{ "id": "1203.0296", "version": "v2", "published": "2012-03-01T20:59:59.000Z", "updated": "2012-05-19T03:48:21.000Z", "title": "The survival of nuclei in jets associated with core-collapse supernovae", "authors": [ "Shunsaku Horiuchi", "Kohta Murase", "Kunihito Ioka", "Peter Meszaros" ], "comment": "v2 (16 pages, 7 figures, 1 table) matches published version (extended discussions, table added, conclusions unchanged)", "journal": "Astrophys.J.753:69,2012", "doi": "10.1088/0004-637X/753/1/69", "categories": [ "astro-ph.HE", "astro-ph.SR" ], "abstract": "Heavy nuclei such as nickel-56 are synthesized in a wide range of core-collapse supernovae (CCSN), including energetic supernovae associated with gamma-ray bursts (GRBs). Recent studies suggest that jet-like outflows are a common feature of CCSN. These outflows may entrain synthesized nuclei at launch or during propagation, and provide interesting multi-messenger signals including heavy ultra-high energy cosmic rays. Here, we investigate the destruction processes of nuclei during crossing from the stellar material into the jet material via a cocoon, and during propagation after being successfully loaded into the jet. We find that nuclei can survive for a range of jet parameters because collisional cooling is faster than spallation. While canonical high-luminosity GRB jets may contain nuclei, magnetic dominated models or low-luminosity jets with small bulk Lorentz factors are more favorable for having a more significant heavy nuclei component.", "revisions": [ { "version": "v2", "updated": "2012-05-19T03:48:21.000Z" } ], "analyses": { "keywords": [ "core-collapse supernovae", "heavy ultra-high energy cosmic rays", "small bulk lorentz factors", "significant heavy nuclei component" ], "tags": [ "journal article" ], "publication": { "journal": "The Astrophysical Journal", "year": 2012, "month": "Jul", "volume": 753, "number": 1, "pages": 69 }, "note": { "typesetting": "TeX", "pages": 16, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1091247, "adsabs": "2012ApJ...753...69H" } } }