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 |
| Published: |
Al-Farabi Kazakh National University
2016-10-01
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| Series: | Physical Sciences and Technology |
| Subjects: | |
| Online Access: | http://phst/index.php/journal/article/view/64 |