ...