Relativistic Plasma Physics. Relativistic Hydrodynamics and Astrophysical Jets.
Akira Mizuta, Tatsuya Yamasaki
Abstract
Open-access reader
Akira Mizuta, Tatsuya Yamasaki
Abstract
Open-access reader
Relativistic flows have been observed in jets and gamma-ray bursts. Such phenomena are not fully understood. In order to study such flows, we need to consider relativistic effects. In this paper, we first explain relativistic hydrodynamic equations. Some characteristics relativistic flows are discussed, namely, the adiabatic exponent and sound speed for high temperature fluid, and shock jump conditions. Second, we show relativistic jets as an example of relativistic flows. Observations of jets and theoretical models for acceleration, collimation, and propagation of jets are given.
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Relativistic flows have been observed in jets and gamma-ray bursts. Such phenomena are not fully understood. In order to study such flows, we need to consider relativistic effects. In this paper, we first explain relativistic hydrodynamic equations. Some characteristics relativistic flows are discussed, namely, the adiabatic exponent and sound speed for high temperature fluid, and shock jump conditions. Second, we show relativistic jets as an example of relativistic flows. Observations of jets and theoretical models for acceleration, collimation, and propagation of jets are given.
Key concepts: Physics, Astrophysical jet, Adiabatic process, Relativistic particle, Relativistic speed, Acceleration, Shock wave, Relativistic beaming