Log-linear analysis

The chirp mass of a binary star system with component masses $m_{1}$ and $m_{2}$ is given by $ℳ = \frac{(m_{1} m_{2})^{3 / 5}}{(m_{1} + m_{2})^{1 / 5}}$ .^[1]^[2] According to general relativity, the chirp mass determines the leading order amplitude and frequency evolution of the gravitational wave signal emitted by the binary during its inspiral.

References

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↑ L. Blanchet, T. Damour, B. R. Iyer, C. M. Will, and A. G. Wiseman, Phys. Rev. Lett. 74, 3515 (1995).
↑ L. Blanchet, B. R. Iyer, C. M. Will, and A. G. Wiseman, Classical Quantum Gravity 13, 575 (1996).

[1] L. Blanchet, T. Damour, B. R. Iyer, C. M. Will, and A. G. Wiseman, Phys. Rev. Lett. 74, 3515 (1995).

[2] L. Blanchet, B. R. Iyer, C. M. Will, and A. G. Wiseman, Classical Quantum Gravity 13, 575 (1996).

[1]

[2]

Log-linear analysis

References

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