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X@C20F20(X=He,Ne,Ar,Kr)几何结构和 电子结构的理论研究

曹青松 邓开明

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X@C20F20(X=He,Ne,Ar,Kr)几何结构和 电子结构的理论研究

曹青松, 邓开明

Theoretical studies of geometric and electronic structures of X@C20F20 (X=He, Ne, Ar, Kr)

Cao Qing-Song, Deng Kai-Ming
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  • 采用密度泛函理论中的广义梯度近似, 对X@C20F20(X=He, Ne, Ar, Kr)几何结构和电子结构进行了计算研究. 几何结构优化发现: 惰性气体原子X内掺到C20F20笼后, 均稳定于碳笼中心, 随着内掺X原子序数的增大, X原子对C20F20笼的影响越来越大. 能隙、内掺能和振动频率计算表明: 内掺X原子使得C20F20的稳定性得到了显著提升, X@C20F20(X=He, Ne, Ar, Kr)都具有良好的稳定性, 并且随着X原子序数的增大, 其稳定性也基本呈现逐渐增强的趋势. 电子结构研究发现: X原子对X@C20F20费米能级附近的占据轨道基本没有贡献, 而对其未占据轨道贡献较大. 计算还发现: 在X@C20F20中, He 和Kr分别从C20F20的C 笼上获得了0.126和0.271个电子, 而Ne和Ar却分别向C笼转移了0.060和0.012个电子. 由此可见: X原子与C原子之间都发生了电荷转移, C笼上的C原子与惰性气体原子X间形成了一定的离子键.
    Several years ago, scientists could already introduced noble gas atoms (He, Ne, Ar, Kr, and Xe) into C60 and higher fullerenes. For the specific cases of He and Ne, the calculations suggested that both atoms are slightly bound inside C60 through simultaneous van der Waals interactions with all 60 carbons. The cavity in dodecahedrane is much smaller than that in C60, but the experimental study found that by bombarding dodecahedrane with fast, neutral helium atoms, He@C20H20 is formed. The structures of C20F20 and C20H20 are similar. Are noble gas atoms also stable in the C20F20? and, are there charges transferring between noble gas atoms and the carbon cage? In this paper, the generalized gradient approximation based on density functional theory is used to analyze the geometric and electronic structures of the endohedral fullerene X@C20F20 (X=He, Ne, Ar, Kr). The geometric optimization shows that the noble gas atoms X are all stable in the center of C20F20 cage. The C-C bond lengths of the X@C20F20 increase with the atomic number X increasing, while the C-F bond length is hardly changed. The inclusion energies of the X@C20F20 (X=He, Ne, Ar, Kr) are 1.359, 3.853, 11.276 and 15.783 eV respectively. These are all positive, which shows that the X@C20F20 have good thermodynamic stabilities, and the thermodynamic stabilities of the X@C20F20 are enhanced with the increase of X atomic number. The energy gaps of the X@C20F20 (X=He, Ne, Ar, Kr) are 5.179, 4.882, 5.874 and 6.205 eV respectively, which are greater than that of C20F20. It indicates that the X@C20F20 have better dynamic stabilities than C20F20. In addition, the vibration frequencies of the X@C20F20 (X=He, Ne, Ar, Kr) are all positive. These indicate that the stability of C20F20 is significantly improved when the X atom is introduced into the cage, and is gradually increasing with the increase of X atomic number. The electronic structures demonstrate that the X atom has no contribution to the occupied molecular orbitals near the Fermi level of X@C20F20, and the contribution of the X atom to the unoccupied molecular orbitals is relatively large. The calculation also shows that the atoms of He and Kr obtain 0.126 and 0.271 electrons from the carbons of the C20F20 cage, while Ar and Ne transfer 0.060 and 0.012 electrons to the carbons of the cage repectively. Thus there are electrons transferring between the X atoms and the carbons of the cage, indicating that the formed C-X bonds of the X@C20F20 are ionic bonds.
      通信作者: 曹青松, qscao@163.com
    • 基金项目: 国家自然科学基金(批准号: 21403111)资助的课题.
      Corresponding author: Cao Qing-Song, qscao@163.com
    • Funds: Project supported by the National Science Foundation of China (Grant No. 21403111).
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    Cao Q S, Yuan Y B, Xiao C Y, Lu R F, Kan E J, Deng K M 2012 Acta Phys. Sin. 61 106101 (in Chinese) [曹青松, 袁勇波, 肖传云, 陆瑞峰, 阚二军, 邓开明 2012 物理学报 61 106101]

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    Zhang C Y, Wu H S, Jiao H J 2007 J. Mol. Model. 13 499

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    Zhang C Y, Wu H S 2007 J. Mol. Struct: Theochem. 815 71

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    Kohn W, Sham L J 1965 Phys. Rev. 140 A1133

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    Holloway J H, Hope E G, Taylor R, Langley G J, Avent A G, Dennis T J, Hare J P, Kroto H W, Walton D R M 1991 J. Chem. Soc. Chem. Commun. 966

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  • [1]

    Kroto H W, Heath J R, O'Brien S C, Curl R F, Smalley R E 1985 Nature 318 162

    [2]

    Cao Q S, Yuan Y B, Xiao C Y, Lu R F, Kan E J, Deng K M 2012 Acta Phys. Sin. 61 106101 (in Chinese) [曹青松, 袁勇波, 肖传云, 陆瑞峰, 阚二军, 邓开明 2012 物理学报 61 106101]

    [3]

    Das S K, Song B, Mahler A, Nesterov V N, Wilson A K, Ito O, D'Souza F 2014 J. Phys. Chem. C 118 3994

    [4]

    Moor K J, Valle D C, Li C H, Kim J H 2015 Environ. Sci. Technol. 49 6190

    [5]

    Saunders M, Jiménez-Vázquez H A, Cross R J, Poreda R J 1993 Science 259 1428

    [6]

    Khong A, Jiménez-Vázquez H A, Saunders M, Cross R J, Laskin J, Peres T, Lifshitz C, Strongin R, Smith III A B 1998 J. Am. Chem. Soc. 120 6380

    [7]

    Paquette L A, Ternansky R J, Balogh D W, Kentgen G 1983 J. Am. Chem. Soc. 105 5446

    [8]

    Cross R J, Saunders M, Prinzbach H 1999 Org. Lett. 1 1479

    [9]

    Jiménez-Vázquez H A, Tamariz J, Cross R J 2001 J. Phys. Chem. A 105 1315

    [10]

    Moran D, Stahl F, Jemmis E D, Schaefer H F, Schleyer P V 2002 J. Phys. Chem. A 106 5144

    [11]

    Chen Z F, Jiao H J, Moran D, Hirsch A, Thiel W, Schleyer Pv R 2003 J. Phys. Chem. A 107 2075

    [12]

    An Y P, Yang C L, Wang M S, Ma X G, Wang D H 2009 J. Phys. Chem. C 113 15756

    [13]

    Prinzbach H, Weber K 1994 Angew. Chem. Int. Ed. Engl. 33 2239

    [14]

    Zhang C Y, Wu H S, Jiao H J 2007 J. Mol. Model. 13 499

    [15]

    Zhang C Y, Wu H S 2007 J. Mol. Struct: Theochem. 815 71

    [16]

    Tang C M, Zhu W H, Deng K M 2010 Chin. Phys. B 19 033604

    [17]

    Becke A D 1993 J. Chem. Phys. 98 5648

    [18]

    Perdew J P, Burke K, Ernzerhof M 1997 Phys. Rev. Lett. 78 1396

    [19]

    Kohn W, Sham L J 1965 Phys. Rev. 140 A1133

    [20]

    Holloway J H, Hope E G, Taylor R, Langley G J, Avent A G, Dennis T J, Hare J P, Kroto H W, Walton D R M 1991 J. Chem. Soc. Chem. Commun. 966

    [21]

    Lu G L, Yuan Y B, Deng K M, Wu H P, Yang J L, Wang X 2006 Chem. Phys. Lett. 424 142

    [22]

    Woodward R B, Hoffmann R 1965 J. Am. Chem. Soc. 87 395

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出版历程
  • 收稿日期:  2015-10-15
  • 修回日期:  2015-12-17
  • 刊出日期:  2016-03-05

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