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Neutron Stars

Notes

Neutron Stars

One-line summary: Stellar remnants so dense that a teaspoon weighs as much as Mount Everest — and dense enough that current physics fails to predict their interiors.

The insight

When a massive star dies, gravity crushes its core until electrons merge with protons into neutrons — a ball of neutrons ~20 miles across but with ~twice the Sun's mass. Per michelle-thaller, these are a frontier of known physics failing: plug measured size and mass into our particle models and "the equations don't work." The interior is likely some interaction of quarks — a state of matter never created in a lab and with no working description. Unlike black-holes, neutron stars are directly observable, which is why NASA's NICER explorer can map their surfaces and see spacetime curve around them.

Evidence

Contradictions / tensions

This is a case of acknowledged model failure, not disagreement between sources: "pretty much every model so far doesn't match what we actually measure." A falsifier for any proposed interior model is whether it reproduces the observed size for the measured mass.

Open questions

  • What is the state of matter at a neutron-star core — discrete neutrons, or a "quark soup"?
  • The same "we don't have the physics" gap applies to black-holes interiors and the pre-Big-Bang state (what-preceded-the-big-bang).

Related

Referenced by