PHYSICS · Subjective · Fermi University Physics · Astrophysics & Cosmology · Stellar structure, energy generation and evolution · Stellar death and compact objects
Stars from the Inside, Ch White dwarfs: the relativistic polytrope, the Chandrasekhar mass and a cooling clock
Problem
Mestel's cooling law gives tcool∝M5/7L−5/7. A 0.6M⊙ carbon-oxygen white dwarf reaches L=10−4L⊙ after a cooling time of 4.4Gyr. Using the same scaling, estimate the cooling time of a 0.9M⊙ white dwarf to reach L=10−3L⊙.