The Evolution of Radio Loud Active Galactic Nuclei as a Function of Black Hole Spin

Abstract

Recent work on the engines of active galactic nuclei jets suggests their power depends strongly and perhaps counter-intuitively on black hole spin. We explore the consequences of this on the radio-loud population of active galactic nuclei and find that the time evolution of the most powerful radio galaxies and radio-loud quasars fits into a picture in which black hole spin varies from retrograde to prograde with respect to the accreting material. Unlike the current view, according to which jet powers decrease in tandem with a global downsizing effect, we argue for a drop in jet power resulting directly from the paucity of retrograde accretion systems at lower redshift $z$ caused by a continuous history of accretion dating back to higher $z$. In addition, the model provides simple interpretations for the basic spectral features differentiating radio-loud and radio-quiet objects, such as the presence or absence of disk reflection, broadened iron lines and signatures of disk winds. We also briefly describe our models' interpretation of microquasar state transitions. We highlight our result that the most radio-loud and most radio-quiet objects both harbor highly spinning black holes but in retrograde and prograde configurations, respectively.

MNRAS accepted

References in corpus (25)

• Black Hole Spin and the Radio Loud/Quiet Dichotomy of Active Galactic Nuclei
• Constraining Black Hole Spin Via X-ray Spectroscopy
• Hot and cold gas accretion and feedback in radio-loud active galaxies
• Stability of Relativistic Jets from Rotating, Accreting Black Holes via Fully Three-Dimensional Magnetohydrodynamic Simulations
• Evidence for powerful AGN winds at high redshift: Dynamics of galactic outflows in radio galaxies during the "Quasar Era"
• The Evolution of Black Hole Mass and Spin in Active Galactic Nuclei
• Broad iron L-line and X-ray reverberation in 1H0707-495
• The X-ray nuclei of intermediate-redshift radio sources
• Black-Hole Spin and Galactic Morphology
• Spitzer Reveals Hidden Quasar Nuclei in Some Powerful FR II Radio Galaxies
• Disk-Jet Coupling in Black Hole Accretion Systems I: General Relativistic Magnetohydrodynamical Models
• Chandra and XMM-Newton Observations of the Nucleus of Centaurus A
• The radio AGN population dichotomy: Green valley Seyferts versus red sequence low-excitation AGN
• Physical Properties of Very Powerful FRII Radio Galaxies
• Models for jet power in elliptical galaxies: A case for rapidly spinning black holes
• Trapping of magnetic flux by the plunge region of a black hole accretion disk
• The spin dependence of the Blandford-Znajek effect
• Maximum Spin of Black Holes Driving Jets
• Structure of the Accretion Flow in Broad-Line Radio Galaxies: The Case of 3C390.3
• The prevalence of FRI radio quasars
• Chandra detection of a parsec scale wind in the Broad Line Radio Galaxy 3C 382
• Bounds on Black Hole Spins
• Towards a New Standard Model for Black Hole Accretion
• Suzaku Observations of the Black Hole H1743-322 in Outburst
• Signatures of black hole spin in galaxy evolution

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