Wendy Mao1,2, Ho-kwang Mao2, Alexander Goncharov2, Viktor Struzhkin2, Quanzhong Guo2, Jingzhu Hu2, Jinfu Shu2, Russell J. Hemley2, Maddury Somayazulu3, Konstantin Lokshin4, & Yusheng Zhao4
1U of Chicago,
2Geophysical Lab, CIW,
3HPCAT, APS,
4LANSCE, LANL
wmao@uchicago.edu
NSLS-X17B (DAC)
Clathrates have attracted attention because of their fundamental physical and chemical significance and their applications to energy, environmental, and astrophysical issues. High-pressure Raman, infrared, x-ray, and neutron studies show that H2 and H2O mixtures crystallize into the sII clathrate structure with an extremely high hydrogen content (H2/H2O ~ 1:2). The clathrate cages are multiply occupied, i.e., a cluster of two H2 molecules in the small cage and four in the large cage. Substantial softening of hydrogen vibrons indicates increased intermolecular interactions. The quenched clathrate is stable up to 145 K at ambient pressure. Retention of hydrogen at such high temperatures could greatly help its condensation in planetary nebulae and play a key role in the evolution of icy bodies.