Title of article
Indirect Techniques in Nuclear Astrophysics. Asymptotic Normalization Coefficient and Trojan Horse Original Research Article
Author/Authors
A.M. Mukhamedzhanov، نويسنده , , L.D. Blokhintsev، نويسنده , , S. Brown، نويسنده , , V. Burjan، نويسنده , , S. Cherubini، نويسنده , , V.Z. Goldberg، نويسنده , , M. Gulino، نويسنده , , B.F. Irgaziev، نويسنده , , E. Johnson، نويسنده , , K. Kemper، نويسنده , , V. Kroha، نويسنده , , M. La Cognata، نويسنده , , L. Lamia، نويسنده , , O. A. Momotyuk، نويسنده , , R.G. Pizzone، نويسنده , , B. Roeder، نويسنده , , G. Rogachev، نويسنده , , S. Romano، نويسنده , , C. Spitaleri، نويسنده , , R.E. Tribble، نويسنده , , et al.، نويسنده ,
Issue Information
هفته نامه با شماره پیاپی سال 2007
Pages
8
From page
321
To page
328
Abstract
We address two important indirect techniques, the asymptotic normalization coefficient (ANC) and the Trojan Horse (TH) methods. We discuss the application of the ANC technique to determine the astrophysical factor for the 13C(α, n)16O reaction which is one of the neutron generators for the s processes in AGB stars. The TH method is a unique indirect technique allowing one to measure astrophysical S factors for rearrangement reactions down to astrophysically relevant energies. We derive equations connecting the cross sections for the binary direct and resonant reactions determined from the indirect TH reactions to direct cross sections measurements.
Journal title
Nuclear physics A
Serial Year
2007
Journal title
Nuclear physics A
Record number
1204532
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