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Properties of blazar jets defined by an economy of power

Journal Article · · Astrophysical Journal Letters
 [1]
  1. Department of Physics and Astronomy, Purdue University, West Lafayette, IN 47907 (United States)
The absolute power of a relativistic black hole jet includes the power in the magnetic field, the leptons, the hadrons, and the radiated photons. A power analysis of a relativistic radio/γ-ray blazar jet leads to bifurcated leptonic synchrotron-Compton (LSC) and leptohadronic synchrotron (LHS) solutions that minimize the total jet power. Higher Doppler factors with increasing peak synchrotron frequency are implied in the LSC model. Strong magnetic fields B{sup ′}≳100 G are found for the LHS model with variability times ≲10{sup 3} s, in accord with highly magnetized, reconnection-driven jet models. Proton synchrotron models of ≳100 GeV blazar radiation can have sub-Eddington absolute jet powers, but models of dominant GeV radiation in flat spectrum radio quasars require excessive power.
OSTI ID:
22868938
Journal Information:
Astrophysical Journal Letters, Journal Name: Astrophysical Journal Letters Journal Issue: 1 Vol. 825; ISSN 2041-8205
Country of Publication:
United States
Language:
English

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