Static and rotating white dwarfs at finite temperatures

Kuantay Boshkayev

Published 2019-09-24Version 1

Static and rotating hot white dwarfs are investigated in Newtonian gravity, employing the well-known Chandrasekhar equation of state. The mass-radius relations of stable white dwarfs are constructed for different temperatures. It is shown that the maximum mass of hot rotating white dwarfs is slightly less than for cold rotating white dwarfs.