Speaker
Tao Xu
(The University of Oklahoma)
Description
The observation of gravitational waves opens a new window for exploring the properties of dark matter. Gravitational wave messengers enable the concurrent measurement of their amplitudes and phases, facilitating a precise analysis of the production and propagation processes. In this talk, I will demonstrate how gravitational waves can be utilized to study the dark matter halo. Specifically, I will use wave dark matter as an example to show that gravitational waveforms, along with further multi-messenger observations involving photon signals, reveal distinctive features to be probed with the ongoing LIGO and upcoming LISA missions.
Authors
Badal Bhalla
(University of Oklahoma)
Fazlollah Hajkarim
(University of Oklahoma)
Kuver Sinha
(University of Oklahoma)
Mudit Rai
(Texas AM University)
Tao Xu
(The University of Oklahoma)
