The field of high energy density (HED) materials science refers to regimes at energy densities greater than ~1012 erg/cm3 or pressures greater then ~1 Mbar, accessible on high energy, pulsed laser facilities. In this talk, a selection of experiments done on the NIF, Omega, and Omega EP lasers will be presented on a variety of materials ranging from deuterium to lead. [1-16] Examples include high pressure equations of state measurements using VISAR diagnostics; and time resolved x-ray diffraction to determine the lattice structure at high pressures. X-ray Thomson scattering has been used to characterize the ionization state, density, and temperature in HED plasma experiments. Radiography has been used to characterize the sample density and optical depth on the Hugoniot at pressures from 25 – 800 Mbar. Strength Rayleigh-Taylor instability experiments have been done in the solid state, plastic flow regime at high pressures and strain rates. Water experiments at 1-4 Mbar have observed the superionic phase whereby the oxygen freezes into a crystalline fcc lattice, whereas the H remains itinerant. And finally, EXAFS experiments for measuring sample temperatures at high pressures have been done on Omega, and are under development on NIF. Examples from the above will be given.
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Publication: [1] Celliers, Peter M., Science 361, 677-682 (2018)<br>[2] F. Coppari, in preparation (2021)<br>[3] T. Döppner, PRL 121, 025001 (2018)<br>[4] Thomas S. Duffy, Frontiers in Earth Science 7, 23 (2019)<br>[5] D.E. Fratanduono, PRL 124, 015701 (2020)<br>[6] D. Kraus PRE 94, 011202(R) (2016)<br>[7] R.G. Kraus, Nature Geoscience 8, 269 (2015)<br>[8] A. L. Kritcher, Nature 584, 51 (2020); ibid., HEDP 10, 27 (2014)<br>[9] A. Krygier, PRL 123, 205701 (2019)<br>[10] A. Lazicki, Nature 589, 532 (2021)<br>[11] M. Millot, Nature 569, 251 (2019); ibid., Nature Physics 14, 297 (2018)<br>[12] H.-S. Park, PoP 28, 060901 (2021)<br>[13] Y. Ping, PRL 111, 065501 (2013)<br>[14] B.A. Remington, PoP 22, 090501 (2015); ibid., PNAS, 116, 18233 (2019)<br>[15] J. R. Rygg, RSI 91, 043902 (2020)<br>[16] R.F. Smith, Nature Astronomy 2, 452 (2018); ibid., Nature 511, 330 (2014)
Presenters
Bruce A Remington
Lawrence Livermore National Laboratory, Lawrence Livermore Natl Lab
Authors
Bruce A Remington
Lawrence Livermore National Laboratory, Lawrence Livermore Natl Lab