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Parameter estimation on gravitational waves from neutron-star binaries with spinning components
Ben Farr, Christopher P. L. Berry, Will M. Farr +14
Inspiraling binary neutron stars are expected to be one of the most significant sources of gravitational-wave signals for the new generation of advanced ground-based detectors. We…
The effect of small inter-pulsar distance variations in stochastic gravitational wave background searches with Pulsar Timing Arrays
Chiara M. F. Mingarelli, Trevor Sidery
One of the primary objectives for Pulsar Timing Arrays (PTAs) is to detect a stochastic background generated by the incoherent superposition of gravitational waves (GWs), in partic…
The First Two Years of Electromagnetic Follow-Up with Advanced LIGO and Virgo
Leo P. Singer, Larry R. Price, Ben Farr +13
We anticipate the first direct detections of gravitational waves (GWs) with Advanced LIGO and Virgo later this decade. Though this groundbreaking technical achievement will be its…
Characterising gravitational wave stochastic background anisotropy with Pulsar Timing Arrays
Chiara M. F. Mingarelli, Trevor Sidery, Ilya Mandel +1
Detecting a stochastic gravitational wave background, particularly radiation from individually unresolvable super-massive black hole binary systems, is one of the primary targets f…
Observing the dynamics of super-massive black hole binaries with Pulsar Timing Arrays
C. M. F. Mingarelli, K. Grover, T. Sidery +2
Pulsar Timing Arrays are a prime tool to study unexplored astrophysical regimes with gravitational waves. Here we show that the detection of gravitational radiation from individual…
The dynamics of pulsar glitches: Contrasting phenomenology with numerical evolutions
T. Sidery, A. Passamonti, N. Andersson
In this paper we consider a simple two-fluid model for pulsar glitches. We derive the basic equations that govern the spin evolution of the system from two-fluid hydrodynamics, acc…