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Volumn 49, Issue 16, 1994, Pages 11421-11424

Shape of large single- and multiple-shell fullerenes

Author keywords

[No Author keywords available]

Indexed keywords

EID: 17044404381 PISSN: 01631829 EISSN: None Source Type: Journal
DOI: 10.1103/PhysRevB.49.11421 Document Type: Article

Times cited : (148)

References (22)

2
- 84911745547
- Canonical Structure of Large Carbon Clusters: Cn, n > 100
- (1993) Europhysics Letters (EPL) , vol.22 , pp. 45
- Ugarte, D.¹

4
- 0008032742
- (1992) J. Chem. Soc. Faraday Trans. , vol.88 , pp. 2815
- Mckay, K.¹

5
- 0002967398
- Molecular Mechanics Calculations of Giant- and Hyperfullerenes with Eicosahedral Symmetry
- (1993) Fullerene Science and Technology , vol.1 , pp. 55
- Yoshida, M.¹ Osawa, E.²

11
- 84864682706
- The divide-and-conquer density-functional approach: Molecular internal rotation and density of states
- (1992) The Journal of Chemical Physics , vol.96 , pp. 2408
- Lee, C.¹ Yang, W.²

14
- 5844386280
- For the original LDA calculations of the graphite see
- (1984) Phys. Rev. B , vol.29 , pp. 6996
- Yin, M.T.¹ Cohen, M.²

15
- 33644817086
- For experimental values see the references cited in the above paper and
- (1990) Phys. Rev. B , vol.42 , pp. 9458
- Brenner, D.W.¹

19
- 84927366891
- If all nearest neighbor hoppings are identical, calculations show that all type I Goldberg series are close shelled. This is generally not true for type II in which N(n)=20n2.

20
- 84927366889
- For spherical morphology, the rotational barrier of inner shell vs outer shell is very small; free rotation is expected. In contrast, for polyhedron morphologies the barriers are very high, which leads to very different intershell vibrational modes. This and related issues will be examined elsewhere.

21
- 33646833936
- After our paper was written we were informed about the paper by, in which they use the Brenner empirical potentials (Ref. 9) to obtain the optimal structure of C240. Their results are almost identical to that of Yoshida and Osawa (Ref. 4). For example, the standard deviation from sphere is 0.17 AA (which was mistakenly stated as 0.085 AA).
- (1992) J. Phys. Chem. , vol.95 , pp. 8737
- Dunlap, B.I.¹

* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.