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Additional Thermodynamic Properties

Internal energy, u, is an intensive property of the system and it represents the energy associated with translation, vibration, and rotational motions and structures of the atoms and molecules. [Pg.66]

Enthalpy is also an intensive property and expressed as a sum of internal energy and product of pressure, p, and specific volume, v [Pg.66]

The specific Gibbs function or Gibbs free energy is defined as [Pg.66]

For a stationary control volume with negligible changes in kinetic energy and potential energy, Equation 3.20 can rewritten as [Pg.67]

The enthalpy of formation for Tmo.ggSe is AHf =-103 7 kcal/mol, determined by the fluorine combustion method by Fritzler [14]. Fig. 167 shows AHf as a function of x in TmxSe, based on more recent investigations with the same method. The increase of AHf (43%) for 0.92 x 0.935 demonstrates the existence of a miscibility gap. Two other miscibility [Pg.340]

94 (hatched) are possibly derived from inhomogeneous samples. [Pg.341]

The difference in energy for stoichiometric TmSe in the intermediate valence state and hypothetical Tm Se is estimated from theenthalpy of solution in aqueous 4 N HCl(see p. 380) to be 42 kcal/mol, Fritzler, Kaldis [6]. A value of AH 46 kcal/mol is estimated for the difference betvy een Tm o.gSe and Tm o2Se. The stabilization energy in TmgSeg due to the ordering of vacancies is estimated to be AH 5 to 7 kcal/mol, Kaldis, Fritzler [16]. [Pg.341]

The electronic contribution to the entropy Sgi, defined as the total entropy minus the lattice and Schottky contributions with and without an external magnetic field H, along the [100] direction between 1.3 and --18K is shown in Fig. 168. The electronic entropy reaches Sei = 0.5 R In 2 at Tn (3.23 K) and H = 0, Berton et al. [12, p. 3507]. [Pg.341]

Electronic contribution to the entropy Sei for nearly stoichiome- q8 trie TmSe with and without an external magnetic field along the [100] direc-  [Pg.341]


Ammonia is readily absorbed ia water to make ammonia liquor. Figure 2 summarizes the vapor—Hquid equiUbria of aqueous ammonia solutions and Figure 3 shows the solution vapor pressures. Additional thermodynamic properties may be found ia the Hterature (1,2). Considerable heat is evolved duriag the solution of ammonia ia water approximately 2180 kJ (520 kcal) of heat is evolved upon the dissolution of 1 kg of ammonia gas. [Pg.336]

Additional thermodynamic properties are related to these and arise by arbitrary definition. Multiplication ofEq. (4-11) hy n and differentiation yields the general expression ... [Pg.515]

All of the primary thermodynamic properties—P, V, T, U, and S—are included in Eq. (6.1). Additional thermodynamic properties arise only by definition in relation to these primary properties. In Chap. 2 the enthalpy was defined as a matter of convenience by the equation ... [Pg.93]

The standard electrode potential is then given as -2.37 V for the Fm + + 2e = Fm° reaction. The authors estimated 5 mV accuracy for the measured half-wave potential seems reasonable, but there is a much larger uncertainty in the estimated amalgamation potential. Because the amalgamation potential represents a large correction in obtaining the standard potential, caution should be exercised in combining this standard potential with other data to calculate additional thermodynamic properties. [Pg.241]

Similar equations are valid for the additional thermodynamic properties to be introduced later. [Pg.20]

Finally, the proton affinities of several atomic metal anions, M" (M -V, Cr, Fe, Co, Mo, and W), have been determined by bracketing methods (47). Combining these data with measured electron affinities of the metals yielded homolytic bond energies for the neutral hydrides, D (M-H). The monohydride bond energies compare favorably with other experimental and theoretical data in the literature and were used to derive additional thermodynamic properties for metal hydride ions and neutrals. [Pg.58]

Of these featores, the pressure-dependence of SCF properties dominates or influences virtually every process conducted on polymers. Pressure governs such properties as density, solubility parameter, and dielectric constant changes of more than an order of magnitude are common when pressure is sufficiently increased to transform a gas into a supercritical fluid. This chapter primarily compiles experimental data on the pressure dependence of physical properties of fluid phase polymer-SCF mixtures. Phase equilibria are addressed, including the solubility of polymers in SCFs, the solubility of SCFs in liquid polymers, and the three-phase solid-fluid-fluid equilibria of crystalline polymers saturated with SCFs. Additional thermodynamic properties include glass transition temperature depressions of polymers, and interfacial tension between SCF-swollen polymers and the SCF. The viscosity of fluid phase polymer-SCF mixtures is also treated. [Pg.319]

For reactions in solntion an additional thermodynamic property that can be helpful is available. The effect of pressure on the equilibrium constant of a reaction yields the volume change of reaction, AT, given by Equation 1.28. [Pg.19]

This paper presents experimental results for the equilibrium adsorption of the shorter unbranched hydrocarbons, ethane, ethene, propane, and propene and of the linear and branched C4 alkanes n-butane and isobutane on Kureha activated carbon, a purely microporous material. The aim of the present study is to investigate comparative packing efficiencies of these light alkanes and alkenes and of the linear and branched C4 alkanes inside the adsorbent pores. An interpretation of the difference in the adsorption behaviour for these six adsorptives is given. In addition, thermodynamic properties like isosteric heat associated with adsorption are presented to characterize interactions between adsorptive and adsorbent and an outlook on mixture adsorption is discussed for this carbon. [Pg.288]

Investigations to find such additive constituent properties of molecules go back to the 1920s and 1930s with work by Fajans [6] and others. In the 1940s and 1950s lhe focus had shifted to the estimation of thermodynamic properties of molecules such as heat of formation, AHf, entropy S°, and heat capacity, C°. [Pg.321]

Thermodynamic properties such as heats of reaction and heats of formation can be computed mote rehably by ab initio theory than by semiempirical MO methods (55). However, the Hterature of the method appropriate to the study should be carefully checked before a technique is selected. Finally, the role of computer graphics in evaluating quantum mechanical properties should not be overlooked. As seen in Figures 2—6, significant information can be conveyed with stick models or various surfaces with charge properties mapped onto them. Additionally, information about orbitals, such as the highest occupied molecular orbital (HOMO) and the lowest unoccupied molecular orbital (LUMO), which ate important sites of reactivity in electrophilic and nucleophilic reactions, can be plotted readily. Figure 7 shows representations of the HOMO and LUMO, respectively, for the antiulcer dmg Zantac. [Pg.163]

Tables 2,3, and 4 outline many of the physical and thermodynamic properties ofpara- and normal hydrogen in the sohd, hquid, and gaseous states, respectively. Extensive tabulations of all the thermodynamic and transport properties hsted in these tables from the triple point to 3000 K and at 0.01—100 MPa (1—14,500 psi) are available (5,39). Additional properties, including accommodation coefficients, thermal diffusivity, virial coefficients, index of refraction, Joule-Thorns on coefficients, Prandti numbers, vapor pressures, infrared absorption, and heat transfer and thermal transpiration parameters are also available (5,40). Thermodynamic properties for hydrogen at 300—20,000 K and 10 Pa to 10.4 MPa (lO " -103 atm) (41) and transport properties at 1,000—30,000 K and 0.1—3.0 MPa (1—30 atm) (42) have been compiled. Enthalpy—entropy tabulations for hydrogen over the range 3—100,000 K and 0.001—101.3 MPa (0.01—1000 atm) have been made (43). Many physical properties for the other isotopes of hydrogen (deuterium and tritium) have also been compiled (44). Tables 2,3, and 4 outline many of the physical and thermodynamic properties ofpara- and normal hydrogen in the sohd, hquid, and gaseous states, respectively. Extensive tabulations of all the thermodynamic and transport properties hsted in these tables from the triple point to 3000 K and at 0.01—100 MPa (1—14,500 psi) are available (5,39). Additional properties, including accommodation coefficients, thermal diffusivity, virial coefficients, index of refraction, Joule-Thorns on coefficients, Prandti numbers, vapor pressures, infrared absorption, and heat transfer and thermal transpiration parameters are also available (5,40). Thermodynamic properties for hydrogen at 300—20,000 K and 10 Pa to 10.4 MPa (lO " -103 atm) (41) and transport properties at 1,000—30,000 K and 0.1—3.0 MPa (1—30 atm) (42) have been compiled. Enthalpy—entropy tabulations for hydrogen over the range 3—100,000 K and 0.001—101.3 MPa (0.01—1000 atm) have been made (43). Many physical properties for the other isotopes of hydrogen (deuterium and tritium) have also been compiled (44).
For cubic crystals, which iaclude sUicon, properties described by other than a zero- or a second-rank tensor are anisotropic (17). Thus, ia principle, whether or not a particular property is anisotropic can be predicted. There are some properties, however, for which the tensor rank is not known. In addition, ia very thin crystal sections, the crystal may have two-dimensional characteristics and exhibit a different symmetry from the bulk, three-dimensional crystal (18). Table 4 is a listing of various isotropic and anisotropic sUicon properties. Table 5 gives values for the more common physical properties and for some of the thermodynamic properties. Figure 5 shows some thermal properties. [Pg.529]

AH the foregoing faciUties form part of the spectmm of options that, in addition to the permanent system data bank, enable the engineer to get the most out of a flow-sheeting system. The following Hst shows the physical properties that are often required for process simulation. The methods of estimating these properties, when direct measurements are not available, are indicated in the references following the properties (also see Thermodynamic properties). [Pg.76]

The increasing ranges of pressure and temperature of interest to technology for an ever-increasing number of substances would necessitate additional tables in this subsection as well as in the subsec tion Thermodynamic Properties. Space restrictions preclude this. Hence, in the present revision, an attempt was made to update the fluid-compressibihty tables for selected fluids and to omit tables for other fluids. The reader is thus referred to the fourth edition for tables on miscellaneous gases at 0°C, acetylene, ammonia, ethane, ethylene, hydrogen-nitrogen mixtures, and methyl chloride. The reader is also... [Pg.184]

Additional data are contained in the subsection Thermodynamic Properties. Data on water are also contained in that subsection. Admtional tables for water are found in Eng. Sci. Data Item 68008, 251 Regent Street, London, England, which contains about 5000 values from 1 to 1000 bar, 0 to 1500°C. [Pg.205]

The values given in the following table for the heats and free energies of formation of inorganic compounds are derived from a) Bichowsky and Rossini, Thermochemistry of the Chemical Substances, Reinhold, New York, 1936 (h) Latimer, Oxidation States of the Elements and Their Potentials in Aqueous Solution, Prentice-Hall, New York, 1938 (c) the tables of the American Petroleum Institute Research Project 44 at the National Bureau of Standards and (d) the tables of Selected Values of Chemical Thermodynamic Properties of the National Bureau of Standards. The reader is referred to the preceding books and tables for additional details as to methods of calculation, standard states, and so on. [Pg.231]

Since we have assumed pairwise additivity, the thermodynamic properties can be obtained from the RDF. For example, the energy is given by... [Pg.138]

By far the most common methods of studying aqueous interfaces by simulations are the Metropolis Monte Carlo (MC) technique and the classical molecular dynamics (MD) techniques. They will not be described here in detail, because several excellent textbooks and proceedings volumes (e.g., [2-8]) on the subject are available. In brief, the stochastic MC technique generates microscopic configurations of the system in the canonical (NYT) ensemble the deterministic MD method solves Newton s equations of motion and generates a time-correlated sequence of configurations in the microcanonical (NVE) ensemble. Structural and thermodynamic properties are accessible by both methods the MD method provides additional information about the microscopic dynamics of the system. [Pg.349]

When an ionic solution contains neutral molecules, their presence may be inferred from the osmotic and thermodynamic properties of the solution. In addition there are two important effects that disclose the presence of neutral molecules (1) in many cases the absorption spectrum for visible or ultraviolet light is different for a neutral molecule in solution and for the ions into which it dissociates (2) historically, it has been mainly the electrical conductivity of solutions that has been studied to elucidate the relation between weak and strong electrolytes. For each ionic solution the conductivity problem may be stated as follows in this solution is it true that at any moment every ion responds to the applied field as a free ion, or must we say that a certain fraction of the solute fails to respond to the field as free ions, either because it consists of neutral undissociated molecules, or for some other reason ... [Pg.38]

R.C. Oliver et al, USDeptCom, Office Tech-Serv ..AD 265822,(1961) CA 60, 10466 (1969) Metal additives for solid proplnts formulas for calculating specific impulse and other proplnt performance parameters are given. A mathematical treatment of the free-energy minimization procedure for equilibrium compn calcns is provided. The treatment is extended to include ionized species and mixing of condensed phases. Sources and techniques for thermodynamic-property calcns are also discussed... [Pg.946]

In addition to deciding on the method of normalization of activity coefficients, it is necessary to undertake two additional tasks first, a method is required for estimating partial molar volumes in the liquid phase, and second, a model must be chosen for the liquid mixture in order to relate y to x. Partial molar volumes were discussed in Section IV. This section gives brief attention to two models which give the effect of composition on liquid-phase thermodynamic properties. [Pg.173]

The implication is that the thermodynamic properties are also additive. Thus... [Pg.535]


See other pages where Additional Thermodynamic Properties is mentioned: [Pg.178]    [Pg.341]    [Pg.345]    [Pg.66]    [Pg.340]    [Pg.178]    [Pg.341]    [Pg.345]    [Pg.66]    [Pg.340]    [Pg.61]    [Pg.325]    [Pg.469]    [Pg.238]    [Pg.335]    [Pg.182]    [Pg.511]    [Pg.851]    [Pg.17]    [Pg.20]    [Pg.25]    [Pg.283]    [Pg.306]    [Pg.61]   


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Additive properties

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