Impact factor of Chinese Physics C is 3.6 in 2023 Impact factor of Chinese Physics C is 3.6 in 2022 2021 Impact Factor 2.944
Advanced Search
×
近期发现有不法分子冒充我刊与作者联系，借此进行欺诈等不法行为，请广大作者加以鉴别，如遇诈骗行为，请第一时间与我刊编辑部联系确认（《中国物理C》（英文）编辑部电话：010-88235947,010-88236950），并作报警处理。
本刊再次郑重声明：
（1）本刊官方网址为cpc.ihep.ac.cn和https://iopscience.iop.org/journal/1674-1137
（2）本刊采编系统作者中心是投稿的唯一路径，该系统为ScholarOne远程稿件采编系统，仅在本刊投稿网网址（https://mc03.manuscriptcentral.com/cpc）设有登录入口。本刊不接受其他方式的投稿，如打印稿投稿、E-mail信箱投稿等，若以此种方式接收投稿均为假冒。
（3）所有投稿均需经过严格的同行评议、编辑加工后方可发表，本刊不存在所谓的“编辑部内部征稿”。如果有人以“编辑部内部人员”名义帮助作者发稿，并收取发表费用，均为假冒。
                  
《中国物理C》（英文）编辑部
2024年10月30日
Chinese Physics C> 2003, Vol. 27> Issue(S1) : 72-76 

Perovskite (Pbnm) structures transformations at high pressure

  •  Beijing Synchrotron Radiation Facility,Institute of High Energy Physics,CAS,Beijing 100039,China2 Department of Geology,Peking University,Beijing 100871,China

  • Perovskite type compounds of general formula ABX3 have the most commonly adopted structure (Pbnm),to some extent distorted from the ideal structure Pm3m.Their structures transformations are diverse at high pressure.Three parameters (t,VA/VB,Etot),which are used to describe the stabilization of perovskite structures,are introduced briefly.Applied threeparameters,all models of perovskite structure (Pbnm) changing at high pressure are summed up.Some of the models suit all perovskites structures.As an example,CaTiO3 (Pbnm) structure changing at high pressure is analyzed by applying several models and qualitatively draws a conclusion that the structure symmetry is reduced with enhancing the pressure.
  • 加载中

  • References

    [1] Dobal P S, Dixit A, Katiyar R S et al. J. Appl. Phys.2001,89 80852 Watanabe S,Koyama Y. Phys. Rev.,2002, B66:1341023 Sleight A W,Cillson J L, Bierstedt P E. Solid State Commun. 1975,17:274 Fontcuberta J, Martinez B,Seffar A et al. Phys. Rev. Lett.,1996 76:11225 Hearne G R, Pasternak M P, Taylor R D et al. Phys. Rev.,1995 51:114956 Glazer A M. Acta Cryst.,1972,B28;33847 Glazer A M. Acta Cryst.,1975,A31 ;7568 Ranjan R, Padey D, Siruguri V et al. J. Phys.:Condensed Matter 1999,11;22339 Redfern S A T. J. Phys.:Condensed Matter, 1996,8:826710 Kennedy B J, Hunter B A. Phys. Rev.,1998,B58:65311 Kennedy B J, Howard C J, Chakoumakos B C et al. Phys. Rev. 1999,B59:402312 Venkateswaran U D, Naik V M,Naik R. Phys. Rev.,1998,B58:1425613 Sani A,Hanfland M,Levy D. J. Phys.:Condensed Matter, 2002 14:1060114 Bouvier P,Kreisel J. J. Phys.:Condensed Matter, 2002, 14:398115 Ming L T, Eto T, Takeda K et al. J. Phys :Condensed Matter:2002,14:1047516 Kudoh Y, Ito E,Takeda. Phys. Chem. Miner.,1987,14:35017 Yamanaka T, Hirai N,Komatsu Y. Amer. Miner.，2002，87:118318 Magyari-Kope B, Vitos L，Johansson B et al. Acta Cryst.，2001，B57:49119 Magyari-Kope B, Vitos L，Johansson B et al. Comput. Mater.Sci.，2002 25:61520 Magyari-Kope B，Vitos L, Johansson B et al. Phys. Rev.，2002,B66:09210321 Shannon R D. Acta Cryst.，1976，A32:75122 Thomas N W. Acta Cryst.，1996，B52:1623 Thomas N W. Acta Cryst.，1998，B54:58524 Zunic T B,Vickovic I. J. Appl. Cryst.，1996，29:30525 Blaha P, Schwarz K，Madsen G et al. WIEN2K-Users Guide,2002:http;//www. wien2k. at/ reg_user/textbooks/26 Howard C J,Stokes H T. Acta Cryst.，1998，B54:78227 Muscat J, Swamy V, Harrison N M. Phys. Rev.，2002，B65:22411228 Lindbaum A, Heathman S, Kresses G et al. J. Phys.:Condensed Matter, 2000, 12:321929 WU X, QIN S, WU Z Y et al. Acta Phys. Sin (in Chinese. in press)(巫翔，秦善，吴白玉等.物理学报，(待发表))30 XIONC D H，MINC L C，Manghnani M H. Phys. Earth. Planet.Inte.，1986, 43:24431 Cillet P, Cuyot F, Price C D et al. Phys. Chem. Miner.，1993，20:15932 Ross N L, Angel R J. Amer Miner.，1999，84:277

  • Access

    加载中

Get Citation
WU Xiang, QIN Shan, WU Zi-Yu, DONG Yu-Hui, LIU Jing and LI Xiao-Dong. Perovskite (Pbnm) structures transformations at high pressure[J]. Chinese Physics C, 2003, 27(S1): 72-76.
WU Xiang, QIN Shan, WU Zi-Yu, DONG Yu-Hui, LIU Jing and LI Xiao-Dong. Perovskite (Pbnm) structures transformations at high pressure[J]. Chinese Physics C, 2003, 27(S1): 72-76. shu
Milestone
Received: 2003-11-21
Revised: 1900-01-01
Article Metric

Article Views(3097)
PDF Downloads(615)
Cited by(0)
Policy on re-use
To reuse of subscription content published by CPC, the users need to request permission from CPC, unless the content was published under an Open Access license which automatically permits that type of reuse.
通讯作者: 陈斌, [email protected]
  • 1. 

    沈阳化工大学材料科学与工程学院 沈阳 110142

  1. 本站搜索
  2. 百度学术搜索
  3. 万方数据库搜索
  4. CNKI搜索

Email This Article

Title:
Email:

Perovskite (Pbnm) structures transformations at high pressure

    Corresponding author: WU Xiang,
  • Beijing Synchrotron Radiation Facility,Institute of High Energy Physics,CAS,Beijing 100039,China2 Department of Geology,Peking University,Beijing 100871,China
  • Received Date: 2003-11-21
  • Accepted Date: 1900-01-01
  • Available Online: 2003-01-02

Abstract: Perovskite type compounds of general formula ABX3 have the most commonly adopted structure (Pbnm),to some extent distorted from the ideal structure Pm3m.Their structures transformations are diverse at high pressure.Three parameters (t,VA/VB,Etot),which are used to describe the stabilization of perovskite structures,are introduced briefly.Applied threeparameters,all models of perovskite structure (Pbnm) changing at high pressure are summed up.Some of the models suit all perovskites structures.As an example,CaTiO3 (Pbnm) structure changing at high pressure is analyzed by applying several models and qualitatively draws a conclusion that the structure symmetry is reduced with enhancing the pressure.

    HTML

Reference (1)

目录

Link
IOPScience
SCOAP3
arXiv
Chinese Physical Society
Journal information
Introduction
Editorial Board
Others
Subscribe
Contact us
QQ: 1307685413
Tel: +86-010-88235947
Fax: +86-010-88233126
E-mail: [email protected]

  • CPC Website

  • IOP Website

  • CPC WeChat

Copyright © Institute of High Energy Physics, Chinese Academy of Sciences, 19B Yuquan Road, Beijing 100049, China 京ICP备05002789号-1

Supported by: Beijing Renhe Information Technology Co. Ltd  E-mail: [email protected]

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return