Benm
0
- Joined
- Aug 16, 2007
- Messages
- 7,896
- Points
- 113
Time is crucial indeed, such spontaneously formed pairs cannot live longer than a plank time, so any process seperating them must act faster than that.
As for radiation emitted from black holes: It's pretty much (like) thermal radiation, and the apparent temperature decreases with the black holes mass. If its heavy enough such that the the apparent temperature is below cosmological background (3 kelvins), the black hole gains mass from cosmological background falling in faster than it loses it from hawking radiation going out.
I'm not sure on what the exact figure is, but its in the order of the mass of the moon. To get an idea on that: such a black hole would be as heavy as the moon, yet much less than 1 mm in schwarszchild radius. If there was one on earth, it would easily gobble up the solar system
As for radiation emitted from black holes: It's pretty much (like) thermal radiation, and the apparent temperature decreases with the black holes mass. If its heavy enough such that the the apparent temperature is below cosmological background (3 kelvins), the black hole gains mass from cosmological background falling in faster than it loses it from hawking radiation going out.
I'm not sure on what the exact figure is, but its in the order of the mass of the moon. To get an idea on that: such a black hole would be as heavy as the moon, yet much less than 1 mm in schwarszchild radius. If there was one on earth, it would easily gobble up the solar system