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Coordinated Universal Time coordination number

The considerations presented in this work suggest that at the percolation threshold the ratio of the shear modulus to the bulk modulus is a universal quantity, which does not depend on the elastic properties of the percolation phase. It is well known, however, that this ratio depends on the coordination number of the lattice on which the percolation takes place. Taking this into account, we conjecture that when the coordination number, Z, of the underlying lattice is more than four times larger than the dimension of the lattice, Z > Ad, Poisson s ratio near the percolation threshold should be negative, irrespective of the value of Poisson s ratio of the percolation phase. [Pg.214]

Coordinated Universal Time (UTC) follows International Atomic Time (TAl) exactly except for an integral number of seconds, presently 32. These leap seconds are inserted on the advice of the International Earth Rotation Service (lERS) to ensure that, on average over the years, the sun is overhead within 0.9 s of 12 00 00 UTC on the meridian of Greenwich. UTC is thus the modern successor of Greenwich Mean Time, GMT, which was used when the unit of time was the mean solar day. [Pg.90]

Coordinated Universal Time (UTC) runs at the same rate as TAI. However, it differs from TAI by an integral number of seconds. This difference increases when leap... [Pg.321]

In order to investigate the quantum number dependence of vibrational dephasing, an analysis was done on two systems C-I stretching mode in neat-CH3I and C-H mode in neat-CHCl3 systems. The C-I and C-H frequencies are widely different (525 cm-1 and 3020 cm-1, respectively) and so also their anharmonic constants. Yet, they both lead to a subquadratic quantum number dependence. The time-dependent friction on the normal coordinate is found to have the universal nonexponential characteristics in both systems—a distinct inertial Gaussian part followed by a slower almost-exponential part. [Pg.169]

The isotropy properties assumed for the model universe imply that it is statistically spherically symmetric about the chosen origin. If, for the sake of simplicity, it is assumed that the characteristic sampling times over which the assumed statistical isotropies become exact are infinitesimal, then the idea of statistical spherical symmetry, gives way to the idea of exact spherical symmetry thereby allowing the idea of some kind of rotationally invariant radial coordinate to exist. As a first step toward defining such an idea, suppose only that the means exists to define a succession of nested spheres, Sj C S2C ClSp, about the chosen origin since the model universe with infinitesimal characteristic sampling times is stationary, then the flux of particles across the spheres is such that these spheres will always contain fixed numbers of particles, say N, N2,. . . , NP, respectively. [Pg.318]

The time-dependent Schrodinger equation (2.43) presents a serious problem from the point of view of relativity theory it does not treat space and time in a symmetric way, because second-order derivatives of the wavefunction with respect to spatial coordinates are accompanied by a first-order derivative with respect to time. One way out, as actually proposed by Schrodinger and later known as the Klein-Gordon equation, would be to have also second-order derivatives with respect to time. However, that would lead to a total probability for the particle under consideration which would be a function of time, and to a variation of the number of particles of the universe (which, at the time, was completely unacceptable). In 1928, Dirac sought the solution for this problem, by accepting first-order derivation in the case of time and forcing the spatial derivatives to also be first order. This requires the wavefunction to have four components (functions of the spatial coordinates alone), often called a four-component spinor . [Pg.42]

In 1930 the Department of Chemistry was established in Osaka University, and Ryutaro Tsuchida( 1903-1962) was appointed the professor of inorganic chemistry. Also Taku Uemura(l893-1980) began the research on coordination chemistry at the Tokyo Institute of Technology at nearly the same time. Both men were former co-workers of Yuji Shibata s. Thus young coordination chemists graduated from these newly established laboratories, and the numbers of published research papers gradually increased. [Pg.141]

Werner has been claimed as a national by the Germans, French and Swiss. He was born in Mulhouse while Alsace was still part of France, remained there after it was seized in the Franco-Prussian War of 1870 (and even served in the German army) but he spent most of his career as an independent researcher in Zurich, coming to the University of Zurich (initially as an organic chemist ) in 1893. By then he had already taken an interest in coordination compounds, which at the time were poorly (if at aU) understood, especially with regard to constitution and structure [11]. The existence of a number of series of species, each containing a metal in combination with the same constituents but in varying numbers, was very hard to reconcile with well-established laws of proportions and valency. [Pg.11]


See other pages where Coordinated Universal Time coordination number is mentioned: [Pg.144]    [Pg.78]    [Pg.219]    [Pg.413]    [Pg.1837]    [Pg.117]    [Pg.6]    [Pg.53]    [Pg.246]    [Pg.218]    [Pg.413]    [Pg.299]    [Pg.76]    [Pg.106]    [Pg.535]    [Pg.499]    [Pg.27]    [Pg.134]    [Pg.36]    [Pg.1596]    [Pg.18]    [Pg.134]    [Pg.2296]    [Pg.8]    [Pg.7]    [Pg.39]    [Pg.85]    [Pg.114]    [Pg.2279]    [Pg.1841]    [Pg.273]    [Pg.274]    [Pg.54]    [Pg.344]    [Pg.358]    [Pg.54]    [Pg.5]    [Pg.2]    [Pg.168]    [Pg.80]    [Pg.48]    [Pg.364]    [Pg.340]   
See also in sourсe #XX -- [ Pg.943 ]




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Coordinated Universal Time

Coordination number

Universal time

Universal time coordinate

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