Experimental Pathways for Detecting Double Superionicity in Planetary Ices
Journal Article
·
· Contributions to Plasma Physics
- University of California, Berkeley, CA (United States)
The ice giant planets Uranus and Neptune are assumed to contain large amounts of planetary ices such as water, methane, and ammonia. The properties of mixtures of such ices at the extreme pressures and temperatures of planetary interiors are not yet well understood. Ab initio computer simulations have predicted that a number of ices exhibit a hydrogen superionic state and a doubly superionic state. Since the latter state has not yet been generated with experiments, we outline here two possible pathways for reaching and detecting such a state with dynamic compression experiments. Here, we suggest X-ray diffraction as the principal tool for detecting when the material becomes doubly superionic and the sublattice of one of the heavy nuclei melts. That would require a temperature of ~3500 K and pressures greater than ~200 GPa for H3NO4, which we use as an example material here. Such conditions can be reached with experiments that employ an initial shock that is followed by a ramp compression wave. Alternatively, one may use triple-shock compression because a single shock does not yield sufficiently high densities.
- Research Organization:
- University of California, San Diego, La Jolla, CA (United States)
- Sponsoring Organization:
- USDOE National Nuclear Security Administration (NNSA)
- Grant/Contract Number:
- NA0004147
- OSTI ID:
- 2568779
- Journal Information:
- Contributions to Plasma Physics, Journal Name: Contributions to Plasma Physics; ISSN 0863-1042; ISSN 1521-3986
- Publisher:
- WileyCopyright Statement
- Country of Publication:
- United States
- Language:
- English
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