Share Email Print
cover

Proceedings Paper

Modelling the effect of the radiation reaction force on the acceleration of ultra-thin foils
Format Member Price Non-Member Price
PDF $14.40 $18.00

Paper Abstract

An investigation of the effects of the radiation reaction force on radiation pressure acceleration is presented. Through 1D(3V) PIC code simulations, it is found that radiation reaction causes a decrease in the target velocity during the interaction of an ultra-intense laser pulse with a solid density thin foil of varying thickness. This change in the target velocity can be related to the loss of backwards-directed electrons due to cooling and reflection in the laser field. The loss of this electron population changes the distribution of the emitted synchrotron radiation. We demonstrate that it is the emission of radiation which leads to the observed decrease in target velocity. Through a modification to the light sail equation of motion (which is used to describe radiation pressure acceleration in thin foils), which accounts for the conversion of laser energy to synchrotron radiation, we can describe this change in target velocity. This model can be tested in future experiments with ultra-high intensity lasers, and will lead to a better understanding of the process of relativistically induced transparency in the new intensity regime.

Paper Details

Date Published: 17 May 2017
PDF: 10 pages
Proc. SPIE 10241, Research Using Extreme Light: Entering New Frontiers with Petawatt-Class Lasers III, 102410V (17 May 2017); doi: 10.1117/12.2267424
Show Author Affiliations
M. J. Duff, Univ. of Strathclyde (United Kingdom)
R. Capdessus, Univ. of Strathclyde (United Kingdom)
M. King, Univ. of Strathclyde (United Kingdom)
D. Del Sorbo, Univ. of York (United Kingdom)
C. P. Ridgers, Univ. of York (United Kingdom)
P. McKenna, Univ. of Strathclyde (United Kingdom)


Published in SPIE Proceedings Vol. 10241:
Research Using Extreme Light: Entering New Frontiers with Petawatt-Class Lasers III
Georg Korn; Luis O. Silva, Editor(s)

© SPIE. Terms of Use
Back to Top