As a classical object with zero temperature it was assumed that black holes had zero entropy.

Another difference between the low inclination (cold) and high inclination (hot) classical objects is the observed number of binary asteroid.

Now one can ask where the boundary lies between objects with quantum properties and classical objects.

He was known to use a lot of classical objects in fresh similes.

In fact, though, associated ruled surfaces were classical objects.

But to be fair, Bohr correspondence was true for every single classical object known up until this one.

These definitions lack precision: in particular the boundary between the classical objects and the scattered disk remains blurred.

There is a sense in which classical objects are like the constraints on the release of energy that permits work to be done.

Kig can handle any classical object of the dynamic geometry, but also:

The paradox is whether a classical object like a cat can behave like a quantum particle.