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?
The discussion centers on the potential role of dark energy in preventing neutron stars from collapsing into black holes. It posits that while gravity typically overcomes neutron degeneracy pressure, quark degeneracy pressure may provide additional resistance to collapse, potentially leading to the formation of quark stars. The conversation also explores the implications of dark energy, suggesting that if it behaves like particles trapped between neutrons, it could exert a repulsive force that counters gravity, thus preventing singularities during black hole formation.
PREREQUISITESAstronomers, astrophysicists, and students of theoretical physics interested in the dynamics of neutron stars, black hole formation, and the role of dark energy in cosmic phenomena.
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.