The stimulated Raman backscatter instability that occurs when short (∼50–100 fs), intense (I≂2×1017 W/cm2) laser pulses are focused into a high density, low temperature plasma is reported on in this article. Results from linear theory, numerical differencing of the coupled mode equations, and one-dimensional particle-in-cell simulations will be discussed. It is found that the growth rate is a function of position along the pulse, and that the maximum growth rate at the peak of the pulse is reduced from the homogeneous long pulse value, γ0 by a factor of 1/√2. A criterion is obtained that predicts when the product of the pulse length and the growth rate is large enough so that the backscatter instability will heat the background electrons to a significant amount above the initial temperature. The usual hot electron component associated with this instability will also be discussed.
No takes yet. Share an insight, caveat, or question.
Wilks et al. (1995) studied this question.
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context: