Laser-driven shock compression of pre-compressed water (up to 1 GPa precompression) produces high-pressure, -temperature conditions in the water inducing two optical phenomena: opacity and reflectivity in the initially transparent water. The onset of reflectivity at infrared wavelengths can be interpreted as a semi-conductor to electronic conductor transition in water and is found at pressures above {approx}130 GPa for single-shocked samples pre-compressed to 1 GPa. This electronic conduction provides an additional contribution to the conductivity required for magnetic field generation in Icy Giant planets like Uranus and Neptune
The study of planetary interiors is a key concern for the purpose of providing a unified framework a...
We present some preliminary results on the equation of state (EOS) of water in a pressure regime of...
International audienceAmmonia is predicted to be one of the major components in the depths of the ic...
Laser-driven shock compression of samples precompressed to 1 GPa produces high-pressure-temperature ...
Laser-driven shock compression of samples precompressed to 1 GPa produces high-pressure-temperature...
The optical reflectance of a strong shock front in water increases continuously with pressure above ...
The interiors of Neptune and Uranus are believed to be primarily composed of a fluid mixture of meth...
An accurate equation of state (EOS) for planetary constituents at extreme conditions is the key to a...
In order to derive models of the interiors of Uranus, Neptune, Jupiter and Saturn, researchers studi...
Characterising the behaviour of planetary interiors’ components at extreme conditions (megabar press...
International audienceWater, methane, and ammonia are commonly considered to be the key components o...
High power lasers are a tool that can be used to determine important parameters in the context of wa...
The study of planetary interiors is a key concern for the purpose of providing a unified framework a...
We present some preliminary results on the equation of state (EOS) of water in a pressure regime of...
International audienceAmmonia is predicted to be one of the major components in the depths of the ic...
Laser-driven shock compression of samples precompressed to 1 GPa produces high-pressure-temperature ...
Laser-driven shock compression of samples precompressed to 1 GPa produces high-pressure-temperature...
The optical reflectance of a strong shock front in water increases continuously with pressure above ...
The interiors of Neptune and Uranus are believed to be primarily composed of a fluid mixture of meth...
An accurate equation of state (EOS) for planetary constituents at extreme conditions is the key to a...
In order to derive models of the interiors of Uranus, Neptune, Jupiter and Saturn, researchers studi...
Characterising the behaviour of planetary interiors’ components at extreme conditions (megabar press...
International audienceWater, methane, and ammonia are commonly considered to be the key components o...
High power lasers are a tool that can be used to determine important parameters in the context of wa...
The study of planetary interiors is a key concern for the purpose of providing a unified framework a...
We present some preliminary results on the equation of state (EOS) of water in a pressure regime of...
International audienceAmmonia is predicted to be one of the major components in the depths of the ic...