"10"^^ . "Trache, L." . "Spitareli, C." . . "Plunkett, A." . "Mr\u00E1zek, Jarom\u00EDr" . "78" . . . "000258636200068" . "Z nam\u011B\u0159en\u00FDch \u00FAhlov\u00FDch rozlo\u017Een\u00ED byly pomoc\u00ED v\u00FDpo\u010Dt\u016F DWBA ur\u010Deny ANC pro p\u0159\u00EDm\u00FD z\u00E1chyt. D\u00E1le byly provedeny v\u00FDpo\u010Dty v r\u00E1mci R-maticov\u00E9 teorie a z\u00EDsk\u00E1n celkov\u00FD astrofyzik\u00E1ln\u00ED faktor reakce 15N(p,gama )16O zahrnuj\u00EDc\u00ED rezonan\u010Dn\u00ED i nerezonan\u010Dn\u00ED proces."@cs . . "Gagliardi, C. A." . . "RIV/61389005:_____/08:00311394!RIV09-AV0-61389005" . . "\u0160ime\u010Dkov\u00E1, Eva" . "1" . . . "0556-2813" . "Physical Review. C" . . "Goldberg, V. Z." . "Nov\u00FD astrofyzik\u00E1ln\u00ED S faktor pro reakci 15N(p,gama)16-O metodou asymptotick\u00FDch normaliza\u010Dn\u00EDch koeficient\u016F"@cs . "Burjan, V\u00E1clav" . "Kroha, V\u00E1clav" . . "P(GA202/05/0302), P(LC07050), Z(AV0Z10480505)" . . "Vesel\u00FD, Franti\u0161ek" . "New astrophysical S factor for the N-15(p,gamma)O-16 reaction via the asymptotic normalization coefficient (ANC) method"@en . "B\u00E9m, Pavel" . "Hons, Zden\u011Bk" . . "Nov\u00E1k, Jan" . "Mukhamedzhanov, A. M." . . . "Romano, S." . . . . . "Tribble, R. E." . "New astrophysical S factor for the N-15(p,gamma)O-16 reaction via the asymptotic normalization coefficient (ANC) method" . "Pizzone, R. G." . "RIV/61389005:_____/08:00311394" . "US - Spojen\u00E9 st\u00E1ty americk\u00E9" . "Nov\u00FD astrofyzik\u00E1ln\u00ED S faktor pro reakci 15N(p,gama)16-O metodou asymptotick\u00FDch normaliza\u010Dn\u00EDch koeficient\u016F"@cs . "The N-15(p,gamma)O-16 reaction provides a path from the CN cycle to the CNO bi-cycle and CNO tri-cycle. The measured astrophysical factor for this reaction is dominated by resonant capture through two strong J(pi) = 1(-) resonances at E-R = 312 and 962 keV and direct capture to the ground state. Asymptotic normalization coefficients (ANCs) for the ground and seven excited states in O-16 were extracted from the comparison of experimental differential cross sections for the N-15(He-3,d)O-16 reaction with distorted-wave Born approximation calculations. Using these ANCs and proton and alpha resonance widths determined from an R-matrix fit to the data from the N-15(p,alpha)C-12 reaction, we carried out an R-matrix calculation to obtain the astrophysical factor for the N-15(p,gamma)O-16 reaction. The results indicate that the direct capture contribution was previously overestimated." . . . "Pisko\u0159, \u0160t\u011Bp\u00E1n" . . . "[B5AD391DE155]" . "8"^^ . . "382504" . "Vincour, Ji\u0159\u00ED" . "New astrophysical S factor for the N-15(p,gamma)O-16 reaction via the asymptotic normalization coefficient (ANC) method"@en . "The N-15(p,gamma)O-16 reaction provides a path from the CN cycle to the CNO bi-cycle and CNO tri-cycle. The measured astrophysical factor for this reaction is dominated by resonant capture through two strong J(pi) = 1(-) resonances at E-R = 312 and 962 keV and direct capture to the ground state. Asymptotic normalization coefficients (ANCs) for the ground and seven excited states in O-16 were extracted from the comparison of experimental differential cross sections for the N-15(He-3,d)O-16 reaction with distorted-wave Born approximation calculations. Using these ANCs and proton and alpha resonance widths determined from an R-matrix fit to the data from the N-15(p,alpha)C-12 reaction, we carried out an R-matrix calculation to obtain the astrophysical factor for the N-15(p,gamma)O-16 reaction. The results indicate that the direct capture contribution was previously overestimated."@en . "ANC"@en . "New astrophysical S factor for the N-15(p,gamma)O-16 reaction via the asymptotic normalization coefficient (ANC) method" . "20"^^ . . . "La Cognata, M." .