Time-dependent modeling of high energy emission of TeV blazars

Details Time-dependent modeling of high energy emission of TeV blazars Time-dependent modeling of high energy emission of TeV blazars

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003newar..47..529s&link_type=abstract

New Astronomy Reviews, Volume 47, Issue 6-7, p. 529-531.

Astronomy and Astrophysics

Astronomy

2

Scientific paper

We present a self-consistent and time-dependent model in order to explain the variability behaviors of extreme or TeV-blazars. This model is based on the `Two-Flow model' involving a relativistic pair plasma beam surrounded by a classical MHD structure. Particular symbiosis between the ultra-relativistic pairs and the turbulence generated by the MHD jet may lead to a preys-predators comportment. We also consider that the pair energy distribution is not a power-law but a `pile-up' one.

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