Speaker
Description
Jets are ubiquitously in association with different celestial objects. However, most of previous theoretical studies of them rely on numerical calculations, not being able to provide a more convenient way for understanding rather abundant observational results. Now we have obtained a general analytical solution for describing a magnetically dominated jet, through separating the jet “core equation” (which maintains the radial dynamic equilibrium) into rotating and non-rotating terms, finding that each of the two-term equations can be solved analytically, and the two solutions match each other very well. The analytical model based on this solution can explain the main results of jet observations and numerical simulations, such as jet shape configuration, acceleration profile (from non-relativistic to relativistic), and polarization pattern etc. Furthermore, the solution is applicable to, e.g., limb-brightening (a hollow jet), periodical variability (a helical jet), and "complex" proper motion pattern (a stratified jet) etc. I this talk, I will present the details of the theory, examples of comparing with observations, and a variety of predictions (Ref. Chen & Zhang, 2021, ApJ, 906, 105).
Keywords
Relativistic jets, Magnetic fields, Gamma-ray bursts, Active galactic nuclei, Charged black holes, Gamma-rays, Cosmic rays, Pulsars, Neutron stars
| Subcategory | Theoretical Results |
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