High energy photon emission from wakefields and its signatures in astrophysical Blazars

Farinella, D.*; Zhang, X.*; Lau, C.*; Taimourzadeh, S.*; Hwang, Y.*; Koga, J. K.; Ebisuzaki, Toshikazu*; Tajima, Toshiki*

Episodic eruptions of accretion disks of AGNs (and Blazars) due to the Magneto-Rotational-Instability are related to the excitation of intense Alfvn waves and their subsequently mode converted EM pulses. These intense pulses are related to the emission of bursts of rays and extreme high energy cosmic ray (EHECR) genesis in AGN and Blazars. Wakefield acceleration and pondermotive acceleration of electrons give rise to ray emissions of the above through synchrotron radiation which can undergo inverse-Compton scattering to attain high X-ray energies. We study additional emissions of rays by the betatron oscillations and QED radiative processes in the intense accelerating fields.

Language	:	English
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Meeting title	:	American Physical Society 57th Annual Meeting of the Division of Plasma Physics (DPP 2015)
Held date	:	2015/11
Location (city)	:	Savannah
Location (country)	:	U.S.A.
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Registration No. : BB20151079
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