NANOGrav spectral index $\gamma =3$ from melting domain walls

Abstract

We discuss cosmic domain walls described by a tension red-shifting with the expansion of the Universe. These melting domain walls emit gravitational waves with the low-frequency spectral shape ${\Omega }_{gw}\propto f^2$ corresponding to the spectral index $\gamma =3$ favoured by the recent NANOGrav 15 yrs data. We discuss a concrete high-energy physics scenario leading to such a melting domain wall network in the early Universe. This scenario involves a feebly coupled scalar field, which can serve as a promising dark matter candidate. We identify parameters of the model matching the gravitational wave characteristics observed in the NANOGrav data. The dark matter mass is pushed to the ultra-light range below $10^{-11}-10^{-12}\text{eV}$ which is accessible through planned observations thanks to the effects of superradiance of rotating black holes.

7 revtex pages, 1 figure; added references and appendix with the calculation of gravitational wave spectrum; matches version accepted in PRD

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