scholarly journals The role of the Weibel instability at the reconnection jet front in relativistic pair plasma reconnection

2008 ◽  
Vol 15 (2) ◽  
pp. 022101 ◽  
Author(s):  
S. Zenitani ◽  
M. Hesse
Keyword(s):  
Weibel Instability ◽  
Pair Plasma ◽  
Relativistic Pair

scholarly journals The Role of the Guide Field in Relativistic Pair Plasma Reconnection

2008 ◽  
Vol 677 (1) ◽  
pp. 530-544 ◽  
Author(s):  
S. Zenitani ◽  
M. Hoshino
Keyword(s):  
Pair Plasma ◽  
Guide Field ◽  
Relativistic Pair

scholarly journals A Study of Gamma Spectral Break in AGN

1994 ◽  
Vol 159 ◽  
pp. 347-347
Author(s):  
A. Marcowith ◽  
G. Henri ◽  
G. Pelletier
Keyword(s):  
Pair Production ◽  
Flow Model ◽  
Photon Absorption ◽  
Compact Region ◽  
Pair Plasma ◽  
Relativistic Jet ◽  
Spectral Break ◽  
Superluminal Motion ◽  
Γ Rays ◽  
Relativistic Pair

Since its launch, CGRO has detected more than 20 γ-ray emitting AGN, most of them associated with powerful, radio-loud, flat-spectrum objects, exhibiting VLBI superluminal motions. In the case of 3C279, the huge value of the apparent luminosity (∼ 1048erg.s−1) and the variability time-scale of a few days (Hartmann et al., 1992) gives a very large compacity lapp ≃ 200, that is, the medium should be completely thick to γ-rays. This contradiction can be explained if the γ-rays originate from a relativistic jet pointing at a small angle with respect to the line of sight (Maraschi et al., 1992). However, the still large value of compacity suggests the existence of an inner, more compact region where pair production can take place efficiently (Henri et al., 1993). This supports the so-called “two-flow” model, where the superluminal motion is attributed to the expansion of a relativistic pair plasma heated by a MHD jet from an accretion disk (Sol et al., 1989). Hence we propose to interpret the spectral break observed in many objects around a few MeV (Lichti et al., 1993) by an opacity effect due to photon-photon absorption by pair production.

scholarly journals Quantum-electrodynamical birefringence vanishing in a thermal relativistic pair plasma

2015 ◽  
Vol 5 (1) ◽  
Author(s):  
Y. S. Huang
Keyword(s):  
Pair Plasma ◽  
Relativistic Pair

Bremsstrahlung radiation from a non-relativistic pair plasma

2008 ◽  
Vol 50 (12) ◽  
pp. 125004 ◽  
Author(s):  
Liang Guo ◽  
Jian Zheng ◽  
Bin Zhao ◽  
Ding Li
Keyword(s):  
Bremsstrahlung Radiation ◽  
Pair Plasma ◽  
Relativistic Pair

Radio Pulses through a Magnetized Relativistic Pair Plasma Flow

2002 ◽  
Vol 572 (1) ◽  
pp. L91-L94 ◽  
Author(s):  
Yu-Qing Lou
Keyword(s):  
Plasma Flow ◽  
Pair Plasma ◽  
Relativistic Pair

scholarly journals BEAMING AND RAPID VARIABILITY OF HIGH-ENERGY RADIATION FROM RELATIVISTIC PAIR PLASMA RECONNECTION

2012 ◽  
Vol 754 (2) ◽  
pp. L33 ◽  
Author(s):  
B. Cerutti ◽  
G. R. Werner ◽  
D. A. Uzdensky ◽  
M. C. Begelman
Keyword(s):  
High Energy ◽  
Rapid Variability ◽  
High Energy Radiation ◽  
Energy Radiation ◽  
Pair Plasma ◽  
Relativistic Pair

scholarly journals Damped Bernstein modes in a weakly relativistic pair plasma

2005 ◽  
Vol 72 (3) ◽  
Author(s):  
E. W. Laing ◽  
D. A. Diver
Keyword(s):  
Pair Plasma ◽  
Relativistic Pair

scholarly journals Self‐Regulation of the Reconnecting Current Layer in Relativistic Pair Plasma Reconnection

2008 ◽  
Vol 684 (2) ◽  
pp. 1477-1485 ◽  
Author(s):  
S. Zenitani ◽  
M. Hesse
Keyword(s):  
Self Regulation ◽  
Current Layer ◽  
Pair Plasma ◽  
Relativistic Pair
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