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Topologically frustrated ionisation in a water-ammonia ice mixture
C Liu1,2, A Mafety1, J A Queyroux1
1Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie (IMPMC), Sorbonne Universités-UPMC Univ. Paris 6, CNRS UMR 7590, IRD UMR 206, MNHN, 4 Place Jussieu, F-75005, Paris, France.
Ammonia monohydrate transforms into a mix of neutral and ionic species at moderate pressures. This study reveals unique high-pressure behavior of water and ammonia mixtures, crucial for understanding icy planet interiors.
Area of Science:
- Planetary Science
- Materials Science
- Physical Chemistry
Background:
- Water and ammonia are key components in icy planet interiors.
- High pressures reveal exotic phases of pure water and ammonia ices.
Purpose of the Study:
- Investigate the high-pressure properties of ammonia monohydrate.
- Understand the phase behavior of equimolar water-ammonia mixtures.
Main Methods:
- Experimental study of ammonia monohydrate under high P-T conditions.
- Ab initio atomistic simulations to model phase behavior.
Main Results:
- Ammonia monohydrate transforms at 7.4 GPa and 300 K.
- Coexistence of neutral water/ammonia with hydroxide and ammonium ions observed.
- Topological frustration explains the neutral/ionic species coexistence.
Conclusions:
- Mild pressures induce significant chemical changes in ammonia monohydrate.
- The findings provide insights into the interior composition of icy celestial bodies.
- This work highlights complex ionisation mechanisms in planetary ices.
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