Silicon Chemistry 2003
DOI: 10.1002/9783527610761.ch2
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Reactions with Matrix‐Isolated SiO Molecules

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Cited by 6 publications
(5 citation statements)
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“…For example, the bond energy in SiO 2 is estimated as being 621.7 kJ/mol. 34 Usually, under moderate temperature conditions, the structure of silicates is restricted to tetrahedral fourfold coordination containing SiO 4 units, with the Si atom at the center and O atoms at the vertices. These structures range from individual silicate anions to covalent neutral threedimensional (3D) tetrahedral networks, such as silica-based compounds.…”
Section: ■ Introductionmentioning
confidence: 99%
See 1 more Smart Citation
“…For example, the bond energy in SiO 2 is estimated as being 621.7 kJ/mol. 34 Usually, under moderate temperature conditions, the structure of silicates is restricted to tetrahedral fourfold coordination containing SiO 4 units, with the Si atom at the center and O atoms at the vertices. These structures range from individual silicate anions to covalent neutral threedimensional (3D) tetrahedral networks, such as silica-based compounds.…”
Section: ■ Introductionmentioning
confidence: 99%
“…There is a variety of silicate minerals and synthetic SiO compounds, stabilized by the high affinity between Si and O atoms during the thermodynamic formation of these materials. For example, the bond energy in SiO 2 is estimated as being 621.7 kJ/mol . Usually, under moderate temperature conditions, the structure of silicates is restricted to tetrahedral fourfold coordination containing SiO 4 units, with the Si atom at the center and O atoms at the vertices.…”
Section: Introductionmentioning
confidence: 99%
“…Interestingly, the monoxide of silicon is also the subject of astrophysical studies, because of its high interstellar abundance. ,, Diatomic SiO, well-known on Earth as a metastable molecule (the Si–O separation is 1.49 Å), has also been detected in sunspots. It was suggested that SiO is the initial condensate in the outflows of oxygen-rich dying stars.…”
Section: Introductionmentioning
confidence: 99%
“…It was suggested that SiO is the initial condensate in the outflows of oxygen-rich dying stars. Some crystalline silicate grains have been observed in the dust shells around those stars at temperatures above 1000 K. There is some theoretical work on SiO nanoaggregates, and oligomers of SiO have been detected and assessed in calculations …”
Section: Introductionmentioning
confidence: 99%
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