欢迎登录材料期刊网

材料期刊网

高级检索

我们进行了Bi2Sr2CaCu2Oy(Bi2212)单晶变温X射线衍射(XRD)研究,定量给出温度从77K变化至300K时,c轴晶格参数和0038主峰的半高宽(FWHM)Δθ的变化.实验发现,从77K至140K,晶格参数c值变化是线性的,随温度较慢地单调增大;从140K附近至300K,c值的变化偏离了原来的线性,随温度较快地单调增大.另外,0038主峰的半高宽Δθ随温度的变化在140K附近出现一个极大值.这表明Bi2212单晶在140K附近发生了明显的反常结构变化.

参考文献

[1] Y He;J Xiang;J Zhang;A He,F Chang F Li .[J].Modern Physics Letters B,1990,4:651.
[2] P V Reddy;Y V Ramana .[J].Solid State Communications,1990,74:377.
[3] A R Anderson;G Gu;K N R Taylor;G J Gussel .[J].Superconductor Science and Technology,1992,5:258.
[4] X H Cheng;H M Shen;Y N Wang .[J].Modern Physics Letters B,1989,3:1241.
[5] H C Huang;D H Zheng;A L Li;F Chen,H C Sun S Y Zhu .[J].Modern Physics Letters B,1990,4:993.
[6] Z Tang;Z Q Chen;S J Wang;C G Ce Z X Zhao .[J].Journal of Physics:Condensed Matter,1993,5:345.
[7] D M Zhang;C Q Tang;T Gen;G Y Li .[J].Physical Review B,1993,47:3435.
[8] E M Gololobov;B V Novysh;N A Prytkova;ZH M Tomilo,N M shimanskaya,YA A Abeliov,G V Maiornikova A B Yagina .[J].Physica Status Solidi A,1991,126:K25.
[9] H Takenaka;K Kamigaki;H Terauchi;A Katsui .[J].Journal of the Physical Society of Japan,1989,58:775.
[10] C Patterson;P D Hatton;R J Nelmes;X Chu,Y F Yan Z X Zhao .[J].Superconductor Science and Technology,1990,3:297.
[11] S T Johnson;P D Hatton;A J S Chowdury;B M Wanklyn .[J].Solid State Communications,1995,94:261.
[12] L Shi;G E Zhou;W B Wu;M L Tian,X G Li,J Shi Y H Zhang .[J].Journal of Physics:Condensed Matter,1995,7:8597.
[13] X F Sun;W B Wu;J S Zhu;Y B Jia,G E Zhou,X G Li Y H Zhang .[J].Superconductor Science and Technology,1996,9:750.
[14] P A Miles;S J Kennedy;A R Anderson;G D Gu,G J Russell N Koshizuka .[J].Physical Review B,1997,55:14632.
[15] X F Sun;W B Wu;X R Zhao;L Zheng,L Shi,G E Zhou,X G Li Y H Zhang .[J].Journal of Physics:Condensed Matter,1996,9:6391.
[16] T Watanabe;T Fujii;A Matsuda .[J].Physical Review Letters,1997,79:2113.
[17] D Jin;P X Luo;W B Wu;X F Sun,Y H Xu,R Y Liang,X G Li Y H Zhang .[J].Physica C,1997,282-287:1341.
上一张 下一张
上一张 下一张
计量
  • 下载量()
  • 访问量()
文章评分
  • 您的评分:
  • 1
    0%
  • 2
    0%
  • 3
    0%
  • 4
    0%
  • 5
    0%