Detection of exoplanets through gravitational wave astronomy

In this seminar I will present a new method for detecting circumbinary exoplanets through gravitational wave
astronomy. I will show that the Laser Interferometer Space Antenna (LISA) mission will be able to both detect
Jupiter-like planets orbiting white dwarfs binaries, and to determine some of their orbital parameters.
This technique is not affected by stellar activity and it will allow us to search for post-main sequence exoplanets
everywhere in the Milky Way and in the Magellanic Clouds.
I will then explain how having a more robust statistics of this planetary population will enable us to find the
connecting thread that runs from formation to the very end of an exoplanet.
Finally, in the spirit of the new era of multi-messenger astronomy, I will discuss the possibilities that
could open for the field of exoplanets when standard electromagnetic techniques work in synergy with Gravitational
Wave astronomy.