- #1
Mark Springer
- 1
- 0
I just read a book by nuclear physicist Carlo Rovelli on the subject of "Time" and he says that 'entropy' is the only non-reversible process in the basic equations of physics, and he believes time and entropy are related (if I understand him correctly). So this started me thinking on entropy:
1. Suppose you have a finite universe that is filled uniformly with Hydrogen atoms. Does this universe have less entropy than a universe that is half empty and the other half filled with the same quantity of Hydrogen atoms?
2. If gravity pulls those atoms together into a star so that they fuse into many different types of atoms (such as Oxygen, Uranium, Silicon etc), then is there more entropy now, or less? Normally, I would think that having a variety of atoms (from which you can build planets, and even life itself, would be a state of less entropy, but that's just intuitive, and must be wrong.
4. Thermal energy is supposed to be the most entropic type of energy. The amount of energy in the universe is conserved. Mass can be converted into energy. Is Mass a low-entropy form of energy? Is kinetic energy a form of energy that has more entropy than 'potential energy'?
5. Carlo Rovelli also says that often the universe contains objects that are stable for a long time. I know this is true of chemical reactions, because sometimes you need a catalyst to make chemicals react, but I think he is talking of objects with entropy and energy that also don't change for a long time - he uses the phrase 'locked in'. Does the universe progress over time to have more such 'locked-in' objects? For example, a universe that started with just Hydrogen atoms would, over time, end up with many other types of atoms that could not easily be broken back down into Hydrogen atoms. Is so, does this increasing 'locked in' direction correlate with time and entropy?
6. An atom bomb can convert mass into energy, but how is energy converted into mass?
7. At the end of the lifespan of the universe, will atoms such as Oxygen and Carbon exist?
That is enough for now. Thanks
1. Suppose you have a finite universe that is filled uniformly with Hydrogen atoms. Does this universe have less entropy than a universe that is half empty and the other half filled with the same quantity of Hydrogen atoms?
2. If gravity pulls those atoms together into a star so that they fuse into many different types of atoms (such as Oxygen, Uranium, Silicon etc), then is there more entropy now, or less? Normally, I would think that having a variety of atoms (from which you can build planets, and even life itself, would be a state of less entropy, but that's just intuitive, and must be wrong.
4. Thermal energy is supposed to be the most entropic type of energy. The amount of energy in the universe is conserved. Mass can be converted into energy. Is Mass a low-entropy form of energy? Is kinetic energy a form of energy that has more entropy than 'potential energy'?
5. Carlo Rovelli also says that often the universe contains objects that are stable for a long time. I know this is true of chemical reactions, because sometimes you need a catalyst to make chemicals react, but I think he is talking of objects with entropy and energy that also don't change for a long time - he uses the phrase 'locked in'. Does the universe progress over time to have more such 'locked-in' objects? For example, a universe that started with just Hydrogen atoms would, over time, end up with many other types of atoms that could not easily be broken back down into Hydrogen atoms. Is so, does this increasing 'locked in' direction correlate with time and entropy?
6. An atom bomb can convert mass into energy, but how is energy converted into mass?
7. At the end of the lifespan of the universe, will atoms such as Oxygen and Carbon exist?
That is enough for now. Thanks