Orbital transmutation and the electronic spectrum of FeSe in the nematic phase

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Orbital transmutation and the electronic spectrum of FeSe in the nematic phase. / Christensen, Morten H.; Fernandes, Rafael M.; Chubukov, Andrey V.

I: Physical Review Research, Bind 2, Nr. 1, 013015, 01.2020.

Publikation: Bidrag til tidsskriftTidsskriftartikelForskningfagfællebedømt

Harvard

Christensen, MH, Fernandes, RM & Chubukov, AV 2020, 'Orbital transmutation and the electronic spectrum of FeSe in the nematic phase', Physical Review Research, bind 2, nr. 1, 013015. https://doi.org/10.1103/PhysRevResearch.2.013015

APA

Christensen, M. H., Fernandes, R. M., & Chubukov, A. V. (2020). Orbital transmutation and the electronic spectrum of FeSe in the nematic phase. Physical Review Research, 2(1), [013015]. https://doi.org/10.1103/PhysRevResearch.2.013015

Vancouver

Christensen MH, Fernandes RM, Chubukov AV. Orbital transmutation and the electronic spectrum of FeSe in the nematic phase. Physical Review Research. 2020 jan.;2(1). 013015. https://doi.org/10.1103/PhysRevResearch.2.013015

Author

Christensen, Morten H. ; Fernandes, Rafael M. ; Chubukov, Andrey V. / Orbital transmutation and the electronic spectrum of FeSe in the nematic phase. I: Physical Review Research. 2020 ; Bind 2, Nr. 1.

Bibtex

@article{425fa1e778174765b0d4defb26da5cd6,
title = "Orbital transmutation and the electronic spectrum of FeSe in the nematic phase",
abstract = "We consider the electronic spectrum near M=(π,π) in the nematic phase of FeSe (T<Tnem) and make a detailed comparison with recent ARPES and STM experiments. Our main focus is the unexpected temperature dependence of the excitations at the M point. These have been identified as having xz and yz orbital character well below Tnem, but remain split at T>Tnem, in apparent contradiction to the fact that in the tetragonal phase the xz and yz orbitals are degenerate. Here we present two scenarios which can describe the data. In both scenarios, hybridization terms present in the tetragonal phase leads to an orbital transmutation, a change in the dominant orbital character of some of the bands, between T>Tnem and T≪Tnem. The first scenario relies on the spin-orbit coupling at the M point. We show that a finite spin-orbit coupling gives rise to orbital transmutation, in which one of the modes, identified as xz (yz) at T≪Tnem, becomes predominantly xy at T>Tnem and hence does not merge with the predominantly yz (xz) mode. The second scenario, complementary to the first, takes into consideration the fact that both ARPES and STM are surface probes. In the bulk, a direct hybridization between the xz and yz orbitals is not allowed at the M point, however, it is permitted on the surface. In the presence of a direct xz/yz hybridization, the orbital character of the xz/yz modes changes from pure xz and pure yz at T≪Tnem to xz±yz at T>Tnem, i.e., the two modes again have mono-orbital character at low T, but do not merge at Tnem. We discuss how these scenarios can be distinguished in polarized ARPES experiments.",
author = "Christensen, {Morten H.} and Fernandes, {Rafael M.} and Chubukov, {Andrey V.}",
note = "Publisher Copyright: {\textcopyright} 2020 authors. Published by the American Physical Society. 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.",
year = "2020",
month = jan,
doi = "10.1103/PhysRevResearch.2.013015",
language = "English",
volume = "2",
journal = "Physical Review Research",
issn = "2643-1564",
publisher = "AMER PHYSICAL SOC",
number = "1",

}

RIS

TY - JOUR

T1 - Orbital transmutation and the electronic spectrum of FeSe in the nematic phase

AU - Christensen, Morten H.

AU - Fernandes, Rafael M.

AU - Chubukov, Andrey V.

N1 - Publisher Copyright: © 2020 authors. Published by the American Physical Society. 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.

PY - 2020/1

Y1 - 2020/1

N2 - We consider the electronic spectrum near M=(π,π) in the nematic phase of FeSe (T<Tnem) and make a detailed comparison with recent ARPES and STM experiments. Our main focus is the unexpected temperature dependence of the excitations at the M point. These have been identified as having xz and yz orbital character well below Tnem, but remain split at T>Tnem, in apparent contradiction to the fact that in the tetragonal phase the xz and yz orbitals are degenerate. Here we present two scenarios which can describe the data. In both scenarios, hybridization terms present in the tetragonal phase leads to an orbital transmutation, a change in the dominant orbital character of some of the bands, between T>Tnem and T≪Tnem. The first scenario relies on the spin-orbit coupling at the M point. We show that a finite spin-orbit coupling gives rise to orbital transmutation, in which one of the modes, identified as xz (yz) at T≪Tnem, becomes predominantly xy at T>Tnem and hence does not merge with the predominantly yz (xz) mode. The second scenario, complementary to the first, takes into consideration the fact that both ARPES and STM are surface probes. In the bulk, a direct hybridization between the xz and yz orbitals is not allowed at the M point, however, it is permitted on the surface. In the presence of a direct xz/yz hybridization, the orbital character of the xz/yz modes changes from pure xz and pure yz at T≪Tnem to xz±yz at T>Tnem, i.e., the two modes again have mono-orbital character at low T, but do not merge at Tnem. We discuss how these scenarios can be distinguished in polarized ARPES experiments.

AB - We consider the electronic spectrum near M=(π,π) in the nematic phase of FeSe (T<Tnem) and make a detailed comparison with recent ARPES and STM experiments. Our main focus is the unexpected temperature dependence of the excitations at the M point. These have been identified as having xz and yz orbital character well below Tnem, but remain split at T>Tnem, in apparent contradiction to the fact that in the tetragonal phase the xz and yz orbitals are degenerate. Here we present two scenarios which can describe the data. In both scenarios, hybridization terms present in the tetragonal phase leads to an orbital transmutation, a change in the dominant orbital character of some of the bands, between T>Tnem and T≪Tnem. The first scenario relies on the spin-orbit coupling at the M point. We show that a finite spin-orbit coupling gives rise to orbital transmutation, in which one of the modes, identified as xz (yz) at T≪Tnem, becomes predominantly xy at T>Tnem and hence does not merge with the predominantly yz (xz) mode. The second scenario, complementary to the first, takes into consideration the fact that both ARPES and STM are surface probes. In the bulk, a direct hybridization between the xz and yz orbitals is not allowed at the M point, however, it is permitted on the surface. In the presence of a direct xz/yz hybridization, the orbital character of the xz/yz modes changes from pure xz and pure yz at T≪Tnem to xz±yz at T>Tnem, i.e., the two modes again have mono-orbital character at low T, but do not merge at Tnem. We discuss how these scenarios can be distinguished in polarized ARPES experiments.

UR - http://www.scopus.com/inward/record.url?scp=85085638920&partnerID=8YFLogxK

U2 - 10.1103/PhysRevResearch.2.013015

DO - 10.1103/PhysRevResearch.2.013015

M3 - Journal article

AN - SCOPUS:85085638920

VL - 2

JO - Physical Review Research

JF - Physical Review Research

SN - 2643-1564

IS - 1

M1 - 013015

ER -

ID: 398068351