scholarly journals Confinement of relativistic electrons in a magnetic mirror en route to a magnetized relativistic pair plasma

2021 ◽  
Vol 28 (9) ◽  
pp. 092508
Author(s):  
J. von der Linden ◽  
G. Fiksel ◽  
J. Peebles ◽  
M. R. Edwards ◽  
L. Willingale ◽  
...  
Keyword(s):  
Magnetic Mirror ◽  
Relativistic Electrons ◽  
Pair Plasma ◽  
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

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 Do Fluid Waves Propagate in Mildly Relativistic Thermal Pair Plasmas?

1994 ◽  
Vol 159 ◽  
pp. 357-357
Author(s):  
P. Pietrini ◽  
J.H. Krolik
Keyword(s):  
Linear Response ◽  
Plasma System ◽  
Pair Plasma ◽  
Central Regions ◽  
Relativistic Pair

Relativistic pair plasmas are implicated in the physics of the central regions of AGNs, and the observed variability of these sources can be related to the dynamics and changes in structure of these plasmas. To this respect a study of the behaviour of waves to which the pair plasma reacts as a fluid is quite relevant. We analyze the linear response to perturbations of a simple thermal mildly relativistic pair plasma system.

Ohm’s law for a relativistic pair plasma

1993 ◽  
Vol 71 (21) ◽  
pp. 3481-3484 ◽  
Author(s):  
Eric G. Blackman ◽  
George B. Field
Keyword(s):  
Ohm’S Law ◽  
Pair Plasma ◽  
Ohm's Law ◽  
Relativistic Pair
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