quote:
Originally posted by incubus:
Thats called the Chandresekar limit
That it is...
quote:
Originally posted by LazyGit:
Yeah, but in real world (space) conditions the star would really need to be over 5 times stellar mass to have a chance of turning into a black hole.Sub atomic stuff is so annoying that you might aswell see a proton as a neutron and an electron together anyway, it saves time.
Depends on the conditions in which the star dies. I'm not an astrophysicist, but 1.7-3 solar masses for an upper limit for the formation of neutron stars is a large range, so I wouldn't be suprised if larger stars did form neutron stars instead of black holes, but I don't think you'd need >5 solar masses to have any chance, just >2 would be enough.
Or a neutron as a proton plus an electron maybe? Just because something decays into something else, doesn't mean that it is composed of soley of the decay products. In order for it to decay, it must be energetically favourable. This means that energy is 'lost' in the transformation, so you can't say that a neutron is a proton plus an electron.
edit: UBB greebles
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"Make things as simple as possible, but no simpler" - Einstein
This message has been edited by masher on February 26, 2001 at 03:30 AM