A neutron star is a type of stellar remnant that can result from the gravitational collapse of a massive star during a Type II, Type Ib or Type Ic supernova event. Neutron stars are the densest and tiniest stars known to exist in the universe; although having only the diameter of about 10 km (6 mi), they may have a mass of several times that of the Sun. Neutron stars probably appear white to the naked eye.
Six miles, gravity quantizes up.
Say what?
Some neutron stars rotate very rapidly and emit beams of electromagnetic radiation as pulsars.
No atom no EM mode, sorry. But the things should support packed nulls at the magnetic level. Say, something like stable neutrinos. When we run the normal integral equations, as if mass were a compressible fluid, the delta radius breaks down near the center, the equations don't work. Einstein calls that general relativity, I call that problems with numerical convergence. You cannot scale up large enough to solve the numerical problem, because its a neutron star, not a quark star; you reach a limit. You can scale up farther, if its a quark star, but I do not think mass is stable at the Higgs level. However, one might just make it with a Higgs wave in motion. We could call it the Higgs fluid matter wave.
A Quark star won't work. Quarks are not uniform, they will have to sort in order to regain maximum entropy, and you still have the problem. As near as I can tell, phase will still use the neutron for numerical integration.
So, in the center is a region where phase imbalance, stored in the neutron, reaches the limit, or we get Higgs kinetic wave energy.
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