Mustang11
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Hi all. I am curious as to why quark stars have not dominated by now, given their inability to decay as they are a mass of fundamental particles. What prevents this?
The discussion centers around the existence and characteristics of quark stars, exploring why they are not prevalent in the universe. Participants examine theoretical motivations, distinctions from neutron stars, and the implications of quark matter under various conditions.
Participants do not reach consensus on the existence of quark stars or the implications of quark matter. Multiple competing views and uncertainties remain throughout the discussion.
Discussions include assumptions about the conditions under which quark matter might exist, the definitions of stability, and the implications of high-pressure environments. There are unresolved questions regarding the behavior of quarks at varying temperatures and pressures.
I gather that a hypothetical quark star would consist of disassociated quarks instead of triplets composing neutrons.mathman said:What is the distinction between a quark star and a neutron star? Neutrons are made of quarks.
As rootone stated, the form of matter is different. Instead of just a bunch of neutrons, it'd be sort of like a single giant nucleon consisting of huge numbers of quarks. It would be a hypothetical intermediate stage between a neutron star and a black hole.mathman said:What is the distinction between a quark star and a neutron star? Neutrons are made of quarks.
According to the models, quark matter is more stable at any pressure.fzero said:Quark stars and quark matter are hypothetical, but I'm unaware of any strong objections to the possibility that they could exist. Quark matter would exist at extremely high temperatures and pressure, where the quarks are asymptotically free, so there is no reason for them to assemble into neutrons. It would be like shoving a huge amount of quark-gluon plasma into a small volume. If some quark matter were ejected from the implosion of a quark star, the ejected components would not necessarily be at the pressure required to remain quark matter and would probably stablize as ordinary matter.
Chalnoth said:According to the models, quark matter is more stable at any pressure.
Chalnoth said:According to the models, quark matter is more stable at any pressure.
Here's a review:PeterDonis said:But at low temperatures, quarks are not asymptotically free; wouldn't they form hadrons? Certainly that happens to quarks inside accelerators like the LHC when they are ejected from collisions--that's how quarks are spotted, by the hadron jets they produce.
Chalnoth said:Here's a review:
http://arxiv.org/abs/astro-ph/0407155