The Weibel instability is investigated theoretically and numerically under three scenarios: counterstreaming electron beams in background plasma, an electron-positron beam and an electron-proton beam in background plasma. These models occur widely in laboratory and astrophysical environments. The Weibel instability growth rates are determined numerically from the corresponding cold-fluid dispersion relations, which are confirmed with two-dimensional particle-in-cell simulations. The maximum growth rates for the counterstreaming beams in background plasma are an order of magnitude smaller than the maximum growth rates for the beams cases in the same range of density ratios and beam energies. The maximum growth rate for the electron-positron ...
Many astrophysical plasmas are prone to beam-plasma instabilities. For relativistic and dilute beams...
The dynamics of two counter-streaming electron-positron-ion unmagnetized plasma shells with zero net...
In certain plasmas, non-thermal electron distributions can produce instabilities. These instabilitie...
International audienceThe development of the Weibel instability during the expansion of a thin plasm...
Plasma (an electrified gas with atoms dissociated into positive ions and negative electrons) is ofte...
textThis thesis focuses on the propagation of charged particle beams in plasmas, and is divided into...
DoctorIn this dissertation, collisionless electromagnetic instabilities, known as Weibel instability...
The energy transportation of High-energy electrons to the compressed fuel and study of affected fact...
This paper investigates how an electrostatic Langmuir wave having large amplitude affects the Weibel...
Aims.We discuss the linear theory of the Weibel instability in a relativistic plasma driven by ultra...
Weibel electromagnetic instability has been studied analytically in relativistic plasma with high pa...
We present comprehensive two-dimensional (2D) particle-in-cell (PIC) simulations on the transport of...
Density filamentation has been observed in many beam-plasma simulations and experiments. Because cur...
A theoretical model is developed to describe the formation of microstructures due to plasma streamin...
We study collective processes for an electron beam propagating through a background plasma using sim...
Many astrophysical plasmas are prone to beam-plasma instabilities. For relativistic and dilute beams...
The dynamics of two counter-streaming electron-positron-ion unmagnetized plasma shells with zero net...
In certain plasmas, non-thermal electron distributions can produce instabilities. These instabilitie...
International audienceThe development of the Weibel instability during the expansion of a thin plasm...
Plasma (an electrified gas with atoms dissociated into positive ions and negative electrons) is ofte...
textThis thesis focuses on the propagation of charged particle beams in plasmas, and is divided into...
DoctorIn this dissertation, collisionless electromagnetic instabilities, known as Weibel instability...
The energy transportation of High-energy electrons to the compressed fuel and study of affected fact...
This paper investigates how an electrostatic Langmuir wave having large amplitude affects the Weibel...
Aims.We discuss the linear theory of the Weibel instability in a relativistic plasma driven by ultra...
Weibel electromagnetic instability has been studied analytically in relativistic plasma with high pa...
We present comprehensive two-dimensional (2D) particle-in-cell (PIC) simulations on the transport of...
Density filamentation has been observed in many beam-plasma simulations and experiments. Because cur...
A theoretical model is developed to describe the formation of microstructures due to plasma streamin...
We study collective processes for an electron beam propagating through a background plasma using sim...
Many astrophysical plasmas are prone to beam-plasma instabilities. For relativistic and dilute beams...
The dynamics of two counter-streaming electron-positron-ion unmagnetized plasma shells with zero net...
In certain plasmas, non-thermal electron distributions can produce instabilities. These instabilitie...