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Lighter elements

The new elements neptunium and plutonium have been produced in quantity by neutron bombardment of uranium. Subsequently many isotopes have been obtained by transmutation and synthetic isotopes of elements such as Ac and Pa are more easily obtained than the naturally occurring species. Synthetic species of lighter elements, e.g. Tc and Pm are also prepared. [Pg.403]

Hafnium [7440-58-6] Hf, is in Group 4 (IVB) of the Periodic Table as are the lighter elements zirconium and titanium. Hafnium is a heavy gray-white metallic element never found free in nature. It is always found associated with the more plentiful zirconium. The two elements are almost identical in chemical behavior. This close similarity in chemical properties is related to the configuration of the valence electrons, and for zirconium and... [Pg.439]

Similar accuracies have been found for thick, homogeneous, complex specimens when corrections for secondary excitation are also included. With appropriate standards, total accuracies of 2% have been demonstrated. Because the determination of the lighter elements (i.e., 5 < Z< 15) are more sensitive to the uncertainties in the data base items listed above, less accuracy should be expected for these elements. [Pg.366]

By the time Ho is reached the Ln radius has been sufficiently reduced to be almost identical with that of Y which is why this much lighter element is invariably associated with the heavier lanthanides. [Pg.1234]

In the early years of this century the periodic table ended with element 92 but, with J. Chadwick s discovery of the neutron in 1932 and the realization that neutron-capture by a heavy atom is frequently followed by j6 emission yielding the next higher element, the synthesis of new elements became an exciting possibility. E. Fermi and others were quick to attempt the synthesis of element 93 by neutron bombardment of but it gradually became evident that the main result of the process was not the production of element 93 but nuclear fission, which produces lighter elements. However, in 1940, E. M. McMillan and P. H. Abelson in Berkeley, California, were able to identify, along with the fission products, a short-lived isotope of... [Pg.1251]

In addition, MNDO uses the approximation, for some of the lighter elements. [Pg.87]

Values of Wk below 0.3 are common for the lighter elements. (See Appendix II, Table 2.)... [Pg.36]

Fig. 9-3. Comparison of 50-kv, 40-ma (dotted line) spectra with 100-kv, 20-ma (solid line) spectra of hafnium and tantalum, showing efficient excitation of the K spectra at the higher voltage. The higher voltage is particularly useful in connection with analyses of niobium-tantalum mixtures and zirconium-hafnium mixtures which are difficult at the lower voltage because of the interference of the K lines of the lighter elements with the L spectra of the heavier elements. (Courtesy of M. L. Salmon, Fluo-X-Spec Analytical Laboratory, Denver, Colo.)... Fig. 9-3. Comparison of 50-kv, 40-ma (dotted line) spectra with 100-kv, 20-ma (solid line) spectra of hafnium and tantalum, showing efficient excitation of the K spectra at the higher voltage. The higher voltage is particularly useful in connection with analyses of niobium-tantalum mixtures and zirconium-hafnium mixtures which are difficult at the lower voltage because of the interference of the K lines of the lighter elements with the L spectra of the heavier elements. (Courtesy of M. L. Salmon, Fluo-X-Spec Analytical Laboratory, Denver, Colo.)...
The chemistry of plutonium is unique in the periodic table. This theme is exemplified throughout much of the research work that is described in this volume. Many of the properties of plutonium cannot be estimated accurately based on experiments with lighter elements, such as uranium and neptunium. Because massive amounts of plutonium have been and are being produced throughout the world, the need to define precisely its chemical and physical properties and to predict its chemical behavior under widely varying conditions will persist. In addition to these needs, there is an intrinsic fundamental interest in an element with so many unusual properties and with so many different oxidation states, each with its own chemistry. [Pg.7]

The only structurally characterized In—Sb adduct is (Me3SiCH2)3 In—Sb(Tms)3 19 [38], featuring an In—Sb bond distance of 300.8(1) pm. Due to the lack of other structurally characterized In—Sb adducts, no structural comparisons can be made. The In—Sb bond length found in 19 is supposed to be at the lower end of the In—Sb dative bond range since the covalent radius of In (r ov 143 pm) is about 17 pm larger than those of the lighter elements Al and Ga. Therefore, In—Sb dative bonds are expected to... [Pg.129]

Group 13/15 heterocycles of the type [R2MER2]x and [RMER ]x containing the lighter elements of group 15, N and P, are usually synthesized by alkane, hydrogen or salt elimination reactions, as can be seen in Scheme 6 [8b, 11],... [Pg.139]

Processes that occur at the upper and lower boundaries of the atmosphere. Many atmospheric constituents are formed, and many undergo a wide range of reactions at the lower boundary. At the upper boundary lighter elements are lost to space and some important substances are acquired. [Pg.132]

Lighter elements show a stronger tendency to develop a stereochemically active lone pair than their heavier homologues. For instance, for antimony(III) more distorted structures are known than for bismuth(III) ]29]. [Pg.17]

The expressions (4.22)-(4.23) found in chap. 4 for the isomer shift 5 in nonrelativ-istic form may be applied to lighter elements up to iron without causing too much of an error. In heavier elements, however, the wave function j/ is subject to considerable modification by relativistic effects, particularly near the nucleus (remember that the spin-orbit coupling coefficient increases with Z ). Therefore, the electron density at the nucleus l /(o)P will be modified as well and the aforementioned equations for the isomer shift require relativistic correction. This has been considered [1] in a somewhat restricted approach by using Dirac wave functions and first-order perturbation theory in this approximation the relativistic correction simply consists of a dimensionless factor S (Z), which is introduced in the above equations for S,... [Pg.546]

The basic function of the spectrometer is to separate the polychromatic beam of radiation coming from the specimen in order that the intensities of each individual characteristic line can be measured. In principle, the wide variety of instruments (WDXRF and EDXRF types) differ only in the type of source used for excitation, the number of elements which they are able to measure at one time and the speed of data collection. Detectors commonly employed in X-ray spectrometers are usually either a gas-flow proportional counter for heavier elements/soft X-rays (useful range E < 6keV 1.5-50 A), a scintillation counter for lighter elements/hard X-rays (E > 6keV 0.2-2 A) or a solid-state detector (0.5-8 A). [Pg.629]

The Gillespie-Nyholm rules can be applied with the aid of this formulation. The occurrence of both kinds of building blocks in Li2Sb, chains and dumbbells, shows that in this case the Peierls distortion contributes only a minor stabilization and is partially overridden by other effects. The Peierls distortion cannot be suppressed that easily with lighter elements. [Pg.137]


See other pages where Lighter elements is mentioned: [Pg.46]    [Pg.155]    [Pg.402]    [Pg.317]    [Pg.216]    [Pg.150]    [Pg.536]    [Pg.172]    [Pg.347]    [Pg.483]    [Pg.13]    [Pg.15]    [Pg.1180]    [Pg.215]    [Pg.850]    [Pg.268]    [Pg.272]    [Pg.21]    [Pg.113]    [Pg.247]    [Pg.297]    [Pg.66]    [Pg.724]    [Pg.180]    [Pg.120]    [Pg.236]    [Pg.202]    [Pg.147]    [Pg.301]    [Pg.641]    [Pg.234]    [Pg.100]    [Pg.171]    [Pg.205]    [Pg.209]   
See also in sourсe #XX -- [ Pg.298 ]




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Spin-orbit effects lighter elements

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