Isotope Effects on the Hydrogen Hugoniot
POSTER
Abstract
The equation of state of hydrogen isotopes in the warm dense matter regime is integral to understanding the evolution of gas giant planets and igniting thermonuclear fusion implosions. While gas giants like Jupiter are composed of the lightest isotope, protium, and thermonuclear fusion implosion capsules employ a mixture of deuterium and tritium, most hydrogen Hugoniot data are from deuterium. Moreover, what protium data does exist seems to deviate from modern models in the vicinity of 20 GPa. This presentation describes recent experiments to collect accurate data on the protium Hugoniot, from a few GPa into and beyond the warm dense matter regime.
Presenters
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Austin Schunke
University of Rochester
Authors
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Austin Schunke
University of Rochester
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J. Ryan Rygg
Laboratory for Laser Energetics, University of Rochester
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Gilbert W Collins
University of Rochester, Department of Physics and Astronomy, University of Rochester, Rochester, NY, United States, Laboratory for Laser Energetics, University of Rochester
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Zaire Sprowal
University of Rochester
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Alexa J LaPierre
University of Rochester
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Arnold K Schwemmlein
University of Rochester