Instruct: Identify the main and secondary category of Arxiv papers based on the titles and abstracts
Query: Equilibrium Configurations of Rotating White Dwarfs at Finite
  Temperatures   In this work, cold and hot, static and rotating white dwarf stars are
investigated within the framework of classical physics, employing the
Chandrasekhar equation of state. The main parameters of white dwarfs such as
the central density, pressure, total mass and radius are calculated fulfilling
the stability criteria for hot rotating stars. To construct rotating
configurations the Hartle approach is involved. It is shown that the effects of
finite temperatures become crucial in low-mass white dwarfs, whereas rotation
is relevant in all mass range. The simultaneous accounting for temperature and
rotation is critical in the calculation of the radii of white dwarfs. The
results obtained in this work can be applied to explain a variety of
observational data for white dwarfs from the Sloan Digital Sky Survey Data
Releases.

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The categories of this paper are: dg-ga
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The categories of this paper are: adap-org
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The categories of this paper are: q-alg
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The categories of this paper are: comp-gas
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The categories of this paper are: nucl-th
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The categories of this paper are: q-bio
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The categories of this paper are: math-ph
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The categories of this paper are: hep-lat
0
The categories of this paper are: hep-ph
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The categories of this paper are: acc-phys
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The categories of this paper are: cond-mat
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The categories of this paper are: econ
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The categories of this paper are: eess
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The categories of this paper are: quant-ph
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The categories of this paper are: atom-ph
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The categories of this paper are: bayes-an