Derives large-eccentricity asymptotics for post-Newtonian eccentric waveform Fourier modes and builds a fast endpoint-constrained analytic approximation with error under 10^{-3} valid to p=200.
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Continuous spin gravity yields GW time-delay deviations of order ρ_g/ω from GR predictions for frequencies above ρ_g, with damping below, enabling sensitivity to spin scales ~10^{-14} eV at ground interferometers and ~10^{-24} eV at PTAs.
FABLE simulation predictions for the nanohertz gravitational wave background are statistically consistent with NANOGrav 15-year data at 1–2.5σ tension, with physically motivated population modifications further improving agreement.
SKAO timing of a handful of binary pulsars can reach unprecedented sensitivity to microhertz gravitational waves from inspiralling massive black hole binaries via resonant perturbations.
Proposes and simulates the use of space-based atomic clock networks for one-way Doppler tracking of gravitational waves in concert with LISA, including noise analysis and preliminary parameter estimation on binary sources.
A perturbative analytical model of gravitational waves on an exact Bianchi IV background is derived via the proper-time method and shown to be stable.
Reports timing solutions and basic properties for 49 pulsars (18 new) from the AO327 survey, with emission feature notes and model comparisons for distances.
VLBI astrometry of nearby MSPs can supply the distance priors needed to localize individual continuous-wave nanohertz GW sources to ~10^{-3} deg².
Simulations forecast 21-51% probability of resolving individual SMBH binaries with PTAs in 0-10 years, with localization areas containing ~190k early-type galaxies on average and a ranking method that excludes roughly half the candidates when galaxy properties are available.
SKAO forecasts show that planned observations will improve SGWB anisotropy constraints but remain insufficient to detect the kinematic dipole even in joint PTA-astrometry analyses.
A review summarizing detection methods, population statistics, and coevolution of supermassive black holes with host galaxies from early universe observations and simulations.
citing papers explorer
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Large-Eccentricity Asymptotics and Fast Analytic Approximation for Fourier modes of Post-Newtonian Eccentric Waveforms
Derives large-eccentricity asymptotics for post-Newtonian eccentric waveform Fourier modes and builds a fast endpoint-constrained analytic approximation with error under 10^{-3} valid to p=200.
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First look at continuous spin gravity: Time delay signatures
Continuous spin gravity yields GW time-delay deviations of order ρ_g/ω from GR predictions for frequencies above ρ_g, with damping below, enabling sensitivity to spin scales ~10^{-14} eV at ground interferometers and ~10^{-24} eV at PTAs.
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Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations
FABLE simulation predictions for the nanohertz gravitational wave background are statistically consistent with NANOGrav 15-year data at 1–2.5σ tension, with physically motivated population modifications further improving agreement.
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Unveiling the Microhertz Gravitational-Wave Sky with the Square Kilometre Array Observatory
SKAO timing of a handful of binary pulsars can reach unprecedented sensitivity to microhertz gravitational waves from inspiralling massive black hole binaries via resonant perturbations.
-
Gravitational-wave astronomy with a space-based optical clock network
Proposes and simulates the use of space-based atomic clock networks for one-way Doppler tracking of gravitational waves in concert with LISA, including noise analysis and preliminary parameter estimation on binary sources.
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Linear perturbations of an exact gravitational wave in the Bianchi IV universe
A perturbative analytical model of gravitational waves on an exact Bianchi IV background is derived via the proper-time method and shown to be stable.
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Discovery and Timing of 49 Pulsars from the Arecibo 327-MHz Drift Survey
Reports timing solutions and basic properties for 49 pulsars (18 new) from the AO327 survey, with emission feature notes and model comparisons for distances.
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VLBI-Enabled Localization of Continuous GW Sources
VLBI astrometry of nearby MSPs can supply the distance priors needed to localize individual continuous-wave nanohertz GW sources to ~10^{-3} deg².
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Prospects of resolving and localising individual supermassive black hole binaries with pulsar timing arrays: the host ranking challenge
Simulations forecast 21-51% probability of resolving individual SMBH binaries with PTAs in 0-10 years, with localization areas containing ~190k early-type galaxies on average and a ranking method that excludes roughly half the candidates when galaxy properties are available.
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Probing Kinematic Anisotropies in the Stochastic Gravitational Wave Background with the SKA
SKAO forecasts show that planned observations will improve SGWB anisotropy constraints but remain insufficient to detect the kinematic dipole even in joint PTA-astrometry analyses.
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Massive black holes and their galaxies
A review summarizing detection methods, population statistics, and coevolution of supermassive black holes with host galaxies from early universe observations and simulations.