Equations of State

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Equations of State Physics 313 Professor Lee Carkner Lecture 4

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Equations of State. Physics 313 Professor Lee Carkner Lecture 4. Exercise #2 Radiation. Size of Alberio stars Find T for each from Wien’s law: T = 2.9X10 7 / l max Star A l max = 6900 A, T = Star B: l max = 2200 A, T = Find area from Stefan-Boltzmann law: P = se AT 4 - PowerPoint PPT Presentation

Transcript of Equations of State

Page 1: Equations of State

Equations of State

Physics 313Professor Lee

CarknerLecture 4

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Exercise #2 Radiation Size of Alberio stars Find T for each from Wien’s law: T = 2.9X107/max

Star A max = 6900 A, T = Star B: max = 2200 A, T =

Find area from Stefan-Boltzmann law: P = AT4

A = P / (T4) AA = (3X1029) / [(5.6703X10-8)(1)(4202)4] = AB = (4.7X1028) / (5.6703X10-8)(1)(13182)4 =

Convert area to radius: A = 4r2

r = (A/4)½

rA = [(1.7X1022) / (4)(p)] ½ = rB = [(2.8X1019) / (4)(p)] ½ = 3.68X1010 / 1.48X109 = 25 times larger (red star compared

to blue) Your blackbody radiation (T = 37 C)

Convert to Kelvin, T = 37 +273 = max = 2.9X107/T = P = (5.6703X10-8)(1)(2)(310)4 ~

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Equilibrium

Mechanical

Chemical

Thermal

Thermodynamic

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Non-Equilibrium

System cannot be described in macroscopic coordinates

If process happens quasi-statically, system is approximately in equilibrium for any point during the process

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Equation of State

System with properties X, Y and Z

Equation relating them is equation of state:

Determined empirically

These constants can be looked up in tables Equations only useful over certain conditions

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Ideal Gas

PV = nRT

or, since v = V/n (molar volume):

Remember ideal gas law is more accurate as the pressure gets lower

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Constants In the previous formulation

R = universal gas constant (8.31 J/mol

K) We can rewrite in terms of:

Rs = specific gas constant (R/M)

The ideal gas law is then:Pvs = RsT

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Hydrostatic Systems

X,Y,Z are P,V,T

Many applications Well determined equations of state

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Types of Hydrostatic Systems

Pure substances

Homogeneous mixture

Heterogeneous mixture

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Homogeneous Pure Gas : Equations of State

Pv = RT

(P + a/v2)(v - b) = RT

P = (RT/v2)(1 - c/vT3)(v+B)-(A/v2)

A = A0(1 - a/v) and B = B0(1 - b/v) Note: a, b and c are constants specific to a particular

gas and are determined experimentally (empirical relations) Ideal gas ignores interactions between particles, the other

two approximate interaction effects

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Differentials

For small changes we use the differential notation, e.g. dV, dT, dP

P, V and T have no meaning for small numbers of molecules

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Differential Relations

For a system of three dependant variables:

dz = (z/x)y dx + (z/y)x dy

The total change in z is equal to the change in z due to changes in x plus the change in z due to changes in y

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State Relations in Hydrostatic Systems

How does the volume of a hydrostatic system change when P and T change?

Volume Expansivity:

= (1/V) (V/ T)P

Isothermal Compressibility:

= -(1/V) (V/ P)T

Both are empirically determined tabulated quantities

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Two Differential Theorems

(x/y)z = 1/(y/x)z

(x/y)z(y/z)x = -(x/ z)y

If we know something about how a system changes, we can tabulate it

We can use the above theorems to relate these known quantities to other changes

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Constant Volume Relations

For hydrostatic systems:dP = (P/ T)V dT + (P/ V)T dV

For constant volume:

But, -(P/ T)V = (P/ V)T (V/ T)P, so:

For constant and with T