Heterocumulene Explained

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. Some authors relax the definition to include species with chains of only two double bonds between consecutive atoms,[1] 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.[2]

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.[2] CCCCN undergoes an isonitrile conversion.[2]

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.[3] SCnS chains can be made by laser ablation with n up to 27.[4]

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
heteroatom1 carbon2 carbon3 carbon4 carbon5 carbon6 carbon7 carbon8 carbon9 carbon
B CCB CCBCC, CCCCB
N NCCCCCN C5N
O C6O C8O[5]
Si CCSi bentCCCSi ringCCCCSi C6Si
P CCP
S C4S[6] SCCCCSC5S SC5S[7] C6S[8] SC7S SC9S
Cl CCCl CCCCl is bent
Se SeCCCSe[9]
IrIrC3[10]
PtPtC3
AuAuC3+

Two different hetero atoms

atom 1HNOS
NHCNHCCCN HCnN n=5,7,9,11 HCNCC[11] HCCNC -SNC -NCS
SHC2-8S (HCS bent)NCS (NCCS bent) NC3-7S[12] OCS
Se-SeCN

Notes and References

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