Asymptotic normalization coefficients in nuclear astrophysics

0185733 - UJF-V 20033049 RIV NL eng J - Článek v odborném periodiku
Kroha, Václav - Azhari, A. - Bém, Pavel - Burjan, Václav - Gagliardi, C. A. - Mukhamedzhanov, A. M. - Novák, Jan - Piskoř, Štěpán - Šimečková, Eva - Tang, X. - Trache, L. - Tribble, R. E. - Vincour, Jiří
Asymptotic normalization coefficients in nuclear astrophysics.
Nuclear Physics. A. Roč. 719, - (2003), s. 119C-122C. ISSN 0375-9474. E-ISSN 1873-1554
Grant CEP: GA ČR GA202/01/0709; GA AV ČR KSK1048102
Výzkumný záměr: CEZ:AV0Z1048901
Klíčová slova: S-factor * C-13(p,gamma)N-14 * Be-9(p, gamma)B-10
Kód oboru RIV: BG - Jaderná, atomová a mol. fyzika, urychlovače
Impakt faktor: 1.761, rok: 2003

The technique of Asymptotic Normalization Coefficients (ANC) provides an effective method of indirect determination of S-factors for the synthesis in astrophysically important reactions. These coefficients can be extracted from the differential cross sections of the peripheral particle transfer reactions. Recent applications include measurements of ANC's for determining of stellar reaction rates of Be-9(p, gamma)B-10, C-13(p, gamma)N-14, C-11 (p, gamma) N-12 and N-14 (p, gamma)O-15.
Trvalý link: http://hdl.handle.net/11104/0082116