Audible curvaton: modulated phase transition as the origin of large-scale curvature perturbations and gravitational wave anisotropies
Abstract
We propose a post-inflationary first-order phase transition modulated by a light spectator field as the origin of primordial large-scale curvature perturbations. Spectator fluctuations acquired during inflation modulate the bubble nucleation history, generating curvature perturbations together with correlated intrinsic gravitational-wave (GW) anisotropies. We show that this mechanism can reproduce the observed amplitude of curvature perturbations while producing a loud stochastic GW background in the frequency bands of space-based detectors such as LISA, Taiji, and TianQin. A concrete benchmark yields strongly enhanced intrinsic GW anisotropies and a local primordial non-Gaussianity signal within reach of future large-scale-structure surveys.
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BibTeX
@misc{ai2026audible,
title = {{Audible curvaton: modulated phase transition as the origin of large-scale curvature perturbations and gravitational wave anisotropies}},
author = {Wen-Yuan Ai and Gabriele Franciolini and Xin Wang and Xiang-Xi Zeng},
howpublished = {arXiv},
year = {2026},
month = oct,
doi = {10.48550/arxiv.2610.18975},
eprint = {2610.18975},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2610.18975},
}
RIS
TY - UNPB
TI - Audible curvaton: modulated phase transition as the origin of large-scale curvature perturbations and gravitational wave anisotropies
AU - Wen-Yuan Ai
AU - Gabriele Franciolini
AU - Xin Wang
AU - Xiang-Xi Zeng
PY - 2026
DA - 2026/10/13
PB - arXiv
DO - 10.48550/arxiv.2610.18975
UR - https://arxiv.org/abs/2610.18975
AB - We propose a post-inflationary first-order phase transition modulated by a light spectator field as the origin of primordial large-scale curvature perturbations. Spectator fluctuations acquired during inflation modulate the bubble nucleation history, generating curvature perturbations together with correlated intrinsic gravitational-wave (GW) anisotropies. We show that this mechanism can reproduce the observed amplitude of curvature perturbations while producing a loud stochastic GW background in the frequency bands of space-based detectors such as LISA, Taiji, and TianQin. A concrete benchmark yields strongly enhanced intrinsic GW anisotropies and a local primordial non-Gaussianity signal within reach of future large-scale-structure surveys.
ER -