通过 ARPES 和 XAS 研究 PrTen(n=2,3)和 ErTe3 中不同的电荷密度波不稳定性

IF 3.1 3区 材料科学 Q2 MATERIALS SCIENCE, MULTIDISCIPLINARY
J.-S. Kang, Seungho Seong, Eunsook Lee, Y. S. Kwon, Kyoo Kim, Junwon Kim, Heejung Kim, B. I. Min
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In this research update, we have investigated the electronic structures of <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><msub><mi>PrTe</mi><mi>n</mi></msub></math> (<math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mrow><mi>n</mi><mo>=</mo><mn>2</mn></mrow></math>, 3) and <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><msub><mi>ErTe</mi><mn>3</mn></msub></math> layered CDW compounds employing angle-resolved photoemission spectroscopy (ARPES) and soft x-ray absorption spectroscopy (XAS). The trivalent valency of <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><msup><mi>R</mi><mrow><mn>3</mn><mo>+</mo></mrow></msup></math> ions is confirmed for <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><msub><mi>PrTe</mi><mi>n</mi></msub></math> (<math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mrow><mi>n</mi><mo>=</mo><mn>2</mn></mrow></math>, 3) and <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><msub><mi>ErTe</mi><mn>3</mn></msub></math>, supporting that <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mi>R</mi></math>-Te slabs serve as charge reservoirs and that the CDW instability occurs in the partially filled Te sheets. Both <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mrow><mi>R</mi><mspace width=\"4pt\"></mspace><mn>4</mn><mi>d</mi><mo>→</mo><mn>4</mn><mi>f</mi></mrow></math> resonant photoemission spectroscopy and photon-energy map measurements provide evidence that <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mrow><mi>R</mi><mspace width=\"4pt\"></mspace><mn>4</mn><mi>f</mi></mrow></math> electrons do not contribute directly to the CDW formation but that the indirect contribution from Pr <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mrow><mn>4</mn><mi>f</mi></mrow></math> electrons through the Pr <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mrow><mn>4</mn><mi>f</mi><mo>−</mo><mi>Te</mi></mrow><mo> </mo><mrow><mn>5</mn><mi>p</mi></mrow></math> hybridization is feasible in <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><msub><mi>PrTe</mi><mi>n</mi></msub></math> (<math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mrow><mi>n</mi><mo>=</mo><mn>2</mn></mrow></math>, 3). Circular and linear dichroism ARPES measurements indicate that the chirality of the Te <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mrow><mn>5</mn><mi>p</mi></mrow></math> orbitals certainly plays a role in the CDW formation of <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mrow><mi>R</mi><msub><mi>Te</mi><mn>3</mn></msub></mrow></math> (<math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mrow><mi>R</mi><mo>=</mo><mi>Pr</mi></mrow></math>, Er) while it is relatively weak in <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><msub><mi>PrTe</mi><mn>2</mn></msub></math>, and that the <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><msub><mi>E</mi><mi mathvariant=\"normal\">F</mi></msub></math>-crossing orbitals, responsible for the CDW formation, are ordered in plane (in the <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mrow><mi>a</mi><mi>c</mi></mrow></math> plane) in all of them. 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The trivalent valency of <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><msup><mi>R</mi><mrow><mn>3</mn><mo>+</mo></mrow></msup></math> ions is confirmed for <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><msub><mi>PrTe</mi><mi>n</mi></msub></math> (<math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mrow><mi>n</mi><mo>=</mo><mn>2</mn></mrow></math>, 3) and <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><msub><mi>ErTe</mi><mn>3</mn></msub></math>, supporting that <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mi>R</mi></math>-Te slabs serve as charge reservoirs and that the CDW instability occurs in the partially filled Te sheets. Both <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mrow><mi>R</mi><mspace width=\\\"4pt\\\"></mspace><mn>4</mn><mi>d</mi><mo>→</mo><mn>4</mn><mi>f</mi></mrow></math> resonant photoemission spectroscopy and photon-energy map measurements provide evidence that <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mrow><mi>R</mi><mspace width=\\\"4pt\\\"></mspace><mn>4</mn><mi>f</mi></mrow></math> electrons do not contribute directly to the CDW formation but that the indirect contribution from Pr <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mrow><mn>4</mn><mi>f</mi></mrow></math> electrons through the Pr <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mrow><mn>4</mn><mi>f</mi><mo>−</mo><mi>Te</mi></mrow><mo> </mo><mrow><mn>5</mn><mi>p</mi></mrow></math> hybridization is feasible in <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><msub><mi>PrTe</mi><mi>n</mi></msub></math> (<math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mrow><mi>n</mi><mo>=</mo><mn>2</mn></mrow></math>, 3). 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引用次数: 0

摘要

了解层状 RTen (n=2, 3) 化合物(R,稀土元素)中不同电荷密度波 (CDW) 不稳定性的起源一直是一个重要问题。在这项最新研究中,我们采用角分辨光发射光谱(ARPES)和软 X 射线吸收光谱(XAS)研究了 PrTen (n=2, 3) 和 ErTe3 层状 CDW 化合物的电子结构。在 PrTen(n=2,3)和 ErTe3 中,R3+ 离子的三价性得到了证实,证明了 R-Te 板是电荷库,而 CDW 的不稳定性发生在部分填充的 Te 片中。R4d→4f 共振光发射光谱和光能图测量结果都证明,R4f 电子并不直接参与 CDW 的形成,但 Pr 4f 电子通过 Pr 4f-Te 5p 杂化间接参与 CDW 的形成在 PrTen(n=2,3)中是可行的。环向和线性二色性 ARPES 测量结果表明,Te 5p 轨道的手性在 RTe3(R=Pr,Er)的 CDW 形成中肯定起了作用,而在 PrTe2 中则相对较弱。RTe3 和 RTe2 中不同的 CDW 引发的费米面重构是由于:(i) RTe3 和 RTe2 中每个单位晶胞分别存在两个 Te 片和一个 Te 片,因此产生的空穴载流子数量不同;(ii) RTen 中 Te 片的晶格参数不同,导致 EF 处的态密度不同。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Distinct charge density wave instabilities in PrTen (n=2, 3) and ErTe3 investigated via ARPES and XAS

Distinct charge density wave instabilities in PrTen (n=2, 3) and ErTe3 investigated via ARPES and XAS
Understanding the origin of distinct charge density wave (CDW) instabilities in layered RTen (n=2, 3) compounds (R, rare earth element) has been an important issue. In this research update, we have investigated the electronic structures of PrTen (n=2, 3) and ErTe3 layered CDW compounds employing angle-resolved photoemission spectroscopy (ARPES) and soft x-ray absorption spectroscopy (XAS). The trivalent valency of R3+ ions is confirmed for PrTen (n=2, 3) and ErTe3, supporting that R-Te slabs serve as charge reservoirs and that the CDW instability occurs in the partially filled Te sheets. Both R4d4f resonant photoemission spectroscopy and photon-energy map measurements provide evidence that R4f electrons do not contribute directly to the CDW formation but that the indirect contribution from Pr 4f electrons through the Pr 4fTe 5p hybridization is feasible in PrTen (n=2, 3). Circular and linear dichroism ARPES measurements indicate that the chirality of the Te 5p orbitals certainly plays a role in the CDW formation of RTe3 (R=Pr, Er) while it is relatively weak in PrTe2, and that the EF-crossing orbitals, responsible for the CDW formation, are ordered in plane (in the ac plane) in all of them. Different CDW-induced Fermi surface reconstructions between RTe3 and RTe2 are due to (i) the existence of two Te sheets and one Te sheet per unit cell in RTe3 and RTe2, respectively, so as to produce different numbers of hole carriers, and (ii) the different lattice parameters of Te sheets in RTen, leading to the different densities of states at EF.
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来源期刊
Physical Review Materials
Physical Review Materials Physics and Astronomy-Physics and Astronomy (miscellaneous)
CiteScore
5.80
自引率
5.90%
发文量
611
期刊介绍: Physical Review Materials is a new broad-scope international journal for the multidisciplinary community engaged in research on materials. It is intended to fill a gap in the family of existing Physical Review journals that publish materials research. This field has grown rapidly in recent years and is increasingly being carried out in a way that transcends conventional subject boundaries. The journal was created to provide a common publication and reference source to the expanding community of physicists, materials scientists, chemists, engineers, and researchers in related disciplines that carry out high-quality original research in materials. It will share the same commitment to the high quality expected of all APS publications.
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