Abstract
We calculate qualitatively the cohesive energy and density of metals which theoretically should condense in high-pressure systems containing high concentrations of muons and various isotopes of hydrogen. The resulting metallic forms are found to be thermally superstable suggesting that they may perhaps exist briefly and in small quantities in some stellar environments.
- Received 3 November 1969
DOI:https://doi.org/10.1103/PhysRevLett.23.1508
©1969 American Physical Society