Charge transport in a polar metal
The fate of electric dipoles inside a Fermi sea is an old issue, yet poorly explored. Sr 1 − x Ca x TiO 3 hosts a robust but dilute ferroelectricity in a narrow ( 0.0018 < x < 0.02 ) window of substitution. This insulator becomes metallic by removal of a tiny fraction of its oxygen atoms. Here...
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Veröffentlicht in: | npj quantum materials 2019-12, Vol.4 (1), Article 61 |
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Format: | Artikel |
Sprache: | eng |
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Zusammenfassung: | The fate of electric dipoles inside a Fermi sea is an old issue, yet poorly explored. Sr
1
−
x
Ca
x
TiO
3
hosts a robust but dilute ferroelectricity in a narrow (
0.0018
<
x
<
0.02
) window of substitution. This insulator becomes metallic by removal of a tiny fraction of its oxygen atoms. Here, we present a detailed study of low-temperature charge transport in Sr
1
−
x
Ca
x
TiO
3
−
δ
, documenting the evolution of resistivity with increasing carrier concentration (
n
). Below a threshold carrier concentration,
n
*
(
x
)
, the polar structural-phase transition has a clear signature in resistivity and Ca substitution significantly reduces the 2 K mobility at a given carrier density. For three different Ca concentrations, we find that the phase transition fades away when one mobile electron is introduced for about
7.9
±
0.6
dipoles. This threshold corresponds to the expected peak in anti-ferroelectric coupling mediated by a diplolar counterpart of Ruderman–Kittel–Kasuya–Yosida (RKKY) interaction. Our results imply that the transition is driven by dipole–dipole interaction, even in presence of a dilute Fermi sea. Charge transport for
n
<
n
*
(
x
)
shows a non-monotonic temperature dependence, most probably caused by scattering off the transverse optical phonon mode. A quantitative explanation of charge transport in this polar metal remains a challenge to theory. For
n
≥
n
*
(
x
)
, resistivity follows a T-square behavior together with slight upturns (in both Ca-free and Ca-substituted samples). The latter are reminiscent of Kondo effect and most probably due to oxygen vacancies. |
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ISSN: | 2397-4648 2397-4648 |
DOI: | 10.1038/s41535-019-0200-1 |