Non-rotating and slowly rotating white dwarfs in classical physics
The equilibrium configurations of uniformly rotating white dwarfs are calculated in the framework of classical physics. The Chandrasekhar and the Salpeter equations of state are used to describe the white dwarf matter. The Hartle formalism is applied to the integration of the equations of hydrostati...
Main Authors: | , , , , , |
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Format: | Article |
Language: | English |
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Al-Farabi Kazakh National University
2016-10-01
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Series: | Physical Sciences and Technology |
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Online Access: | http://phst/index.php/journal/article/view/64 |
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author | K. Boshkayev J.A. Rueda R. Ruffini B. Zhami Zh. Kalymova G. Balgimbekov |
author_facet | K. Boshkayev J.A. Rueda R. Ruffini B. Zhami Zh. Kalymova G. Balgimbekov |
author_sort | K. Boshkayev |
collection | DOAJ |
description | The equilibrium configurations of uniformly rotating white dwarfs are calculated in the framework of classical physics. The Chandrasekhar and the Salpeter equations of state are used to describe the white dwarf matter. The Hartle formalism is applied to the integration of the equations of hydrostatic equilibrium and field equations. The equations of structure have been expanded in powers of the angular velocity Ω of the white dwarf, and terms of higher order than Ω |
first_indexed | 2024-03-11T14:44:22Z |
format | Article |
id | doaj.art-6f9fc0189bff4adba60c7769e03616bd |
institution | Directory Open Access Journal |
issn | 2409-6121 |
language | English |
last_indexed | 2024-03-11T14:44:22Z |
publishDate | 2016-10-01 |
publisher | Al-Farabi Kazakh National University |
record_format | Article |
series | Physical Sciences and Technology |
spelling | doaj.art-6f9fc0189bff4adba60c7769e03616bd2023-10-30T13:11:33ZengAl-Farabi Kazakh National UniversityPhysical Sciences and Technology2409-61212016-10-0121Non-rotating and slowly rotating white dwarfs in classical physicsK. Boshkayev0J.A. Rueda1R. Ruffini2B. ZhamiZh. KalymovaG. BalgimbekovAl-Farabi Kazakh National University, IETP, al-Farabi 71, 050040 Almaty, Kazakhstan Dipartimento di Fisica and ICRA, Università di Roma “La Sapienza”, Piazzale Aldo Moro 5, I-00185 Roma, ItalyDipartimento di Fisica and ICRA, Università di Roma “La Sapienza”, Piazzale Aldo Moro 5, I-00185 Roma, ItalyDipartimento di Fisica and ICRA, Università di Roma “La Sapienza”, Piazzale Aldo Moro 5, I-00185 Roma, ItalyThe equilibrium configurations of uniformly rotating white dwarfs are calculated in the framework of classical physics. The Chandrasekhar and the Salpeter equations of state are used to describe the white dwarf matter. The Hartle formalism is applied to the integration of the equations of hydrostatic equilibrium and field equations. The equations of structure have been expanded in powers of the angular velocity Ω of the white dwarf, and terms of higher order than Ωhttp://phst/index.php/journal/article/view/64Key wordswhite dwarfsuniform rotationHartle’s formalismequilibrium configurationsmoment of inertia |
spellingShingle | K. Boshkayev J.A. Rueda R. Ruffini B. Zhami Zh. Kalymova G. Balgimbekov Non-rotating and slowly rotating white dwarfs in classical physics Physical Sciences and Technology Key words white dwarfs uniform rotation Hartle’s formalism equilibrium configurations moment of inertia |
title | Non-rotating and slowly rotating white dwarfs in classical physics |
title_full | Non-rotating and slowly rotating white dwarfs in classical physics |
title_fullStr | Non-rotating and slowly rotating white dwarfs in classical physics |
title_full_unstemmed | Non-rotating and slowly rotating white dwarfs in classical physics |
title_short | Non-rotating and slowly rotating white dwarfs in classical physics |
title_sort | non rotating and slowly rotating white dwarfs in classical physics |
topic | Key words white dwarfs uniform rotation Hartle’s formalism equilibrium configurations moment of inertia |
url | http://phst/index.php/journal/article/view/64 |
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