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

P4.2010 On the role of non-equilibrium relativistic hot electron populations in Target Normal Sheath Acceleration

11 Jul 2019, 14:00
2h
Building U6 (University of Milano-Bicocca UNIMIB)

Building U6

University of Milano-Bicocca UNIMIB

Piazza dell’Ateneo Nuovo, 1 20126 Milan, Italy
BPIF Poster P4

Speaker

A. Maffini (EPS 2019)

Description

See the full abstract here:
http://ocs.ciemat.es/EPS2019ABS/pdf/P4.2010.pdf

Laser-driven ion acceleration is a long-standing topic of great appeal in the field of laserplasma interaction, both because of the rich physics at play and the foreseen applications [1]. Various laser-ion acceleration mechanisms have been identified in the literature. Among them, Target Normal Sheath Acceleration (TNSA) has emerged as the most robust and reliable one, being active in a wide range of experimental conditions, including advanced target configurations [2]. Considerable theoretical effort has been put into understanding the role played by several key parameters in TNSA experiments, as for the case of static models that feature a self-consistent electrostatic potential, which have been proven to be a simple, yet effective approximate tool to describe the physics of TNSA [3,4]. In this work, we overcome a number of severe limitations affecting such approach, by proposing a fully relativistic, self-consistent model that includes non-thermal features in the theoretical description of TNSA. By means of an analytical investigation we show how the presence of non-equilibrium features in the relativistic electron population affect the ion acceleration process. In addition, complementary 3D PIC simulations demonstrate that nonthermal processes are particularly relevant, especially in the case of advanced target configurations involving a nanostructured, near-critical plasma layer. Therefore, besides its fundamental interest, the model hereby proposed can serve as a predictive tool to design future experiments investigating enhanced TNSA scenarios.

[1] A. Macchi et al., Reviews of Modern Physics 85.2 (2013): 751.
[2] M. Passoni et al., Phys. Rev. Acc. Beams 19, 061301 (2016)
[3] M. Passoni and M. Lontano, Physical review letters 101.11 (2008): 115001.
[4] D. Bennaceur-Doumaz et al,. Jour. App. Physics 117, 043303 (2015).

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