{ "id": "1605.03690", "version": "v1", "published": "2016-05-12T06:01:59.000Z", "updated": "2016-05-12T06:01:59.000Z", "title": "The production of proton-rich isotopes beyond iron: The $γ$ process in stars", "authors": [ "Marco Pignatari", "Kathrin Göbel", "René Reifarth", "Claudia Travaglio" ], "comment": "51 pages, 14 figures, invited review", "journal": "International Journal of Modern Physics E, Vol. 25, No. 4 (2016) 1630003", "doi": "10.1142/S0218301316300034", "categories": [ "astro-ph.SR" ], "abstract": "Beyond iron, a small fraction of the total abundances in the Solar System is made of proton-rich isotopes, the p nuclei. The clear understanding of their production is a fundamental challenge for nuclear astrophysics. The p nuclei constrain the nucleosynthesis in core-collapse and thermonuclear supernovae. The $\\gamma$ process is the most established scenario for the production of the p nuclei, which are produced via different photodisintegration paths starting on heavier nuclei. A large effort from nuclear physics is needed to access the relevant nuclear reaction rates far from the valley of stability. This review describes the production of the heavy proton-rich isotopes by the $\\gamma$ process in stars, and explores the state of the art of experimental nuclear physics to provide nuclear data for stellar nucleosynthesis.", "revisions": [ { "version": "v1", "updated": "2016-05-12T06:01:59.000Z" } ], "analyses": { "subjects": [ "26.30.-k", "97.10.Tk", "97.60.Bw" ], "keywords": [ "production", "relevant nuclear reaction rates far", "experimental nuclear physics", "heavy proton-rich isotopes", "total abundances" ], "tags": [ "review article", "journal article" ], "publication": { "publisher": "World Scientific", "journal": "International Journal of Modern Physics E", "year": 2016, "month": "Apr", "volume": 25, "number": 4, "pages": 1630003 }, "note": { "typesetting": "TeX", "pages": 51, "language": "en", "license": "arXiv", "status": "editable", "adsabs": "2016IJMPE..2530003P" } } }