No, I mean it is over.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?
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.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.
The matter at the core of a neutron star is made up of extremely dense and tightly packed neutrons. This is due to the immense gravitational forces present in the core, which compress the atoms and strip them of their electrons.
The pressure at the core of a neutron star is so immense that it can reach up to 10^34 times the pressure found at the Earth's core. This is strong enough to overcome the repulsive force between neutrons and cause them to merge together.
The matter at the core of a neutron star is responsible for its small size and high density. The core is typically only about 10 kilometers in diameter, but can have a mass up to twice that of the Sun. This extreme density is due to the tightly packed neutrons in the core.
The temperature at the core of a neutron star can reach up to 10^12 Kelvin. This high temperature is a result of the immense pressure and energy released during the formation of the star. However, as the star ages, it gradually cools down.
The matter at the core of a neutron star is also responsible for its strong magnetic field. As the core rotates, it creates a dynamo effect, generating a magnetic field that is a trillion times stronger than the Earth's. This can also lead to powerful bursts of radiation from the star's poles, known as pulsars.