# Dipolar Spin Ice Under Uniaxial Pressure

**Authors:** Richard Edberg, Lise {\O}rduk Sandberg, Ingrid Marie Bergh Bakke,, Morten Lunn Haubro, Lucile Mangin-Thro, Malcolm Guthrie, Alexander Holmes,, Magnus S{\o}rby, Kim Lefmann, Pascale Petronella Deen, Patrik Henelius

arXiv: 1907.03638 · 2019-10-30

## TL;DR

This study investigates how uniaxial pressure influences the magnetic ordering in classical spin ice materials, combining theoretical modeling and neutron scattering experiments to reveal pressure-induced transitions and the role of dipolar interactions.

## Contribution

The paper presents a combined theoretical and experimental analysis of pressure effects on spin ice, highlighting the impact of dipolar interactions on pressure-induced magnetic ordering transitions.

## Key findings

- Pressure induces magnetic ordering in Dy2Ti2O7.
- Dipolar interactions significantly influence the transition.
- Experimental neutron data aligns with theoretical predictions.

## Abstract

The magnetically frustrated spin ice family of materials is host to numerous exotic phenomena such as magnetic monopole excitations and macroscopic residual entropy extending to low temperature. A finite-temperature ordering transition in the absence of applied fields has not been experimentally observed in the classical spin ice materials Dy2Ti2O7 and Ho2Ti2O7. Such a transition could be induced by the application of pressure, and in this work we consider the effects of uniaxial pressure on classical spin ice systems. Theoretically we find that the pressure induced ordering transition in Dy2Ti2O7 is strongly affected by the dipolar interaction. We also report measurements on the neutron structure factor of Ho2Ti2O7 under pressure, and compare the experimental results to the predictions of our theoretical model.

## Full text

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## Figures

21 figures with captions in the complete paper: https://tomesphere.com/paper/1907.03638/full.md

## References

28 references — full list in the complete paper: https://tomesphere.com/paper/1907.03638/full.md

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Source: https://tomesphere.com/paper/1907.03638