Surfatron acceleration of the high energy protons in the relativistic jets

Abstract

This paper describes the acceleration of high energies protons captured by electrostatic waves in the frame of jet arising in the area of instability of relativistic jet, where spiral structures are excited. The wave has a spatially heterogeneous structure of $\exp (i{k}_{\parallel }z+i{m}_{\varphi }\varphi )$. Protons can be captured in potential wells created by spiral waves, and thereby experience acceleration with a mechanism known as surfatron acceleration. Expressions of the maximum energy ($E_p\simeq 10^{19}eV$) and the energy spectrum from jet parameters are obtained.

arXiv comment7 pages, 3 figures, regular paper

References in corpus (10)

• Neutrino emission from the direction of the blazar TXS 0506+056 prior to the IceCube-170922A alert
• Relativistic Jets in Active Galactic Nuclei
• The Nature of SS433 and the Ultraluminous X-ray Sources
• Observational evidence for the origin of high-energy neutrinos in parsec-scale nuclei of radio-bright active galaxies
• Bethe-Heitler emission in BL Lacs: filling the gap between X-rays and $\gamma$-rays
• Reading M87's DNA: A Double Helix revealing a large scale Helical Magnetic Field
• The inner jet of radio galaxy NGC 315 as observed with Chandra and the VLA
• MAGIC observations of the giant radio galaxy M87 in a low-emission state between 2005 and 2007
• Acceleration of high energy protons in AGN relativistic jets
• Centrifugal acceleration of protons by a supermassive black hole