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Direct evidence of real-space pairing in BaBiO3

A. P. Menushenkov, A. Ivanov, V. Neverov, A. Lukyanov, A. Krasavin, A. A. Yastrebtsev, I. A. Kovalev, Y. Zhumagulov, A. V. Kuznetsov, V. Popov, G. Tselikov, I. Shchetinin, O. Krymskaya, A. Yaroslavtsev, R. Carley, L. Mercadier, Z. Yin, S. Parchenko, L. P. Hoang, N. Ghodrati, Y. Y. Kim, J. Schlappa, M. Izquierdo, S. Molodtsov, and A. Scherz
Phys. Rev. Research 6, 023307 – Published 21 June 2024

Abstract

The parent compound BaBiO3 of bismuthate high-temperature superconductors (HTSCs) BaBi(Pb)O3 and Ba(K)BiO3 with perovskitelike structure exhibits unusual electronic and structural properties, which can be satisfactorily explained if we assume that all charge carriers are in the paired state. However, the prior experiments and the first-principle calculations only indirectly indicate the existence of paired charge carriers in BaBiO3. In this work, we report the direct evidence of initially paired electrons and holes in the upper antibonding Bi 6sO2pσ* orbital of the neighboring octahedral complexes in the ground state of BaBiO3 using the time-resolved x-ray absorption spectroscopy (XAS) to monitor the electron dynamics after the femtosecond resonant 633 nm laser excitation. We observe strong changes in the oxygen K-edge XAS preedge region, defined by the Bi6sO2pσ* orbitals. We interpret them as a fast (0.3 ps) breaking of charge carrier pairs and slower (0.3–0.8 ps) lattice rearrangement from the distorted monoclinic structure into the new metastable state with a cubic lattice, which persists at least up to 60 ps after the excitation. Analysis of the intermediate state at the fast excitation shows that the bond disproportionation and monoclinic distortion of BaBiO3 structure are energetically favorable due to the charge carrier pairing. Thus the compound BaBiO3 forms a new quantum state that we define as a local pair density wave. Taking into account a large number of similarities between bismuthate and cuprate high-temperature superconductors, we believe that our work will give a new impetus to understanding the nature of superconductivity in perovskite HTSCs.

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  • Received 13 December 2023
  • Revised 29 March 2024
  • Accepted 17 May 2024

DOI:https://doi.org/10.1103/PhysRevResearch.6.023307

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

A. P. Menushenkov1,*, A. Ivanov1, V. Neverov1, A. Lukyanov1, A. Krasavin1, A. A. Yastrebtsev1, I. A. Kovalev1, Y. Zhumagulov2, A. V. Kuznetsov1, V. Popov1, G. Tselikov3, I. Shchetinin4, O. Krymskaya1, A. Yaroslavtsev5, R. Carley6, L. Mercadier6, Z. Yin6, S. Parchenko6, L. P. Hoang6, N. Ghodrati6, Y. Y. Kim6, J. Schlappa6, M. Izquierdo6, S. Molodtsov6,7,8, and A. Scherz6

  • *Corresponding author: menushen@gmail.com

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Vol. 6, Iss. 2 — June - August 2024

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