Construct · 1 fields · 1 citations

quasinormal modes: a standalone construct

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Gravitational physics

damped characteristic oscillations of a perturbed black hole whose frequencies depend only on its mass and spin.

In gravitational physics, quasinormal modes refers to damped characteristic oscillations of a perturbed black hole whose frequencies depend only on its mass and spin. This meaning comes from Vishveshwara (1970) in Nature.[1]

Unit
Recovery means
Measured by

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Nearby constructs

hole3 fields · 5 citationsjingle · one word, three constructs mass3 fields · 9 citationsjingle · one word, three constructs spin4 fields · 4 citationsjingle · one word, four constructs

References

Vishveshwara, C. V. (1970). Scattering of Gravitational Radiation by a Schwarzschild Black-hole. Nature, 227(5261), 936-938. https://doi.org/10.1038/227936a0

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