The Structures of S 4 N⊖, S 3 N 2 O 2 and S 4 N 3
Part of the potential surface of S 4 N⊖ has been investigated using the MNDO method. It is found that the cis-trans isomer 1b is more stable by 20-30 kJ/mol than the trans-trans isomer (1 c) and the cis-cis isomer (1 a). The stability of 1 b is traced back to stabilization of the HOMO and to a Coulo...
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Veröffentlicht in: | Zeitschrift für Naturforschung. B, A journal of chemical sciences A journal of chemical sciences, 1981-04, Vol.36 (4), p.492-497 |
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container_title | Zeitschrift für Naturforschung. B, A journal of chemical sciences |
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creator | Gleiter, Rolf Bartetzko, Richard |
description | Part of the potential surface of S
4
N⊖ has been investigated using the MNDO method. It is found that the cis-trans isomer 1b is more stable by 20-30 kJ/mol than the trans-trans isomer (1 c) and the cis-cis isomer (1 a). The stability of 1 b is traced back to stabilization of the HOMO and to a Coulomb attraction. For S
3
N
2
O
2
(2) the MNDO calculations favour those isomers (2a and 2b) with two sickle-like arrangements for the same reasons. For S
4
N
3
e (3) only one isomer (3a) is favoured due to the stabilization of the HOMO. The similarity in the transannular interaction present in 1-3 and that in trithiapentalenes and related compounds is pointed out. The PE spectrum of 2 has been reinvestigated. The first five bands can be interpreted by comparison between the measured ionization potentials and the calculated (MNDO) orbital energies. |
doi_str_mv | 10.1515/znb-1981-0418 |
format | Article |
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4
N⊖ has been investigated using the MNDO method. It is found that the cis-trans isomer 1b is more stable by 20-30 kJ/mol than the trans-trans isomer (1 c) and the cis-cis isomer (1 a). The stability of 1 b is traced back to stabilization of the HOMO and to a Coulomb attraction. For S
3
N
2
O
2
(2) the MNDO calculations favour those isomers (2a and 2b) with two sickle-like arrangements for the same reasons. For S
4
N
3
e (3) only one isomer (3a) is favoured due to the stabilization of the HOMO. The similarity in the transannular interaction present in 1-3 and that in trithiapentalenes and related compounds is pointed out. The PE spectrum of 2 has been reinvestigated. The first five bands can be interpreted by comparison between the measured ionization potentials and the calculated (MNDO) orbital energies.</description><identifier>ISSN: 0932-0776</identifier><identifier>EISSN: 1865-7117</identifier><identifier>DOI: 10.1515/znb-1981-0418</identifier><language>eng</language><ispartof>Zeitschrift für Naturforschung. B, A journal of chemical sciences, 1981-04, Vol.36 (4), p.492-497</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c828-de9355b5f16737bb5731431f2990fb2d12859d2716595f595ca51c8d030f7b383</citedby></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids></links><search><creatorcontrib>Gleiter, Rolf</creatorcontrib><creatorcontrib>Bartetzko, Richard</creatorcontrib><title>The Structures of S 4 N⊖, S 3 N 2 O 2 and S 4 N 3</title><title>Zeitschrift für Naturforschung. B, A journal of chemical sciences</title><description>Part of the potential surface of S
4
N⊖ has been investigated using the MNDO method. It is found that the cis-trans isomer 1b is more stable by 20-30 kJ/mol than the trans-trans isomer (1 c) and the cis-cis isomer (1 a). The stability of 1 b is traced back to stabilization of the HOMO and to a Coulomb attraction. For S
3
N
2
O
2
(2) the MNDO calculations favour those isomers (2a and 2b) with two sickle-like arrangements for the same reasons. For S
4
N
3
e (3) only one isomer (3a) is favoured due to the stabilization of the HOMO. The similarity in the transannular interaction present in 1-3 and that in trithiapentalenes and related compounds is pointed out. The PE spectrum of 2 has been reinvestigated. The first five bands can be interpreted by comparison between the measured ionization potentials and the calculated (MNDO) orbital energies.</description><issn>0932-0776</issn><issn>1865-7117</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1981</creationdate><recordtype>article</recordtype><recordid>eNotj81KAzEUhYMoOFaX7vMARu_NzZ0kSyn-QWkXnX2YzExQ0VaSdqGP4AP4gD6JM9TFxzlw4MAnxCXCNTLyzdcmKvQOFRh0R6JCV7OyiPZYVOBJK7C2PhVnpbwCoDcGKkHN8yDXu7zvdvs8FLlNci2NXP5-_1yNjeRSarkaaTf9YZF0Lk5S-1aGi_-cieb-rpk_qsXq4Wl-u1Cd0071gyfmyAlrSzZGtoSGMGnvIUXdo3bse22xZs9ppGsZO9cDQbKRHM2EOtx2eVtKHlL4yC_vbf4MCGESDqNwmITDJEx_1sBDjA</recordid><startdate>19810401</startdate><enddate>19810401</enddate><creator>Gleiter, Rolf</creator><creator>Bartetzko, Richard</creator><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>19810401</creationdate><title>The Structures of S 4 N⊖, S 3 N 2 O 2 and S 4 N 3</title><author>Gleiter, Rolf ; Bartetzko, Richard</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c828-de9355b5f16737bb5731431f2990fb2d12859d2716595f595ca51c8d030f7b383</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1981</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Gleiter, Rolf</creatorcontrib><creatorcontrib>Bartetzko, Richard</creatorcontrib><collection>CrossRef</collection><jtitle>Zeitschrift für Naturforschung. B, A journal of chemical sciences</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Gleiter, Rolf</au><au>Bartetzko, Richard</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The Structures of S 4 N⊖, S 3 N 2 O 2 and S 4 N 3</atitle><jtitle>Zeitschrift für Naturforschung. B, A journal of chemical sciences</jtitle><date>1981-04-01</date><risdate>1981</risdate><volume>36</volume><issue>4</issue><spage>492</spage><epage>497</epage><pages>492-497</pages><issn>0932-0776</issn><eissn>1865-7117</eissn><abstract>Part of the potential surface of S
4
N⊖ has been investigated using the MNDO method. It is found that the cis-trans isomer 1b is more stable by 20-30 kJ/mol than the trans-trans isomer (1 c) and the cis-cis isomer (1 a). The stability of 1 b is traced back to stabilization of the HOMO and to a Coulomb attraction. For S
3
N
2
O
2
(2) the MNDO calculations favour those isomers (2a and 2b) with two sickle-like arrangements for the same reasons. For S
4
N
3
e (3) only one isomer (3a) is favoured due to the stabilization of the HOMO. The similarity in the transannular interaction present in 1-3 and that in trithiapentalenes and related compounds is pointed out. The PE spectrum of 2 has been reinvestigated. The first five bands can be interpreted by comparison between the measured ionization potentials and the calculated (MNDO) orbital energies.</abstract><doi>10.1515/znb-1981-0418</doi><tpages>6</tpages></addata></record> |
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identifier | ISSN: 0932-0776 |
ispartof | Zeitschrift für Naturforschung. B, A journal of chemical sciences, 1981-04, Vol.36 (4), p.492-497 |
issn | 0932-0776 1865-7117 |
language | eng |
recordid | cdi_crossref_primary_10_1515_znb_1981_0418 |
source | Alma/SFX Local Collection |
title | The Structures of S 4 N⊖, S 3 N 2 O 2 and S 4 N 3 |
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