The evolution of stars, as discussed in Section 33-2, can lead to a white dwarf, a neutron

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The evolution of stars, as discussed in Section 33-2, can lead to a white dwarf, a neutron star, or even a black hole, depending on the mass.

(a) Referring to Sections 33-2 and 33-4, give the radius of (i) a white dwarf of 1 solar mass, (ii) a neutron star of 1.5 solar masses, and (iii) a black hole of 3 solar masses.

(b) Express these three radii as ratios (ri: rii: riii).

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