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An Upper Limit on the Stochastic Gravitational-Wave Background of Cosmological Origin
The LIGO Scientific Collaboration, the Virgo Collaboration
A stochastic background of gravitational waves is expected to arise from a superposition of a large number of unresolved gravitational-wave sources of astrophysical and cosmologica…
Conformally curved binary black hole initial data including tidal deformations and outgoing radiation
Nathan K. Johnson-McDaniel, Nicolas Yunes, Wolfgang Tichy +1
(Abridged) By asymptotically matching a post-Newtonian (PN) metric to two tidally perturbed Schwarzschild metrics, we generate approximate initial data (in the form of a 4-metric)…
Stacking Gravitational Wave Signals from Soft Gamma Repeater Bursts
P. Kalmus, K. C. Cannon, S. Marka +1
Soft gamma repeaters (SGRs) have unique properties that make them intriguing targets for gravitational wave (GW) searches. They are nearby, their burst emission mechanism may invol…
How photon astronomy affects searches for continuous gravitational waves
Benjamin J. Owen
Due to their computational limitations, searches for continuous gravitational waves (GW) are significantly more sensitive when informed by observational photon astronomy and theore…
Probing neutron stars with gravitational waves
Benjamin J. Owen
Within the next decade gravitational-wave (GW) observations by Advanced LIGO in the United States, Advanced Virgo and GEO HF in Europe, and possibly other ground-based instruments…