Post-Keplerian waveform model for binary compact object as sources of space-based gravitational wave detector and its implications

Understand

Binary compact objects will be among the important sources for the future space-based gravitational wave detectors.

• Such binary compact objects include stellar massive binary black hole, binary neutron star, binary white dwarf and mixture of these compact objects.
• Regarding to the relatively low frequency, the gravitational interaction between the two objects of the binary is weak.
• Post-Newtonian approximation of general relativity is valid.