{ "id": "1103.5746", "version": "v4", "published": "2011-03-29T20:00:02.000Z", "updated": "2011-09-14T13:20:10.000Z", "title": "Gamma-Ray Burst without Baryonic and Magnetic Load?", "authors": [ "Kunihito Ioka", "Yutaka Ohira", "Norita Kawanaka", "Akira Mizuta" ], "comment": "10 pages, 3 figures, final version to be published in Progress of Theoretical Physics", "journal": "Prog. Theor. Phys. 126 (2011), 555-564", "doi": "10.1143/PTP.126.555", "categories": [ "astro-ph.HE" ], "abstract": "We show that, contrary to common belief, internal shocks can arise in an accelerating radiation-dominated jet if it is confined even weakly to a converging opening angle because the acceleration declines. The radiation-dominated internal shock (RDIS) enables a very efficient yet highly nonthermal emission by Fermi-like photon acceleration, keeping the electron-positron ($e^{\\pm}$) pair photosphere and inertia up to a high Lorentz factor >1000. In gamma-ray bursts (GRBs), a weak confinement would persist beyond the progenitor star or surrounding matter because of the fast cocoon accompanying the breakout jet. The simplest model predicts few high-energy cosmic rays and neutrinos, and a correlation between the early afterglow and the GeV-TeV prompt emission. The central engine allows a less fine-tuned baryon load than previously thought, even including pure-leptonic unmagnetized outflows.", "revisions": [ { "version": "v4", "updated": "2011-09-14T13:20:10.000Z" } ], "analyses": { "keywords": [ "gamma-ray burst", "magnetic load", "internal shock", "high lorentz factor", "simplest model predicts" ], "tags": [ "journal article" ], "publication": { "journal": "Progress of Theoretical Physics", "year": 2011, "month": "Sep", "volume": 126, "number": 3, "pages": 555 }, "note": { "typesetting": "TeX", "pages": 10, "language": "en", "license": "arXiv", "status": "editable", "inspire": 894533, "adsabs": "2011PThPh.126..555I" } } }