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Dive into the research topics where Stephen A. Slutz is active.

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Featured researches published by Stephen A. Slutz.


Physics of Plasmas | 2010

Pulsed-power-driven cylindrical liner implosions of laser preheated fuel magnetized with an axial field

Stephen A. Slutz; Mark Herrmann; Roger Alan Vesey; Adam B Sefkow; Daniel Brian Sinars; Dean C. Rovang; Kyle Peterson; M. E. Cuneo

The radial convergence required to reach fusion conditions is considerably higher for cylindrical than for spherical implosions since the volume is proportional to r2 versus r3, respectively. Fuel magnetization and preheat significantly lowers the required radial convergence enabling cylindrical implosions to become an attractive path toward generating fusion conditions. Numerical simulations are presented indicating that significant fusion yields may be obtained by pulsed-power-driven implosions of cylindrical metal liners onto magnetized (>10 T) and preheated (100–500 eV) deuterium-tritium (DT) fuel. Yields exceeding 100 kJ could be possible on Z at 25 MA, while yields exceeding 50 MJ could be possible with a more advanced pulsed power machine delivering 60 MA. These implosions occur on a much shorter time scale than previously proposed implosions, about 100 ns as compared to about 10 μs for magnetic target fusion (MTF) [I. R. Lindemuth and R. C. Kirkpatrick, Nucl. Fusion 23, 263 (1983)]. Consequently t...


Physics of Plasmas | 2005

Pulsed-power-driven high energy density physics and inertial confinement fusion research

M. Keith Matzen; M. A. Sweeney; R. G. Adams; J. R. Asay; J. E. Bailey; Guy R. Bennett; D.E. Bliss; Douglas D. Bloomquist; T. A. Brunner; Robert B. Campbell; Gordon Andrew Chandler; C.A. Coverdale; M. E. Cuneo; Jean-Paul Davis; C. Deeney; Michael P. Desjarlais; G. L. Donovan; Christopher Joseph Garasi; Thomas A. Haill; C. A. Hall; D.L. Hanson; M. J. Hurst; B. Jones; M. D. Knudson; R. J. Leeper; R.W. Lemke; M.G. Mazarakis; D. H. McDaniel; T.A. Mehlhorn; T. J. Nash

The Z accelerator [R. B. Spielman, W. A. Stygar, J. F. Seamen et al., Proceedings of the 11th International Pulsed Power Conference, Baltimore, MD, 1997, edited by G. Cooperstein and I. Vitkovitsky (IEEE, Piscataway, NJ, 1997), Vol. 1, p. 709] at Sandia National Laboratories delivers ∼20MA load currents to create high magnetic fields (>1000T) and high pressures (megabar to gigabar). In a z-pinch configuration, the magnetic pressure (the Lorentz force) supersonically implodes a plasma created from a cylindrical wire array, which at stagnation typically generates a plasma with energy densities of about 10MJ∕cm3 and temperatures >1keV at 0.1% of solid density. These plasmas produce x-ray energies approaching 2MJ at powers >200TW for inertial confinement fusion (ICF) and high energy density physics (HEDP) experiments. In an alternative configuration, the large magnetic pressure directly drives isentropic compression experiments to pressures >3Mbar and accelerates flyer plates to >30km∕s for equation of state ...


Physical Review Letters | 2004

Hot Dense Capsule-Implosion Cores Produced by Z -Pinch Dynamic Hohlraum Radiation

J. E. Bailey; Gordon Andrew Chandler; Stephen A. Slutz; Igor E. Golovkin; P. Lake; J. J. MacFarlane; R. C. Mancini; T.J. Burris-Mog; G. W. Cooper; R. J. Leeper; Thomas Alan Mehlhorn; T. C. Moore; T. J. Nash; Nielsen Ds; C. L. Ruiz; D. G. Schroen; W. Varnum

Hot dense capsule implosions driven by Z-pinch x rays have been measured using a approximately 220 eV dynamic Hohlraum to implode 1.7-2.1 mm diameter gas-filled CH capsules. The capsules absorbed up to approximately 20 kJ of x rays. Argon tracer atom spectra were used to measure the T(e) approximately 1 keV electron temperature and the n(e) approximately 1-4 x 10(23) cm(-3) electron density. Spectra from multiple directions provide core symmetry estimates. Computer simulations agree well with the peak emission values of T(e), n(e), and symmetry, indicating reasonable understanding of the Hohlraum and implosion physics.


Journal of Applied Physics | 1985

Time-resolved proton focus of a high-power ion diode

D. J. Johnson; R. J. Leeper; W. A. Stygar; R. S. Coats; Thomas Alan Mehlhorn; J. P. Quintenz; Stephen A. Slutz; M. A. Sweeney

An improved understanding of the factors that control the axial focus of applied‐B ion diodes was obtained from time‐resolved diagnostics of ion‐beam trajectories. This resulted in a new selection of anode shape that produced a proton focus of 1.3‐mm diameter from a 4.5‐cm‐radius diode, which is a factor of 2 improvement over previous results. We have achieved a peak proton power density of 1.5±0.2 TW/cm2 on the 1‐TW Proto I accelerator. The radial convergence of this proton beam, defined as the ratio of the anode diameter to focused beam FWHM, is 70. Time‐resolved information about virtual cathode evolution, the self‐ and applied‐magnetic‐field bending, and the horizontal focus of the beam was also obtained. In addition, the diffusion of the magnetic field into the anode plasma is estimated by measuring the horizontal focal position as a function of time. Finally, we discuss the effects of gas cell scattering on the beam focus.


Physics of Plasmas | 2003

Dynamic hohlraum driven inertial fusion capsules

Stephen A. Slutz; J. E. Bailey; Gordon Andrew Chandler; Guy R. Bennett; G. W. Cooper; Joel Staton Lash; S. Lazier; P. Lake; R.W. Lemke; Thomas Alan Mehlhorn; T. J. Nash; D. S. Nielson; J. McGurn; T. C. Moore; C. L. Ruiz; Diana Grace Schroen; J. Torres; W. Varnum; Roger Alan Vesey

A dynamic hohlraum is formed when an imploding annular cylindrical Z-pinch driven plasma collides with an internal low density convertor. This collision generates an inward traveling shock wave that emits x rays, which are trapped by the optically thick Z-pinch plasma and can be used to drive an inertial fusion capsule embedded in the convertor. This scheme has the potential to efficiently drive high yield capsules due to the close coupling between the intense radiation generation and the capsule. In prior dynamic hohlraum experiments [J. E. Bailey et al., Phys. Rev Lett. 89, 095004 (2002)] the convertor shock wave has been imaged with gated x-ray pinhole cameras. The shock emission was observed to be very circular and to be quite narrow in the radial direction. This implies that there is minimal Rayleigh–Taylor imprinting on the shock wave. Thus, the dominant source of radiation asymmetry is not random and in principle could be significantly decreased by proper design. Due to the closed geometry of the d...


Journal of Applied Physics | 2005

Magnetically accelerated, ultrahigh velocity flyer plates for shock wave experiments

R.W. Lemke; M. D. Knudson; D.E. Bliss; Kyle Robert Cochrane; Jean-Paul Davis; A. A. Giunta; H.C. Harjes; Stephen A. Slutz

The intense magnetic field produced by the 20 MA Z accelerator is used as an impulsive pressure source to accelerate metal flyer plates to high velocity for the purpose of performing plate impact, shock wave experiments. This capability has been significantly enhanced by the recently developed pulse shaping capability of Z, which enables tailoring the rise time to peak current for a specific material and drive pressure to avoid shock formation within the flyer plate during acceleration. Consequently, full advantage can be taken of the available current to achieve the maximum possible magnetic drive pressure. In this way, peak magnetic drive pressures up to 490 GPa have been produced, which shocklessly accelerated 850μm aluminum (6061-T6) flyer plates to peak velocities of 34km∕s. We discuss magnetohydrodynamic (MHD) simulations that are used to optimize the magnetic pressure for a given flyer load and to determine the shape of the current rise time that precludes shock formation within the flyer during ac...


Physics of Plasmas | 2011

Measurements of magneto-Rayleigh–Taylor instability growth during the implosion of initially solid metal liners a)

Daniel Brian Sinars; Stephen A. Slutz; Mark Herrmann; R. D. McBride; M. E. Cuneo; Christopher A. Jennings; J. P. Chittenden; A.L. Velikovich; Kyle Peterson; Roger Alan Vesey; C. Nakhleh; E.M. Waisman; B.E. Blue; K. Killebrew; D. G. Schroen; Kurt Tomlinson; Aaron Edens; M. R. Lopez; I. C. Smith; Jonathon Shores; V. Bigman; Guy R. Bennett; Briggs Atherton; M. E. Savage; W. A. Stygar; G. T. Leifeste; John L. Porter

A recent publication [D. B. Sinars et al., Phys. Rev. Lett. 105, 185001 (2010)] describes the first controlled experiments measuring the growth of the magneto-Rayleigh–Taylor instability in fast (∼100 ns) Z-pinch plasmas formed from initially solid aluminum tubes (liners). Sinusoidal perturbations on the surface of these liners with wavelengths of 25–400 μm were used to seed single-mode instabilities. The evolution of the outer liner surface was captured using multiframe 6.151 keV radiography. The initial paper shows that there is good agreement between the data and 2-D radiation magneto-hydrodynamic simulations down to 50 μm wavelengths. This paper extends the previous one by providing more detailed radiography images, detailed target characterization data, a more accurate comparison to analytic models for the amplitude growth, the first data from a beryllium liner, and comparisons between the data and 3D simulations.


Physics of Plasmas | 2014

Design of magnetized liner inertial fusion experiments using the Z facilitya)

Adam B Sefkow; Stephen A. Slutz; Joseph Matthew Koning; M. M. Marinak; Kyle Peterson; Daniel Brian Sinars; Roger Alan Vesey

The magnetized liner inertial fusion concept has been presented as a path toward obtaining substantial thermonuclear fusion yields using the Z accelerator [S. A. Slutz et al., Phys. Plasmas 17, 056303 (2010)]. We present the first integrated magnetohydrodynamic simulations of the inertial fusion targets, which self-consistently include laser preheating of the fuel, the presence of electrodes, and end loss effects. These numerical simulations provided the design for the first thermonuclear fusion neutron-producing experiments on Z using capabilities that presently exist: peak currents of Imax = 18–20 MA, pre-seeded axial magnetic fields of Bz0=10 T, laser preheat energies of about Elas = 2 kJ delivered in 2 ns, DD fuel, and an aspect ratio 6 solid Be liner imploded to 70 km/s. Specific design details and observables for both near-term and future experiments are discussed, including sensitivity to laser timing and absorbed preheat energy. The initial experiments measured stagnation radii rstag<75 μm, temper...


Physics of Plasmas | 2013

Beryllium liner implosion experiments on the Z accelerator in preparation for magnetized liner inertial fusion

Ryan D McBride; M. R. Martin; R.W. Lemke; J. B. Greenly; Christopher A. Jennings; Dean C. Rovang; Daniel Brian Sinars; M. E. Cuneo; Mark Herrmann; Stephen A. Slutz; C. Nakhleh; D. D. Ryutov; Jean-Paul Davis; Dawn G. Flicker; B.E. Blue; Kurt Tomlinson; D. G. Schroen; R. M. Stamm; G. E. Smith; J. K. Moore; T. J. Rogers; G. K. Robertson; R. J. Kamm; I. C. Smith; M. E. Savage; W. A. Stygar; G. A. Rochau; M. Jones; M. R. Lopez; John L. Porter

Multiple experimental campaigns have been executed to study the implosions of initially solid beryllium (Be) liners (tubes) on the Z pulsed-power accelerator. The implosions were driven by current pulses that rose from 0 to 20 MA in either 100 or 200 ns (200 ns for pulse shaping experiments). These studies were conducted in support of the recently proposed Magnetized Liner Inertial Fusion concept [Slutz et al., Phys. Plasmas 17, 056303 (2010)], as well as for exploring novel equation-of-state measurement techniques. The experiments used thick-walled liners that had an aspect ratio (initial outer radius divided by initial wall thickness) of either 3.2, 4, or 6. From these studies, we present three new primary results. First, we present radiographic images of imploding Be liners, where each liner contained a thin aluminum sleeve for enhancing the contrast and visibility of the liners inner surface in the images. These images allow us to assess the stability of the liners inner surface more accurately and more directly than was previously possible. Second, we present radiographic images taken early in the implosion (prior to any motion of the liners inner surface) of a shockwave propagating radially inward through the liner wall. Radial mass density profiles from these shock compression experiments are contrasted with profiles from experiments where the Z accelerators pulse shaping capabilities were used to achieve shockless (“quasi-isentropic”) liner compression. Third, we present “micro-B” measurements of azimuthal magnetic field penetration into the initially vacuum-filled interior of a shocked liner. Our measurements and simulations reveal that the penetration commences shortly after the shockwave breaks out from the liners inner surface. The field then accelerates this low-density “precursor” plasma to the axis of symmetry.


IEEE Transactions on Plasma Science | 2012

Magnetically Driven Implosions for Inertial Confinement Fusion at Sandia National Laboratories

Michael Edward Cuneo; Mark Herrmann; Daniel Brian Sinars; Stephen A. Slutz; W. A. Stygar; Roger Alan Vesey; A. B. Sefkow; Gregory A. Rochau; Gordon Andrew Chandler; J. E. Bailey; John L. Porter; R. D. McBride; D. C. Rovang; M.G. Mazarakis; E. P. Yu; Derek C. Lamppa; Kyle Peterson; C. Nakhleh; Stephanie B. Hansen; A. J. Lopez; M. E. Savage; Christopher A. Jennings; M. R. Martin; R.W. Lemke; Briggs Atherton; I. C. Smith; P. K. Rambo; M. Jones; M.R. Lopez; P. J. Christenson

High current pulsed-power generators efficiently store and deliver magnetic energy to z-pinch targets. We review applications of magnetically driven implosions (MDIs) to inertial confinement fusion. Previous research on MDIs of wire-array z-pinches for radiation-driven indirect-drive target designs is summarized. Indirect-drive designs are compared with new targets that are imploded by direct application of magnetic pressure produced by the pulsed-power current pulse. We describe target design elements such as larger absorbed energy, magnetized and pre-heated fuel, and cryogenic fuel layers that may relax fusion requirements. These elements are embodied in the magnetized liner inertial fusion (MagLIF) concept [Slutz “Pulsed-power-driven cylindrical liner implosions of laser pre-heated fuel magnetized with an axial field,” Phys. Plasmas, 17, 056303 (2010), and Stephen A. Slutz and Roger A. Vesey, “High-Gain Magnetized Inertial Fusion,” Phys. Rev. Lett., 108, 025003 (2012)]. MagLIF is in the class of magneto-inertial fusion targets. In MagLIF, the large drive currents produce an azimuthal magnetic field that compresses cylindrical liners containing pre-heated and axially pre-magnetized fusion fuel. Scientific breakeven may be achievable on the Z facility with this concept. Simulations of MagLIF with deuterium-tritium fuel indicate that the fusion energy yield can exceed the energy invested in heating the fuel at a peak drive current of about 27 MA. Scientific breakeven does not require alpha particle self-heating and is therefore not equivalent to ignition. Capabilities to perform these experiments will be developed on Z starting in 2013. These simulations and predictions must be validated against a series of experiments over the next five years. Near-term experiments are planned at drive currents of 16 MA with D2 fuel. MagLIF increases the efficiency of coupling energy (=target absorbed energy/driver stored energy) to targets by 10-150X relative to indirect-drive targets. MagLIF also increases the absolute energy absorbed by the target by 10-50X relative to indirect-drive targets. These increases could lead to higher fusion gains and yields. Single-shot high yields are of great utility to national security missions. Higher efficiency and higher gains may also translate into more compelling (lower cost and complexity) fusion reactor designs. We will discuss the broad goals of the emerging research on the MagLIF concept and identify some of the challenges. We will also summarize advances in pulsed-power technology and pulsed-power driver architectures that double the efficiency of the driver.

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Daniel Brian Sinars

Sandia National Laboratories

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Kyle Peterson

Sandia National Laboratories

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Roger Alan Vesey

Sandia National Laboratories

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Michael Edward Cuneo

Sandia National Laboratories

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Mark Herrmann

Sandia National Laboratories

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Adam B Sefkow

Sandia National Laboratories

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J. E. Bailey

Sandia National Laboratories

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Thomas Alan Mehlhorn

Sandia National Laboratories

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