Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1085..475t&link_type=abstract
HIGH ENERGY GAMMA-RAY ASTRONOMY: Proceedings of the 4th International Meeting on High Energy Gamma-Ray Astronomy. AIP Conferenc
Astronomy and Astrophysics
Astronomy
1
Particle Acceleration, Quasars, Gamma-Ray Sources, Gamma-Ray Bursts
Scientific paper
We take the time constraints obtained from recent observations of rapid TeV variability of minute-scale flares in TeV Blazars, and combine them with the time-scale estimates of different particle acceleration mechanisms. We compare the processes and estimate their suitability in producing sufficiently high-energy particles in short enough time to have significance in being able to (i) energise particles to produce rapid flaring, (ii) account for gradual acceleration that could explain the energy-dependent time delays in a recent gamma-ray flare of Markarian 501. We are able to exclude the neutron-based converter mechanism and the shear acceleration as the main processes for energisation of the radiating particles, and suggest the stochastic acceleration as a promising candidate for the time delay in Mkn 501.
Duffy Peter
Tammi Joni
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