Abstract

We have developed a conceptual design of a next-generation pulsed-power accelerator that is optimized for megajoule-class dynamic-material-physics experiments. Sufficient electrical energy is delivered by the accelerator to a physics load to achieve—within centimeter-scale samples—material pressures as high as 1 TPa. The accelerator design is based on an architecture that is founded on three concepts: single-stage electrical-pulse compression, impedance matching, and transit-time-isolated drive circuits. The prime power source of the accelerator consists of 600 independent impedance-matched Marx generators. Each Marx comprises eight 5.8-GW bricks connected electrically in series, and generates a 100-ns 46-GW electrical-power pulse. A 450-ns-long water-insulated coaxial-transmission-line impedance transformer transports the power generated by each Marx to a system of twelve 2.5-m-radius water-insulated conical transmission lines. The conical lines are connected electrically in parallel at a 66-cm radius by a water-insulated 45-post sextuple-post-hole convolute. The convolute sums the electrical currents at the outputs of the conical lines, and delivers the combined current to a single solid-dielectric-insulated radial transmission line. The radial line in turn transmits the combined current to the load. Since much of the accelerator is water insulated, we refer to it as Neptune. Neptune is 40 m in diameter, stores 4.8 MJ of electrical energy in its Marx capacitors, and generates 28 TW of peak electrical power. Since the Marxes are transit-time isolated from each other for 900 ns, they can be triggered at different times to construct–over an interval as long as 1 μs–the specific load-current time history required for a given experiment. Neptune delivers 1 MJ and 20 MA in a 380-ns current pulse to an 18−mΩ load; hence Neptune is a megajoule-class 20-MA arbitrary waveform generator. Neptune will allow the international scientific community to conduct dynamic equation-of-state, phase-transition, mechanical-property, and other material-physics experiments with a wide variety of drive-pressure time histories.3 MoreReceived 25 January 2016DOI:https://doi.org/10.1103/PhysRevAccelBeams.19.070401This article is available under the terms of the Creative Commons Attribution 3.0 License. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI.Published by the American Physical SocietyPhysics Subject Headings (PhySH)Physical SystemsPulsed-power acceleratorsAccelerators & Beams

Highlights

  • We have developed a conceptual design of a next-generation pulsed-power accelerator that is optimized for megajoule-class dynamic-material-physics experiments

  • Since the bricks are transit-time isolated from each other, they can be triggered at different times to construct, with a high-degree of precision, the specific load-current time history required for a given experiment

  • The singleMarx load-current time history is plotted by Fig. 7

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Summary

INTRODUCTION

In the late 1990s, Reisman and colleagues [1] and Hall and coworkers [2,3] developed a novel experimental platform for dynamic-material-physics experiments: an inductive short-circuit load that was driven by the Z pulsed-power accelerator [4,5,6,7,8,9,10,11,12,13,14,15,16]. The success of these experiments has motivated the development of a number of megampere-class pulsed-power accelerators that are optimized for material-science research [30,31,32,33,34,35,36] These machines deliver as much as 5 MA to a load and achieve pressures as high as 100 GPa. To maximize the peak load current, the drive circuits of the machines are connected as closely as possible to the load, which minimizes the inductance of the connections. We propose that the machine be powered by ∼600 drive circuits that are transit-time isolated over time intervals of interest This would make it possible to construct, with unprecedented precision and reproducibility, the specific load-current time history required for a given experiment. Numbered equations of this article are in SI units throughout

CONCEPTUAL DESIGN OF NEPTUNE
CIRCUIT MODEL OF NEPTUNE
M ntCbV
RESULTS
ENERGY EFFICIENCY OF THE NEPTUNE-LOAD SYSTEM
SUGGESTIONS FOR FUTURE WORK
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