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Thermodynamic Systems Physics 313 Professor Lee Carkner Lecture 5

Thermodynamic Systems Physics 313 Professor Lee Carkner Lecture 5

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Page 1: Thermodynamic Systems Physics 313 Professor Lee Carkner Lecture 5

Thermodynamic Systems

Physics 313Professor Lee

CarknerLecture 5

Page 2: Thermodynamic Systems Physics 313 Professor Lee Carkner Lecture 5

Exercise #3 Equations of State

Ideal gas pressure: P = RT/v = (8.31)(150)/(1.1733) = 1062.39 kPa

Beattie-Bridgeman pressure: P = (RT/v2)(1-(c/vT3))(v+B)-(A/v2) P = [(8.31)(150)/(1.1733)2][1-((4.2X104)/(1.1733)(150)3)]

(1.1733+0.05076)-(133.193/1.17332) = 999.84 kPa

Savings Design A requires 1062.39-999.84 = 62.55 kPa more

Page 3: Thermodynamic Systems Physics 313 Professor Lee Carkner Lecture 5

Temperature Dependence

Can use the equation of state to find dependence

Can use differential theorems to relate

Page 4: Thermodynamic Systems Physics 313 Professor Lee Carkner Lecture 5

Generic Relations

Consider a system with interdependent properties x, y and z:

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

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

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

Can use these along with: Tabulated x,y,z dependencies (expansivity, bulk

modulus etc.)

Page 5: Thermodynamic Systems Physics 313 Professor Lee Carkner Lecture 5

Stretched Wire A wire under tension is a

thermodynamic system that can be described with three variables:

differential changes can be related by:

dL = (L/T) dT + (L/)T d

Page 6: Thermodynamic Systems Physics 313 Professor Lee Carkner Lecture 5

Wire Relations

Linear Expansivity:

= (1/L)(L/T)

Isothermal Young’s Modulus:

Y = (L/A)(/L)T

These are well known for most normal conditions

Page 7: Thermodynamic Systems Physics 313 Professor Lee Carkner Lecture 5

Wires and Sound Vibrating strings can produce notes of a

given frequency

Frequency depends on wave speed and wavelength, which are properties of the string:

is usually fixed

based on string (linear density) is usually fixed

How does the tension change?

Page 8: Thermodynamic Systems Physics 313 Professor Lee Carkner Lecture 5

Surfaces Surfaces (such as films) act like 2-D wires

The surface tension is a force that pulls in the plane of the surface

Surface tension relations often depend on the type of system

e.g. vapor above liquid, oil film on water

Page 9: Thermodynamic Systems Physics 313 Professor Lee Carkner Lecture 5

Boundaries as Surfaces

For surface defined as the boundary between a liquid and its vapor:

= 0[1 - (T/TC)]n

where: •

• n is between 1 and 2

• Higher T means lower tension•

Page 10: Thermodynamic Systems Physics 313 Professor Lee Carkner Lecture 5

Oil on Water

A film of oil on water increases the surface tension:

( - w)A = aT

Sort of a 2-D equation of state

Page 11: Thermodynamic Systems Physics 313 Professor Lee Carkner Lecture 5

Electrochemical Cell

A battery produces emf through chemical reactions

The emf depends on the amount of charge transferred

Batteries can be recharged

Page 12: Thermodynamic Systems Physics 313 Professor Lee Carkner Lecture 5
Page 13: Thermodynamic Systems Physics 313 Professor Lee Carkner Lecture 5

Equation of State We can relate the emf to 2 other variables

The equation of state is: = 20 + (T-20) + (T-20)2 + (T-20)3

Constants depend on materials and chemicals

Page 14: Thermodynamic Systems Physics 313 Professor Lee Carkner Lecture 5

Dielectric Slab Material in an electric field will undergo polarization

(molecules become polar) The total polarization depends on the electric field and

the temperature

Equation of state:P/V = [a + (b/T)]E

Where P/V is the polarization per unit volume

Thermal “forces” compete with electrical

Page 15: Thermodynamic Systems Physics 313 Professor Lee Carkner Lecture 5

Paramagnetic Rod Paramagnetic materials develop magnetization in a

magnetic field

Non-magnetic materials become magnetic

Properties:

Equation of state:M = CH/T

M decreases at higher temperature

This assumes a long thin shape

Page 16: Thermodynamic Systems Physics 313 Professor Lee Carkner Lecture 5

The Eagle Nebula - Interstellar Dust

Page 17: Thermodynamic Systems Physics 313 Professor Lee Carkner Lecture 5

Paramagnetism and Interstellar Dust

Page 18: Thermodynamic Systems Physics 313 Professor Lee Carkner Lecture 5

Intensive Extensive

Independent of mass

Tension emf Magnetic field

Proportional to mass Length Charge Total magnetization

Page 19: Thermodynamic Systems Physics 313 Professor Lee Carkner Lecture 5

Concepts

How do system properties vary with temperature?

What are the differential relations?

How can the differential relations be rewritten?