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High-pressure chemistry of hydrocarbons relevant to planetary interiors and inertial confinement fusion

  • Author(s): Kraus, D
  • Hartley, NJ
  • Frydrych, S
  • Schuster, AK
  • Rohatsch, K
  • Rödel, M
  • Cowan, TE
  • Brown, S
  • Cunningham, E
  • Van Driel, T
  • Fletcher, LB
  • Galtier, E
  • Gamboa, EJ
  • Laso Garcia, A
  • Gericke, DO
  • Granados, E
  • Heimann, PA
  • Lee, HJ
  • Macdonald, MJ
  • Mackinnon, AJ
  • McBride, EE
  • Nam, I
  • Neumayer, P
  • Pak, A
  • Pelka, A
  • Prencipe, I
  • Ravasio, A
  • Redmer, R
  • Saunders, AM
  • Schölmerich, M
  • Schörner, M
  • Sun, P
  • Turner, SJ
  • Zettl, A
  • Falcone, RW
  • Glenzer, SH
  • Döppner, T
  • Vorberger, J
  • et al.

Published Web Location

https://doi.org/10.1063/1.5017908
Abstract

© 2018 Author(s). Diamond formation in polystyrene (C8H8)n, which is laser-compressed and heated to conditions around 150 GPa and 5000 K, has recently been demonstrated in the laboratory [Kraus et al., Nat. Astron. 1, 606-611 (2017)]. Here, we show an extended analysis and comparison to first-principles simulations of the acquired data and their implications for planetary physics and inertial confinement fusion. Moreover, we discuss the advanced diagnostic capabilities of adding high-quality small angle X-ray scattering and spectrally resolved X-ray scattering to the platform, which shows great prospects of precisely studying the kinetics of chemical reactions in dense plasma environments at pressures exceeding 100 GPa.

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