A resolution of the Gibbs paradox gives rise to a formula for this quantity in a mono-atomic ideal gas, the Sackur-Tetrode equation.
For black holes, this quantity is proportional to the event horizon's surface area. A resolution of the Gibbs paradox gives rise to a formula for this quantity in a mono-atomic ideal gas, the Sackur-Tetrode equation. It is equal to Boltzmann's constant times natural log of the number of microstates. This quantity approaches a minimum value at absolute zero, according to the third law of thermodynamics, and always increases up to a maximum value at equilibrium, according to the second law. For 10 points, name this measure of disorder in a system.
For black holes, this quantity is proportional to the event horizon's surface area.
{entropy} [do not accept "{enthalphy}"]