An approach to obtaining substantial
amounts of data from a hazardous starting material that can only be
obtained and handled in small quantities is demonstrated by the investigation
of a single small-scale reaction of cyclooctatetraene, C8H8, with a solution obtained from the reduction of Cp′3Pu (Cp′ = C5H4SiMe3) with potassium graphite. This one reaction coupled with oxidation
of a product has provided single-crystal X-ray structural data on
three organoplutonium compounds as well as information on redox chemistry
thereby demonstrating an efficient route to new reactivity and structural
information on this highly radioactive element. The crystal structures
were obtained from the reduction of C8H8 by
a putative Pu(II) complex, (Cp′3PuII)1−, generated in situ, to form the Pu(III) cyclooctatetraenide
complex, [K(crypt)][(C8H8)2PuIII], 1-Pu, and the tetra(cyclopentadienyl) Pu(III)
complex, [K(crypt)][Cp′4PuIII], 2-Pu. Oxidation of the sample of 1-Pu with Ag(I)
afforded a third organoplutonium complex that has been structurally
characterized for the first time, (C8H8)2PuIV, 3-Pu. Complexes 1-Pu and 3-Pu contain Pu sandwiched between parallel (C8H8)2– rings. The (Cp′4PuIII)− anion in 2-Pu features three η5-Cp′ rings and one η1-Cp′ ring, which is a rare example of a formal Pu–C
η1-bond. In addition, this study addresses the challenge
of small-scale synthesis imparted by radiological and material availability
of transuranium isotopes, in particular that of pure metal samples.
A route to an anhydrous Pu(III) starting material from the more readily
available PuIVO2 was developed to facilitate
reproducible syntheses and allow complete spectroscopic analysis of 1-Pu and 2-Pu. PuIVO2 was
converted to PuIIIBr3(DME)2 (DME
= CH3OCH2CH2OCH3) and
subsequently PuIIIBr3(THF)
x
, which was used to independently synthesize 1-Pu, 2-Pu, and 3-Pu.
The compound Rh2(esp)2 (esp = α,α,α',α'-tetramethyl-1,3-benzenediproponoate) is the most generally effective catalyst for nitrenoid amination of C-H bonds. However, much of its fundamental coordination chemistry is unknown. In this work, we study the effects of axial ligand coordination to the catalyst Rh2(esp)2. We report here crystal structures, cyclic voltammetry, UV-vis, IR, Raman, and (1)H NMR spectra for the complexes Rh2(esp)2L2 where L = pyridine, 3-picoline, 2,6-lutidine, acetonitrile, and methanol. The compounds all show well-defined π* → σ* electronic transitions in the 16500 to 20500 cm(-1) range, and Rh-Rh stretching vibrations in the range from 304 to 322 cm(-1). Taking these data into account we find that the strength of axial ligand binding to Rh2(esp)2 increases in the series CH3OH ∼ 2,6-lutidine < CH3CN < 3-methylpyridine ∼ pyridine. Quasi-reversible Rh2(4+/5+) redox waves are only obtained when either acetonitrile or no axial ligand is present. In the presence of pyridines, irreversible oxidation waves are observed, suggesting that these ligands destabilize the Rh2 complex under oxidative conditions.
A new undergraduate inorganic chemistry
laboratory experiment is
presented. An introduction of the spectrochemical series and ligand
exchange is explored using the coordination complex dirhodium tetraacetate,
Rh2(OAc)4. Students have measured the absorption
spectra of the Rh2 complex in the presence of various ligand
environments. In dichloromethane solution, Rh2(OAc)4 displays an absorption feature at 661 nm (222 M–1 cm–1), which shifts to higher energy upon introduction
of neutral axial ligands. The magnitude of the shift corresponds to
the ligand’s placement within the spectrochemical series. Experimental
techniques of synthetic coordination chemistry and UV–vis spectroscopy
are emphasized in this experiment as well as concepts such as molecular
orbital (MO) diagrams and the spectrochemical series.
In
this study, the synthesis, characterization, and pressure response
of a 1D californium mellitate (mellitate = 1,2,3,4,5,6-benzenehexacarboxylate)
coordination polymer, Cf2(mell)(H2O)10·4H2O (Cf-1), are reported. The Cf–O
lengths within the crystal structure are compared to its gadolinium
(Gd-1) and holmium (Ho-1) analogs as well.
These data show that the average Cf–O bond distance is slightly
longer than the average Gd–O bond, consistent with trends in
effective ionic radii. UV–vis-NIR absorption spectra as a function
of pressure were collected using diamond-anvil techniques for both Cf-1 and Ho-1. These experiments show that the
Cf(III) f → f transitions have a stronger dependence on pressure
than that of the holmium analog. In the former case, the shift is
nearly linear with applied pressure and averages 6.6 cm–1/GPa, whereas in the latter, it is <3 cm–1/GPa.
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