{ "id": "0909.4819", "version": "v2", "published": "2009-09-25T23:40:41.000Z", "updated": "2009-09-30T21:48:51.000Z", "title": "Transformation of the Poynting flux into the kinetic energy in relativistic jets", "authors": [ "Y. E. Lyubarsky" ], "comment": "Submitted to MNRAS Minor changes in the Conclusions", "categories": [ "astro-ph.HE" ], "abstract": "The acceleration of relativistic jets from the Poynting to the matter dominated stage is considered. The are generally two collimation regimes, which we call equilibrium and non-equilibrium, correspondingly. In the first regime, the jet is efficiently accelerated till the equipartition between the kinetic and electro-magnetic energy. We show that after the equilibrium jet ceases to be Poynting dominated, the ratio of the electro-magnetic to the kinetic energy decreases only logarithmically so that such jets become truly matter dominated only at extremely large distances. Non-equilibrium jets remain generally Poynting dominated till the logarithmically large distances. In the only case when a non-equilibrium jet is accelerated till the equipartition level, we found that the flow is not continued to the infinity but is focused towards the axis at a finite distance from the origin.", "revisions": [ { "version": "v2", "updated": "2009-09-30T21:48:51.000Z" } ], "analyses": { "keywords": [ "relativistic jets", "poynting flux", "large distances", "transformation", "kinetic energy decreases" ], "tags": [ "journal article" ], "publication": { "doi": "10.1111/j.1365-2966.2009.15877.x", "journal": "Monthly Notices of the Royal Astronomical Society", "year": 2010, "month": "Feb", "volume": 402, "number": 1, "pages": 353 }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 832309, "adsabs": "2010MNRAS.402..353L" } } }