Non-RPA behavior of the valence plasmon in SrTi1−𝑥⁢ Nb𝑥⁢O3

Caitlin S. Kengle, Samantha I. Rubeck, Melinda Rak, Jin Chen, Faren Hoveyda, Simon Bettler, Ali Husain, Matteo Mitrano, Alexander Edelman, Peter Littlewood, Tai Chang Chiang, Fahad Mahmood, Peter Abbamonte*

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract

Doped SrTi1-x NbxO3 is a dilute polaronic metal that exhibits superconductivity and a mid-infrared optical response suggesting parallels with copper oxides. A peculiar feature of SrTi1-x NbxO3 is that its plasma frequency, ωp, is highly temperature dependent, increasing by more than a factor of 2 when the system is cooled from 300 to 100 K [F. Gervais et al., Phys. Rev. B 47, 8187 (1993); D. M. Eagles et al., Phys. Rev. B 54, 22 (1996); C. Z. Bi et al., J. Phys.: Condens. Matter 18, 2553 (2006). There is still no generally accepted explanation for this dramatic shift. Here, we present momentum-resolved electron energy-loss spectroscopy measurements of SrTi1-x NbxO3 at nonzero momentum, q. We also calculate the collective excitations of SrTi1-x NbxO3 using the random phase approximation (RPA), to assess whether the behavior of the collective modes conforms to established explanations. We find that the plasmon energy and linewidth are momentum independent, in contrast to RPA predictions, and that its shift with temperature takes place everywhere in the Brillouin zone, from q=0 to the zone boundary, q=0.5 reciprocal lattice units. We also find that the phonon frequencies do not shift with q in the expected way, suggesting the screening properties of the material deviate significantly from RPA predictions. We conclude that a radically different starting point, perhaps based on lattice anharmonicity, may be needed to explain the collective charge excitations of SrTi1-x NbxO3.

Original languageEnglish
Article number205102
Number of pages9
JournalPhysical Review B - Condensed Matter and Materials Physics
Volume108
Issue number20
Early online date1 Nov 2023
DOIs
Publication statusPublished - 15 Nov 2023

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