kurious
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How can gravity overcome the degeneracy pressure of neutrons in a neutron star? Isn't such a thing the same as violating the uncertainty principle?
I'm not sure anyone has done the calculations to see if there's another plateau of stability below 'quark degeneracy'. Even if they have, my guess would be we'd be into a region where the Standard Model isn't a reliable guide any more ... it's in an energy (etc) regime that's not well explored in Earthly accelerators (or not explored at all), and 'beyond the SM' physics has essentially no observational basis today.kurious said:Presumably if the quarks don't hold out then they have structure and form
smaller particles or the quarks form heavier quarks pentaquarks etc?
The photo on that link is great.