Symmetries of spacetime infinitely far away from gravitational fields may hint at new laws of nature
LIGO-Virgo
Is the common-spectrum process observed with pulsar timing arrays a precursor to the detection?
Evaluating data analysis challenges in the 3G detector era and discussing the solutions
We model red noise and link exponential dips in residuals with pulse shape changes
Understanding millisecond pulsar spin noise and neutron star physics
Artist's sketch of accreting neutron star, a possible source of gravitational waves. Image: NASA.
Artist's representation of a GRB jets (NASA), and a 3D model of the Lomonosov satellite (MSU).