collaborators

6 papers

astro-ph.CO2026

Revisiting the Chern-Simons interaction during inflation with a non-canonical pseudo-scalar

Jun'ya Kume, Marco Peloso, Nicola Bartolo

A Chern-Simons interaction between a pseudo-scalar field and a U(1) gauge field results in the generation of a chiral gravitational wave background. The detection of this signal is…

hep-ph2025

On the inefficiency of fermion level-crossing under the parity-violating spin-2 gravitational field

Kohei Kamada, Jun'ya Kume

Gravitational chiral anomaly connects the topological charge of spacetime and the chirality of fermions. It has been known that the chirality is carried by the particles (or the ex…

gr-qc2025

Assessing the Impact of Unequal Noises and Foreground Modeling on SGWB Reconstruction with LISA

Jun'ya Kume, Marco Peloso, Mauro Pieroni +1

In the search for stochastic gravitational wave backgrounds (SGWB) of cosmological origin with LISA, it is crucial to account for realistic complications in the noise and astrophys…

astro-ph.CO2025

Reconstructing Primordial Curvature Perturbations via Scalar-Induced Gravitational Waves with LISA

Jonas El Gammal, Aya Ghaleb, Gabriele Franciolini +17

Many early universe scenarios predict an enhancement of scalar perturbations at scales currently unconstrained by cosmological probes. These perturbations source gravitational wave…

gr-qc2025

Gravitational effects on fluid dynamics in cosmological first-order phase transitions

Ryusuke Jinno, Jun'ya Kume

Cosmological first-order phase transition (FOPT) sources the stochastic gravitational wave background (SWGB) through bubble collisions, sound waves, and turbulence. So far, most st…

astro-ph.CO2025

Revised bounds on local cosmic strings from NANOGrav observations

Jun'ya Kume, Mark Hindmarsh

In a recent paper, the NANOGrav collaboration studied new physics explanations of the observed pulsar timing residuals consistent with a stochastic gravitational wave background (S…