Speaker
Yun-Long Zhang
(NAOC(National Astronomical Observatories, CAS))
Description
Chiral gravitational wave backgrounds are predicted in many well-motivated mechanisms. We investigate the detection of Chiral GWBs using a network of detectors under arbitrary configurations. We also propose a dipole pulsar timing array, which demonstrates sensitivity to Chiral gravitational wave backgrounds from the nanohertz to microhertz regime.
Primary author
Yun-Long Zhang
(NAOC(National Astronomical Observatories, CAS))
