The consequence of jet interacting with a warped disc
S. F. Zou, B. P. Gong

TL;DR
This paper presents a novel analogy between jet interactions with warped accretion discs in active galactic nuclei and a sprinkler mechanism, explaining broad-line region features and angular momentum dissipation.
Contribution
It introduces a new conceptual model linking jet-disc interactions to observed AGN phenomena and addresses the angular momentum problem in accretion disc theory.
Findings
Explains broad-line region features via jet-baryon collisions.
Provides a natural mechanism for angular momentum dissipation.
Suggests a new analogy for jet-disc interactions in AGNs.
Abstract
The sprinkler pivots on a bearing on top of its threaded attachment nut. It is driven in a circular motion by a spring-loaded arm pushed back by the water stream which returns to "impact" the stream. The water stream can thus rotate around a fix axis. Analogously in our universe, the outflow or jet formed by the relativistic plasma corresponds to the water stream of a sprinkler; and the baryons in the tilted outer accretion disc or torus play the role of "impact arm". Then the jet aligning with the inner parts of a warped disc can directly "touch" the outer region of the disc. The resultant collision between such rapid leptons and slow baryons automatically accounts for the main features of broad-line region of active galactic nuclei. Moreover, it naturally provides a channel of dissipating the angular momentum of an accretion disc, which has long been a problem in theory of accretion…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsFluid Dynamics and Turbulent Flows · Advanced Numerical Analysis Techniques · Computational Fluid Dynamics and Aerodynamics
