Looking at the NANOGrav Signal Through the Anthropic Window of Axion-Like Particles
Alexander S. Sakharov, Yury N. Eroshenko, Sergey G. Rubin

TL;DR
This paper investigates how axion-like particles formed during inflation could produce gravitational wave signals matching the NANOGrav observations, revealing new links between early universe physics and gravitational wave data.
Contribution
It introduces a novel model connecting ALP domain walls from inflation to the NANOGrav gravitational wave excess, analyzing their spectrum and potential observable effects.
Findings
The characteristic strain spectrum matches the NANOGrav signal slope.
Parameter combinations can produce signals saturating the NANOGrav excess.
Closed domain walls may form wormholes affecting gravitational wave background.
Abstract
We explore the inflationary dynamics leading to formation of closed domain walls in course of evolution of an axion like particle (ALP) field whose Peccei-Quinn-like phase transition occurred well before inflationary epoch. Evolving after inflation, the domain walls may leave their imprint in stochastic gravitational waves background, in the frequency range accessible for the pulsar timing array measurements. We derive the characteristic strain power spectrum produced by the distribution of the closed domain walls and relate it with the recently reported NANOGrav signal excess. We found that the slope of the frequency dependence of the characteristic strain spectrum generated by the domain walls is very well centered inside the range of the slopes in the signal reported by the NANOGrav. Analyzing the inflationary dynamics of the ALP field, in consistency with the isocurvature…
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