
Entropy and the second law
PHYS 220 · Second Law and Entropy
Entropy is a state function that quantifies energy dispersal and microscopic multiplicity. This lesson introduces entropy and the second law of thermodynamics.
Key equations
\Delta S_{isolated}\geq 0dS=\frac{\delta Q_{rev}}{T}\Delta S=\int_i^f \frac{\delta Q_{rev}}{T}S=k_B\ln\Omega\Delta S_{universe}=\Delta S_{system}+\Delta S_{surroundings}>0\Delta S_{universe}=0Learning objectives
- State the second law in entropy form.
- Define entropy using reversible heat transfer.
- Explain Boltzmann's statistical interpretation of entropy.
- Compare Clausius and Kelvin-Planck statements of the second law.
- Analyze entropy changes of system plus surroundings.
Direction in thermodynamics
The first law says energy is conserved, but it does not tell us which processes happen naturally. A hot object cools in a cold room, but the reverse process would not violate energy conservation by itself. Energy could, in principle, flow from the cold room into the hot object while total energy remains constant. Yet this does not happen spontaneously.
The second law of thermodynamics addresses direction. It says that for an isolated system, entropy never decreases:
Natural irreversible processes increase total entropy. Ideal reversible processes keep total entropy constant.
What entropy means
Entropy, written , is a thermodynamic state function. It can be introduced macroscopically through heat transfer in a reversible process:
dS=rac{delta Q_{rev}}{T}
For a finite reversible path,
Delta S=int_i^f rac{delta Q_{rev}}{T}
The subscript is important. Entropy change is a state function, so it can be calculated using any convenient reversible path between the same states, even if the actual process is irreversible.
Statistical meaning
In statistical mechanics, entropy is related to the number of microscopic arrangements consistent with a macroscopic state. Boltzmann's formula is
where is Boltzmann's constant and is the number of accessible microstates.
A macrostate with many possible microstates has higher entropy. Natural systems tend to evolve from less probable macrostates to more probable macrostates because there are overwhelmingly more microscopic ways to be in the high-entropy state.
Energy dispersal
Entropy is often associated with energy spreading out or becoming less available to do organized work. When a hot object and cold object reach a common temperature, energy is still conserved, but it is more evenly distributed. The final state has higher total entropy.
This does not mean entropy is simply disorder in a vague sense. Disorder can be a helpful image, but entropy has precise thermodynamic and statistical definitions.
Clausius statement
One statement of the second law is the Clausius statement: heat does not spontaneously flow from a colder body to a hotter body. Refrigerators can move heat from cold to hot, but only by using external work.
This statement explains why heat transfer has a natural direction.
Kelvin-Planck statement
Another statement is the Kelvin-Planck form: no heat engine operating in a cycle can convert all absorbed heat into work with no other effect. Some heat must be rejected to a lower-temperature reservoir.
This sets fundamental limits on engines and power plants.
Entropy of the universe
For any real spontaneous process,
For an ideal reversible process,
The system's entropy can decrease, but only if the surroundings' entropy increases by at least as much. Freezing water lowers the water's entropy, but heat released to the surroundings increases total entropy.
The big idea
The second law explains why energy-conserving processes still have preferred directions. Entropy is a state function connected to reversible heat transfer and to microscopic multiplicity. In isolated systems, entropy never decreases, making entropy one of the deepest concepts in physics.
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