A Dynamical Equilibrium Linking Nanohertz Stochastic Gravitational Wave Background to Cosmic Structure Formation
Manjia Liang, Peng Xu, Ruijun Shi, Zhoujian Cao, Ziren Luo, Minghui Du, Qiong Deng, Bo Liang, Jiaxiang Liang

TL;DR
This paper proposes a new dynamical framework linking the nanohertz gravitational wave background to cosmic structure formation, supported by data fitting and theoretical modeling within general relativity.
Contribution
It introduces a coupled non-equilibrium system model of SGWB and matter, deriving a spectrum with a cutoff and scale-dependent coupling, connecting gravitational waves to cosmic structure.
Findings
Fitted the model to NANOGrav data with a high Bayes factor.
Identified a screening mass scale overlapping with cosmic structure transition mass.
Predicted scale-dependent effects testable by future surveys.
Abstract
The stochastic gravitational wave background (SGWB) is conventionally treated as a passive relic of its astrophysical and cosmological sources, with negligible back-reaction on the matter content of the Universe. Here we show that this assumption needs to be modified once the SGWB and matter are treated as a dynamically coupled non-equilibrium system. Combining linearized general relativity with the fluctuation-dissipation theorem, we derive a generalized Langevin framework that drives the coupled system toward a dynamical equilibrium, which is characterized by a distinctive strain spectrum with a high-frequency cutoff , and a scale-dependent coupling parameter that screens gravity progressively for the most massive structures. Three findings support this framework. Fitting the equilibrium spectrum to the NANOGrav 15-year dataset yields a Bayes factor of over…
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