Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/24715
Title: | Shell and explosive hydrogen burning. Nuclear reaction rates for hydrogen burning in RGB, AGB and Novae | Authors: | Boeltzig, A. Bruno, C. G. Cavanna, F. CRISTALLO, Sergio Davinson, T. Depalo, R. deBoer, R. J. Di Leva, A. Ferraro, F. Imbriani, G. Marigo, P. Terrasi, F. Wiescher, M. |
Issue Date: | 2016 | Journal: | THE EUROPEAN PHYSICAL JOURNAL. A, HADRONS AND NUCLEI | Number: | 52 | Issue: | 4 | First Page: | 75 | Abstract: | The nucleosynthesis of light elements, from helium up to silicon, mainly occurs in Red Giant and Asymptotic Giant Branch stars and Novae. The relative abundances of the synthesized nuclides critically depend on the rates of the nuclear processes involved, often through non-trivial reaction chains, combined with complex mixing mechanisms. In this paper, we summarize the contributions made by LUNA experiments in furthering our understanding of nuclear reaction rates necessary for modeling nucleosynthesis in AGB stars and Novae explosions. | URI: | http://hdl.handle.net/20.500.12386/24715 | URL: | https://link.springer.com/article/10.1140%2Fepja%2Fi2016-16075-4 | ISSN: | 1434-6001 | DOI: | 10.1140/epja/i2016-16075-4 | Bibcode ADS: | 2016EPJA...52...75B | Fulltext: | open |
Appears in Collections: | 1.01 Articoli in rivista |
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File | Description | Size | Format | |
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1611.06244.pdf | postprint | 888.09 kB | Adobe PDF | View/Open |
Boeltzig_2016_EPJ_A_52_75.pdf | [administrators only] | 710.09 kB | Adobe PDF |
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