Results 1 to 10 of about 240,141 (195)
Magnetic Dissipation in Relativistic Jets [PDF]
The most promising mechanisms for producing and accelerating relativistic jets, and maintaining collimated structure of relativistic jets involve magnetohydrodynamical (MHD) processes.
Yosuke Mizuno +7 more
doaj +6 more sources
Relativistic Jets of Blazars [PDF]
To appear in New Astronomy Reviews special volume '100 Years of Astrophysical Jets' (eds. Rob Fender and Ralph Wijers).
Talvikki Hovatta, Elina Lindfors
exaly +8 more sources
Stationary relativistic jets. [PDF]
AbstractIn this paper we describe a simple numerical approach which allows to study the structure of steady-state axisymmetric relativistic jets using one-dimensional time-dependent simulations. It is based on the fact that for narrow jets with $v_{z}\approx c$ v z
Komissarov SS, Porth O, Lyutikov M.
europepmc +7 more sources
Jets from a stellar-mass black hole are as relativistic as those from supermassive black holes [PDF]
Relativistic jets from supermassive black holes in active galactic nuclei are amongst the most powerful phenomena in the universe. Similar jets from stellar-mass black holes offer a chance to study the phenomena on accessible observation time scales ...
X. Zhang +17 more
doaj +2 more sources
Particle-in-Cell Simulations of Astrophysical Relativistic Jets
Astrophysical relativistic jets in active galactic nuclei, gamma-ray bursts, and pulsars is the main key subject of study in the field of high-energy astrophysics, especially regarding the jet interaction with the interstellar or intergalactic ...
Ken-Ichi Nishikawa, Athina Meli
exaly +3 more sources
The particle-in-cell (PIC) method was developed to investigate microscopic phenomena, and with the advances in computing power, newly developed codes have been used for several fields, such as astrophysical, magnetospheric, and solar plasmas.
Ken-Ichi Nishikawa +2 more
exaly +3 more sources
Applying Relativistic Reconnection to Blazar Jets
Rapid and luminous flares of non-thermal radiation observed in blazars require an efficient mechanism of energy dissipation and particle acceleration in relativistic active galactic nuclei (AGN) jets.
Krzysztof Nalewajko
exaly +3 more sources
Quasi-periodic oscillations of GHz-band polarization in a black hole [PDF]
Relativistic jets from accreting black holes radiate non-thermal emission which is highly variable in different time scales. Previous studies on black holes of different mass scales, including supermassive and stellar-mass black holes, only report flux ...
Wei Wang +12 more
doaj +2 more sources
Microscopic Processes in Global Relativistic Jets Containing Helical Magnetic Fields
In the study of relativistic jets one of the key open questions is their interaction with the environment on the microscopic level. Here, we study the initial evolution of both electron–proton ( e − – p + ) and electron–positron ( e ± )
Ken-Ichi Nishikawa +2 more
exaly +3 more sources
GRMHD Simulations and Modeling for Jet Formation and Acceleration Region in AGNs
Relativistic jets are collimated plasma outflows with relativistic speeds. Astrophysical objects involving relativistic jets are a system comprising a compact object such as a black hole, surrounded by rotating accretion flows, with the relativistic jets
Yosuke Mizuno
doaj +1 more source

