Formation of neutron stars and black holes.

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SUMMARY

Neutron stars form from massive stars that undergo gravitational collapse after exhausting their nuclear fuel, while black holes arise from even more massive stars. During this collapse, the star's core compresses, leading to the formation of neutrons as electrons combine with protons under extreme pressure. The distinction between neutron stars and black holes lies in the mass; neutron stars are incredibly dense but still retain a physical structure, whereas black holes represent a point of singularity where gravity overcomes all other forces. The discussion clarifies that neutron stars are not merely supermassive atomic nuclei but rather a unique state of matter under extreme conditions.

PREREQUISITES
  • Understanding of stellar evolution and lifecycle
  • Familiarity with nuclear fusion processes in stars
  • Knowledge of gravitational collapse and its effects on stellar remnants
  • Basic concepts of atomic structure and particle physics
NEXT STEPS
  • Research the process of stellar nucleosynthesis in massive stars
  • Study the characteristics and formation of black holes, particularly the Schwarzschild radius
  • Explore the properties of neutron stars, including their density and structure
  • Learn about gravitational waves and their relation to neutron star mergers
USEFUL FOR

Astronomy students, astrophysicists, and anyone interested in the lifecycle of stars and the formation of compact objects in the universe.

LogicalAcid
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First of all, I know that that very large stars tend to form black holes, and smaller stars, but still massive in comparison to our sun, tend to form neutron stars. My question is, if matter is lost when a star collapses into a black hole, but can still form one, why is it that it is a star first if it has more mass than the original black hole?
 
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LogicalAcid said:
why is it that it is a star first if it has more mass than the original black hole?
During its normal life, the nuclear reactions in the star's core creates outward pressure that compensate the gravity. It is only when the star has radiated most of its energy from nuclear reactions that it has trouble fighting gravity. Depending on its mass at this point, it may collapse to a white dwarf, a neutron star, or a black hole.
 
I understand that a neutron star is a star so effected by gravity that the electron shells have been foced into the protons to form neutrons. Presumably these neutrons are packed in tightly together as they have no repulsive charges and are under enormous gravitational pressure. Also, most of an atom is empty space between the nucleus and the electon quanta. If there are no electrons, does that mean that we have effectively a supermassive atomic nucleus? Or is that black hole territory? Or (most likely) I'm missing something!
 

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