Matches in SemOpenAlex for { <https://semopenalex.org/work/W2572057611> ?p ?o ?g. }
- W2572057611 endingPage "136" @default.
- W2572057611 startingPage "136" @default.
- W2572057611 abstract "This is the second in a series of companion papers showing that when an efficient dynamo can be maintained by accretion disks around supermassive black holes in active galactic nuclei, it can lead to the formation of a powerful, magnetically driven, and mediated helix that could explain both the observed radio jet/lobe structures and ultimately the enormous power inferred from the observed ultrahigh-energy cosmic rays. In the first paper, we showed self-consistently that minimizing viscous dissipation in the disk naturally leads to jets of maximum power with boundary conditions known to yield jets as a low-density, magnetically collimated tower, consistent with observational constraints of wire-like currents at distances far from the black hole. In this paper we show that these magnetic towers remain collimated as they grow in length at nonrelativistic velocities. Differences with relativistic jet models are explained by three-dimensional magnetic structures derived from a detailed examination of stability properties of the tower model, including a broad diffuse pinch with current profiles predicted by a detailed jet solution outside the collimated central column treated as an electric circuit. We justify our model in part by the derived jet dimensions in reasonable agreement with observations. Using these jet properties, we also discuss the implications for relativistic particle acceleration in nonrelativistically moving jets. The appendices justify the low jet densities yielding our results and speculate how to reconcile our nonrelativistic treatment with general relativistic MHD simulations." @default.
- W2572057611 created "2017-01-26" @default.
- W2572057611 creator A5005601328 @default.
- W2572057611 creator A5018603529 @default.
- W2572057611 creator A5021358807 @default.
- W2572057611 creator A5035961360 @default.
- W2572057611 creator A5067290528 @default.
- W2572057611 creator A5067580630 @default.
- W2572057611 date "2015-11-09" @default.
- W2572057611 modified "2023-09-25" @default.
- W2572057611 title "QUASI-STATIC MODEL OF MAGNETICALLY COLLIMATED JETS AND RADIO LOBES. II. JET STRUCTURE AND STABILITY" @default.
- W2572057611 cites W1829802794 @default.
- W2572057611 cites W1885275909 @default.
- W2572057611 cites W1891583834 @default.
- W2572057611 cites W1954011629 @default.
- W2572057611 cites W1963968588 @default.
- W2572057611 cites W1966102813 @default.
- W2572057611 cites W1966870157 @default.
- W2572057611 cites W1972382298 @default.
- W2572057611 cites W1972402856 @default.
- W2572057611 cites W1975944132 @default.
- W2572057611 cites W1979140081 @default.
- W2572057611 cites W1982166331 @default.
- W2572057611 cites W1985413883 @default.
- W2572057611 cites W1987200687 @default.
- W2572057611 cites W1988370772 @default.
- W2572057611 cites W1992502792 @default.
- W2572057611 cites W1992717256 @default.
- W2572057611 cites W1995724457 @default.
- W2572057611 cites W1996621510 @default.
- W2572057611 cites W1998801057 @default.
- W2572057611 cites W2002691002 @default.
- W2572057611 cites W2006108427 @default.
- W2572057611 cites W2011084739 @default.
- W2572057611 cites W2011974859 @default.
- W2572057611 cites W2013780225 @default.
- W2572057611 cites W2015741683 @default.
- W2572057611 cites W2023347320 @default.
- W2572057611 cites W2025557213 @default.
- W2572057611 cites W2027168596 @default.
- W2572057611 cites W2028998331 @default.
- W2572057611 cites W2030249860 @default.
- W2572057611 cites W2033083917 @default.
- W2572057611 cites W2035004694 @default.
- W2572057611 cites W2038613834 @default.
- W2572057611 cites W2040619705 @default.
- W2572057611 cites W2046945127 @default.
- W2572057611 cites W2053931845 @default.
- W2572057611 cites W2054218231 @default.
- W2572057611 cites W2058237260 @default.
- W2572057611 cites W2061700805 @default.
- W2572057611 cites W2063856513 @default.
- W2572057611 cites W2063986325 @default.
- W2572057611 cites W2064000978 @default.
- W2572057611 cites W2064856088 @default.
- W2572057611 cites W2066469971 @default.
- W2572057611 cites W2071724415 @default.
- W2572057611 cites W2072545981 @default.
- W2572057611 cites W2076752333 @default.
- W2572057611 cites W2085977426 @default.
- W2572057611 cites W2090432756 @default.
- W2572057611 cites W2097446146 @default.
- W2572057611 cites W2099390171 @default.
- W2572057611 cites W2101010207 @default.
- W2572057611 cites W2106444943 @default.
- W2572057611 cites W2107572729 @default.
- W2572057611 cites W2122968988 @default.
- W2572057611 cites W2133916915 @default.
- W2572057611 cites W2137771656 @default.
- W2572057611 cites W2140587776 @default.
- W2572057611 cites W2149924898 @default.
- W2572057611 cites W2156621121 @default.
- W2572057611 cites W2494455406 @default.
- W2572057611 cites W2597667062 @default.
- W2572057611 cites W2802818114 @default.
- W2572057611 cites W2985443361 @default.
- W2572057611 cites W3020898290 @default.
- W2572057611 cites W3098164397 @default.
- W2572057611 cites W3098829393 @default.
- W2572057611 cites W3099998938 @default.
- W2572057611 cites W3100647909 @default.
- W2572057611 cites W3100782618 @default.
- W2572057611 cites W3102353399 @default.
- W2572057611 cites W3102655688 @default.
- W2572057611 cites W3103632766 @default.
- W2572057611 cites W3103675869 @default.
- W2572057611 cites W3103702603 @default.
- W2572057611 cites W3103896318 @default.
- W2572057611 cites W3104181489 @default.
- W2572057611 cites W3106192069 @default.
- W2572057611 cites W3106233724 @default.
- W2572057611 cites W3106456014 @default.
- W2572057611 cites W3106467044 @default.
- W2572057611 cites W4234559081 @default.
- W2572057611 cites W4237602324 @default.
- W2572057611 cites W4238874417 @default.
- W2572057611 cites W4299527096 @default.
- W2572057611 doi "https://doi.org/10.1088/0004-637x/813/2/136" @default.