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Internal energy density

Figure 4.1. Profile of a steady shock wave, risetime imparting a particle velocity, e.g., Uj, pressure Pi, and internal energy density E, propagating with velocity U, into material that is at rest at density pQ and internal energy density Eq. Figure 4.1. Profile of a steady shock wave, risetime imparting a particle velocity, e.g., Uj, pressure Pi, and internal energy density E, propagating with velocity U, into material that is at rest at density pQ and internal energy density Eq.
We can compare this to the expression derived from experimental data for transition in internal energy density. Good agreement between the empirical model and the experimentally derived curve is observed (Figure 5.15). [Pg.172]

U, U, u Internal energy, internal energy per mole (or particle), internal energy density J, J mol-1, J m-3... [Pg.668]

The rate of change in the local internal energy density, du/dt, and the component concentrations, dcfdt. are obtained from an energy balance and n component balances similar to Eq. (A.29) ... [Pg.385]

Let us subtract (6.2.6) from (6.2.7) this yields an expression for the rate of change of internal energy density ... [Pg.541]

In Eqs. (6.2.8) and (6.2.9) JQ was identified as a heat flux vector, yet this quantity corresponds to e, the internal energy density. Consult Sections 1.8 and 1.16 and explain again why this particular designation is appropriate. [Pg.545]

The WK model completely reparametrizes TIP4P. Charges are scaled to reproduce the quadrupole moment of the isolated molecule. The dipole moment, on the other hand, is close to its value in the liquid phase, assumed 2.6 D as in ice [158-161]. The LJ parameters are then adjusted to reproduce internal energy, density and 0-0 pair correlation function of the liquid at 25 C. [Pg.394]

The total energy density of a system involves contributions from the internal energy density e, the kinetic energy density JC, and the potential energy density V. [Pg.350]

Henceforth we neglect motion of the center of mass (setting i> = 0) and we now consider the time derivative of the internal energy density, given by... [Pg.351]

In looking ahead to the theoretical development in later sections it is expedient to separate out from the right-hand side of Eq. (6.1.17a) the last three terms and to sum the remaining contributions as a time rate of change of the internal energy density, e. Thus, we set... [Pg.352]

This equation relates the change in entropy density to the changes in the internal energy density and the molar concentration. This equation can be alternatively expressed as... [Pg.331]

The starting point of the investigation is the introduction of a scalar microstruc-tural parameter k which contributes to the total energy E of the body under study as pointed out in Refs. [38] and 39]. In Eq. (1) p, s and x are the mass density, the specific internal energy density and the velocity, respectively. The parameter k in the product pk describes microstructural properties and transfers the square of the rate of k to the dimensions of a specific energy density. In addition, the energy supply Ri and the energy flux R2 are also modified in the form of Eqs. (2) and (3), wherein pb is the body force density, pg is the supply of K, and p r is the heat supply. Further quantities are the stress vector t = T n associated to the Cauchy stress tensor T and to the outer normal n, the microstructural flux s = S n and the heat flux qi = —q n. [Pg.322]

The thermal energy of a liquid particle is defined by the internal energy density, which depends on parameters of local thermodynamic condition. According to the first law of thermodynamics. [Pg.61]

Represents internal energy density that must be coupled to the load. Coupling will reduce energy density hy a factor of 2 at least. [Pg.1671]

In CFAST, a set of equations that predict state variables (pressure, temperamre, etc.) are solved based on the enthalpy and mass flux over small increments of time. These equations are derived from the conservation equations for mass, momentum, energy and the ideal gas law together with plume models, vent flow equations, radiation and combustion models. Forney and Moss reviewed that there are 11 variables to be solved the mass, internal energy, density, temperature and volume for the upper and lower layers (Mu, Eu, qu, Tu, Vu and ML, EL, qL, TL, VL), and the pressure R Because there are seven constraints, any four of those variables have to be chosen as solution variables. The four variables solved are the pressure... [Pg.903]

A compartment is divided into two control volumes, a relatively hot upper layer and a relatively cool lower layer, as illustrated in Fig. 4. The gas in each layer has attributes of mass, internal /energy, density, temperature, and volume denoted respectively by m, Ei, ni, Ti, and Vi where i = Lfoi the lower layer and / = U for the upper layer. The compartment as a whole has the attribute of pressure P. These 11 variables are related by means of the following seven constraints (counting density, internal eneigy and the ideal gas law twice, once for each Iayer)[14]. [Pg.903]

From the internal energy density u and entropy density s, we obtain the local variables of... [Pg.120]

The finite width of the transition region is reflected in the position dependent profiles of mass density p(z), internal energy density e z) and stress tensor which can all be obtained from Monte Carlo simulations. In ac-... [Pg.268]

By combining (1), (2) and (3), we can evaluate the system by expressing the properties (internal energy, density and enthalpy) as a function of pressure. Since heat leak iq) is dependent on the container geometry, supports and insulation quality, it is difficult to provide a useful general expression. [Pg.273]

Extending Eq. (3.84) by this electrostatic energy the infinitesirrral change in internal energy density becomes... [Pg.56]

Internal energy density t/ is a thermodynamic potential in conjunction with independent variables a, Dj and Sx. The partial derivatives of this potential with respect to these variables yield the quantities ,E, and Tx, respectively. [Pg.57]

Example 3.1 (Elastic material under small strain condition). Under small strain theory the variables of internal energy u in the course of mechanical and thermal fields are the strain and the entropy s which are extensive variables thus the increment of internal energy density du(e, s) can be written as... [Pg.102]

As understood from (3.107), the internal energy density u of an elastic material is a function of the strain if no temperature change is involved. In this case ( ) is the strain energy, and we have... [Pg.103]

In a closed system if the kinetic energy density k defined by (3.19)2 and the internal energy density u are used, the inequality (D.71) is reduced to... [Pg.338]

To investigate the thermo-mechanical interactions, the laws of thermodynamics are applied. The first law of thermodynamics can be considered as a balance equation with the internal energy density m and the heat fluxes q and r due to close-range and long-range effects, respectively. Considering the direct energy production density f one can obtain... [Pg.75]

From the internal energy density uix) and entropy density s(x), we obtain the local variables of (du/ds)yjj = T(x), -(duldV)s j = P, and (ds/dNi )u = -tx x)IT x). The densities in Eqs. (3.1) and (3.2) are dependent on the locally well-defined temperature. In a nonequilibrium system, therefore, the total entropy S is generally not a function of the total entropy U and the total volume V. Also, the classical thermodynamic equations such as the Gibbs and the Gibbs-Duhem equations... [Pg.98]


See other pages where Internal energy density is mentioned: [Pg.722]    [Pg.86]    [Pg.222]    [Pg.165]    [Pg.14]    [Pg.224]    [Pg.98]    [Pg.384]    [Pg.68]    [Pg.34]    [Pg.452]    [Pg.34]    [Pg.496]    [Pg.722]    [Pg.236]    [Pg.161]    [Pg.273]    [Pg.58]    [Pg.296]    [Pg.340]    [Pg.57]   
See also in sourсe #XX -- [ Pg.165 ]




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