2015
DOI: 10.1017/s0022377815000513
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Radiation reaction induced non-monotonic features in runaway electron distributions

Abstract: Runaway electrons, which are generated in a plasma where the induced electric field exceeds a certain critical value, can reach very high energies in the MeV range. For such energetic electrons, radiative losses will contribute significantly to the momentum space dynamics. Under certain conditions, due to radiative momentum losses, a non-monotonic feature -a "bump" -can form in the runaway electron tail, creating a potential for bump-on-tail-type instabilities to arise. Here we study the conditions for the exi… Show more

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Cited by 25 publications
(46 citation statements)
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“…Both radiative energy loss channels can therefore be significant at densities characteristic of disruptions and are included in this paper. The synchrotron radiation reaction force is given by [28,29]…”
Section: Radiation Lossesmentioning
confidence: 99%
“…Both radiative energy loss channels can therefore be significant at densities characteristic of disruptions and are included in this paper. The synchrotron radiation reaction force is given by [28,29]…”
Section: Radiation Lossesmentioning
confidence: 99%
“…Further work highlighted the important role of synchrotron damping in elevating the threshold electric field above E C [7,8], and several experiments have since yielded evidence of the elevated threshold [9][10][11][12]. These observations motivated the development of a rigorous analytical theory [13] and computational tools [14][15][16][17][18][19] that clarified the importance of the effects of pitch-angle scattering and synchrotron damping. Alongside quantifying the enhancement of the threshold field, these works predict phase-space circulation around an attractor resulting in a pileup of REs at specific energies potentially resulting in nonmonotonic features in the RE distribution function (f e ).…”
mentioning
confidence: 99%
“…Inclusion of synchrotron radiation losses associated with the gyromotion of electrons in a straight magnetic field has been shown to be an important energy-loss mechanism [17][18][19][20][21]. Figure 1(b) shows that, in conjunction with bremsstrahlung losses, synchrotron losses (modeled as in [17]) shift the distribution towards lower energies but does not change its qualitative features. The difference between the Boltzmann and mean-force models is reduced in such cases, as the extent of the distribution when full bremsstrahlung effects are included is reduced by the synchrotron effect.…”
Section: Numerical Resultsmentioning
confidence: 98%
“…The difference between the Boltzmann and mean-force models is reduced in such cases, as the extent of the distribution when full bremsstrahlung effects are included is reduced by the synchrotron effect. When bremsstrahlung losses are ignored, and synchrotron emission alone is responsible for the energy loss by radiation, a non-monotonic runaway tail can also form (solutions to this problem have been characterized in [17,20]). However, for the present values of density, magnetic and electric fields this occurs at the significantly higher momentum [6,20] .…”
Section: Numerical Resultsmentioning
confidence: 99%