Experimental values of the astrophysical S factor for the 15N(p,γ0)16O reaction are fitted using both an R-matrix formula and an alternative formula, and values of the zero-energy S factor are derived
The astrophysical S factors of E1 and E2 capture data of 12C( α , γ) reaction at 300 keV have been c...
The 14N(p,γ)15O low-energy S-factor is analyzed using the R-matrix model. We find that the g.s. cont...
The astrophysical S(E) factor of 14N(p,γ)15O has been measured for effective center-of-mass energies...
Experimental values of the astrophysical S factor for the 15N(p,α0)12C reaction are available both f...
The 15N(p,γ)16O reaction represents a breakout reaction linking the first and second cycles of the C...
The 15N(p,\u3b3)16O reaction represents a breakout reaction linking the first and second cycles of t...
The 15N(p,γ)16O reaction represents a breakout reaction linking the first and second cycles of the C...
The 15N(p,γ)16O reaction represents a breakout reaction linking the first and second cycles of the C...
The 15N(p,γ)16O reaction represents a breakout reaction linking the first and second cycles of the C...
The N14(p,γ)O15 reaction is the slowest reaction of the carbon-nitrogen cycle of hydrogen burning an...
The N14(p,γ)O15 reaction is the slowest reaction of the carbon-nitrogen cycle of hydrogen burning an...
The N14(p,γ)O15 reaction is the slowest reaction of the carbon-nitrogen cycle of hydrogen burning an...
Abstract. The astrophysical S(E) factor of 14N(p; °)15O has been measured for e®ective center-of-mas...
The astrophysical S-factor of 14N(p,gamma)15O has been measured for effective center-of-mass energie...
Journals published by the American Physical Society can be found at http://publish.aps.org/We presen...
The astrophysical S factors of E1 and E2 capture data of 12C( α , γ) reaction at 300 keV have been c...
The 14N(p,γ)15O low-energy S-factor is analyzed using the R-matrix model. We find that the g.s. cont...
The astrophysical S(E) factor of 14N(p,γ)15O has been measured for effective center-of-mass energies...
Experimental values of the astrophysical S factor for the 15N(p,α0)12C reaction are available both f...
The 15N(p,γ)16O reaction represents a breakout reaction linking the first and second cycles of the C...
The 15N(p,\u3b3)16O reaction represents a breakout reaction linking the first and second cycles of t...
The 15N(p,γ)16O reaction represents a breakout reaction linking the first and second cycles of the C...
The 15N(p,γ)16O reaction represents a breakout reaction linking the first and second cycles of the C...
The 15N(p,γ)16O reaction represents a breakout reaction linking the first and second cycles of the C...
The N14(p,γ)O15 reaction is the slowest reaction of the carbon-nitrogen cycle of hydrogen burning an...
The N14(p,γ)O15 reaction is the slowest reaction of the carbon-nitrogen cycle of hydrogen burning an...
The N14(p,γ)O15 reaction is the slowest reaction of the carbon-nitrogen cycle of hydrogen burning an...
Abstract. The astrophysical S(E) factor of 14N(p; °)15O has been measured for e®ective center-of-mas...
The astrophysical S-factor of 14N(p,gamma)15O has been measured for effective center-of-mass energie...
Journals published by the American Physical Society can be found at http://publish.aps.org/We presen...
The astrophysical S factors of E1 and E2 capture data of 12C( α , γ) reaction at 300 keV have been c...
The 14N(p,γ)15O low-energy S-factor is analyzed using the R-matrix model. We find that the g.s. cont...
The astrophysical S(E) factor of 14N(p,γ)15O has been measured for effective center-of-mass energies...
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