Speaker
Andrew Miller
Description
The third observing run of advanced LIGO, Virgo and KAGRA brought unprecedented sensitivity towards a variety of quasi-monochromatic, persistent gravitational-wave signals. Continuous waves allow us to probe not just the canonical asymmetrically rotating neutron stars, but also different forms of dark matter, thus showing the wide-ranging astrophysical implications of using a relatively simple signal model. In this talk, I will summarize recent results from searches for dark matter in the form of asteroid-mass primordial black holes, dark matter clouds that could form around rotating black holes, and even dark matter that could interact with the detectors themselves.
Details
Andrew Miller / Nikhef and Utrecht University
| Is this abstract from experiment? | Yes |
|---|---|
| Name of experiment and experimental site | LIGO/Virgo/KAGRA |
| Is the speaker for that presentation defined? | Yes |
| Internet talk | Yes |
Author
Andrew Miller
