Series
Hydrostatic equilibrium — the series
2 essays on one idea, from the one that introduces it to the one that assumes the rest.
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A star is held up by its own weight
A star has a central temperature because it has a central pressure, and it has a central pressure because everything above is pressing down. The nuclear reactions do not set that temperature — they obey it.
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A floor under the centre that assumes nothing
There is a lower bound on the pressure at the centre of any body in hydrostatic equilibrium, and it needs no equation of state, no composition and no temperature — only a mass and a radius. For the Sun it is nearly useless. For a neutron star it says which theory of gravity the interior needs.