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 12.1 Heat and Temperature 12.2 The Kinetic Theory of Gases & the Ideal Gas Law 12.3 The Laws of Thermodynamics 12.4 Heat Engines

 12.5 Key Formulas 12.6 Practice Questions 12.7 Explanations
The Laws of Thermodynamics
Dynamics is the study of why things move the way they do. For instance, in the chapter on dynamics, we looked at Newton’s Laws to explain what compels bodies to accelerate, and how. The prefix thermo denotes heat, so thermodynamics is the study of what compels heat to move in the way that it does. The Laws of Thermodynamics give us the whats and whys of heat flow.
The laws of thermodynamics are a bit strange. There are four of them, but they are ordered zero to three, and not one to four. They weren’t discovered in the order in which they’re numbered, and some—particularly the Second Law—have many different formulations, which seem to have nothing to do with one another.
There will almost certainly be a question on the Second Law on SAT II Physics, and quite possibly something on the First Law. The Zeroth Law and Third Law are unlikely to come up, but we include them here for the sake of completion. Questions on the Laws of Thermodynamics will probably be qualitative: as long as you understand what these laws mean, you probably won’t have to do any calculating.
Zeroth Law
If system A is at thermal equilibrium with system B, and B is at thermal equilibrium with system C, then A is at thermal equilibrium with C. This is more a matter of logic than of physics. Two systems are at thermal equilibrium if they have the same temperature. If A and B have the same temperature, and B and C have the same temperature, then A and C have the same temperature.
The significant consequence of the Zeroth Law is that, when a hotter object and a colder object are placed in contact with one another, heat will flow from the hotter object to the colder object until they are in thermal equilibrium.
First Law
Consider an isolated system—that is, one where heat and energy neither enter nor leave the system. Such a system is doing no work, but we associate with it a certain internal energy, U, which is related to the kinetic energy of the molecules in the system, and therefore to the system’s temperature. Internal energy is similar to potential energy in that it is a property of a system that is doing no work, but has the potential to do work.
The First Law tells us that the internal energy of a system increases if heat is added to the system or if work is done on the system and decreases if the system gives off heat or does work. We can express this law as an equation:
where U signifies internal energy, Q signifies heat, and W signifies work.
The First Law is just another way of stating the law of conservation of energy. Both heat and work are forms of energy, so any heat or work that goes into or out of a system must affect the internal energy of that system.
Example
 Some heat is added to a gas container that is topped by a movable piston. The piston is weighed down with a 2 kg mass. The piston rises a distance of 0.2 m at a constant velocity. Throughout this process, the temperature of the gas in the container remains constant. How much heat was added to the container?
The key to answering this question is to note that the temperature of the container remains constant. That means that the internal energy of the system remains constant (), which means that, according to the First Law, . By pushing the piston upward, the system does a certain amount of work, , and this work must be equal to the amount of heat added to the system, .
The amount of work done by the system on the piston is the product of the force exerted on the piston and the distance the piston is moved. Since the piston moves at a constant velocity, we know that the net force acting on the piston is zero, and so the force the expanding gas exerts to push the piston upward must be equal and opposite to the force of gravity pushing the piston downward. If the piston is weighed down by a two-kilogram mass, we know that the force of gravity is:
Since the gas exerts a force that is equal and opposite to the force of gravity, we know that it exerts a force of 19.6 N upward. The piston travels a distance of 0.2 m, so the total work done on the piston is:
Since in the equation for the First Law of Thermodynamics is positive when work is done on the system and negative when work is done by the system, the value of is –3.92 J. Because , we can conclude that J, so 3.92 J of heat must have been added to the system to make the piston rise as it did.
Second Law
There are a number of equivalent forms of the Second Law, each of which sounds quite different from the others. Questions about the Second Law on SAT II Physics will invariably be qualitative. They will usually ask that you identify a certain formulation of the Second Law as an expression of the Second Law.
The Second Law in Terms of Heat Flow
Perhaps the most intuitive formulation of the Second Law is that heat flows spontaneously from a hotter object to a colder one, but not in the opposite direction. If you leave a hot dinner on a table at room temperature, it will slowly cool down, and if you leave a bowl of ice cream on a table at room temperature, it will warm up and melt. You may have noticed that hot dinners do not spontaneously get hotter and ice cream does not spontaneously get colder when we leave them out.
The Second Law in Terms of Heat Engines
One consequence of this law, which we will explore a bit more in the section on heat engines, is that no machine can work at 100% efficiency: all machines generate some heat, and some of that heat is always lost to the machine’s surroundings.
The Second Law in Terms of Entropy
The Second Law is most famous for its formulation in terms of entropy. The word entropy was coined in the 19th century as a technical term for talking about disorder. The same principle that tells us that heat spontaneously flows from hot to cold but not in the opposite direction also tells us that, in general, ordered systems are liable to fall into disorder, but disordered systems are not liable to order themselves spontaneously.
Imagine pouring a tablespoon of salt and then a tablespoon of pepper into a jar. At first, there will be two separate heaps: one of salt and one of pepper. But if you shake up the mixture, the grains of salt and pepper will mix together. No amount of shaking will then help you separate the mixture of grains back into two distinct heaps. The two separate heaps of salt and pepper constitute a more ordered system than the mixture of the two.
Next, suppose you drop the jar on the floor. The glass will break and the grains of salt and pepper will scatter across the floor. You can wait patiently, but you’ll find that, while the glass could shatter and the grains could scatter, no action as simple as dropping a jar will get the glass to fuse back together again or the salt and pepper to gather themselves up. Your system of salt and pepper in the jar is more ordered than the system of shattered glass and scattered condiments.
Entropy and Time
You may have noticed that Newton’s Laws and the laws of kinematics are time-invariant. That is, if you were to play a videotape of kinematic motion in reverse, it would still obey the laws of kinematics. Videotape a ball flying up in the air and watch it drop. Then play the tape backward: it goes up in the air and drops in just the same way.
By contrast, you’ll notice that the Second Law is not time-invariant: it tells us that, over time, the universe tends toward greater disorder. Physicists suggest that the Second Law is what gives time a direction. If all we had were Newton’s Laws, then there would be no difference between time going forward and time going backward. So we were a bit inaccurate when we said that entropy increases over time. We would be more accurate to say that time moves in the direction of entropy increase.
Third Law
It is impossible to cool a substance to absolute zero. This law is irrelevant as far as SAT II Physics is concerned, but we have included it for the sake of completeness.
 Jump to a New ChapterIntroduction to the SAT IIIntroduction to SAT II PhysicsStrategies for Taking SAT II PhysicsVectorsKinematicsDynamicsWork, Energy, and PowerSpecial Problems in MechanicsLinear MomentumRotational MotionCircular Motion and GravitationThermal PhysicsElectric Forces, Fields, and PotentialDC CircuitsMagnetismElectromagnetic InductionWavesOpticsModern PhysicsPhysics GlossaryPractice Tests Are Your Best Friends
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