2012
DOI: 10.1021/om301087e
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Synthesis and Molecular Structures of Meta-Substituted Arylcalcium Iodides

Abstract: The reduction of meta-methyl-substituted iodobenzene with activated calcium in tetrahydrofuran (THF) yields [(3-MeC 6 H 4 )CaI(thf) 4 ] (1) and [(3,5-Me 2 C 6 H 3 )CaI(thf) 4 ] (2). The reaction of 3-halo-1-iodobenzene with calcium powder leads to the formation of the corresponding post-Grignard reagents [(3-XC 6 H 4 )CaI(thf) 4 ] [X = F (3), Cl (4), Br (5), and I (6)]. The synthesis of the thf adducts of 3-methoxyphenylcalcium iodide (7) and β-naphthylcalcium iodide (8) follows the same strategy. All post-Gri… Show more

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Cited by 19 publications
(12 citation statements)
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“…The presence of two strongly basic carbanions in the coordination sphere of calcium leads to lengthening of the metal carbon bonds in comparison to naphthylcalcium halide complexes 9. 1517 For the known compound [Ca(α ‐ Naph){N(SiMe 3 ) 2 }(thf) 3 ]15 an analogous finding might be expected due to the presence of a strongly basic amide, but here the simultaneous reduction of the coordination number from six to five, which leads to an overall contraction, overcompensates this effect. Selected bond lengths and angles of 1 and 2 are listed together with the corresponding values of naphthylcalcium halides and amides in Table 1.…”
Section: Resultsmentioning
confidence: 99%
See 1 more Smart Citation
“…The presence of two strongly basic carbanions in the coordination sphere of calcium leads to lengthening of the metal carbon bonds in comparison to naphthylcalcium halide complexes 9. 1517 For the known compound [Ca(α ‐ Naph){N(SiMe 3 ) 2 }(thf) 3 ]15 an analogous finding might be expected due to the presence of a strongly basic amide, but here the simultaneous reduction of the coordination number from six to five, which leads to an overall contraction, overcompensates this effect. Selected bond lengths and angles of 1 and 2 are listed together with the corresponding values of naphthylcalcium halides and amides in Table 1.…”
Section: Resultsmentioning
confidence: 99%
“…Calcium was activated by dissolution in liquid NH 3 and subsequent reduction of the deep‐blue solution to dryness, resulting in finely divided calcium powders. The complexes [CaI(Ph)(thf) 4 ],10 [CaI(Tol)(thf) 4 ],10 and [CaI(β‐Naph)(thf) 4 ]17 were prepared according to known procedures and recrystallized from THF prior to use. Compounds 1 and 4 were synthesized as preliminarily reported 12.…”
Section: Methodsmentioning
confidence: 99%
“…Bond lengths Ca1C4 and Ca1I1 of 253.0(4) and 318.63(8) pm, respectively, were established. The closely related α‐ and β‐naphthylcalcium iodides [Ca(α‐Naph)(I)(thf) 4 ], [Ca(β‐Naph)(I)(thf) 4 ], and [Ca(β‐Naph)(I)(thf) 4 ] showed similar CaC bond lengths of 255.2(6),19 252.8(5),20 and 253.4(6) pm,21 respectively. The Ca1O bond lengths of 2 varied between 236.9(3) and 241.5(3) pm.…”
Section: Methodsmentioning
confidence: 99%
“…To take into account an appropriate mass-loss for the SC stars, we consider the stellar evolutionary models of rotating MS stars by Köhler & Langer (2012) which encompass the SC mass range and are computed for the LMC metallicity. The above authors use the one-dimensional hydrodynamic binary evolution code of Heger et al (2000) which includes direct treatments of stellar rotation, magnetic field and detailed stellar winds.…”
Section: Evolution Of Super-canonical Stars: the Effect Of Stellar Windsmentioning
confidence: 99%
“…Stellar wind is the most important factor for the evolution of the mass of an isolated massive star during its main sequence. In the computations by Köhler & Langer (2012), the MS stellar wind of Vink et al ( 2001) is applied that includes the bi-stability jump. During the bi-stability jump, a linear interpolation is applied as in Brott et al (2011).…”
Section: Evolution Of Super-canonical Stars: the Effect Of Stellar Windsmentioning
confidence: 99%