THE COSMOLOGICAL IMPACT OF LUMINOUS TeV BLAZARS. I. IMPLICATIONS OF PLASMA INSTABILITIES FOR THE INTERGALACTIC MAGNETIC FIELD AND EXTRAGALACTIC GAMMA-RAY BACKGROUND

• Published in: The Astrophysical journal Vol. 752; no. 1; pp. 1 - 23
• Main Authors: BRODERICK, Avery E, CHANG, Philip, PFROMMER, Christoph
• Format: Journal Article
• Language: English
• Published: Bristol IOP 10-06-2012
• Subjects: ANNIHILATION; ASTRONOMY; ASTROPHYSICS; ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; BL LACERTAE OBJECTS; Blazars; COMPARATIVE EVALUATIONS; COMPTON EFFECT; COSMIC PHOTONS; DENSITY; Earth, ocean, space; ENERGY LOSSES; Exact sciences and technology; GAMMA RADIATION; Gamma rays; GEV RANGE; Instability; Inverse; LUMINOSITY; MAGNETIC FIELDS; PAIR PRODUCTION; PHOTON EMISSION; PLASMA INSTABILITY; QUASARS; RED SHIFT; RELATIVISTIC RANGE; Stability; TEV RANGE; radiation mechanisms: non-thermal; Intergalactic matter; Plasma; Red shift; Luminosity; GeV range; BL Lacertae objects; Plasma instability; Cosmic radio sources; gamma rays: general; Energetics; Quasars; plasmas; Cooling rate; Intergalactic magnetic fields; Blazar; instabilities; Extragalactic source; Radiation mechanism; Gamma radiation; Inverse Compton scattering; Two-stream instability; Energy losses; BL Lacertae objects: general; Magnetic fields; Luminosity function
• ISSN: 0004-637X; 1538-4357
• DOI: 10.1088/0004-637x/752/1/22

Inverse Compton cascades (ICCs) initiated by energetic gamma rays (E [> ~] 100 GeV) enhance the GeV emission from bright, extragalactic TeV sources. The absence of this emission from bright TeV blazars has been used to constrain the intergalactic magnetic field (IGMF), and the stringent limits placed on the unresolved extragalactic gamma-ray background (EGRB) by Fermi have been used to argue against a large number of such objects at high redshifts. However, these are predicated on the assumption that inverse Compton scattering is the primary energy-loss mechanism for the ultrarelativistic pairs produced by the annihilation of the energetic gamma rays on extragalactic background light photons. Here, we show that for sufficiently bright TeV sources (isotropic-equivalent luminosities [> ~]10 super(42) erg s super(-1)) plasma beam instabilities, specifically the "oblique" instability, present a plausible mechanism by which the energy of these pairs can be dissipated locally, heating the intergalactic medium. Since these instabilities typically grow on timescales short in comparison to the inverse Compton cooling rate, they necessarily suppress the ICCs. As a consequence, this places a severe constraint on efforts to limit the IGMF from the lack of a discernible GeV bump in TeV sources. Similarly, it considerably weakens the Fermi limits on the evolution of blazar populations. Specifically, we construct a TeV-blazar luminosity function from those objects currently observed and find that it is very well described by the quasar luminosity function at z ~ 0.1, shifted to lower luminosities and number densities, suggesting that both classes of sources are regulated by similar processes. Extending this relationship to higher redshifts, we show that the magnitude and shape of the EGRB above ~10 GeV are naturally reproduced with this particular example of a rapidly evolving TeV-blazar luminosity function.