{ "id": "1008.0429", "version": "v1", "published": "2010-08-03T00:33:44.000Z", "updated": "2010-08-03T00:33:44.000Z", "title": "Diffusive Shock Acceleration in Test-Particle Regime", "authors": [ "Hyesung Kang", "Dongsu Ryu" ], "comment": "17 pages, 5 figures, to appear in ApJ", "categories": [ "astro-ph.HE" ], "abstract": "We examine the test-particle solution for diffusive shock acceleration, based on simple models for thermal leakage injection and Alfv'enic drift. The critical injection rate, \\xi_c, above which the cosmic ray (CR) pressure becomes dynamically significant, depends mainly on the sonic shock Mach number, M, and preshock gas temperature, T_1. In the hot-phase interstellar medium (ISM) and intracluster medium, \\xi_c < 10^{-3} for shocks with M < 5, while \\xi_c ~ 10^{-4}(T_1/10^6 K)^{1/2} for shocks with M > 10. For T_1=10^6 K, for example, the test-particle solution would be valid if the injection momentum, p_{inj} > 3.8 p_{th}. This leads to the postshock CR pressure less than 10% of the shock ram pressure. If the Alfv'en speed is comparable to the sound speed in the preshock flow, as in the hot-phase ISM, the power-law slope of CR spectrum can be significantly softer than the canonical test-particle slope. Then the CR spectrum at the shock can be approximated by the revised test-particle power-law with an exponential cutoff at the highest accelerated momentum, p_{max}(t). An analytic form of the exponential cutoff is also suggested.", "revisions": [ { "version": "v1", "updated": "2010-08-03T00:33:44.000Z" } ], "analyses": { "keywords": [ "diffusive shock acceleration", "test-particle regime", "test-particle solution", "exponential cutoff", "cr spectrum" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/0004-637X/721/1/886", "journal": "The Astrophysical Journal", "year": 2010, "month": "Sep", "volume": 721, "number": 1, "pages": 886 }, "note": { "typesetting": "TeX", "pages": 17, "language": "en", "license": "arXiv", "status": "editable", "inspire": 864287, "adsabs": "2010ApJ...721..886K" } } }