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Density expansion coefficients

The same result can also be obtained directly from the virial equation of state given above and the low-density fonn of g(r). B2(T) is called the second virial coefficient and the expansion of P in powers of is known as the virial expansion, of which the leading non-ideal temi is deduced above. The higher-order temis in the virial expansion for P and in the density expansion of g(r) can be obtained using the methods of cluster expansion and cumulant expansion. [Pg.423]

The density is computed as p(r) = 2. n i ). (/ )p. Often, p(r) is expanded in an AO basis, which need not be the same as the basis used for the and the expansion coefficients of p are computed in tenns of those of the It is also connnon to use an AO basis to expand p (r) which, together with p, is needed to evaluate the exchange-correlation fiinctionaTs contribution toCg. [Pg.2183]

Metal Crystal 22° C stmeture 1000° c Melting point, °C Density, g/cm Thermal expansion coefficient at RT, ioV°c Thermal conductivity at RT, W/(m-K)" Young s modulus, GPa "... [Pg.109]

Ultrasonic Spectroscopy. Information on size distribution maybe obtained from the attenuation of sound waves traveling through a particle dispersion. Two distinct approaches are being used to extract particle size data from the attenuation spectmm an empirical approach based on the Bouguer-Lambert-Beerlaw (63) and a more fundamental or first-principle approach (64—66). The first-principle approach implies that no caHbration is required, but certain physical constants of both phases, ie, speed of sound, density, thermal coefficient of expansion, heat capacity, thermal conductivity. [Pg.133]

AUoy Constituents, wt % Be Co Density, g/mL Elastic modulus GPa Thermal expansion coefficient, ppm/°C Thermal conductivity, W/(m-K) Melting range, °C... [Pg.70]

The expansion coefficient of a solid can be estimated with the aid of an approximate thermodynamic equation of state for solids which equates the thermal expansion coefficient with the quantity where yis the Griineisen dimensionless ratio, C, is the specific heat of the solid, p is the density of the material, and B is the bulk modulus. For fee metals the average value of the Griineisen constant is near 2.3. However, there is a tendency for this constant to increase with atomic number. [Pg.1127]

Material Density Melting or decomposition ID) lemperalvre (Kj Modulus (GNm- l Expansion coefficient X 10 (K- ) Thermal conductivity at lOOOK (Wm- K- I Fracture toughness K.IMNm- )... [Pg.206]

The specific heats of polymers are large - typically 5 times more than those of metals when measured per kg. When measured per m, however, they are about the same because of the large differences in density. The coefficients of thermal expansion of polymers are enormous, 10 to 100 times larger than those of metals. This can lead to problems of thermal stress when polymers and metals are joined. And the thermal conductivities are small, 100 to 1000 times smaller than those of metals. This makes polymers attractive for thermal insulation, particularly when foamed. [Pg.226]

Physical characteristics Molecular weight Vapour density Specific gravity Melting point Boiling point Solubility/miscibility with water Viscosity Particle size size distribution Eoaming/emulsification characteristics Critical temperature/pressure Expansion coefficient Surface tension Joule-Thompson effect Caking properties... [Pg.4]

Both the Fock matrix—through the density matrix—and the orbitals depend on the molecular orbital expansion coefficients. Thus, Equation 31 is not linear and must be solved iteratively. The procedure which does so is called the Self-Consistent Field... [Pg.263]

The moments of the distribution function can be amply related to the expansion coefficients. Using the fact that ( ) andF (0,9>) are unity, we have for the number density ... [Pg.27]

The terms p, T, and v are characteristic reducing parameters which may be obtained by fitting pressure-volume-temperature data (density, thermal expansion coefficient, and thermal pressure coefficient) for each pure component in the mixture (3,12). Values of p, v, and T are given in Tables I and II. [Pg.188]

Extended Hiickel calculations are performed with a nonorthogonalized AO basis set therefore, the spin densities are to be evaluated by gross atomic populations and not simply by squares of expansion coefficients. [Pg.349]

For neutral radicals, the most significant term in eq. (144) is that which is first order in the overlap. This term contains expansion coefficients of directly interacting positions where in dimerization a new a bond is formed. The higher the values of these expansion coefficients, the larger is the interaction energy, in accord with chemical anticipation for dimerization to occur in positions of the highest spin densities. With radical ions, also, the last terms in eqs. (143) and (144) are important, since they stand for coidombic interactions. [Pg.375]

The expansion coefficients, which actually contain all relevant information about the charge density, are usually collected in the so-called density matrix P with elements... [Pg.112]

Since we have chosen the coK to be orthonormal, the expansion coefficients cK are related to the density matrix according to... [Pg.126]


See other pages where Density expansion coefficients is mentioned: [Pg.698]    [Pg.666]    [Pg.98]    [Pg.389]    [Pg.114]    [Pg.698]    [Pg.666]    [Pg.98]    [Pg.389]    [Pg.114]    [Pg.449]    [Pg.472]    [Pg.473]    [Pg.297]    [Pg.475]    [Pg.500]    [Pg.505]    [Pg.502]    [Pg.128]    [Pg.212]    [Pg.208]    [Pg.503]    [Pg.188]    [Pg.13]    [Pg.397]    [Pg.398]    [Pg.1177]    [Pg.866]    [Pg.9]    [Pg.266]    [Pg.331]    [Pg.374]    [Pg.97]    [Pg.597]    [Pg.185]    [Pg.190]    [Pg.217]    [Pg.138]   
See also in sourсe #XX -- [ Pg.389 ]




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Density expansion

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