JCTthatsME
- 6
- 0
I have been studying self-gravitating systems and their unusual property of negative heat capacity. This makes me wonder how far such a thermodynamic description can be extended.
Does the concept of self-gravitation apply only to bound stellar systems, or could it also be applicable at the galactic scale?
In particular, is there any relation (or contrast) between this thermodynamic perspective and the MOND approach to flat galactic rotation curves?
Could it be said that the 'reach' of a self-gravitating system naturally ends where MOND-type effects begin?
Does the concept of self-gravitation apply only to bound stellar systems, or could it also be applicable at the galactic scale?
In particular, is there any relation (or contrast) between this thermodynamic perspective and the MOND approach to flat galactic rotation curves?
Could it be said that the 'reach' of a self-gravitating system naturally ends where MOND-type effects begin?