Skip navigation

DSpace

機構典藏 DSpace 系統致力於保存各式數位資料(如:文字、圖片、PDF)並使其易於取用。

點此認識 DSpace
DSpace logo
English
中文
  • 瀏覽論文
    • 校院系所
    • 出版年
    • 作者
    • 標題
    • 關鍵字
    • 指導教授
  • 搜尋 TDR
  • 授權 Q&A
    • 我的頁面
    • 接受 E-mail 通知
    • 編輯個人資料
  1. NTU Theses and Dissertations Repository
  2. 理學院
  3. 物理學系
請用此 Handle URI 來引用此文件: http://tdr.lib.ntu.edu.tw/jspui/handle/123456789/28754
完整後設資料紀錄
DC 欄位值語言
dc.contributor.advisor林昭吟,陳政弦
dc.contributor.authorMei-Chung Linen
dc.contributor.author林美君zh_TW
dc.date.accessioned2021-06-13T00:20:58Z-
dc.date.available2007-07-30
dc.date.copyright2007-07-30
dc.date.issued2007
dc.date.submitted2007-07-27
dc.identifier.citation[1] T. C. Han and J. G. Lin, J. Magn. Mater., 304 (2006) e424
[2] W. Prellier, M. P. Singh, and P. Murugavel, J. Phys.: Condens. Matter, 17 (2005) R803
[3] http://www.ncnr.nist.gov/staff/jeff/Multiferroics.html
[4] H. Sugie, N. Iwata, and K. Kohn, J. Phys. Soc. Jpn., 71 (2002) 1558
[5] Z. J. Huang, Y. Cao, Y. Y. Sun, Y. Y. Xue, and C. W. Chu, Phys. Rev. B 56 (1997) 2623
[6] A. Munoz, J. A. Alonso, M. J. Martinez-Lope, M. T. Casais, J. L. Martinez, and M. T. Fernandez-Diaz, Phys. Rev. B 62 (2000) 9498
[7] C. dela Cruz, F. Yen, B. Lorenz, Y. Q. Wang, Y. Y. Sun, M. M. Gospodinov, and C. W. Chu, Phys. Rev. B 71 (2005) 060407
[8] P. A. Sharma, J. S. Ahn, N. Hur, S. Park, S. –B. Kim, S. Lee, J. –G. Park, S. Guha, and S. –W. Cheong, Phys. Rev. Lett. 93 (2004) 1770202
[9] M. Fiebig, Th. Lottermoser, D. Frohlich, A. V. Goltsev, and R. V. Pisarev, Nature 419 (2002) 818
[10] D. G. Tomuta, S. Ramakrishnan, G. J. Nieuwenhuys, and J. A. Mydosh, J. Phys.: Condens. Matter 13 (2001) 4543
[11] B. F. Woodfield, M. L. Wilson, and J. M. Byers, Phys. Rev. Lett. 78 (1997) 3201
[12] T. Katsufuji, S. Mori, M. Masaki, Y. Moritomo, N. Yamamoto, and H. Takagi, Phys. Rev. B 64 (2001) 104419
[13] I. Munawar and S. H. Curnoe, J. Phys.: Condens. Matter 18 (2006) 9575
[14] N. Iwata and K. Kohn, J. Phys. Soc. Jpn., 67 (1998) 3318
[15] P. Murugavel, J. –H. Lee, D. Lee, and T. W. Noh, et al.: App. Phys. Lett. 90 (2007) 142902
dc.identifier.urihttp://tdr.lib.ntu.edu.tw/jspui/handle/123456789/28754-
dc.description.abstract在固態反應合成下,稀土錳氧化物RMnO3 ( R = 稀土元素或釔 )依據R3+ 離子半徑的大小可形成二種晶體結構,分別為:(1)當R為半徑較大的La、Ce、Pr、Nd、Sm、Eu、Gd、Tb、Dy時,則會形成正方結構的RMnO3;(2)當R為半徑較小的Ho、Er、Tm、Yb、Lu、Y,則會形成六方結構的RMnO3。這個研究利用固態反應法備製了一系列六方結構的RMnO3(R = Ho、Er、Tm、Yb、Lu、Y)的樣品,藉由X光繞射儀斷定其結構,繼而測量其磁性、電性和比熱的特性,探討不同R3+離子對於整個化合物的物性影響。
研究發現,在磁性的數據中顯示,只有在YMnO3、YbMnO3和LuMnO3清楚出現了反鐵磁的轉變溫度,分別為73 K、87 K和83 K;而由比熱的量測發現,磁性轉變溫度清楚的反應在比熱的性質中,由比熱的轉變溫度可以歸納出,轉變溫度隨R的離子半徑變小而增高。在介電常數的量測中,發現在所有磁轉變溫度附近都出現不正常的轉折現象,證實磁和電性的強關聯性。综而言之,我們的這個研究提供了重要的實驗數據,有助於未來多磁體的理論發展。
zh_TW
dc.description.abstractThe rare earth manganites RMnO3 (R = rare earth element or Y) exhibit strong magnetic exchange interactions between the magnetic moments of the Mn3+ ions as well as some of the magnetic R3+. Depending on the size of rare earth ion, RMnO3 crystallizes into two different structures:(1) orthorhombic phase for R = La, Ce, Pr, Nd, Sm, Eu, Gd, Tb, or Dy which has a larger ionic radius compared with that of Ho;and (2)hexagonal phase for R = Ho, Er, Tm, Yb, Lu or Y which possesses a smaller ionic radius. In this work, we have prepared a series of hexagonal RMnO3 with R = Ho, Er, Tm, Yb, Lu and Y and employed the techniques of X-ray powder diffraction, magnetic susceptibility, heat capacity and dielectric permeability in order to systematically study their R-dependent structural, magnetic and electric properties.
In the data of magnetic susceptibility of these six samples, only YMnO3, YbMnO3 and LuMnO3 show antiferromagnetic transitions near 73 K, 87 K and 83 K respectively. However, the magnetic transition temperatures of all samples are clearly observed in the data of specific heat. It is found that the transition temperature increases with decreasing the radius of R-ion, which is attributed to the enhancement of exchange interaction between Mn3+-ions. In the data of temperature dependent dielectric permeability vs. temperature, anomalies appear near TN in all samples, implying a strong coupling between ferroelectric and magnetic orders in the hexagonal RMnO3 compounds. The results of this study provide important information for the future development of theoretical model for multiferroism.
en
dc.description.provenanceMade available in DSpace on 2021-06-13T00:20:58Z (GMT). No. of bitstreams: 1
ntu-96-R94222069-1.pdf: 3173486 bytes, checksum: b68d7544e3e569dc073653c35f2fbadb (MD5)
Previous issue date: 2007
en
dc.description.tableofcontentsContents
口試委員審定書 i
致謝 ii
Abstract (in Chinese) iii
Abstract (in English) iv
Contents v
List of figures vi
List of tables viii

Chapter 1. Introduction 1
Chapter 2. Experimental 5
2-1 Experiment flow chart 5
2-2 Sample preparation 6
2-3 Measurements 8
2-3-1 Structure analysis 8
2-3-2 Magnetic analysis 8
2-3-3 Specific heat analysis 8
2-3-4 Dielectric analysis 9
Chapter 3. Results and Discussion 10
3-1 Structures of hexagonal RMnO3 10
3-2 Magnetic properties of hexagonal RMnO3 10
3-3 Specific heat properties of hexagonal RMnO3 12
3-4 Dielectric properties of hexagonal RMnO3 14
Chapter 4. Conclusion 17
References 18


List of figures
Fig. 1-1 View of the ferroelectric phase from the perpendicular to the c axis, showing the layered nature of the hexagonal RMnO3. 19
Fig. 1-2 Schematic representation of the magnetic structure of YMnO3. 19
Fig. 2-1 X-ray diffraction machine Bruker D8. 20
Fig. 2-2 JEOL 6700 Scanning Electron Microscopy. 20
Fig. 2-3 Superconducting quantum interference device (SQUID) Quantum Design. 21
Fig. 2-4 PPMS (Quantum Design Model 6000). 21
Fig. 2-5 The set-up of thermal relation measurement. (a) view from the side; (b) view from the top. 22
Fig. 2-6 (a) LCR-Meter Agilent 4294A); (b) home-made probe. 22
Fig. 3-1 X-ray diffraction patterns of RMnO3 samples with R= Ho, Er, Tm, Yb, Lu and Y. 23
Fig. 3-2 Lattice parameter of RMnO3 as a function of the size of the rare earth (RE). 23
Fig. 3-3 Scanning electron micrographs of a sintered pellet of HoMnO3 taken at a magnification of 5.000 times. 24
Fig. 3-4 Scanning electron micrographs of a sintered pellet of ErMnO3 taken at a magnification of 2000 times. 24
Fig. 3-5 Scanning electron micrographs of a sintered pellet of TmMnO3 taken at a magnification of 5000 times. 25
Fig. 3-6 Scanning electron micrographs of a sintered pellet of YbMnO3 taken at a magnification of 5000 times. 25
Fig. 3-7 Scanning electron micrographs of a sintered pellet of LuMnO3 taken at a magnification of 5000 times. 26
Fig. 3-8 Scanning electron micrographs of a sintered pellet of YMnO3 taken at a magnification of 5000 times. 26

Fig. 3-9 Inverse susceptibility of HoMnO3 in the zero-field-
cooled and the field-cooled. 27
Fig. 3-10 Inverse susceptibility of ErMnO3 in the zero-field-
cooled and the field-cooled. 27
Fig. 3-11 Inverse susceptibility of TmMnO3 in the zero-field-
cooled and the field-cooled. 28
Fig. 3-12 Inverse susceptibility of YbMnO3 in the zero-field-
cooled and the field-cooled. 28
Fig. 3-13 Inverse susceptibility of LuMnO3 in the zero-field-
cooled and the field-cooled. 29
Fig. 3-14 Inverse susceptibility of YMnO3 in the zero-field-
cooled and the field-cooled. 29
Fig. 3-15 Magnetization isotherms of YMnO3. 30
Fig. 3-16 Magnetization isotherms of TmMnO3. 30
Fig. 3-17 Specific heat v.s. temperature of YMnO3 at zero magnetic field. The solid line is the lattice contribution. 31
Fig. 3-18 Specific heat v.s. temperature of HoMnO3 at zero magnetic field. The solid line is the lattice contribution. 31
Fig. 3-19 Specific heat v.s. temperature of ErMnO3 at zero magnetic field. The solid line is the lattice contribution. 32
Fig. 3-20 Specific heat v.s. temperature of TmMnO3 at zero magnetic field. The solid line is the lattice contribution. 32
Fig. 3-21 Specific heat v.s. temperature of YbMnO3 at zero magnetic field. The solid line is the lattice contribution. 33
Fig. 3-22 Specific heat v.s. temperature of LuMnO3 at zero magnetic field. The solid line is the lattice contribution. 33
Fig. 3-23 Excess specific heat of YMnO3 after subtraction of the lattice contribution. 34
Fig. 3-24 Excess specific heat of HoMnO3 after subtraction of the lattice contribution. 34

Fig. 3-25 Excess specific heat of ErMnO3 after subtraction of the lattice contribution. 35
Fig. 3-26 Excess specific heat of TmMnO3 after subtraction of the lattice contribution. 35
Fig. 3-27 Excess specific heat of YbMnO3 after subtraction of the lattice contribution. 36
Fig. 3-28 Excess specific heat of LuMnO3 after subtraction of the lattice contribution. 36
Fig. 3-29 Temperature dependence of the dielectric constant (ε) of YMnO3. 37
Fig. 3-30 Temperature dependence of the dielectric constant (ε) of HoMnO3. 37
Fig. 3-31 Temperature dependence of the dielectric constant (ε) of ErMnO3. 38
Fig. 3-32 Temperature dependence of the dielectric constant (ε) of TmMnO3. 38
Fig. 3-33 Temperature dependence of the dielectric constant (ε) of YbMnO3. 39
Fig. 3-34 Temperature dependence of the dielectric constant (ε) of LuMnO3. 39
Fig. 3-35 Frequency dependence of the dielectric constant of RMnO3 at room temperature. 40
Fig. 3-36 Frequency dependence of the tanδ of RMnO3 at room temperature. 40

List of table
Table 1. Lattice parameters and magnetic transition temperature in RMnO3. 41
dc.language.isoen
dc.subject六角柱zh_TW
dc.subject稀釷氧化物zh_TW
dc.subject多磁體zh_TW
dc.subjecthexagonalen
dc.subjectmultiferroicen
dc.subjectRMnO3en
dc.title多磁體RMnO3 (R=Ho, Er, Tm, Yb, Lu and Y)的物性研究zh_TW
dc.titleThe study on the physical properties of multiferroic RMnO3 (R=Ho, Er, Tm, Yb, Lu and Y)en
dc.typeThesis
dc.date.schoolyear95-2
dc.description.degree碩士
dc.contributor.oralexamcommittee張慶瑞,胡崇德
dc.subject.keyword多磁體,稀釷氧化物,六角柱,zh_TW
dc.subject.keywordmultiferroic,RMnO3,hexagonal,en
dc.relation.page41
dc.rights.note有償授權
dc.date.accepted2007-07-27
dc.contributor.author-college理學院zh_TW
dc.contributor.author-dept物理研究所zh_TW
顯示於系所單位:物理學系

文件中的檔案:
檔案 大小格式 
ntu-96-1.pdf
  未授權公開取用
3.1 MBAdobe PDF
顯示文件簡單紀錄


系統中的文件,除了特別指名其著作權條款之外,均受到著作權保護,並且保留所有的權利。

社群連結
聯絡資訊
10617臺北市大安區羅斯福路四段1號
No.1 Sec.4, Roosevelt Rd., Taipei, Taiwan, R.O.C. 106
Tel: (02)33662353
Email: ntuetds@ntu.edu.tw
意見箱
相關連結
館藏目錄
國內圖書館整合查詢 MetaCat
臺大學術典藏 NTU Scholars
臺大圖書館數位典藏館
本站聲明
© NTU Library All Rights Reserved