Publications

Vesey, Roger A.; Slutz, Stephen A.

Abstract not provided.

Slutz, Stephen A.; Vesey, Roger A.

Abstract not provided.

Slutz, Stephen A.; Vesey, Roger A.; Herrmann, Mark H.

Abstract not provided.

Vesey, Roger A.; Herrmann, Mark H.; Slutz, Stephen A.; Cuneo, M.E.

Abstract not provided.

Vesey, Roger A.; Herrmann, Mark H.; Slutz, Stephen A.; Cuneo, M.E.; Mehlhorn, Thomas A.

Abstract not provided.

Plasma Physics and Controlled Fusion

Bailey, James E.; Chandler, Gordon A.; Leeper, Ramon J.; Mehlhorn, Thomas A.; Peterson, Kyle J.; Lemke, Raymond W.; Slutz, Stephen A.; Ruiz, Carlos L.

Abstract not provided.

Physical Review Letters

Slutz, Stephen A.; Vesey, Roger A.; Herrmann, Mark H.

Abstract not provided.

Slutz, Stephen A.; Vesey, Roger A.; Herrmann, Mark H.

Abstract not provided.

Physical Review Letters

Slutz, Stephen A.; Vesey, Roger A.; Herrmann, Mark H.

Abstract not provided.

Chandler, Gordon A.; Ruiz, Carlos L.; Bailey, James E.; Coverdale, Christine A.; Rochau, G.A.; Slutz, Stephen A.; Leeper, Ramon J.; Mehlhorn, Thomas A.

Abstract not provided.

Slutz, Stephen A.

Abstract not provided.

Slutz, Stephen A.; Vesey, Roger A.; Herrmann, Mark H.

Abstract not provided.

Bailey, James E.; Peterson, Kyle J.; Chandler, Gordon A.; Slutz, Stephen A.

Abstract not provided.

Vesey, Roger A.; Slutz, Stephen A.; Yu, Edmund Y.; Herrmann, Mark H.; Lemke, Raymond W.; Christenson, Peggy J.; Cuneo, M.E.; Desjarlais, Michael P.; Mehlhorn, Thomas A.

Abstract not provided.

Vesey, Roger A.; Slutz, Stephen A.; Yu, Edmund Y.; Herrmann, Mark H.; Lemke, Raymond W.; Christenson, Peggy J.; Cuneo, M.E.; Desjarlais, Michael P.; Mehlhorn, Thomas A.

Abstract not provided.

Bailey, James E.; Lake, Patrick W.; Leeper, Ramon J.; Lemke, Raymond W.; Mehlhorn, Thomas A.; Nash, Thomas J.; Chandler, Gordon A.; Nielsen, D.S.; Peterson, Kyle J.; Ruiz, Carlos L.; Rochau, G.A.; Slutz, Stephen A.

Abstract not provided.

Mehlhorn, Thomas A.; Slutz, Stephen A.

We examine the scaling to ignition of the energy deposition of laser generated electrons in compressed fast ignition cores. Relevant cores have densities of several hundred g/cm{sup 3}, with a few keV initial temperature. As the laser intensities increase approaching ignition systems, on the order of a few 10{sup 21}W/cm{sup 2}, the hot electron energies expected to approach 100MeV. Most certainly anomalous processes must play a role in the energy transfer, but the exact nature of these processes, as well as a practical way to model them, remain open issues. Traditional PIC explicit methods are limited to low densities on current and anticipated computing platforms, so the study of relevant parameter ranges has received so far little attention. We use LSP to examine a relativistic electron beam (presumed generated from a laser plasma interaction) of legislated energy and angular distribution is injected into a 3D block of compressed DT. Collective effects will determine the stopping, most likely driven by magnetic field filamentation. The scaling of the stopping as a function of block density and temperature, as well as hot electron current and laser intensity is presented. Sub-grid models may be profitably used and degenerate effects included in the solution of this problem.

Lemke, Raymond W.; Knudson, Marcus D.; Davis, Jean-Paul D.; Bliss, David E.; Slutz, Stephen A.; Giunta, Anthony A.; Harjes, Henry C.

The intense magnetic field generated in the 20 MA Z-machine is used to accelerate metallic flyer plates to high velocity for the purpose of generating strong shocks in equation of state experiments. We present results pertaining to experiments in which a 0.085 cm thick Al flyer plate is magnetically accelerated across a vacuum gap into a quartz target. Peak magnetic drive pressures up to 4.9 Mbar were produced, which yielded a record 34 km/s flyer velocity without destroying it by shock formation or Joule heating. Two-dimensional MHD simulation was used to optimize the magnetic drive pressure on the flyer surface, shape the current pulse to accelerate the flyer without shock formation (i.e., quasi-isentropically), and predict the flyer velocity. Shock pressures up to 11.5 Mbar were produced in quartz. Accurate measurements of the shock velocity indicate that a fraction of the flyer is at solid density when it arrives at the target. Comparison of measurements and simulation results yields a consistent picture of the flyer state at impact with the quartz target.

Bailey, James E.; Rochau, G.A.; Chandler, Gordon A.; Slutz, Stephen A.; Lake, Patrick W.; Mehlhorn, Thomas A.; Lemke, Raymond W.

Abstract not provided.

Mehlhorn, Thomas A.; Slutz, Stephen A.

Abstract not provided.

Mehlhorn, Thomas A.; Slutz, Stephen A.

Abstract not provided.

Slutz, Stephen A.; Vesey, Roger A.; Mehlhorn, Thomas A.; Cuneo, M.E.

Abstract not provided.

Proposed for publication in the Journal of Applied Physics.

Lemke, Raymond W.; Knudson, Marcus D.; Bliss, David E.; Harjes, Henry C.; Slutz, Stephen A.

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 850 {micro}m aluminum (6061-T6) flyer plates to peak velocities of 34 km/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 acceleration to peak velocity. In addition, we present results pertaining to plate impact, shock wave experiments in which the aluminum flyer plates were magnetically accelerated across a vacuum gap and impacted z-cut, {alpha}-quartz targets. Accurate measurements of resulting quartz shock velocities are presented and analyzed through high-fidelity MHD simulations enhanced using optimization techniques. Results show that a fraction of the flyer remains at solid density at impact, that the fraction of material at solid density decreases with increasing magnetic pressure, and that the observed abrupt decrease in the quartz shock velocity is well correlated with the melt transition in the aluminum flyer.

Proposed for publication in the Journal of Quantitative Spectroscopy and Radiative Transfer.

Bailey, James E.; Chandler, Gordon A.; Rochau, G.A.; Slutz, Stephen A.; Lake, Patrick W.; Lemke, Raymond W.; Mehlhorn, Thomas A.

A dynamic hohlraum is created when an annular z-pinch plasma implodes onto a cylindrical 0.014 g/cc 6-mm-diameter CH{sub 2} foam. The impact launches a radiating shock that propagates toward the axis at {approx}350 {micro}m/ns. The radiation trapped by the tungsten z-pinch plasma forms a {approx}200 eV hohlraum that provides X-rays for indirect drive inertial confinement fusion capsule implosion experiments. We are developing the ability to diagnose the hohlraum interior using emission and absorption spectroscopy of Si atoms added as a tracer to the central portion of the foam. Time- and space-resolved Si spectra are recorded with an elliptical crystal spectrometer viewing the cylindrical hohlraum end-on. A rectangular aperture at the end of the hohlraum restricts the field of view so that the 1D spectrometer resolution corresponds approximately to the hohlraum radial direction. This enables distinguishing between spectra from the unshocked radiation-heated foam and from the shocked foam. Typical spectral lines observed include the Si Ly{alpha} with its He-like satellites and the He-like resonance sequence including He{alpha}, He{beta}, and He{gamma}, along with some of their associated Li-like satellites. Work is in progress to infer the hohlraum conditions using collisional-radiative modeling that accounts for the radiation environment and includes both opacity effects and detailed Stark broadening calculations. These 6-mm-scale radiation-heated plasmas might eventually also prove suitable for testing Stark broadening line profile calculations or for opacity measurements.

Proposed for publication in Physics of Plasmas.

Slutz, Stephen A.; Vesey, Roger A.

A series of numerical simulations have been performed to determine scaling laws for fast ignition break even of a hot spot formed by energetic particles created by a short pulse laser. Hot spot break even is defined to be when the fusion yield is equal to the total energy deposited in the hot spot through both the initial compression and the subsequent heating. In these simulations, only a small portion of a previously compressed mass of deuterium-tritium fuel is heated on a short time scale, i.e., the hot spot is tamped by the cold dense fuel which surrounds it. The hot spot tamping reduces the minimum energy required to obtain break even as compared to the situation where the entire fuel mass is heated, as was assumed in a previous study [S. A. Slutz, R. A. Vesey, I. Shoemaker, T. A. Mehlhorn, and K. Cochrane, Phys. Plasmas 7, 3483 (2004)]. The minimum energy required to obtain hot spot break even is given approximately by the scaling law E{sub T} = 7.5({rho}/100){sup -1.87} kJ for tamped hot spots, as compared to the previously reported scaling of E{sub UT} = 15.3({rho}/100){sup -1.5} kJ for untamped hotspots. The size of the compressed fuel mass and the focusability of the particles generated by the short pulse laser determines which scaling law to use for an experiment designed to achieve hot spot break even.