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Modern Engineering Thermodynamics

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102 CHAPTER 4: The First Law of <strong>Thermodynamics</strong> and Energy Transport Mechanisms<br />

or<br />

The energy rate balance is<br />

or<br />

E G = E T (4.1)<br />

_E G = _E T + _E P ðas required by the first lawÞ<br />

_E G = _E T (4.2)<br />

From now on, we frequently use the phrases energy balance and energy rate balance in identifying the proper<br />

equation to use in an analysis. So, for simplicity, we introduce the following abbreviations:<br />

and<br />

EB = energy balance<br />

ERB = energy rate balance<br />

In Chapter 3, we introduce the components of the total system energy E as the internal energy U, the kinetic<br />

energy mV 2 /2g c , and the potential energy mgZ/g c ,or 3<br />

E = U + mV 2<br />

2g c<br />

+ mgZ<br />

g c<br />

(3.9)<br />

In this equation, V is the magnitude of the velocity of the center of mass of the entire system, Z is the height of<br />

the center of mass above a ground (or zero) potential datum, and g c is the dimensional proportionality factor<br />

(see Table 1.2 of Chapter 1). In Chapter 3, we also introduce the abbreviated form of this equation:<br />

E = U + KE + PE (3.10)<br />

and similarly for the specific energy e,<br />

and<br />

e = E m = u + V 2<br />

2g c<br />

+ gZ<br />

g c<br />

(3.12)<br />

e = u + ke + pe (3.13)<br />

In these equations, we continue the practice introduced in Chapter 2 of using uppercase letters to denote extensive<br />

properties and lowercase letters to denote intensive (specific) properties. The energy concepts described in these<br />

equations are illustrated in Figure 4.1.<br />

Center of<br />

mass<br />

Velocity V<br />

In equilibrium thermodynamics, the proper energy balance is given by Eq. (4.1),<br />

where the gain in energy E G is to be interpreted as follows. The system is initially<br />

in some equilibrium state (call it state 1), and after the application of some “process,”<br />

the system ends up in a different equilibrium state (call it state 2). If we<br />

now add a subscript to each symbol to denote the state at which the property is<br />

to be evaluated (E 1 is the total energy of the system in state 1 and so forth), then<br />

we can write the energy gain of the system as<br />

Height = Z<br />

Internal<br />

energy<br />

U<br />

FIGURE 4.1<br />

System energy components.<br />

Z = 0<br />

System (either<br />

open or closed)<br />

System boundary<br />

or<br />

E G = Final total energy − Initial total energy (4.3)<br />

E G = E 2 − E 1 (4.4)<br />

and extending this to Eq. (3.9), we obtain<br />

E G = U 2 − U 1 + m<br />

<br />

ðV2 2 2g − V2 1 Þ + mg <br />

c<br />

g<br />

ðZ 2 − Z 1 Þ (4.5)<br />

c<br />

or<br />

<br />

E G = m u 2 − u 1 + V 2 2 − V2 1<br />

+ g <br />

2g c<br />

g<br />

ðZ 2 − Z 1 Þ<br />

(4.6)<br />

c<br />

3 In this text, we use the symbol V to represent the magnitude of the average velocity |V|, and the symbol V to represent volume.

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