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20242026
most citedSTOLAS: STOchastic LAttice Simulation of cosmic inflation

19 citations · 25 across the 8 of their papers we have counts for

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7 papers · 1 filter

astro-ph.CO2026

QCD Crossover Transfer Functions for Scalar-Induced Gravitational Waves in the PTA Band

Gabriele Franciolini, Xavier Pritchard, Yuichiro Tada

Pulsar timing array (PTA) collaborations have reported evidence for a stochastic gravitational wave (GW) background in the nHz band. Should scalar-induced GWs, sourced at second or…

astro-ph.CO2026

Constant-Roll Inflation: Analytical Formulae for Power Spectrum and Implications for Induced Gravitational Waves

Hayato Motohashi, Shi Pi, Yuichiro Tada +1

Constant-roll inflation provides a simple and analytically tractable framework for describing transient departures from slow roll, including non-attractor phases that can enhance t…

astro-ph.CO2026

Domain-wall Quintessence

Nobufusa Kobayashi, Yuichiro Tada, Fuminobu Takahashi +1

We investigate a dark energy model driven by a planar domain-wall-like structure with a thickness comparable to, or larger than, the current Hubble radius, focusing on its intrinsi…

astro-ph.CO2026

STOchastic LAttice Simulation of hybrid inflation

Tomoaki Murata, Yuichiro Tada

We investigate the spatial profile of the curvature perturbation generated in multi-waterfall hybrid inflation models, which are known to produce various topological defects. Using…

astro-ph.CO2025★ 2 cited

Stochastic-tail of the curvature perturbation in hybrid inflation

Tomoaki Murata, Yuichiro Tada

The exponential-tail behaviours of the probability density function (PDF) of the primordial curvature perturbation are confirmed in the mild-waterfall variants of hybrid inflation…

astro-ph.CO2025★ 4 cited

Dip and non-linearity in the curvature perturbation from inflation with a transient non-slow-roll stage

Tomohiro Fujita, Ryodai Kawaguchi, Misao Sasaki +1

We consider models of inflation that contain a transient non-slow-roll stage and investigate the conditions under which a dip appears in the power spectrum of the curvature perturb…