quote:
Free neutrons undergo beta decay with a mean lifetime of about 10 minutes
Serway, R.A., 1996, Physics for Scientists and Engineers: with Modern Physics 4th Ed., Saunders College Publishing, Philadelphia, p. 1382.The key word here is 'free'. That is, a neutron all by itself. After about 10 mins, it will spit out an electron and transform into a proton.
.
quote:
The density of a neutron start is about 1.2x10^14 gcm^-3 ... slightly less than the density of a neutron, which is about 4x10^14 gcm^-3 ... we can conclude that the gravitational pressure of the neutron star is balanced by the repulsive component, due to the exclusion principle, of the strong nuclear force between the neutrons.
Tipler, P.A, 1992, Elementary Modern Physics, Worth Publishers, New York, pp. 314-315.
Also, a neutron star with the mass of our sun will have a radius of 12.7 km. As the mass increases, the radius decreases, until you get a black hole. About 1.7 - 3 solar masses is the limit for neutron stars. After this you get black holes.
------------------
"Make things as simple as possible, but no simpler" - Einstein