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Energy of expansion

The essential features of the earlier commercial models were that the two piston engines were vertically arranged inside the large finned heat exchanger in a static atmosphere of helium with LHe from the Joule-Thomson expansion collecting in the bottom of the dewar. This liquid could be either used in situ or transferred to all external storage dewar. The energy of expansion was absorbed in a crosshead on top of the dewar assembly. [Pg.140]

Another surface parameter of interest is the hysteresis area (AG), which is indicative of energy trapped in a monolayer. The hysteresis area is the difference between the free energy of compression and free energy of expansion which is calculated from the area under corresponding surface pressure - area isotherms. [Pg.175]

Low values of the heat of water absorption can be obtained. These values smaller than the liquefaction energy may result from the superposition of an endothermal mechanism breaking of some bonds (4), further cristallization of the polymers (5), expansion of the macromolecules with change of volume. For this last case, which does not correspond to an expansion mechanism described by the Flory model one has to take into account the enthalpy and free energy of expansion (6,7) or the internal pressure due to the polymer (8). [Pg.15]

Determinations of the calorific value (C.V.) of many gaseous fuels, and of all solid fuels, are performed in constant volume calorimeters. That is to say, values of qp= AV are determined. When the fuel is burnt, however, at one atmosphere pressure, additional energy of expansion (+ve or -ve) against the atmosphere is involved, and the value of q actually realized, that is qp=AH, may be significantly different. We start with equation 2.7 ... [Pg.20]

For example, if we have a gas in a container with a piston, we can access the energy of expansion. If the container is adiabatically insulated, we cannot access the... [Pg.56]

In (Ms way, a system is a transfonner of energy forms. This is not tme in general. A necessary condition to transform energy forms is that the intensive variables are functions of the extensive variables. In order to transform thermal energy into energy of expansion we must have... [Pg.72]

Again, if only the exchange of volume energy, i.e., the energy of compression and the energy of expansion is in between the two gases, is allowed, we will rewrite... [Pg.201]

Note that the first term within the brackets is equivalent to the isothermal energy of expansion. The second term within the parenthesis represents the loss of energy as a result of the second law of thermodynamics. The result predicted by Eq. (3.13) is smaller than the result predicted assuming an isothermal expansion, but greater than the result assuming an adiabatic expansion. [Pg.161]

Another concept is to treat each individual chain as a thermodynamic system subject to elastic energies of expansion and thermodynamic free energies of dilution by solvent. With both the theory of elasticity and the concept of the interaction of two subunits as a mixing phenomenon, the highly repulsive limit derived by the first method was extended to include solvents where the interaction energy for chain subunits was more favorable than the interaction with the solvent. [Pg.16]

Now consider die case where Ais itself a time-independent operator, such as that for the position, momenPiin or angidar momenPiin of a particle or even the energy of the benzene molecule. In these cases, the time-dependent expansion coefficients are unaffected by application of the operator, and one obtains... [Pg.14]

Bell R J 1970 Multipolar expansion for the non-additive third-order interaction energy of three atoms J. [Pg.212]

In 1972 Wegner [25] derived a power-series expansion for the free energy of a spin system represented by a Flamiltonian roughly equivalent to the scaled equation (A2.5.28). and from this he obtained power-series expansions of various themiodynamic quantities around the critical point. For example the compressibility... [Pg.650]

Kirkwood generalized the Onsager reaction field method to arbitrary charge distributions and, for a spherical cavity, obtained the Gibbs free energy of solvation in tenns of a miiltipole expansion of the electrostatic field generated by the charge distribution [12, 1 3]... [Pg.837]

This fomi is called a Ginzburg-Landau expansion. The first temi f(m) corresponds to the free energy of a homogeneous (bulk-like) system and detemiines the phase behaviour. For t> 0 the fiinction/exliibits two minima at = 37. This value corresponds to the composition difference of the two coexisting phases. The second contribution specifies the cost of an inhomogeneous order parameter profile. / sets the typical length scale. [Pg.2370]

Undoubtedly the most successful model of the nematic-smectic A phase transition is the Landau-de Gennes model [201. It is applied in the case of a second-order phase transition by combining a Landau expansion for the free energy in tenns of an order parameter for smectic layering with the elastic energy of the nematic phase [20]. It is first convenient to introduce an order parameter for the smectic stmcture, which allows both for the layer periodicity (at the first hannonic level, cf equation (C2.2A)) and the fluctuations of layer position ur [20] ... [Pg.2559]

Irude model only considers the dipole-dipole interaction if higher-order terms, due to e-quadrupole, quadrupole-quadrupole, etc., interactions are included as well as other i in the binomial expansion, then the energy of the Drude model is more properly an as a series expansion ... [Pg.224]

The eleetronie energy of a moleeule, ion, or radieal at geometries near a stable strueture ean be expanded in a Taylor series in powers of displaeement eoordinates as was done in the preeeding seetion of this Chapter. This expansion leads to a pieture of uneoupled harmonie vibrational energy levels... [Pg.356]

The molecular quantities can be best understood as a Taylor series expansion. For example, the energy of the molecule E would be the sum of the energy without an electric field present, Eq, and corrections for the dipole, polarizability, hyperpolarizability, and the like ... [Pg.256]


See other pages where Energy of expansion is mentioned: [Pg.337]    [Pg.135]    [Pg.174]    [Pg.36]    [Pg.135]    [Pg.57]    [Pg.61]    [Pg.270]    [Pg.286]    [Pg.565]    [Pg.337]    [Pg.135]    [Pg.174]    [Pg.36]    [Pg.135]    [Pg.57]    [Pg.61]    [Pg.270]    [Pg.286]    [Pg.565]    [Pg.213]    [Pg.491]    [Pg.503]    [Pg.503]    [Pg.508]    [Pg.509]    [Pg.2439]    [Pg.442]    [Pg.149]    [Pg.152]    [Pg.153]    [Pg.153]    [Pg.68]    [Pg.133]    [Pg.174]    [Pg.185]    [Pg.211]    [Pg.455]    [Pg.608]    [Pg.121]    [Pg.172]   
See also in sourсe #XX -- [ Pg.36 ]




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Cumulant Expansion of the Free Energy

Many-body expansion of interaction energy

Perturbation expansion of the correlation energy

Taylor Expansion of Potential and Energy

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