This might not be what you are interested in, but log probabilities in statistical physics are closely related to the concepts of energy and entropy. For a physical system in equilibrium at temperature $T$ (in kelvin), the difference in energy between two microstates A and B is related to the logarithm of the probabilities that the system is in state A or state B:
$$E_\mathrm{A} - E_\mathrm{B} =-k_\mathrm{B}T \left[ \ln(P_\mathrm{A}) - \ln( P_\mathrm{B}) \right]$$
So, statistical physicists often work with log probabilities (or scaled versions of them), because they are physically meaningful. For example, the potential energy of a gas molecule in an atmosphere at a fixed temperature under a uniform gravitation field (a good approximation near the surface of the Earth) is $mgh$, where $m$ is the mass of the gas molecule, $g$ is the acceleration of gravity, and $h$ is the height of the molecule above the surface. The probability of finding a gas molecule in the top floor of the building versus in the bottom floor (assuming the floors have the same volume and the floor-to-ceiling height is small) is given by:
$$mg (h_\mathrm{top} - h_\mathrm{bottom}) \approx -k_\mathrm{B} T \left[ \ln (P_\mathrm{top}) - \ln(P_\mathrm{bottom}) \right]$$
This probability is trivially related to the concentration of the gas on the two floors. Higher floors have a lower concentration and the concentration of heavier molecules decays more quickly with height.
In statistical physics, it is often useful to switch back and forth between quantities proportional to log probabilities (energy, entropy, enthalpy, free energy) and quantities proportional to probability (number of microstates, partition function, density of states).