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By:
B.Christopaul
EU/PGS/2012/MSCED/12
Faculty Of Science
EUSL
Teaching Classical Physics
MSED 2558
Thermodynamics in Physics
MSED 2558
Temperature and Heat
• Everyone has a qualitative understanding of temperature, but it is not
very exact.
• Question: Why can you put your hand in a 400 F oven and not get
instantly burned, but if you touch the metal rack, you do?
• Answer: Even though the air and the rack are at the same
temperature, they have very different energy contents.
Units of Heat
• J - Joules
• Cal - calorie
• Btu - British Thermal Unit
• Conversions:
1 cal =4.186 J
1Btu = 252 cal
Thermodynamics
Contributions made by:
• Benjamin Thompson (1753-1814) - (Count Rumford)
• Sadi Carnot (1796-1832)
• James Joule (1818-1889)
• Rudolf Clausius (1822-1888)
• William Thompson (1824-1907) - (Lord Kelvin)
• Robert Boyle (1627-1691)
• Charles (1746-1823)
• Gay-Lussac (1778-1823)
• Amedeo Avogadro (1776-1856)
• Daniel Bernoulli (1700-1782)
• John Dalton (1766-1844)
• Ludwig Boltzmann (1844-1906)
• J. Willard Gibbs (1939-1903)
• James Clerk Maxwell (1831-1879)
5
Construction of a Temperature Scale
• Absolute or Kelvin Scale
•K=C+273
 32
9
5
C
CelsiuswantandFahrenheitknowweIf
32
5
9
FahrenheitwantandCelsiusknowweIf


F
CF
Expansion
Gas Laws
Heat Transfer Mechanisms
1. Conduction: (solids--mostly) Heat transfer without mass transfer.
2. Convection: (liquids/gas) Heat transfer with mass transfer.
3. Radiation: Takes place even in a vacuum.
Conduction
 Thickness
Difference
eTemperatur
Area
Contact
tyConductivi
Thermal
Heat Flow
ofRate 























Convection
• Typically very complicated.
• Very efficient way to transfer energy.
• Vortex formation is very common feature.
Radiation
• Everything that has a temperature radiates energy.
• Method that energy from sun reaches the earth
44
)( TconsteAT
t
Q
P  
Specific Heat
• Observational Fact: It is easy to change the temperature of some things (e.g. air)
and hard to change the temperature of others (e.g. water)
• The amount of heat (Q) added into a body of mass m to change its temperature
an amount T is given by
Q=m C T
• C is called the specific heat and depends on the material and the units
used.
• Note: since we are looking at changes in temperature, either Kelvin or
Celsius will do.
Heat Capacity of Ideal Gas
• CV = heat capacity at constant volume
CV = 3/2 R
• CP = heat capacity at constant pressure
CP = 5/2 R
• For constant volume
Q = nCVΔT = ΔU
• The universal gas constant R = 8.314 J/mol·K
Work Done by a Gas
• Work=(Force)x(distance)
=Fy
• Force=(Presssure)x(Area)
• W=P(Ay)
=PV
The Laws of Thermodynamics
• First law: The change in the internal energy ΔU of a system is equal to the heat Q
added to a system plus the work W done by the system
ΔU = Q + W
• Secondlaw: It is not possible to convert heat completely into work without some
other change taking place.
• The “zeroth” law: Two systems in thermal equilibrium with a third system are in
thermal equilibrium with each other.
• Third law: It is not possible to achieve an absolute zero temperature
16
First law
Isothermal Process
• An isothermal process is a constant temperature process. Any heat
flow into or out of the system must be slow enough to maintain
thermal equilibrium
• For ideal gases, if ΔT is zero, ΔU = 0
• Therefore, Q = W
• Any energy entering the system (Q)
• must leave as work (W)
First law
Isobaric Process
• An isobaric process is a constant pressure process. ΔU, W, and Q are
generally non-zero, but calculating the work done by an ideal gas is
straightforward
W = P·ΔV
• Water boiling in a saucepan is an example of an isobar process
First law
Isochoric Process
• An isochoric process is a constant volume process. When the volume
of a system doesn’t change, it will do no work on its surroundings. W
= 0
ΔU = Q
• Heating gas in a closed container is an isochoric process
Primary Results
• Internal energy U directly related to the average molecular kinetic energy
• Average molecular kinetic energy directly related to absolute temperature
• Internal energy equally distributed among the number of degrees of
freedom (f) of the system
(NA = Avogadro’s Number)
20
Other Primary Results
2. Maxwell derives a relation for the molecular speed distribution f (v):
3. Boltzmann contributes to determine the root-mean-square of the
molecular speed
Thus relating energy to the temperature for an ideal gas
21
black body radiation
Simulation

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Theromo physics

  • 3. Temperature and Heat • Everyone has a qualitative understanding of temperature, but it is not very exact. • Question: Why can you put your hand in a 400 F oven and not get instantly burned, but if you touch the metal rack, you do? • Answer: Even though the air and the rack are at the same temperature, they have very different energy contents.
  • 4. Units of Heat • J - Joules • Cal - calorie • Btu - British Thermal Unit • Conversions: 1 cal =4.186 J 1Btu = 252 cal
  • 5. Thermodynamics Contributions made by: • Benjamin Thompson (1753-1814) - (Count Rumford) • Sadi Carnot (1796-1832) • James Joule (1818-1889) • Rudolf Clausius (1822-1888) • William Thompson (1824-1907) - (Lord Kelvin) • Robert Boyle (1627-1691) • Charles (1746-1823) • Gay-Lussac (1778-1823) • Amedeo Avogadro (1776-1856) • Daniel Bernoulli (1700-1782) • John Dalton (1766-1844) • Ludwig Boltzmann (1844-1906) • J. Willard Gibbs (1939-1903) • James Clerk Maxwell (1831-1879) 5
  • 6. Construction of a Temperature Scale • Absolute or Kelvin Scale •K=C+273  32 9 5 C CelsiuswantandFahrenheitknowweIf 32 5 9 FahrenheitwantandCelsiusknowweIf   F CF
  • 9. Heat Transfer Mechanisms 1. Conduction: (solids--mostly) Heat transfer without mass transfer. 2. Convection: (liquids/gas) Heat transfer with mass transfer. 3. Radiation: Takes place even in a vacuum.
  • 10. Conduction  Thickness Difference eTemperatur Area Contact tyConductivi Thermal Heat Flow ofRate                        
  • 11. Convection • Typically very complicated. • Very efficient way to transfer energy. • Vortex formation is very common feature.
  • 12. Radiation • Everything that has a temperature radiates energy. • Method that energy from sun reaches the earth 44 )( TconsteAT t Q P  
  • 13. Specific Heat • Observational Fact: It is easy to change the temperature of some things (e.g. air) and hard to change the temperature of others (e.g. water) • The amount of heat (Q) added into a body of mass m to change its temperature an amount T is given by Q=m C T • C is called the specific heat and depends on the material and the units used. • Note: since we are looking at changes in temperature, either Kelvin or Celsius will do.
  • 14. Heat Capacity of Ideal Gas • CV = heat capacity at constant volume CV = 3/2 R • CP = heat capacity at constant pressure CP = 5/2 R • For constant volume Q = nCVΔT = ΔU • The universal gas constant R = 8.314 J/mol·K
  • 15. Work Done by a Gas • Work=(Force)x(distance) =Fy • Force=(Presssure)x(Area) • W=P(Ay) =PV
  • 16. The Laws of Thermodynamics • First law: The change in the internal energy ΔU of a system is equal to the heat Q added to a system plus the work W done by the system ΔU = Q + W • Secondlaw: It is not possible to convert heat completely into work without some other change taking place. • The “zeroth” law: Two systems in thermal equilibrium with a third system are in thermal equilibrium with each other. • Third law: It is not possible to achieve an absolute zero temperature 16
  • 17. First law Isothermal Process • An isothermal process is a constant temperature process. Any heat flow into or out of the system must be slow enough to maintain thermal equilibrium • For ideal gases, if ΔT is zero, ΔU = 0 • Therefore, Q = W • Any energy entering the system (Q) • must leave as work (W)
  • 18. First law Isobaric Process • An isobaric process is a constant pressure process. ΔU, W, and Q are generally non-zero, but calculating the work done by an ideal gas is straightforward W = P·ΔV • Water boiling in a saucepan is an example of an isobar process
  • 19. First law Isochoric Process • An isochoric process is a constant volume process. When the volume of a system doesn’t change, it will do no work on its surroundings. W = 0 ΔU = Q • Heating gas in a closed container is an isochoric process
  • 20. Primary Results • Internal energy U directly related to the average molecular kinetic energy • Average molecular kinetic energy directly related to absolute temperature • Internal energy equally distributed among the number of degrees of freedom (f) of the system (NA = Avogadro’s Number) 20
  • 21. Other Primary Results 2. Maxwell derives a relation for the molecular speed distribution f (v): 3. Boltzmann contributes to determine the root-mean-square of the molecular speed Thus relating energy to the temperature for an ideal gas 21