The electronic and magnetic properties of the 3d transition metal intercalates of TiS2

The introduction of 3d transition metals (M) into the van der Waals gaps between the weakly coupled layers of transition metal dichalcogenides TX₂ (T:transition metal, X:chalcogen) produces an interesting family of intercalation compounds, M _x TX₂, the physical properties of which are different from those of the host TX₂ matrix because of ‘host-guest’ interactions. In this article we shall review the salient features of the M _x TiS₂ family with the simple 1T-CdI₂ type layered structure, which have been extensively studied by structural, transport, specific heat and lattice dynamic, magnetic and photoemission spectroscopic measurements. In contrast with the previously reported series of intercalation complexes of the Group V transition metal dichalcogenides, a characteristic of the M _x TiS₂ materials is strong hybridisation between the guest atom M 3d orbitals and the host Ti 3d and S 3p orbitals, leading to changes in the Fermi energy E _F of the conduction band, the density of states at E _F and various types of magnetic orderings. These properties are understood in terms of an itinerant electron or band picture for the intercalant, rather than a rigid band or localised model.     

Thermodynamics for Coulomb systems: A problem at vanishing particle densities

In this paper I combine techniques recently developed by Charles Fefferman with the well-known methods of Joel Lebowitz and Elliott Lieb to resolve some technical problems left unsettled by Lebowitz and Lieb's fundamental 1972 paper The constitution of matter: Existence of thermodynamics for systems composed of electrons and nuclei.     

Precise measurement of electronic gJ value of helium,gJ(4He,23S1)

We report the measurement of $\text{g}{}_{\mathrm{J}}\text{(}{}^4\text{He,2}{}^3\text{S}{}_1\text{)}\text{g}{}_{\mathrm{J}}\text{(}{}^{85}\text{Rb}\text{,5}{}^2\text{S}{}_{\mathrm{<mtext>1</mtext><mtext>2</mtext>}}\text{)}$ by the atomic beam magnetic reson ance method using separated oscillating fields, and hence the determination $\text{g}{}_{\mathrm{J}}\text{(}{}^4\text{He,2}{}^3\text{S}{}_1\text{)}\text{g}{}_{\mathrm{J}}\text{(H,1}{}^2\text{S}{}_{\mathrm{<mtext>1</mtext><mtext>2</mtext>}}\text{)}\text{? 1? (23.19±0.07) × 10}{}^{\mathrm{?6}}$, which agrees with theory and with other less precise recent measurements.     

Sorption kinetics of uranium-238 and neptunium-237 on a glacial sediment

Studies of uptake of radionuclides by natural materials have shown that sorption may occur via fast equilibrium exchange and/or slow kinetic processes, which can be described using a series of box models. This paper describes the use of such models to evaluate the solid-solution partitioning of ²³⁸U and ²³⁷Np on a clay rich sediment. Experimental data are obtained using the batch sorption technique, which are then analysed using 1, 2, and 3 box kinetic models. Uptake of ²³⁸U is initially rapid, with approximately 90% sorbed within the first 30 minutes. Sorption continues, but at a slower rate. Uptake of ²³⁷Np is initially slower than U, with approximately 30% sorbed within the first 30 minutes. Sorption again continues, at a slower rate. Analysis of the experimental data indicates that sorption can be described using 2 and 3 box kinetic models. The results demonstrate that sorption of uranium and neptunium on clay rich sediments occurs via equilibrium and kinetically controlled pathways, with neptunium being controlled by kinetics to a greater extent than uranium. The 2 or 3 box model can describe sorption of neptunium, uranium requires the 3 box model.