Speaker
Yutong He
(Stockholm University)
Description
Radio telescopes can be used as detectors for gravitational waves (GWs) in both the low ($\sim$nHz) and high ($\gg$kHz) frequency regimes. These GWs provide a unique insight into, e.g., the physics at QCD phase transition, primordial black holes, or the nature of gravity. The upcoming SKA is expected to improve the constraints on GW background from existing radio telescopes.
Authors
Alberto ROPER POL
(APC)
Axel Brandenburg
(Stockholm University)
Yutong He
(Stockholm University)
