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Preprint . 2010
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Asymptotic theory of relativistic, magnetized jets

descriptionPublicationkeyboard_double_arrow_right Article , Preprint 05 Jan 2011Embargo end date: 01 Jan 2010 English Publisher:American Physical Society (APS)Journal:Physical Review E, volume 83 (issn: 1539-3755, eissn: 1550-2376, Copyright policy )
Authors: Lyubarsky, Yuri;

doi: 10.1103/physreve.83.016302 , 10.48550/arxiv.1012.2517

pmid: 21405769

arXiv: 1012.2517

Asymptotic theory of relativistic, magnetized jets

Abstract

The structure of a relativistically hot, strongly magnetized jet is investigated at large distances from the source. Asymptotic equations are derived describing collimation and acceleration of the externally confined jet. Conditions are found for the transformation of the thermal energy into the fluid kinetic energy or into the Poynting flux. Simple scalings are presented for the jet collimation angle and Lorentz factors.

To appear in Phys.RevE

Related Organizations
Keywords

High Energy Astrophysical Phenomena (astro-ph.HE), FOS: Physical sciences, Astrophysics - High Energy Astrophysical Phenomena

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    influence
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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
15
Top 10%
Average
Top 10%
Green
bronze