Indirect methods in nuclear astrophysics
arXiv:1511.08859 · doi:10.1088/1742-6596/703/1/012007
Abstract
We discuss recent developments in indirect methods used in nuclear astrophysics to determine the capture cross sections and subsequent rates of various stellar burning processes, when it is difficult to perform the corresponding direct measurements. We discuss in brief, the basic concepts of Asymptotic Normalization Coefficients, the Trojan Horse Method, the Coulomb Dissociation Method, (d,p), and charge-exchange reactions.
9 pages, three figures, Proceedings of the Eighth European Summer school on Experimental Nuclear Astrophysics, 2015, edited by C. Spitaleri, L. Lamia and R.G. Pizzone
Cited by in corpus (5)
- Astronuclear Physics: a Tale of the Atomic Nuclei in the Skies
- Structural effects of Na in the Na(n,Na radiative capture reaction
- Sensitivity of transfer cross sections to the bound-state wave functions
- New determination of proton spectroscopic factors and reduced widths for Be states in the MeV excitation energy region via the study of the Li(He,d)Be transfer reaction at E MeV
- Investigating the rate of Be(n,)Be radiative capture reaction within the FRDWBA framework