메뉴 건너뛰기




Volumn 81, Issue 4, 2010, Pages

Load transfer between cross-linked walls of a carbon nanotube

Author keywords

[No Author keywords available]

Indexed keywords


EID: 77954787958     PISSN: 10980121     EISSN: 1550235X     Source Type: Journal    
DOI: 10.1103/PhysRevB.81.045429     Document Type: Article
Times cited : (43)

References (42)
  • 6
    • 77954770419 scopus 로고    scopus 로고
    • See Ref. and references therein.
    • See Ref. and references therein.
  • 8
    • 0033743089 scopus 로고    scopus 로고
    • 10.1002/(SICI)1521-4095(200005)12:10<750::AID-ADMA750>3.0.CO;2-6
    • P. M. Ajayan, L. S. Schadler, C. Giannaris, and A. Rubio, Adv. Mater. 12, 750 (2000). 10.1002/(SICI)1521-4095(200005)12:10<750::AID-ADMA750>3.0. CO;2-6
    • (2000) Adv. Mater. , vol.12 , pp. 750
    • Ajayan, P.M.1    Schadler, L.S.2    Giannaris, C.3    Rubio, A.4
  • 11
    • 0034725776 scopus 로고    scopus 로고
    • 10.1126/science.289.5479.602
    • J. Cumings and A. Zettl, Science 289, 602 (2000). 10.1126/science.289. 5479.602
    • (2000) Science , vol.289 , pp. 602
    • Cumings, J.1    Zettl, A.2
  • 16
    • 0001195497 scopus 로고    scopus 로고
    • 10.1088/0034-4885/62/8/201
    • F. Banhart, Rep. Prog. Phys. 62, 1181 (1999). 10.1088/0034-4885/62/8/201
    • (1999) Rep. Prog. Phys. , vol.62 , pp. 1181
    • Banhart, F.1
  • 22
    • 42749105636 scopus 로고    scopus 로고
    • 10.1103/PhysRevB.69.233408
    • Z. Xia and W. A. Curtin, Phys. Rev. B 69, 233408 (2004). 10.1103/PhysRevB.69.233408
    • (2004) Phys. Rev. B , vol.69 , pp. 233408
    • Xia, Z.1    Curtin, W.A.2
  • 26
    • 55349087530 scopus 로고    scopus 로고
    • 10.1016/j.physb.2008.07.010
    • S. HaiYang and Z. XinWei, Physica B 403, 3798 (2008). 10.1016/j.physb.2008.07.010
    • (2008) Physica B , vol.403 , pp. 3798
    • Haiyang, S.1    Xinwei, Z.2
  • 30
    • 77954808614 scopus 로고    scopus 로고
    • Another reason for considering the SP3 defect is that we have performed a comparative study between the Frenkel pair and the SP3 defect type in DWNTs and observed that the Frenkel pair is less stable than the SP3. We also have done some high-temperature molecular-dynamics simulations that show that Frenkel pair defects evolve to SP3 ones.
    • Another reason for considering the SP 3 defect is that we have performed a comparative study between the Frenkel pair and the SP 3 defect type in DWNTs and observed that the Frenkel pair is less stable than the SP 3. We also have done some high-temperature molecular-dynamics simulations that show that Frenkel pair defects evolve to SP 3 ones.
  • 33
    • 33644817086 scopus 로고
    • 10.1103/PhysRevB.42.9458
    • D. W. Brenner, Phys. Rev. B 42, 9458 (1990). 10.1103/PhysRevB.42.9458
    • (1990) Phys. Rev. B , vol.42 , pp. 9458
    • Brenner, D.W.1
  • 36
    • 33244484558 scopus 로고    scopus 로고
    • 10.1103/PhysRevB.73.081401
    • B. Shan and K. Cho, Phys. Rev. B 73, 081401 (R) (2006). 10.1103/PhysRevB.73.081401
    • (2006) Phys. Rev. B , vol.73 , pp. 081401
    • Shan, B.1    Cho, K.2
  • 37
    • 0038218041 scopus 로고    scopus 로고
    • 10.1103/PhysRevB.67.115407
    • C. Wei, K. Cho, and D. Srivastava, Phys. Rev. B 67, 115407 (2003). 10.1103/PhysRevB.67.115407
    • (2003) Phys. Rev. B , vol.67 , pp. 115407
    • Wei, C.1    Cho, K.2    Srivastava, D.3
  • 39
    • 77954797367 scopus 로고    scopus 로고
    • Our estimates of the energy barrier to break the s p3 bond between the inner and outer walls and recover the perfect DWNT, using the AIREBO potential, is ∼1eV per s p3 bond. This value is similar to the corresponding energy barrier for a Frenkel pair defect in two layers of graphene, ∼1.4eV (see Ref.).
    • Our estimates of the energy barrier to break the s p 3 bond between the inner and outer walls and recover the perfect DWNT, using the AIREBO potential, is ∼ 1 eV per s p 3 bond. This value is similar to the corresponding energy barrier for a Frenkel pair defect in two layers of graphene, ∼ 1.4 eV (see Ref.).


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.