Bulletin of the American Physical Society
60th Annual Meeting of the APS Division of Plasma Physics
Volume 63, Number 11
Monday–Friday, November 5–9, 2018; Portland, Oregon
Session CO4: Direct and Indirect Drive, Shock and Fast Ignition |
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Chair: Wolfgang Theobald, University of Rochester Room: OCC B110-112 |
Monday, November 5, 2018 2:00PM - 2:12PM |
CO4.00001: Revolver Designs for the National Ignition Facility Using Current and Optimized Phase Plates R. Stephen Craxton, Yujia Yang, Emma M Garcia, Patrick W McKenty, Mark Jude Schmitt, Kim Molvig The three-shell Revolver target[1] proposed for direct-drive ignition at the National Ignition Facility has a diameter (~6 mm) much larger than that of conventional designs. Simulations carried out using the 2-D hydrodynamics code SAGE[2] illustrate the advantages and challenges of the design. The absorption is almost 100%, the absorption occurs at a significant distance from the ablation surface, and the average intensity reaching the quarter-critical surface is low (just over 1 x 1014 W/cm2). However, uniformity presents a challenge, especially if the current phase plates are used. An optimized design, taking into account the full 3-D energy-deposition pattern, results in an implosion velocity nonuniformity of ~2.5% rms with the nonuniformity modes dominated by the small beam sizes. This can be improved to ~1.2% using custom phase plates with larger beam spots. Further improvement should be realized through thermal smoothing of azimuthal variations, not accounted for in the simulations. [1] K. Molvig et al., Phys. Rev. Lett. 116, 255003 (2016). [2] R. S. Craxton and R. L. McCrory, J. Appl. Phys. 56, 108 (1984). |
Monday, November 5, 2018 2:12PM - 2:24PM |
CO4.00002: Numerical Investigation of Laser-Imprint Mitigation in Revolver Ignition Designs Patrick McKenty, Timothy J Collins, John A Marozas, E. M. Campbell, Kim Molvig, Mark Jude Schmitt The three-shell Revolver target[1] proposed for direct-drive ignition at the National Ignition Facility (NIF) utilizes a large 6-mm beryllium shell as an ablator. This ablator will be subjected to significant levels of laser imprint arising directly from the NIF laser beams illuminating the target without sufficient laser smoothing. Initial studies[2] have indicated that such imprint can severely distort the incoming shell and lead to ignition failure. Two-dimensional simulation results, employing nonlocal electron thermal transport and cross‑beam energy transport, will be presented investigating the implementation of several laser-smoothing techniques, as well as tamper layers within the target, to evaluate their efficacy in limiting the ensuing perturbation growth. [1] K. Molvig et al., Phys Rev. Lett. 116, 255003 (2016). [2] P. W. McKenty et al., Bull. Am. Phys. Soc. 62, BAPS.2017.DPP.NO7.5 (2017). |
Monday, November 5, 2018 2:24PM - 2:36PM |
CO4.00003: Direct-Drive Ignition Designs with Gradient-Density Double Shells S. X. Hu, R. Epstein, V. N. Goncharov, E. M. Campbell Double-shell ignition designs have been studied with the indirect-drive inertial confinement fusion (ICF) in both simulations and experiments [1-3]. Such indirect-drive double-shell designs might provide a viable path to breakeven with a gain of G = 1~3. Since the direct-drive ICF can couple more energy to the in-flight shell, we have performed a study on direct-drive, double-shell ignition designs with our state-of-the-art physics models in DRACO. To mitigate a classical unstable interface, we have proposed using tungsten (W) inner shell with a gradient-density tamper layer of W-doped beryllium (Be) [4]. Due to its high ablation velocity, the Be outer shell is driven symmetrically by a high-adiabat (a = 6-8) laser pulse of 1.8 MJ. Our laser-imprint DRACO simulations indicate that neutron yield energies of 5~10 MJ could be possible with direct-drive, double-shell implosions on NIF-scale facilities. This material is based upon work supported by the Department of Energy National Nuclear Security Administration under Award No. DE-NA0001944. [1] P. Amendt et al., Phys. Plasmas 9, 2221 (2002). [2] J. L. Milovich et al., Phys. Plasmas 11, 1552 (2004). [3] E. C. Merritt et al., Bull. Am. Phys. Soc. 61, DPP.PO5.3 (2016). [4] H. Xu et al., Fusion Sci. Tech. 73, 354 (2018). |
Monday, November 5, 2018 2:36PM - 2:48PM |
CO4.00004: Experiments on Indirect-driven Double-shell implosion at the ShenGuang-III laser facility with 100kJ laser energy Ji Yan, Xing Zhang, JiWei Li, Zhensheng Dai The double-shell implosion is a favorable candidate for the ignition by ICF. The double-shell implosion experiments have been carried out on OMEGA with 15kJ laser energy and the highest DD neutron yield is 108. Recent years, double-shell implosion work were carried out on NIF with 1MJ laser energy. In our work, double-shell implosion with 6 shots have been performed on ShenGuang-III laser facility with 96kJ and 48 laser beams.Two type capsules(undoped ablator and doped ablator) were used to study the influence of M-band preheat and Pusher-Gas mix on double-shell implosion. In our experiments, the highest DD neutron yield of 9.1×109 and 27% YOC1D are obtained by undoped ablator shot.Simultaneously,1.5×107 secondary DD neutrons are produced and 14mg/cm2 fuel area density(~80% of 1D simulated) is inferred. On the other hand, the doped ablator shot get a lower neutron yield and YOC1D is less than 10%. Furthermore, fall-line method was used to analysis two type implosions. And we proposed that the measured neutron yield is very close to “clean” neutron from Fall-line. The doped ablator implosion had a lower YOC1D was comes from Pusher-gas mix. In sum, the fall-line analysis is very useful and the pusher-gas mix is very important in double-shell implosion. |
Monday, November 5, 2018 2:48PM - 3:00PM |
CO4.00005: Laser–Plasma Interaction Experiments at Direct-Drive Ignition-Relevant Scale Lengths at the National Ignition Facility Michael Rosenberg, Andrey Solodov, Russell Follett, Wolf Seka, Sean P Regan, Reuben Epstein, Alison R Christopherson, Riccardo Betti, Andrei V Maximov, Timothy J Collins, Valeri N Goncharov, Robert W Short, David Turnbull, Dustin H Froula, P.B Radha, Jason F Myatt, Pierre A Michel, Matthias Hohenberger, Laurent Pierre Masse, George F Swadling, James Ross, Thomas D Chapman, John D Moody, Jason Wilson Bates, Andrew J Schmitt Experiments at the National Ignition Facility have probed laser-plasma interactions and hot-electron production at plasma conditions relevant to direct-drive ignition, with predicted density scale lengths of Ln ~500-700 μm, electron temperatures of Te ~4-5 keV, and overlapped laser intensities of I ~6-15 × 1014 W/cm2. The fraction of laser energy converted to hot electrons is 1-3%, while the hot-electron temperature is 45-60 keV. Only a sharp red-shifted feature is observed around ω/2, along with significant stimulated Raman scattering (SRS), including sidescattering, at lower densities, suggesting that SRS dominates hot-electron production, unlike in shorter-scale-length plasmas on OMEGA that are dominated by two-plasmon decay (TPD). This difference in regime is explained based on absolute SRS and TPD threshold considerations. Subsequent measurements of 3ω/2 emission have revealed evidence of TPD; upcoming experiments will identify dominant plasma waves. The coupling of hot electrons to an implosion will be measured in new experiments, which will determine the need for preheat mitigation strategies for direct-drive ignition. |
Monday, November 5, 2018 3:00PM - 3:12PM |
CO4.00006: Implementation of the Low-Noise, 3-D Ray-Trace, Inverse-Projection Method in the Radiation–Hydrodynamics Code HYDRA John A Marozas, Scott Sepke, Gary D Kerbel, Michael M Marinak Hydrodynamic simulations of direct-drive inertial confinement fusion (ICF) targets require low-noise laser-energy deposition to achieve high-fidelity implosions. Directly driven ICF targets are especially susceptible to laser-deposition noise because of the proximity of the coronal absorption profile to the ablation surface as well as the high laser energy coupling efficiency. Using the inverse-projection method, judicious selection of the simulated laser rays’ origination points dramatically reduces the deposition noise in comparison to random spatial distributions coupled with temporal averaging. The significantly lower ray number density required using the inverse-projection method also improves computational efficiency. The inverse-projection method, originally developed as one part of the Mazinisin 3-D laser ray-trace in the 2-D radiation-hydro code DRACO, has been was extended to the 3-D radiation–hydro code HYDRA. The initial results of 3-D polar-direct-drive implosion simulations demonstrating the improved noise characteristics will be shown as part of the introduction of the inverse-projection method into HYDRA. |
Monday, November 5, 2018 3:12PM - 3:24PM |
CO4.00007: Cross-Beam Energy Transfer Platform Development on OMEGA Aaron Michael Hansen, David Turnbull, Daniel J Haberberger, Joe Katz, Dino Mastrosimone, Adam Bennett Sefkow, Russell Follett, John Palastro, Dustin H Froula A cross-beam energy transfer (CBET) platform was activated on OMEGA. A gas jet was heated by ten 500-ps, 351-nm beams that used phase plates to generate a ~2-mm-diam spherical plasma. Optical Thomson scattering measured a peak temperature of ~700 eV over a uniform ~5 x 1019 cm–3 electron density plateau of ~1 mm. These results are in good agreement with radiation–hydrodynamics simulations performed by HYDRA. To study CBET, a wavelength‑tunable UV beam (Δλ3w ~ 3.5 nm) and a 351-nm beam act as the probe and pump beams, respectively. The frequency of the probe was tuned so that the beat frequency of the crossed beams was resonant with ion-acoustic waves in the plasma, causing Brillouin scattering, which transferred energy between the beams. The results will be compared to LPSE simulations to understand limitations of linear CBET modeling. |
Monday, November 5, 2018 3:24PM - 3:36PM |
CO4.00008: Density Measurements of the Inner Shell Release Daniel J Haberberger, Alex Shvydky, Suxing Hu, Valeri N Goncharov, Dustin H Froula In inertial confinement fusion implosions, the release of plasma off the inner surface of the target shell after the shock breakout is an important parameter to the performance of the design. If the release has a higher density or longer scale length than that predicted by hydrodynamic simulations, the mass increase in the hot spot can decrease its compressibility and reduce performance compared to what is expected from the simulations. Experiments on OMEGA EP at the Laboratory for Laser Energetics were performed to measure the plasma expanding on the back side of a CH shell driven by two UV laser beams with a total of 6 kJ of energy in a 5-ns pulse focused to a 750-mm spot. The peak position of the driven shell was tracked using x-ray radiography streaked over 4 ns. The low-density plasma expanding off the undriven side of the shell after the shock breaks through was measured using the 4ω interferometer and angular filter refractometer. The experimental data will be presented and compared to the hydrodynamic simulations using 2-D radiation–hydrodynamic code DRACO. |
Monday, November 5, 2018 3:36PM - 3:48PM |
CO4.00009: Numerical Simulations of Shock-Release OMEGA EP Experiments A. Shvydky, D. J Haberberger, D. H. H Froula, V. N. N Goncharov, S. X. Hu, I. V. Igumenshchev, J. A. A Marozas, A. V. V Maximov, P. B. Radha Release of shocked material from the inner side of the shell after the shock breakout is an important process in an inertial confinement fusion implosion that affects formation of the hot spot and thereby the implosion performance. Experiments on OMEGA EP at the Laboratory for Laser Energetics were performed to measure the low-density profile of the plasma in the rarefaction wave that follows the shock breakout from the back side of a CH shell driven by two OMEGA EP beams. The shell trajectory was measured using x-ray radiography. The low-density plasma inside the rarefaction wave was measured using 4w interferometry and angular filter refractometry. Results of radiation–hydrodynamic code DRACO simulations of the evolution of the density profile in the rarefaction wave will be presented and compared with the experimental data. Sensitivity of the density profile to the equation of state will be discussed. |
Monday, November 5, 2018 3:48PM - 4:00PM |
CO4.00010: Shock-ignition targets: Effects of low-to-intermediate mode implosion asymmetries Stefano Atzeni, Angelo Schiavi, Arianna Serpi In inertial fusion shock-ignition schemes [1,2], generation of the required central hot spot is "assisted" by a strong converging shock-wave, driven by a final laser spike. This process differs from hot spot formation in the conventional ignition scheme. In particular, interaction of shock waves in the nearly stagnating fuel affects both sensitvity to implosion asymmetries and growth of deceleration-phase Rayleigh-Taylor instability. To address these issues, we perform 2D numerical simulations of targets consisting of a cryogenic DT layer and a plastic ablator. We consider both single-mode and multi-mode perturbations of the velocity field (with mode numbers l in the range 1-12). We study yield degradation as a function of perturbation mode and perturbation amplitude, for different values of laser compression power, laser spike power, and DT vapour density. The relation between sensitivity to drive asymmetries and ignition threshold factors computed with 1D simulations is also discussed. [1] R. Betti et al., Phys. Rev. Lett. 98, 155001 (2007). [2] S. Atzeni et al., Nucl. Fusion 54, 054008 (2014).
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Monday, November 5, 2018 4:00PM - 4:12PM |
CO4.00011: Shock Ignition Simulations and Experiments in ignition-scale plasma conditions Robbie Scott, Kevin Glize, Luca Antonelli, Nigel Woolsey, Wolfgang R. Theobald, Matthew Khan, Mingsheng Wei, Alexis Casner, Vladimir Tikhonchuk, Stefano Atzeni, Warren Garbett, Dimitri Batani, Tony Arber, Keith Bennett, Sean P Regan, Michael J Rosenberg, Chikang Li, Alex Seaton, Riccardo Betti Shock ignition (SI) is a promising route to direct drive ignition. As the implosion velocity is reduced below the self-ignition threshold, ignition is instead initiated by a strong shock. Consequently, SI has potential advantages over other laser fusion schemes; the laser energy requirements for ignition appear to be well within those possible on NIF and, as the implosion velocity can be lower, the susceptibility to fluid instabilities (Rayleigh-Taylor) is reduced. Finally, because more fuel mass can be imploded for a given driver energy, there is the potential for high gain at modest laser energies. However as shock ignition requires increased laser intensity at the end of the drive pulse, laser plasma interaction instabilities (LPI) increasingly dominate the absorption of laser light and can create significant populations of hot-electrons. Depending on their energy spectrum, these hot-electrons may enhance the ignitor shock. This talk will discuss the first experiments – performed on Omega 60 – to combine the laser intensity required for shock ignition (~1e16W/cm2) with NIF-like plasma conditions. We describe the novel targetry used to achieve these plasma conditions and the experimental results. |
Monday, November 5, 2018 4:12PM - 4:24PM |
CO4.00012: Magnetic field guiding of electron beam for reduction of ignition requirement in fast ignition laser fusion Tomoyuki Johzaki, Mie Horio, Shijuro Takeda, Wookyung Kim, Takuma Endo, Hideo Nagatomo, Shinsuke Fujioka, Atsushi Sunahara One of most important issues in fast ignition laser fusion is efficient core heating by laser produced relativistic electron beam (REB). The large angular divergence of REB, however, inhibits the efficient core heating[1]. To solve this problem, the beam guiding using externally applied kilo-tesla class magnetic field has been proposed [2], and its availability has been numerically[3] and experimentally[4] demonstrated. The effect of external field is not only beam guiding, but also the effective range reduction due to Larmor motion. In addition, the convergence field configuration is formed through implosion, then the beam focusing is also expected for the moderate mirror ratio case. On the basis of hybrid simulation, we will show the enhancement in heating efficiency and reduction in ignition threshold due to external fields. [1] S. Fujioka, et al., Phys. Rev. E 91, 063102 (2015). [2] D. J. Strozzi et al., Phys Plasmas 19, 072711 (2012). [3 ]T. Johzaki, et al., Plasma Phys. Control. Fusion 59, 014045 (2017). [4]M. Bailly-Grandvaux, et al., Nat. Commun. 9, 102 (2018).
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Monday, November 5, 2018 4:24PM - 4:36PM |
CO4.00013: Wave-Function Amplitude Analysis of the 5He Resonance in the TT Neutron Spectrum Zaarah Mohamed, James P Knauer, Chad Forrest, Maria Gatu Johnson An understanding of the TT neutron spectrum is necessary for accurate modeling of neutron spectra as well as for analysis of experimental data from ICF implosions. The 5He resonance is an important component of the TT spectrum. Available OMEGA data suitable to study the 5He state include neutron time-of-flight spectra collected at three different ion temperatures. 1 These data are used in a multi-step least-squares analysis that models the resonance line shape for the individual reaction branches involved in TT fusion including 5He (ground state) + n and 5He* (first excited state) + n. This analysis reveals a first excited state at ~2 MeV (Ref. 2) in 5He. The shape of the 5He resonance changes with ion temperature as expected and the width of each state is used to determine its lifetime. 1 M. Gatu Johnson et al., “First Experimental Evidence of a Variant Neutron Spectrum from the T(T,2n)α Reaction at Center-of-Mass Energies in the Range of 16–50 keV,” submitted to Physical Review Letters. 2 C. Wong, J. D. Anderson, and J. W. McClure, Nucl. Phys. 71, 106 (1965).
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