Matter at the core of neutron star

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Discussion Overview

The discussion revolves around the properties of matter in the core of neutron stars, focusing on fundamental characteristics such as particle composition and states of matter. Participants explore concepts related to the ratios of neutrons, protons, and electrons, as well as the nature of these particles in terms of being free, gas, fluid, or superfluid.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant inquires about the fundamental properties of matter in neutron star cores, specifically asking for a description that excludes strange matter and focuses on neutrons, electrons, and protons.
  • Another participant suggests that matter may exist as a superfluid of neutrons, protons, and electrons, with a higher percentage of neutrons at greater depths.
  • A different viewpoint describes the core as a mixture of superfluid neutrons, superconducting/superfluid protons, and an electron "gas," noting that the density at the center is about ten times that of an atomic nucleus.
  • One participant mentions the possibility of a quark-gluon fluid in the core, suggesting it could explain the mass differences between neutron stars and black holes.
  • Several posts reiterate the initial question about the properties of matter in neutron stars, indicating a lack of responses and encouraging further research on the topic.

Areas of Agreement / Disagreement

Participants express differing views on the state and composition of matter in neutron star cores, with no consensus reached on the exact nature of the matter present.

Contextual Notes

Some claims depend on specific definitions of states of matter and may involve unresolved assumptions about the conditions within neutron stars.

Vrbic
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How would you approximately describe matter in the core of underlying neutron star? I am asking for really fundamental properties. No strange matter, consider just n,e,p. A ratio, can we describe particles as free? Gas x fluid x superfluid? etc.
 
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Thanks for the post! Sorry you aren't generating responses at the moment. Do you have any further information, come to any new conclusions or is it possible to reword the post?
 
Greg Bernhardt said:
Thanks for the post! Sorry you aren't generating responses at the moment. Do you have any further information, come to any new conclusions or is it possible to reword the post?
No, I mean it is over.
 
I can't give any details, but I've heard that matter exists in the form of a superfluid of neutrons, protons, and electrons. The deeper you go, the higher the percentage of neutrons compared to protons and electrons.
 
Vrbic said:
How would you approximately describe matter in the core of underlying neutron star? I am asking for really fundamental properties. No strange matter, consider just n,e,p. A ratio, can we describe particles as free? Gas x fluid x superfluid? etc.

As with all questions of this sort, you will get better and more helpful answers if you research the topic yourself, and then come back here with more specific questions about what you found. In this case, the wikipedia pages on"neutron stars" and "degenerate matter" are pretty good.
 
Vrbic said:
How would you approximately describe matter in the core of underlying neutron star? I am asking for really fundamental properties. No strange matter, consider just n,e,p. A ratio, can we describe particles as free? Gas x fluid x superfluid? etc.
It is a mixture of superfluid neutrons, superconducting/superfluid protons, and an electron "gas." Toward the center there are only a few percent electrons and protons. The whole thing is believed to be penetrated by a great many tiny electromagnetic vortices. There is no empty space whatsoever. At the center the density is about ten times that of an atomic nucleus.
 
Conditions in the core of neutron stars strongly hints at a quark - gluon fluid. I find that very Interesting. It may explain the disparity between the most massive neutron stars and lowest mass black holes.
 

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