2017
DOI: 10.1063/1.5002554
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Orbital angular momentum of a π-pulse emission by dense relativistic cold electron beam

Abstract: Using a quantum fluid model, a set of three paraxial coupled equations to describe the FEL instability is derived. These equations are solved numerically considering Laguerre-Gaussian modes as the initial conditions to study the transfer of orbital angular momentum (OAM) between them, which satisfies the total angular momentum conservation as matching condition. The amplification and compression of the output radiation is observed and using the separation of variables method, the set of coupled equations, whic… Show more

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Cited by 3 publications
(2 citation statements)
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“…In addition, we have shown the possibility of having a spiral phase in a plasma wave and a helical profile in its intensity. This opens the possibility of applying this technique to generate helical electron beams [16,17]. Finally, we are conscious of the limitations in the three wave interaction scheme discussed here.…”
Section: Discussionmentioning
confidence: 90%
“…In addition, we have shown the possibility of having a spiral phase in a plasma wave and a helical profile in its intensity. This opens the possibility of applying this technique to generate helical electron beams [16,17]. Finally, we are conscious of the limitations in the three wave interaction scheme discussed here.…”
Section: Discussionmentioning
confidence: 90%
“…These types of waves have the property of reduced parasitic backscattering [25], but since they do not have a beat-wave waveform, no improvement in the maximum intensity is expected. These results should also carry over to using a multifrequency plasma seed instead of a seed laser [41] or to pulses with nonzero orbital angular momentum [42].…”
Section: Discussionmentioning
confidence: 91%