2018 Impact factor 2.481
Hadrons and Nuclei
Eur. Phys. J. A 15, 69-73 (2002)
DOI: 10.1140/epja/i2001-10228-6

Asymptotic normalization coefficients in nuclear astrophysics and structure

C.A. Gagliardi1, A. Azhari1, V. Burjan2, F. Carstoiu3, V. Kroha2, A.M. Mukhamedzhanov1, A. Sattarov1, X. Tang1, L. Trache1 and R.E. Tribble1

1  Cyclotron Institute, Texas A&M University, College Station, TX 77843, USA
2  Institute for Nuclear Physics, Czech Academy of Sciences, Prague-Rez, Czech Republic
3  Institute for Atomic Physics, Bucharest, Romania

cggroup@comp.tamu.edu

(Received: 21 March 2002 / Published online: 31 October 2002)

Abstract
The asymptotic normalization coefficient (ANC) for a nuclear system specifies the normalization of the tail of the nuclear overlap function. ANCs may be determined experimentally by measuring peripheral nuclear reactions. They may be used to calculate the astrophysical S-factors for radiative capture reactions at stellar energies and to determine the halo structure of loosely bound nuclei. A brief introduction to ANCs is given and applications to the 7Be( $p,\gamma$) 8B and 11C( $p,\gamma$) 12N reactions and the halo structure of 8B are described.

PACS
26.30.+k - Nucleosynthesis in novae, supernovae and other explosive environments.
26.20.+f - Hydrostatic stellar nucleosynthesis.
25.60.Je - Transfer reactions.
25.60.Gc - Breakup and momentum distributions.

© Società Italiana di Fisica, Springer-Verlag 2002