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  1. 原著論文

Chemical and orbital fluctuations in Ba3CuSb2O9

https://repo.qst.go.jp/records/47956
https://repo.qst.go.jp/records/47956
3f33b71a-b685-40fc-8adc-fa2881753c93
Item type 学術雑誌論文 / Journal Article(1)
公開日 2017-05-22
タイトル
タイトル Chemical and orbital fluctuations in Ba3CuSb2O9
言語
言語 eng
資源タイプ
資源タイプ識別子 http://purl.org/coar/resource_type/c_6501
資源タイプ journal article
アクセス権
アクセス権 metadata only access
アクセス権URI http://purl.org/coar/access_right/c_14cb
著者 Wakabayashi, Yusuke

× Wakabayashi, Yusuke

WEKO 481456

Wakabayashi, Yusuke

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Nakajima, Daisuke

× Nakajima, Daisuke

WEKO 481457

Nakajima, Daisuke

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Ishiguro, Yuki

× Ishiguro, Yuki

WEKO 481458

Ishiguro, Yuki

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Kimura, Kenta

× Kimura, Kenta

WEKO 481459

Kimura, Kenta

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Kimura, Tsuyoshi

× Kimura, Tsuyoshi

WEKO 481460

Kimura, Tsuyoshi

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Tsutsui, Satoshi

× Tsutsui, Satoshi

WEKO 481461

Tsutsui, Satoshi

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Q., R. Baron Alfred

× Q., R. Baron Alfred

WEKO 481462

Q., R. Baron Alfred

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Hayashi, Kouichi

× Hayashi, Kouichi

WEKO 481463

Hayashi, Kouichi

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Happo, Naohisa

× Happo, Naohisa

WEKO 481464

Happo, Naohisa

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Hosokawa, Shinya

× Hosokawa, Shinya

WEKO 481465

Hosokawa, Shinya

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大和田, 謙二

× 大和田, 謙二

WEKO 481466

大和田, 謙二

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Nakatsuji, Satoru

× Nakatsuji, Satoru

WEKO 481467

Nakatsuji, Satoru

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大和田 謙二

× 大和田 謙二

WEKO 481468

en 大和田 謙二

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抄録
内容記述タイプ Abstract
内容記述 Structural fluctuation in Ba3CuSb2O9, which is proposed to exhibit a spin-orbital entangled state, has been studied by diffuse x-ray scattering, x-ray fluorescence holography, and inelastic x-ray scattering. Two kinds of spatial fluctuations are observed: temperature-independent and temperature-dependent ones. The former is related to Cu/Sb arrangement. The short-range chemical correlation in Ba3CuSb2O9 is honeycomblike, whereas the correlation length is as short as the diameter of the honeycomb unit. The temperature variation of ferro- and antiferro-orbital correlations is extracted from Huang scattering intensity distributions. Both of these correlations increase with decreasing temperature down to 60 K, which corresponds to the energy of magnetic interaction of Ba3CuSb2O9. A wide distribution of the characteristic time scale of the orbital motion is proposed from the spatial fluctuation of the ionic arrangement in Ba3CuSb2O9.
書誌情報 Physical Review B

巻 93, 号 24, p. 245117, 発行日 2016-07
出版者
出版者 American Physical Society
ISSN
収録物識別子タイプ ISSN
収録物識別子 2469-9950
DOI
識別子タイプ DOI
関連識別子 10.1103/PhysRevB.93.245117
関連サイト
識別子タイプ URI
関連識別子 http://journals.aps.org/prb/abstract/10.1103/PhysRevB.93.245117
関連名称 http://journals.aps.org/prb/abstract/10.1103/PhysRevB.93.245117
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