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Relativistic stars with a linear equation of state: analogy with classical isothermal spheres and black holes - MaRDI portal

Relativistic stars with a linear equation of state: analogy with classical isothermal spheres and black holes (Q3516854)

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Relativistic stars with a linear equation of state: analogy with classical isothermal spheres and black holes
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    Relativistic stars with a linear equation of state: analogy with classical isothermal spheres and black holes (English)
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    12 August 2008
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    hydrodynamics
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    instabilities
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    relativity
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    stars: neutron
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    gravitation
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    Black hole physics
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