Abstract

The nature of the hydrogen sublattice of an HCl-doped ice VI sample after cooling at 1.8 GPa has been a topic of recent interest. The samples are interpreted either as the new H-ordered ice phase ice β-XV with a thermodynamic stability region in the phase diagram [T. M. Gasser et al., Chem. Sci., 2018, 9, 4224], or alternatively as H-disordered, deep glassy ice VI [A. Rosu-Finsen and C. G. Salzmann, Chem. Sci., 2019, 10, 515]. Here we provide a comprehensive Raman spectroscopic study on ice β-XV, ice XV and ice VI, with the following key findings: (i) the Raman spectra of ice β-XV differ fundamentally from those of ice VI and ice XV, where the degree of H-order is even higher than in ice XV. (ii) Upon cooling ice VI there is competition between formation of ice XV and ice β-XV domains, where ice XV forms at 0.0 GPa, but ice β-XV at 1.8 GPa. Domains of ice β-XV are present in literature "ice XV" at 1.0 GPa. This result clarifies the puzzling earlier observation that the degree of H-order in ice XV apparently improves upon heating and recooling at ambient pressure. In reality, this procedure leaves the H-order in ice XV unaffected, but removes ice β-XV domains by transforming them to ice XV. (iii) Upon heating, the samples experience the transition sequence ice β-XV → ice XV → ice VI, i.e., an order-order transition at 103 K followed by an order-disorder transition at 129 K. The former progresses via a disordered transient state. (iv) D2O ice β-XV forms upon cooling DCl-doped D2O-ice VI, albeit at a much lower pace than in the hydrogenated case so that untransformed D2O ice VI domains are present even after slow cooling. The librational band at 380 cm-1 is identified to be the characteristic spectroscopic feature of deuterated ice β-XV. Taken together these findings clarify open questions in previous work on H-ordering in the ice VI lattice, rule out a glassy nature of ice β-XV and pave the way for a future neutron diffraction study to refine the crystal structure of D2O ice β-XV.

Highlights

  • Polymorphism in H2O-ices is intimately linked with hydrogen and oxygen atom order.[1,2,3,4,5,6,7] An ice polymorph may transform from an H-disordered high-temperature variant to its H-ordered low-temperature proxy, while the network of O-atoms is barely affected.[8]

  • We have investigated the question of how to clearly differentiate between a new H-ordered ice and deep glassy, H-disordered ice

  • We demonstrate that Raman spectroscopy is suitable to discriminate between H-order and H-disorder, as done in previous studies, and to discriminate between distinct types of H-order

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Summary

Introduction

An interesting phenomenon was observed by heating ice XV at (sub)ambient pressure from 77 K to T o To–d, followed by recooling to liquid nitrogen temperature.[1,5,14,15] While for all other H-ordered ices the degree of order is not affected upon 15452 | Phys. Thereby, one has to keep in mind that such a ferroelectric hydrogen ordering would oppose the antiferroelectric hydrogen ordering of ice XV.[10,14] calculations reveal that there is close competition between the structure with the strongest local hydrogen bonding (ferroelectric Cc structure)[19] and the one with the most favorable ‘‘delocalized’’ hydrogen bond cooperativity effects (antiferroelectric P1% structure).[20,21] Raman spectra calculated for the antiferroelectric structure by DFT14 are ‘‘in essential agreement with experimental spectra of ice XV’’, and so are the calculated structures for this structure by MB-MD.[22] This explanation leaves some room for speculation, which prompted Gasser et al to investigate the influence of pressure and cooling rate on H-ordering quantitatively and systematically.[1] By combining X-ray, differential scanning calorimetry (DSC), Ramanand dielectric relaxation spectroscopy experiments they identified a different cause for the complex behaviour that was not observed for any other ice polymorph before. They are more convenient to describe H-bonding than coupled OH-bonds and can, better be distinguished by substructure.[30]

Results
Section 2: the influence of pressure
Section 3: ice b-XV upon heating
Conclusion
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