{ "id": "1504.05635", "version": "v1", "published": "2015-04-22T02:34:11.000Z", "updated": "2015-04-22T02:34:11.000Z", "title": "The jets-accretion relation, mass-luminosity relation in Fermi blazars", "authors": [ "Xiaoling Yu", "Xiong Zhang", "Haojing Zhang", "Dingrong Xiong", "Bijun Li", "Yongjuan Cha", "Yongyun Chen", "Xia Huang", "Yuwei Wang" ], "comment": "14pages,8figures, has been accepted for publication in Ap&SS", "categories": [ "astro-ph.HE" ], "abstract": "A sample of 111 Fermi blazars each with a well-established radio core luminosity, broad-line luminosity, bolometric luminosity and black hole mass has been compiled from the literatures.We present a significant correlation between radio core and broad-line emission luminosities that supports a close link between accretion processes and relativistic jets. Analysis reveals a relationship of $\\rm{LogL_{BLR}\\sim(0.81\\pm0.06)LogL_{R}^{C}}$ which is consistant with theoretical predicted coefficient and supports that blazar jets are powered by energy extraction from a rapidly spinning Kerr black hole through the magnetic field provided by the accretion disk. Through studying the correlation between the intrinsic bolometric luminosity and the black hole mass, we find a relationship of $\\rm{{Log}\\frac{L_{in}}{L_{\\odot}}=(0.95\\pm0.26){Log}\\frac{M}{M_{\\odot}}+(3.53\\pm2.24)}$ which supports mass-luminosity relation for Fermi blazars derived in this work is a powerlaw relation similar to that for main-sequence stars. Finally, evolutionary sequence of blazars is discussed.", "revisions": [ { "version": "v1", "updated": "2015-04-22T02:34:11.000Z" } ], "analyses": { "keywords": [ "fermi blazars", "jets-accretion relation", "spinning kerr black hole", "black hole mass", "radio core" ], "publication": { "doi": "10.1007/s10509-015-2309-4" }, "note": { "typesetting": "TeX", "pages": 14, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1364325 } } }