activity
20242026
collaborators

7 papers

astro-ph.CO2026

Adding electromagnetic birefringence to pulsar timing and astrometry to detect gravitational waves

Keisuke Inomata, Marc Kamionkowski

It was recently shown that the time variation of the polarization of electromagnetic waves from pulsars can be used, in cross-correlation with pulsar timing, to probe the chirality…

astro-ph.CO2026

Note on pulsar timing array correlation functions induced by peculiar velocities

Neha Anil Kumar, Keisuke Inomata, Marc Kamionkowski

Several papers have recently calculated the contribution to pulsar timing array overlap reduction functions (ORFs) induced by our peculiar velocity with respect to the rest frame o…

astro-ph.CO2025

Gravitational Waves from Particles Produced from Bubble Collisions in First-Order Phase Transitions

Keisuke Inomata, Marc Kamionkowski, Kentaro Kasai +1

We discuss a new source of gravitational waves (GWs) from first-order phase transitions. The collisions of bubbles of the new phase can efficiently produce particles that couple to…

astro-ph.CO2025

Constraints on the Sharpness of the Curvature Power Spectrum

Keisuke Inomata, Xuheng Luo

Motivated by the fact that a sharply peaked curvature spectrum is often considered in the literature, we examine theoretical constraints on the sharpness of such a spectrum. In par…

astro-ph.CO2025

Parity-breaking galaxy 4-point function from lensing by chiral gravitational waves

Keisuke Inomata, Leah Jenks, Marc Kamionkowski

Recent searches for parity breaking in the galaxy four-point correlation function, as well as the prospects for greatly improved sensitivity to parity breaking in forthcoming surve…

astro-ph.CO2024

Inflationary Butterfly Effect: Non-perturbative Dynamics From Small-Scale Features

Angelo Caravano, Keisuke Inomata, Sébastien Renaux-Petel

For the first time, we investigate the non-perturbative dynamics of single field inflation with a departure from slow-roll. Using simulations, we find that oscillatory features in…