The N-14(p,gamma)O-15 reaction has been investigated by LUNA at the National Laboratory of Gran Sasso (LNGS) using two different techniques. The first study has been performed using a solid target and detecting the gamma-rays coming from the single transitions with a HPGe detector in very close geometry to the target. In a second phase a windowless gas target sorrounded by a nearly 4 pi BGO summing crystal has been used and the total S-factor has been measured down to E-b=80 keV
We report on a new measurement of the 14N(p,\u3b3) 15O capture cross section at Ep=140 to 400 keV us...
The rate of the carbon-nitrogen-oxygen (CNO) cycle of hydrogen burning is controlled by the 14N(p,γ ...
The astrophysical S(E) factor of N-14(p,gamma)O-15 has been measured for effective center-of-mass en...
The N-14(p,gamma)O-15 reaction has been investigated by LUNA at the National Laboratory of Gran Sass...
The 14N(p,gamma )15O reaction has been investigated by LUNA at the National Laboratory of Gran Sasso...
The 14N(p, gamma )15O reaction has been investigated by the LUNA experiment at the National Laborato...
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...
I will describe the measurement of 14N(p,γ)15O done in the context of the LUNA experiment. The deter...
We report on a new measurement of the 14N(p, \u3b3 )15O capture cross section at Ep = 140 to 400 keV...
The astrophysical S-factor of 14N(p,gamma)15O has been measured for effective center-of-mass energie...
The rate of the carbon-nitrogen-oxygen (CNO) cycle of hydrogen burning is controlled by the 14N(p,\u...
We report on a new measurement of the 14N(p,γ)15O capture cross section at Ep=140 to 400 keV using t...
We report on a new measurement of the 14N(p,γ) 15O capture cross section at Ep=140 to 400 keV using ...
We report on a new measurement of the 14N(p,\u3b3) 15O capture cross section at Ep=140 to 400 keV us...
The rate of the carbon-nitrogen-oxygen (CNO) cycle of hydrogen burning is controlled by the 14N(p,γ ...
The astrophysical S(E) factor of N-14(p,gamma)O-15 has been measured for effective center-of-mass en...
The N-14(p,gamma)O-15 reaction has been investigated by LUNA at the National Laboratory of Gran Sass...
The 14N(p,gamma )15O reaction has been investigated by LUNA at the National Laboratory of Gran Sasso...
The 14N(p, gamma )15O reaction has been investigated by the LUNA experiment at the National Laborato...
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...
I will describe the measurement of 14N(p,γ)15O done in the context of the LUNA experiment. The deter...
We report on a new measurement of the 14N(p, \u3b3 )15O capture cross section at Ep = 140 to 400 keV...
The astrophysical S-factor of 14N(p,gamma)15O has been measured for effective center-of-mass energie...
The rate of the carbon-nitrogen-oxygen (CNO) cycle of hydrogen burning is controlled by the 14N(p,\u...
We report on a new measurement of the 14N(p,γ)15O capture cross section at Ep=140 to 400 keV using t...
We report on a new measurement of the 14N(p,γ) 15O capture cross section at Ep=140 to 400 keV using ...
We report on a new measurement of the 14N(p,\u3b3) 15O capture cross section at Ep=140 to 400 keV us...
The rate of the carbon-nitrogen-oxygen (CNO) cycle of hydrogen burning is controlled by the 14N(p,γ ...
The astrophysical S(E) factor of N-14(p,gamma)O-15 has been measured for effective center-of-mass en...