We present an investigation of the electromagnetic instabilities which are triggered when an ultra relativistic electron beam passes through a plasma. The linear growth rate is computed for every direction of propagation of the unstable modes, and temperatures are modelled using simple waterbag distribution functions. The ultra relativistic unstable spectrum is located around a very narrow band centered on a critical angle whose value is given analytically. The growth rate of modes propagating in this direction decreases like $k^{-1/3}$
International audienceAn electron or electron-positron beam streaming through a plasma is notoriousl...
International audienceAn electron or electron-positron beam streaming through a plasma is notoriousl...
International audienceAn electron or electron-positron beam streaming through a plasma is notoriousl...
We present an investigation of the electromagnetic instabilities which are trig gered when an ultra ...
We study the linear instabilities experienced by a relativistic electron beam passing through a plas...
We study the linear instabilities experienced by a relativistic electron beam passing through a plas...
The interest in relativistic beam-plasma instabilities has been greatly rejuvenated over the past tw...
The annihilation of TeV photons from extragalactic TeV sources and the extragalactic background ligh...
The linearized, relativistic Vlasov equations are analyzed for the stability of flute‐like modes in ...
International audienceRecent work on Fermi acceleration at ultra-relativistic shock waves has demons...
International audienceRecent work on Fermi acceleration at ultra-relativistic shock waves has demons...
An electromagnetic wave is expected to propagate through an overdense plasma, provided that its ampl...
An electromagnetic wave is expected to propagate through an overdense plasma, provided that its ampl...
International audienceAn electron or electron-positron beam streaming through a plasma is notoriousl...
Axisymmetric radial modes of fast electron beams propagating through dense background plasmas with a...
International audienceAn electron or electron-positron beam streaming through a plasma is notoriousl...
International audienceAn electron or electron-positron beam streaming through a plasma is notoriousl...
International audienceAn electron or electron-positron beam streaming through a plasma is notoriousl...
We present an investigation of the electromagnetic instabilities which are trig gered when an ultra ...
We study the linear instabilities experienced by a relativistic electron beam passing through a plas...
We study the linear instabilities experienced by a relativistic electron beam passing through a plas...
The interest in relativistic beam-plasma instabilities has been greatly rejuvenated over the past tw...
The annihilation of TeV photons from extragalactic TeV sources and the extragalactic background ligh...
The linearized, relativistic Vlasov equations are analyzed for the stability of flute‐like modes in ...
International audienceRecent work on Fermi acceleration at ultra-relativistic shock waves has demons...
International audienceRecent work on Fermi acceleration at ultra-relativistic shock waves has demons...
An electromagnetic wave is expected to propagate through an overdense plasma, provided that its ampl...
An electromagnetic wave is expected to propagate through an overdense plasma, provided that its ampl...
International audienceAn electron or electron-positron beam streaming through a plasma is notoriousl...
Axisymmetric radial modes of fast electron beams propagating through dense background plasmas with a...
International audienceAn electron or electron-positron beam streaming through a plasma is notoriousl...
International audienceAn electron or electron-positron beam streaming through a plasma is notoriousl...
International audienceAn electron or electron-positron beam streaming through a plasma is notoriousl...