A heterocumulene is a molecule or ion containing a chain of at least three double bonds between consecutive atoms, in which one or more atoms in the doubly bonded chain is a heteroatom. Such species are analogous to a cumulene in which the chain of doubly bonded atoms contains only carbon, except that at least one carbon is replaced by a heteroatom.[1] Some authors relax the definition to include species with chains of only two double bonds between consecutive atoms,[2] also known as heteroallenes.

Because of the double bond rule, heterocumulenes are rarely isolated. Instead they tend to polymerize. Many are however common in the interstellar medium, where they exist as a dilute gas. Most of the longer ones are very unstable and reactive, and thus have a transient existence, or can only survive when dilute or in an inert matrix. Molecular clouds in space are very dilute and allow heterocumulenes to exist long enough to be detected. Some simple heterocumulenes are common chemicals or ions. These include carbon dioxide, carbon disulfide, carbon diselenide, cyanate, and thiocyanate. Some definitions of heterocumulenes include compounds that contain concatenated double bonds with more than one element, but may have other parts to them. This class includes ketene, sulfur diimide, sulfine, and dicyclohexylcarbodiimide. Some heterocumulenes can act as ligands with various metals.

Reactions

Some energised heterocumulenes can cyclise by bending into a circle and bonding the two ends of the chain. Molecules that can do this are CCCB, CCCAl, CCCSi, CCCN, and CCCP.[3]

Other four-atom heterocumulenes include CCBO, tricarbon monoxide (CCCO), and CCCS.

Four-atom heterocumulenes when cyclised can have two forms. In the kite (or rhombic) form, a triangle of carbon has two of its atoms bonded to the heteroatom. In the fan form the hetero atom links to three carbon atoms arranged in a fan shape. CCCSi has linear, rhombic or fan isomers. The rhombic form is known in space near the carbon star IRC+10216.

CCCCO cyclises to a three-member ring.[3] CCCCN undergoes an isonitrile conversion.[3]

Molecules

Other known five-atom heterocumulenes include CCBCC, CCCCB, CCOCC, CCCCSi, CNCCO, HCCCO, HCCCS, and NCCCN. CCCCSi is known as a linear molecule in space.

CCCCBO turns into a six-member ring. Other six atom heterocumulenes include OCCCCN and HCNCNH.

Seven atom heterocumulenes include NCCCCCN, HCCBCCH.

A known nine atom heterocumulene is HCCCCCCCH.

Thiocumulenes have a sulfur atom. They include dicarbon monosulfide CCS and tricarbon monosulfide CCCS, both known from molecular clouds.[4] SCnS chains can be made by laser ablation with n up to 27.[5]

Table of molecules

This table lists heterocumulene molecules. Heterocumulenes are supposed to be straight, but some combinations of elements result in bent or cyclic molecules.

one kind of heteroatom
heteroatom 1 carbon 2 carbon 3 carbon 4 carbon 5 carbon 6 carbon 7 carbon 8 carbon 9 carbon
BCCBCCBCC, CCCCB
NCCN NCCNCCCN[6] NCCCNCCCCN NCCCCNNCCCCCN C5N[6]
OOCOCCO[7]CCCO OCCCO >CCCOC4O[7] C4O2OC5OC6O[7]C8O[7]
SiCCSi bentCCCSi ringCCCCSi[6]C6Si[6]
PCCP
SSCSCCS SCCSCCCS SCCCSC4S[8] SCCCCS[8]C5S[8] SC5S[8][9]C6S[10]SC7S[10]SC9S[10]
ClCCClCCCCl is bent
SeCSe2SeCCCSe[11]
Ir IrC3–[12]
Pt PtC3[12]
Au AuC3+[12]

Two different hetero atoms

atom 1 H N O S
N HCNHCCCN HCnN n=5,7,9,11 HCNCC[6] HCCNC[6]-OCN -NCO-SNC -NCS
S HC2-8S (HCS bent)[13] NCS (NCCS bent) NC3-7S[13] OCS
Se -SeCN

References

  1. ↑ IUPAC, Compendium of Chemical Terminology, 2nd ed. (the "Gold Book") (1997). Online corrected version: (2006–) "heterocumulenes". doi:10.1351/goldbook.H02797
  2. ↑ Kumar, Akshai; Samuelson, Ashoka G. (January 2011). "Metathesis of carbon dioxide and phenyl isocyanate catalysed by group(IV) metal alkoxides: An experimental and computational study" (PDF). Journal of Chemical Sciences. 123 (1): 29–36. doi:10.1007/s12039-011-0069-4.
  3. 1 2 3 Wang, Tianfang; Bowie, John H. (November 2011). "Studies of cyclization reactions of linear cumulenes and heterocumulenes using the neutralization-reionization procedure and/or ab initio calculations". Mass Spectrometry Reviews. 30 (6): 1225–1241. Bibcode:2011MSRv...30.1225W. doi:10.1002/mas.20328. PMID 21400561.
  4. ↑ Yamamoto, Satoshi; Saito, Shuji; Kawaguchi, Kentarou; Kaifu, Norio; Suzuki, Hiroko (June 1987). "Laboratory detection of a new carbon-chain molecule C3S and its astronomical identification". The Astrophysical Journal. 317: L119. Bibcode:1987ApJ...317L.119Y. doi:10.1086/184924.
  5. ↑ Burnin, Andrei; BelBruno, Joseph J. (November 2003). "SCnS Linear Chain Production by Direct Laser Ablation". The Journal of Physical Chemistry A. 107 (45): 9547–9553. Bibcode:2003JPCA..107.9547B. doi:10.1021/jp0304071.
  6. 1 2 3 4 5 6 Botschwina, Peter (2003). "Spectroscopic properties of interstellar molecules: Theory and experiment". Physical Chemistry Chemical Physics. 5 (16): 3337. Bibcode:2003PCCP....5.3337B. doi:10.1039/b303753n.
  7. 1 2 3 4 Ohshima, Yasuhiro; Endo, Yasuki; Ogata, Teruhiko (22 January 1995). "Fourier‐transform microwave spectroscopy of triplet carbon monoxides, C2O, C4O, C6O, and C8O". The Journal of Chemical Physics. 102 (4): 1493–1500. Bibcode:1995JChPh.102.1493O. doi:10.1063/1.468881.
  8. 1 2 3 4 Szczepanski, Jan; Hodyss, Robert; Fuller, Jason; Vala, Martin (April 1999). "Infrared Absorption Spectroscopy of Small Carbon−Sulfur Clusters Isolated in Solid Ar". The Journal of Physical Chemistry A. 103 (16): 2975–2981. Bibcode:1999JPCA..103.2975S. doi:10.1021/jp984700q.
  9. ↑ Thorwirth, S.; Salomon, T.; Fanghänel, S.; Kozubal, J.R.; Dudek, J.B. (September 2017). "High-resolution infrared fingerprints of carbon-sulfur clusters: The ν1 band of C5S". Chemical Physics Letters. 684: 262–266. Bibcode:2017CPL...684..262T. doi:10.1016/j.cplett.2017.06.032.
  10. 1 2 3 Wang, Haiyan; Szczepanski, Jan; Cooke, Andrew; Brucat, Philip; Vala, Martin (2005). "Vibrational absorption spectra of CnS (n = 2, 6) and CnS2 (n = 7, 9, 11, 13, 15) linear carbon-sulfur clusters". International Journal of Quantum Chemistry. 102 (5): 806–819. Bibcode:2005IJQC..102..806W. doi:10.1002/qua.20383.
  11. ↑ Pu, Liang; Zhao, Xiao; Zhang, Zhong; King, R. Bruce (May 2017). "Heavier Carbon Subchalcogenides as C3 Sources for Tungsten-Capped Cumulenes: A Theoretical Study". Inorganic Chemistry. 56 (10): 5567–5576. doi:10.1021/acs.inorgchem.6b02958. PMID 28459557.
  12. 1 2 3 Liu, Xuegang; Li, Gang; Liu, Zhiling; Yang, Wenshao; Fan, Hongjun; Jiang, Ling; Xie, Hua (2021-12-23). "Isoelectronic IrC 3 – , PtC 3 , and AuC 3 + Clusters Featuring the Structural and Bonding Resemblance to OC 3". The Journal of Physical Chemistry Letters. 13 (1): 12–17. doi:10.1021/acs.jpclett.1c03754. ISSN 1948-7185. PMID 34941270. S2CID 245444740.
  13. 1 2 McCarthy, M. C.; Cooksy, A. L.; Mohamed, S.; Gordon, V. D.; Thaddeus, P. (February 2003). "Rotational Spectra of the Nitrogen‐Sulfur Carbon Chains NCnS, n = 1–7" (PDF). The Astrophysical Journal Supplement Series. 144 (2): 287–297. Bibcode:2003ApJS..144..287M. doi:10.1086/344727. hdl:2152/26169. S2CID 122233232.
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