Magneto-Rayleigh-Taylor instabiliity mitigation in multi-species gas-puff Z-pinches
ORAL
Abstract
The gas-puff Z-pinch is a well-known, efficient source of X-rays and/or neutrons, in which an axially applied current interacts with the azimuthal self-magnetic field to drive a radial implosion. It is highly susceptible to the magneto-Rayleigh-Taylor instability (MRTI), which can disrupt the pinch if unmitigated. Axial pre-magnetization can mitigate MRTI growth but tends to reduce yield [1] as the initial field, Bz0, is increased. Here, we present 2-D magnetohydrodynamic simulations [2] of Ne-liner, deuterium-target gas-puff loads driven by an 850 kA, 160 ns driver which show that the tradeoff between stability and yield can be reduced by adding a second liner. A Bz0 of 0.7 T is required to stabilize the single-liner implosion with initial radius 2.5 cm, but thermonuclear neutron yield decreases from 1.2x109 with Bz0 = 0 T to 1.0x107 with Bz0 = 0.7 T. When a second liner is added with radius 1.25 cm, the required Bz0 is reduced to 0.3 T. Consequently, the penalty to yield is significantly reduced: from 1.2x109 with Bz0 = 0 T to 9.8x108 with Bz0 = 0.3 T. We show this concept scales favorably with current to 10 MA, at which level thermonuclear yields of ~1013 are predicted.
[1] F. Conti et al., Phys. Plasmas 27, 012702 (2020).
[2] J. Narkis et al., Phys. Rev. E (under review).
[1] F. Conti et al., Phys. Plasmas 27, 012702 (2020).
[2] J. Narkis et al., Phys. Rev. E (under review).
*This material is based upon work supported by the Department of Energy, National Nuclear Security Administration under Award Number DE-NA0003842.
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Publication: J. Narkis, F. Conti, A. Velikovich, and F. N. Beg, Phys. Rev. E (under review).
Presenters
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Jeff Narkis
- University of California, San Diego