Equilibrium Configurations of Rotating White Dwarfs at Finite Temperatures View Full Text


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Article Info

DATE

2018-12

AUTHORS

K. Boshkayev

ABSTRACT

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. More... »

PAGES

847-852

References to SciGraph publications

  • 2014-09. General relativistic white dwarfs and their astrophysical implications in JOURNAL OF THE KOREAN PHYSICAL SOCIETY
  • 2018-04. General relativistic effects in the structure of massive white dwarfs in GENERAL RELATIVITY AND GRAVITATION
  • 2007. Neutron Stars 1 in NONE
  • Identifiers

    URI

    http://scigraph.springernature.com/pub.10.1134/s106377291812017x

    DOI

    http://dx.doi.org/10.1134/s106377291812017x

    DIMENSIONS

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