Speaker
NGAI CHUN LUNG
(NTHU)
Description
In the poster, I will represent our recent work on gravitational wave physics. In particular, we are interested in the signals from compact binary coalescences in the sub-solar mass region. According to our knowledge, there are no formation channels for black holes and neutron stars in such mass region. Detection of such signals allows us to give hints to new physics and constraint some dark matter models. We will also present how our algorithm is developed and is deployed for detection.
Author
NGAI CHUN LUNG
(NTHU)