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2007

Gravitational waveforms for finite mass binaries

Vasúth, Mátyás, Majár, János

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One of the promising sources of gravitational radiation is a binary system composed of compact stars.

It is an important question how the rotation of the bodies and the eccentricity of the orbit affect the detectable signal.
Here we present a method to evaluate the gravitational wave polarization states for inspiralling compact binaries with comparable mass.
We consider eccentric orbits and the spin-orbit contribution in the case of one spinning object up to 1.5 post-Newtonian order.

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