Why Don't Neutron Stars Collapse > Likes and Comments

There are some things in the universe whose form is easy in theory, like black holes. Bring a fairly large volume in a compact volume and it is more difficult to avoid gravity If you accumulated a lot of things in one place and let gravity do its work, you would eventually pass a significant limit, where the need to escape gravity would exceed the speed of light.Reach this point, and you create a black hole
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Neutron stars are supported by neutron degeneracy pressure, which is a consequence of neutrons not wanting to be squeezed together too tightly (Pauli Exclusion Principle).

Thomas wrote: "Neutron stars are supported by neutron degeneracy pressure, which is a consequence of neutrons not wanting to be squeezed together too tightly (Pauli Exclusion Principle)."
​"Spot on, Thomas! The Pauli Exclusion Principle is indeed the quantum foundation here—preventing identical fermions from occupying the exact same quantum state.
​From an information physics perspective, it's fascinating to view degeneracy pressure not just as a physical force, but as a fundamental information density limit. Spacetime simply refuses to overlap identical quantum states beyond a critical information threshold until gravity forces a collapse past the Tolman–Oppenheimer–Volkoff (TOV) limit into a black hole."