- #1
DarkStar42
- 20
- 0
So when a star collapses, if the event horizon doesn't form, but the object remains in ordinary space, in increasing gravitational time-dilated collapse, what problems with these objects would be solved or more easily addressed?
I would think at least the information loss problem, and then there is the conservation of rotational momentum, and then there is the production of the magnetic field.
I would think at least the information loss problem, and then there is the conservation of rotational momentum, and then there is the production of the magnetic field.