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Rotating Stars in Relativity

Stergioylas, Nikolaos

Rotating relativistic stars have been studied extensively in recent years, both theoretically and observationally, because of the information they might yield about the equation of state of matter at extremely high densities and because they are considered to be promising sources of gravitational waves. The latest theoretical understanding of rotating stars in relativity is reviewed in this updated article. The sections on the equilibrium properties and on the nonaxisymmetric instabilities in f-modes and r-modes have been updated and several new sections have been added on analytic solutions for the exterior spacetime, rotating stars in LMXBs, rotating strange stars, and on rotating stars in numerical relativity

Article / Άρθρο
info:eu-repo/semantics/article

Stability
Oscillations
Numerical relativity
Relativistic stars
Cosmic rotation

Αριστοτέλειο Πανεπιστήμιο Θεσσαλονίκης (EL)
Aristotle University of Thessaloniki (EN)

2009-06-29T16:58:45Z
2003


Αριστοτέλειο Πανεπιστήμιο Θεσσαλονίκης, Σχολή Θετικών Επιστημών, Τμήμα Φυσικής

Living Reviews in Relativity, vol.6 [2003] p.1-109 [Published Version]

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info:eu-repo/semantics/openAccess



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