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Ultrafast transient absorption spectroscopy of the charge-transfer insulator NiO: Beyond the dynamical Franz-Keldysh effect

Nicolas Tancogne-Dejean, Michael A. Sentef, and Angel Rubio
Phys. Rev. B 102, 115106 – Published 3 September 2020
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Abstract

We demonstrate that a dynamical modification of the Hubbard U in the model charge-transfer insulator NiO can be observed with state-of-the-art time-resolved absorption spectroscopy. Using a self-consistent time-dependent density functional theory plus U computational framework, we show that the dynamical modulation of screening and Hubbard U significantly changes the transient optical spectroscopy. Whereas we find the well-known dynamical Franz-Keldysh effect when the U is frozen, we observe a dynamical band-gap renormalization for dynamical U. The renormalization of the optical gap is found to be smaller than the renormalization of U. This work opens up the possibility of driving a light-induced transition from a charge transfer into a Mott insulator phase.

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  • Received 26 June 2019
  • Revised 5 February 2020
  • Accepted 16 August 2020

DOI:https://doi.org/10.1103/PhysRevB.102.115106

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. Open access publication funded by the Max Planck Society.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

Nicolas Tancogne-Dejean1,*, Michael A. Sentef1, and Angel Rubio1,2,†

  • 1Max Planck Institute for the Structure and Dynamics of Matter and Center for Free-Electron Laser Science, Luruper Chaussee 149, 22761 Hamburg, Germany
  • 2Center for Computational Quantum Physics (CCQ), The Flatiron Institute, 162 Fifth Avenue, New York 10010, New York

  • *nicolas.tancogne-dejean@mpsd.mpg.de
  • angel.rubio@mpsd.mpg.de

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Vol. 102, Iss. 11 — 15 September 2020

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