Implications of gravitational-wave production from dark photon resonance to pulsar-timing observations and effective number of relativistic species
Ryo Namba, Motoo Suzuki
Abstract
The coherent oscillation of axionic fields naturally drives copious production of dark photon particles in the early Universe, due to resonance and tachyonic enhancement. During the process, energy is abruptly transferred from the former to the latter, sourcing gravitational-wave generation. The resulting gravitational waves are eventually observed today as stochastic background. We report analytical results of this production and connect them to the recent pulsar-timing results from the NANOGrav Collaboration. We show an available parameter space for our mechanism to account for the signal around the mass ${m}_{\ensuremath{\phi}}\ensuremath{\sim}{10}^{\ensuremath{-}13}\text{ }\text{ }\mathrm{eV}$ and the decay constant ${f}_{\ensuremath{\phi}}\ensuremath{\sim}{10}^{16}\text{ }\text{ }\mathrm{GeV}$, with a dimensionless coupling of $\mathcal{O}(1)$. A mechanism to keep the axion from dominating the Universe is a necessary ingredient of this model, and we discuss a possibility to recover a symmetry and render the axion massless after the production. We also comment on potential implications of the required effective number of relativistic species for the determination of the present Hubble constant.