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Mccandless, P. C.

Publications and source records attributed to Mccandless, P. C..

Electronic energy gap of molecular hydrogen from electrical conductivity measurements at high shock pressures

Electrical conductivities were measured for liquid D2 and H2 shock compressed to pressures of 10-20 GPa (100-200 kbar), molar volumes near 8 cu cm/mol, and calculated temperatures of 2900-4600 K. The semiconducting energy gap derived from the conductivities is 12 eV, in good agreement with recent quasi-particle calculations and with oscillator frequencies measured in diamond-anvil cells.

Nellis, W. J.↗

Planetary fluids at high shock pressures and temperatures

The electrical conductivity of liquid H2 was measured at shock pressures in the range 10-20 GPa and shock temperatures in the range 3000-4500 K. Electrical conductivities of H2 are needed for kinematic or dynamo calculation of the magnetic fields of Jupiter and Saturn. Conductivity measurements also enable observations of the narrowing of the electronic energy bandgap of dense H2 with density as its approaches metallization.

Nellis, W. J.↗

Interior structure of Neptune - Comparison with Uranus

Measurements of rotation rates and gravitational harmonics of Neptune made with the Voyager 2 spacecraft allow tighter constraints on models of the planet's interior. Shock measurements of material that may match the composition of Neptune, the so-called planetary 'ice', have been carried out to pressures exceeding 200 gigapascals (2 megabars). Comparison of shock data with inferred pressure-density profiles for both Uranus and Neptune shows substantial similarity through most of the mass of both planets. Analysis of the effect of Neptune's strong differential rotation on its gravitational harmonics indicates that differential rotation involves only the outermost few percent of Neptune's mass.

Hubbard, W. B.↗