8–12 Jul 2019
University of Milano-Bicocca UNIMIB
Europe/Rome timezone

O5.204 Nonlinear dynamics of plasma grating in a static ponderomotive potential

12 Jul 2019, 12:25
15m
Aula U6-06, Building U6 (University of Milano-Bicocca UNIMIB)

Aula U6-06, Building U6

University of Milano-Bicocca UNIMIB

Piazza dell’Ateneo Nuovo, 1 20126 Milan (Italy)
BPIF BPIF

Speaker

H. Peng (EPS 2019)

Description

See the full abstract here http://ocs.ciemat.es/EPS2019ABS/pdf/O5.204.pdf

The plasma devices can stand for much larger energy fluency than solid optical devices. Thus plasma devices become a hot topic recently, as the laser power is promoted to Petawatt order. Plasma grating is one of these appealing plasma devices. Plasma grating can act as laser polarizer and waveplate for both long, moderately intense laser[1, 2, 3] and short, superintense laser[4]. And it also can be used as photonic crystal[5]. On the surface of solid target, it is generated as plasma hologram for ultraintense laser[6]. It is also used for coupling the laser into surface plasma wave instead of solid grating[7].
The growth of the plasma grating is thought to be brought by the deepening of the ion velocity. Its collapse is also believed to be induced by the X-type breaking of the grating[8, 9]. Forslund et al. compares the momentum of ions with initial velocity distribution to the maximum possible thermal potential, to explain the X-type breaking[10].
Here in this work, we analyze the plasma grating grows in a static ponderomotive potential generated by two identical counterpropagating lasers. The details of the building and collapsing process are shown with both fluid and PIC simulation. The mechanism is discussed in details. We find good agreement between fluid and PIC simulation.

References
[1] P. Michel, et al. Phys. Rev. Lett.113, 205001 (2014)
[2] D. Turnbull et al. Phys. Rev. Lett. 116, 205001 (2016)
[3] D. Turnbull et al. Phys. Rev. Lett. 118, 015001 (2017)
[4] G. Lehmann and K. H. Spatschek, Phys. Rev. E 97, 063201 (2018)
[5] G. Lehmann and K. H. Spatschek, Phys. Rev. Lett. 116, 225002 (2016)
[6] A. Leblanc et al. Nat. Phys. 13, 440 (2017)
[7] S. MonchocÈ et al. Phys. Rev. Lett. 112, 145008 (2014)
[8] D. W. Forslund, J. M. Kindel, and E. L. Lindman, Phys. Fluids 18, 1017 (1975)
[9] A. A. Andreev et al. Phys. Plasmas 13, 053110 (2006)
[10] D. W. Forslund et al. Phys Fluids 22, 462 (1979)

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