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Does the pressure within a neutron star compress the neutrons to a smaller size?
The size of neutrons in a neutron star remains unchanged despite extreme pressure; instead, the pressure compresses the electron cloud, neutralizing protons and resulting in a nucleus composed solely of densely packed neutrons. The diameter of this neutron-rich nucleus ranges from 11 km to 11.5 km, containing a mass between 1 to 2 solar masses. This unique structure allows neutrons to coexist closely without repulsion, leading to the formation of a massive nucleus. The discussion also touches on the implications of mass variations just below the threshold for singularity collapse.
PREREQUISITESAstronomers, astrophysicists, and students studying nuclear physics and stellar evolution will benefit from this discussion, particularly those interested in the characteristics and behaviors of neutron stars.
The numbers at this link do go up to about 20km. Why do you say no more than 11.5kM?GoMario said:It measures no less than 11km and no more than 11.5km in diameter,