Comparison of the evolution of Rayleigh–Taylor instability during the coasting phase of the central ignition and the double-cone ignition schemes

Author:

Lei Y. Y.12ORCID,Wu F. Y.134ORCID,Ramis R.4ORCID,Zhang J.123ORCID

Affiliation:

1. Key Laboratory for Laser Plasmas (MoE) and School of Physics and Astronomy, Shanghai Jiao Tong University 1 , Shanghai 200240, China

2. Zhiyuan College, Shanghai Jiao Tong University 2 , Shanghai 200240, China

3. IFSA Collaborative Innovation Center and DCI joint team, Shanghai Jiao Tong University 3 , Shanghai 200240, China

4. E.T.S.I. Aeronautica y del Espacio, Universidad Politecnica de Madrid 4 , Madrid 28040, Spain

Abstract

The Rayleigh–Taylor (RT) instability has been a great challenge for robust fusion ignition. In this paper, the evolution of the RT instability at the fuel inner interface during the coasting phase is investigated for the central ignition scheme [Hurricane et al., Rev Mod Phys. 95, 025005 (2023)] and the double-cone ignition (DCI) scheme [Zhang et al., Philos. Trans. R. Soc. A. 378, 20200015 (2020)]. It is found that the spherical convergent effect can be helpful for smoothing the disturbance by merging the spikes in the azimuthal direction. For the DCI scheme, the pressure gradient in the same direction with the density gradient at the fuel inner interface can further prevent the disturbance from growing. For the example case with an initial disturbance amplitude as large as 20 μm, the DCI scheme can still reach a high-density isochoric plasma with an areal density of 2.18 g/cm2 at the stagnation moment, providing favorable conditions for fast ignition by the relativistic electron beam.

Funder

Strategic Priority Research Program of Chinese Academy of Science

National Natural Science Foundation of China

Shanghai Municipal Science and Technology Key Project

Shanghai Pujiang Program

Publisher

AIP Publishing

Subject

Condensed Matter Physics

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