activity
20242026
most citedWaveform Modelling for the Laser Interferometer Space Antenna

39 citations · 42 across the 4 of their papers we have counts for

collaborators

6 papers

gr-qc2026

Finite Populations & Finite Time: The Non-Gaussianity of a Gravitational Wave Background

William G. Lamb, Jeremy M. Wachter, Andrea Mitridate +5

Strong evidence for an isotropic, Gaussian gravitational wave background (GWB) has been found by multiple pulsar timing arrays (PTAs). The GWB is expected to be sourced by a finite…

gr-qc202639 cited

Waveform Modelling for the Laser Interferometer Space Antenna

LISA Consortium Waveform Working Group, Niayesh Afshordi, Sarp Akçay +144

LISA, the Laser Interferometer Space Antenna, will usher in a new era in gravitational-wave astronomy. As the first anticipated space-based gravitational-wave detector, it will exp…

gr-qc20262 cited

More accurate gravitational wave backgrounds from cosmic strings

Jeremy M. Wachter, Ken D. Olum, Jose J. Blanco-Pillado

We derive a general procedure for calculating the gravitational wave background (GWB) from cosmic string loops whose typical shape evolves over time, as in gravitational backreacti…

gr-qc2025

Numerical gravitational backreaction on cosmic string loops from simulation

Jeremy M. Wachter, Ken D. Olum, Jose J. Blanco-Pillado +2

We report on the results of performing computational gravitational backreaction on cosmic string loops taken from a network simulation. The principal effect of backreaction is to s…

astro-ph.CO2025

Gravitational waves from cosmic strings in LISA: reconstruction pipeline and physics interpretation

Jose J. Blanco-Pillado, Yanou Cui, Sachiko Kuroyanagi +6

We initiate the LISA template databank for stochastic gravitational wave backgrounds sourced by cosmic strings. We include two templates, an analytical template, which enables more…

astro-ph.IM2024

Deep Neural Emulation of the Supermassive Black-hole Binary Population

Nima Laal, Stephen R. Taylor, Luke Zoltan Kelley +13

While supermassive black-hole (SMBH)-binaries are not the only viable source for the low-frequency gravitational wave background (GWB) signal evidenced by the most recent pulsar ti…