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Astrophysics > High Energy Astrophysical Phenomena

arXiv:1601.02423 (astro-ph)
[Submitted on 11 Jan 2016]

Title:Classical and relativistic flux of energy conservation in astrophysical jets

Authors:L. Zaninetti
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Abstract:The conservation of the energy flux in turbulent jets which propagate in the intergalactic medium (IGM) allows deducing the law of motion in the classical and relativistic cases. Three types of IGM are considered: constant density, hyperbolic and inverse power law decrease of density. An analytical law for the evolution of the magnetic field along the radio-jets is deduced using a linear relation between the magnetic pressure and the rest density. Astrophysical applications are made to the centerline intensity of synchrotron emission in NGC315 and to the magnetic field of 3C273.
Comments: 17 pages and 11 figures. arXiv admin note: text overlap with arXiv:1508.00360
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE)
Cite as: arXiv:1601.02423 [astro-ph.HE]
  (or arXiv:1601.02423v1 [astro-ph.HE] for this version)
  https://doi.org/10.48550/arXiv.1601.02423
Journal reference: Journal of High Energy Physics, Gravitation and Cosmology, (2016), 2, 41-56
Related DOI: https://doi.org/10.4236/jhepgc.2016.21005

Submission history

From: Lorenzo Zaninetti [view email]
[v1] Mon, 11 Jan 2016 12:48:25 UTC (107 KB)
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