scholarly journals Equations of state for two alkali metals at high temperatures

2008 ◽  
Vol 98 (3) ◽  
pp. 032023 ◽  
Author(s):  
K V Khishchenko
1984 ◽  
Vol 29 (12) ◽  
pp. 6489-6499 ◽  
Author(s):  
Rosemary A. MacDonald ◽  
Ramesh C. Shukla ◽  
David K. Kahaner

1890 ◽  
Vol 35 (2) ◽  
pp. 429-469
Author(s):  
W. Dittmar

The fragmentary nature of our knowledge of the behaviour of the more strongly basilous hydrates and carbonates at high temperatures is owing chiefly to the absence of a suitable material for the necessary crucibles. Unfortunately there is no metal which combines the infusibility of platinum with the chemical inertness of gold, in opposition to fiery-fluid caustic alkalies. But the corrosive action of these on platinum, as I showed some years ago, is a function only of the peroxides formed from them by the action of atmospheric oxygen, and, consequently, can easily be prevented by operating in an atmosphere of hydrogen or nitrogen.


2013 ◽  
Vol 8 (2) ◽  
pp. 137-145

Coals contain elements which, although usually found in concentrations lower than 1% (trace elements), can give rise to environmental or technological problems. After gasification most of these elements may occur in gas phase in different proportions. In order to avoid the problems that the presence of trace elements in gas phase can originate during coal gasification processes, a suitable technology needs to be developed. The systems currently being studied and developed for gas cleaning in coal gasification, focus on the removal of sulphur, particulate matter, nitrogen, alkali metals and halogens but not on corrosive or toxic trace elements. Nevertheless, the reduction of trace elements using solid sorbents in gas phase at high temperatures appears to be a promising method for combustion systems. The main objectives of this work were to determine the capacity of different solid sorbents for retaining arsenic, selenium, cadmium and zinc species in gases from coal gasification systems at 550 and 750 ºC and to find out how the sorbent characteristics and operational variables (temperature and gas composition) influence retention. To attain these objectives the sorption capacity (mg of element per g of sorbent) and the efficiency (percentage of element retention) were determined. The study was carried out in a laboratory scale reactor, in which the sorbent was employed as a fixed bed, using synthetic gas mixtures. At the end of each experiment, the sorbent bed (mixture of sorbent + sand) was finely ground and dissolved in a microwave oven with HF, HNO3 and H3BO3, and the element in solution was determined by ICP-MS. The results are discussed in the light of the data for combustion conditions reported in the literature, and possible retention mechanisms are proposed. Different amounts of arsenic, selenium, cadmium, and zinc can be retained in solid sorbents at high temperatures. It was observed that, in a coal gasification atmosphere, limestone, fly ashes and metallic oxide mixtures containing spinels, were the best sorbents, though in each case the retention capacity depended on temperature and atmosphere. Retention capacities between 16-24 mg g-1 were obtained using limestone and fly ashes for arsenic retention. For selenium, the maximum retention capacities ranging between 50-56 mg g-1 were attained using limestone. Alumina in a gasification atmosphere containing HCl was the best sorbent for zinc removal (52 mg g-1). The lowest retention capacities were obtained for cadmium, these being <1 mg g-1 for the different sorbents tested. Retention probably proceeds through different mechanisms, but in most cases a chemical reaction is involved.


1974 ◽  
Vol 65 ◽  
pp. 329-335
Author(s):  
R. S. Hawke

Since Jupiter and Saturn are considered to be composed primarily of hydrogen, its pressure-density equation of state is needed for computational models of their interiors. Until recently, experimental data were limited to 20 kbar statically and 40 kbar dynamically. Since the majority of a major planet is at a pressure in excess of this, there were only theoretical calculations available for modeling.Wigner-Seitz type calculations have been shown to be accurate at determining the equations of state of the alkali metals. Hence, it has been assumed that the equation of state of metallic hydrogen can be calculated in the same way with fair confidence. However, the molecular hydrogen equation of state has been much more ellusive. The many attempts at modeling the interatomic forces have led to rather scattered pressure density relationships.The planetary model situation is further complicated by the expectation that the transition from the molecular to the metallic phase will be in conjunction with a relatively large density change.Recently, data from new experiments have become available; in one case up to 8 Mbar. The data are not in disagreement with many calculations on hydrogen, but the resolution is not yet adequate to determine accurately and confidently, the pressure and the densities of the molecular to metallic phase transition. The accuracy of these parameters in turn affect the models of the planetary interiors, such as the radii of the metallic sphere and high density core.This paper will discuss the details of these relations and the possible affects of the speculative properties of metallic hydrogen.


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