Nonvalidity of I-Love-Q Relations for Hot White Dwarf Stars
arXiv:1709.04593 · doi:10.1093/mnras/sty1227
Abstract
The equilibrium configurations of uniformly rotating white dwarfs at finite temperatures are investigated, exploiting the Chandrasekhar equation of state for different isothermal cores. The Hartle-Thorne formalism is applied to construct white dwarf configurations in the framework of Newtonian physics. The equations of structure are considered in the slow rotation approximation and all basic parameters of rotating hot white dwarfs are computed to test the so-called moment of inertia, tidal Love number and quadrupole moment (-Love-) relations. It is shown that even within the same equation of state the -Love- relations are not universal for white dwarfs at finite temperatures.
7 pages, 12 figures
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Cited by in corpus (9)
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- I-Love-Q Relations for Realistic White Dwarfs
- Rotating white dwarf models with finite-temperature envelope
- Equilibrium Configurations of Rotating White Dwarfs at Finite Temperatures
- Dark Matter-admixed Rotating White Dwarfs as Peculiar Compact Objects
- Oscillations and tidal deformations of crystallized white dwarfs
- Compact star deformation and universal relationship for magnetized white dwarfs
- Dark I-Love-Q