# Anomalous Thermodynamic Properties of Electron Accumulation Layer in   SrTiO$_{3}$

**Authors:** Michael Sammon, Han Fu, B. I. Shklovskii

arXiv: 1706.01179 · 2017-10-18

## TL;DR

This paper investigates the unusual thermodynamic behavior of electron accumulation layers in SrTiO$_{3}$ caused by nonlinear dielectric effects, revealing diverging properties and potential experimental probes through capacitance measurements.

## Contribution

It demonstrates how the nonlinear dielectric response leads to a long electron density tail causing divergent thermodynamic quantities and explores how sample width, dielectric constant, and back gate voltage influence these anomalies.

## Key findings

- Magnetization and specific heat diverge due to the long tail of $n(x)$.
- Finite sample width W truncates the divergence.
- Capacitance measurements can reveal the shape of the $n(x)$ tail.

## Abstract

Due to the nonlinear dielectric response within SrTiO$_{3}$ (STO), an accumulation layer created by positive charges at the surface of the STO sample ($x=0$) has an electron density profile $n(x)$ that slowly decays as $1/x^{12/7}$. Here we show that the long tail of $n(x)$ causes the magnetization and the specific heat of the accumulation layer to diverge at large $x$. We explore the truncation of the tail by the finite sample width $W$, the transition from the nonlinear to linear dielectric response with dielectric constant $\kappa$, and the use of a back gate with a negative voltage $-|V|$. We find that both the magnetization and specific heat are anomalously large and obey nontrivial power law dependences on $W$, $\kappa$, or $|V|$. We conclude with a discussion of how the capacitance as a function of the back gate voltage may be used to study the shape of the $n(x)$ tail in thin samples.

## Full text

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## Figures

9 figures with captions in the complete paper: https://tomesphere.com/paper/1706.01179/full.md

## References

39 references — full list in the complete paper: https://tomesphere.com/paper/1706.01179/full.md

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Source: https://tomesphere.com/paper/1706.01179