http://arxiv.org/abs/2111.14084
Even though Pulsar Timing Arrays already have the potential to detect the gravitational wave background by finding a quadrupole correlation in the timing residuals, this goal has not yet been achieved. Motivated by some theoretical arguments, we analyzed some advantages of including the millisecond pulsars within globular clusters, especially those in their cores, in current and future Pulsar Timing Array projects for detecting the gravitational waves emitted by an ensemble of supermassive black holes.
M. Maiorano, F. Paolis, A. Nucita, et. al.
Tue, 30 Nov 21
53/105
Comments: 8 pages, 4 figures, proceeding of the Sixteenth Marcel Grossmann Meeting