arXiv · 2507.07665
Whispers from the Early Universe: The Ringdown of Primordial Black Holes
Abstract
We investigate the stochastic gravitational wave background (SGWB) generated by the ringdown phase of primordial black holes (PBHs) formed in the early universe. As the ringdown signal is independent of the PBH formation mechanism, the resulting SGWB offers a model-independent probe of PBHs. We numerically compute the ringdown waveform and derive the corresponding SGWB. We show that such a signal could be detected by future pulsar timing arrays (PTAs) for PBHs heavier than the solar mass. Additionally, we evaluate the SGWB from binary PBH mergers and demonstrate that it lies within the sensitivity bands of next-generation ground-based interferometers such as Cosmic Explorer and Einstein Telescope, suggesting a multi-band observational strategy for probing the PBH dark matter scenario.
Explore related subjects
Keep this discovery
Chen Yuan, Zhen Zhong, Qing-Guo Huang. 2025-07-10. Whispers from the Early Universe: The Ringdown of Primordial Black Holes. https://arxiv.org/abs/2507.07665
Cite the original work for its findings. Save a collection to share your selection of sources.