Calculating the Radius of a Neutron Star

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Discussion Overview

The discussion revolves around the hypothetical scenario of the Sun collapsing into a neutron star and seeks to determine the resulting radius of such a neutron star. Participants explore theoretical implications, calculations, and the conditions necessary for such a collapse, touching on concepts from astrophysics and stellar evolution.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • One participant questions the feasibility of the Sun becoming a neutron star, stating it is too small and would instead become a white dwarf.
  • Another participant suggests that if the Sun could be compressed into a neutron star, the critical density required for such a transformation should be considered to calculate the radius.
  • A calculation approach is proposed using the mass of the Sun and the critical density to find the volume of the neutron star, followed by deriving the radius from the volume of a sphere.
  • One participant hypothesizes that if the Sun were to collapse into a neutron star, its diameter could be approximately 14 kilometers, based on a comparison to atomic nuclei and the significant reduction in size during the collapse.

Areas of Agreement / Disagreement

Participants express differing views on whether the Sun could become a neutron star, with some asserting it cannot due to its mass, while others explore the hypothetical scenario without consensus on the feasibility of such a collapse.

Contextual Notes

The discussion includes assumptions about critical density and the conditions under which a star collapses into a neutron star, which are not fully resolved. The calculations proposed depend on these assumptions and the definitions of density and volume.

sammyz
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The question is: Suppose the sun collapses into a neutron star. What will its radius be?

The question gave a brief backround explaining that stars are powered by nuclear reactions that fuse hydrogen and helium. When the hydrogen is used up the star collapses into a neutron star. The force of gravity becomes so large that protons and electrons are fused into neutrons. The entire star is then a tightly packed ball of neutrons with the density of nuclear matter.

I am not even sure how to begin. Any help would be appreciated. Thanks.
 
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For starters, the sun is too small to end up as a neutron star - it would collapse to a white dwarf.
 
If you somehow had an enormous compressor to put the Sun in, you could squash it into being a neutron star. The how big would its radius be?

If i remember correctly there is some critical density that a star must attain for collapse into a neutron star so that the gravitation can overcome the degeneracy pressure. The easy way to find the answer is to take this critical density as an approximation to the real density, use it with the mass of the sun to find the volume if it was a neutron star, and then finally you can use the volume of a sphere, \frac{4}{3} \pi r^2, to get the radius out of that figure.
 
sammyz said:
The question is: Suppose the sun collapses into a neutron star. What will its radius be?

The question gave a brief backround explaining that stars are powered by nuclear reactions that fuse hydrogen and helium. When the hydrogen is used up the star collapses into a neutron star. The force of gravity becomes so large that protons and electrons are fused into neutrons. The entire star is then a tightly packed ball of neutrons with the density of nuclear matter.

I am not even sure how to begin. Any help would be appreciated. Thanks.

In a sense an atomic nucleus is like neutron star and the electron cloud would have been the size of the star before the collapse, therefore its diameter must have shrunk by approx 1/100,000 so if the sun with a diameter of 1,400,000k were converted to a nuetron star its diameter would be 14 kilometers hypotheically
 

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