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Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law

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Page 1: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law

Phys 160 Thermodynamics and Statistical

Physics

Lecture 3

Heat, Work and the First Law

Page 2: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law

• Simple! Temperature is what you measure with a thermometer!

• Temperature is the thing that is the

same for two objects after they have been in contact long enough.

• Temperature is a measure of the ten- dency of an object to absorb or lose energy spontaneously- energy going from a body at a higher temperature to a body at a lower temperature.

Page 3: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law

• The condition for thermal equilibrium between several assemblies is the equality of a certain single-valued function of the thermodynamic states of the assemblies, which may be called the temperature t

• Zeroeth law of thermodynamics

Page 4: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law
Page 5: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law

• We have a wonderful result from this model: The average translati-onal KE of the molecules in a gas is given by a constant time the temperature.

• The temperature of a gas is a direct measure of the average KE of gas molecules. .

Page 6: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law
Page 7: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law

Boltzmann's kinetic theory of gases seemed to presuppose the reality of atoms and molecules, but almost all German philosophers and many scientists like Ernst Mach and the physical chemist Wilhelm Ostwald opposed their existence.

Page 8: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law

Much of the physics establishment did not share his belief in the reality of atoms and molecules — a belief shared, however, by Maxwell in Scotland and Gibbs in the United States; and by most chemists since the discoveries of John Dalton in 1808. He had a long-running dispute with the editor of the preeminent German physics journal of his day, who refused to let Boltzmann refer to atoms and molecules as anything other than convenient

Page 9: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law

theoretical constructs. Only a couple of years after Boltzmann's death, Perrin's studies of colloidal suspensions (1908–1909), based on Einstein's theoretical studies of 1905, confirmed the values of Avogadro's number and Boltzmann's constant, and convinced the world that the tiny particles really exist.

Page 10: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law

To quote Planck, "The logarithmic connection between entropy and probability was first stated by L. Boltzmann in his kinetic theory of gases". This famous formula for entropy S is where k = 1.3806505(24) × 10−23 J K−1 is Boltzmann's constant, and the logarithm is taken to the natural base e.

Page 11: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law

On September 5, 1906, while on a summer vacation in Duino, near Trieste, Boltzmann hanged himself during an attack of depression.

Page 12: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law

Boltzmann was also one of the founders of quantum mechanics due to his suggestion in 1877 that the energy levels of a physical system could be discrete. The equation for S is engraved on Boltzmann's tombstone at the Vienna Zentralfriedhof — his second grave.

Page 13: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law
Page 14: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law
Page 15: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law

Uranium hexafluoride is a chemical compound consisting of one atom of uranium combined with six atoms of fluorine. It is the chemical form of uranium that is used during the uranium enrichment process. Within a reasonable range of temperature and pressure, it can be a solid, liquid, or gas.

Page 16: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law
Page 17: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law
Page 18: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law
Page 19: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law
Page 20: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law
Page 21: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law
Page 22: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law
Page 23: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law
Page 24: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law
Page 25: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law
Page 26: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law
Page 27: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law
Page 28: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law
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Page 35: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law
Page 36: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law
Page 37: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law
Page 38: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law
Page 39: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law

Heat and Work Much of thermodynamics deals with three closely -related concepts; temperature, energy, and heat.

• Temperature, fundamentally, is a measure of an object's tendency to spontaneously give up energy. • Energy is the most fundamental

dynamical concept in all of physics

Page 40: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law

• For this reason, how to express energy in terms of anything more fundamental?

• We can only state what we know definitely. The law of conservation of energy.

• There are many ways to put energy into a system or taken out.

Page 41: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law

• In Thermodynamics, we classify these mechanisms as Heat and Work

• Heat is defined as spontaneous flow of energy from one object to another due to difference in temperature. • Work is defined as any other

transfer of energy into or out of a system.

Page 42: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law

• Usually with work an agent is involved in putting in energy; it is not spontaneous

• Both heat and work refers to energy in transit; there is no heat or work in a system. Heat enters a system; work is done on a system. .

Page 43: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law

• Define symbols: • U for the total energy inside a

system.

• Q and W represent the energy that enters and leave the system as heat and work. Q + W is the total energy that enters the system

• By the conservation law, • U = Q + W . U is the change in energy.

Page 44: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law
Page 45: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law

• Can we say similarly change in Q and W? Q and W are infinitesimal quantities.

• This statement U = Q + W is what is know as the first law of thermodynamics

• The SI unit for energy is the Joule kg.m2/s2. Traditional unit is calorie. 1 cal = 4.186 J.

Page 46: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law

• Three modes of heat transfer. • Conduction, convection and

radiation

• Conduction by molecular contact, convection by bulk motion of gas or liquid, radiation by the emission of EM waves, mostly IR at room temperature, and visible light at highr temperature.

Page 47: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law

• Estimate how long it would take to bring a cup of water (200g) in a micro-wave oven of 600W capacity to boil. Make any reasonable assumptions necessary. How much heat is involved in this process?

• Let us say the initial temperature is 200C. The final temperature is

• 1000C

Page 48: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law

• The total energy needed is • m.c. T =200g.80deg. 1cal/g. • = 16000cal =16000cal*4.186J/cal • = 66976J = 67000J

• 600W = 600J/s; • hence the time needed to raise the

temperature is 67000J/(600J/s) • = 110s.

• No heat but electromagnetic work!

Page 49: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law
Page 50: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law
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• Compression Work –important type of work done on a system (gas)

• W = F. dr = F x =P.A. x (volume change should be very slow-quasistatic)

Page 55: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law

• What happens if the pressure changes significantly?

.

Page 56: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law
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Page 59: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law
Page 60: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law

• Simple! Temperature is what you measure with a thermometer!

• Temperature is the thing that is the

same for two objects after they have been in contact long enough.

• Temperature is a measure of the ten- dency of an object to absorb or lose energy spontaneously- energy going from a body at a higher temperature to a body at a lower temperature.

Page 61: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law
Page 62: Phys 160 Thermodynamics and Statistical Physics - sjsu.edu · Phys 160 Thermodynamics and Statistical Physics Lecture 3 Heat, Work and the First Law