Construct · 1 fields · 1 citations

Hartle-Thorne approximation: a standalone construct

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Gravitational physics

the perturbative treatment of slowly and rigidly rotating relativistic stars to second order in angular velocity.

In gravitational physics, Hartle-Thorne approximation refers to the perturbative treatment of slowly and rigidly rotating relativistic stars to second order in angular velocity. This meaning comes from Hartle (1967) in The Astrophysical Journal.[1]

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Nearby constructs

order4 fields · 6 citationsjingle · one word, four constructs treatment1 fields · 1 citationsanchor · a standalone construct velocity6 fields · 14 citationsjingle · one name, six constructs

References

Hartle, J. B. (1967). Slowly Rotating Relativistic Stars. I. Equations of Structure. The Astrophysical Journal, 150, 1005. https://doi.org/10.1086/149400

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