kurious
- 633
- 0
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 explores the relationship between dark energy and neutron stars, specifically whether dark energy could prevent neutron stars from collapsing into black holes. It includes theoretical considerations, speculative models, and the implications of quantum mechanics in extreme environments.
Participants express various hypotheses regarding the role of dark energy and the behavior of quarks under extreme conditions, but no consensus is reached on any particular model or explanation.
There are limitations regarding the assumptions made about the behavior of quarks and dark energy, as well as the applicability of the Standard Model in extreme conditions. The discussion also highlights the lack of experimental data in relevant energy regimes.
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.