Can a secluded self-interacting dark sector generate detectable gravitational waves?

Can a secluded self-interacting dark sector generate detectable gravitational waves?
Song Li, Jin Min Yang, Mengchao Zhang, Yang Zhang, Rui Zhu
arXiv:2502.04108v3 Announce Type: replace-cross
Abstract: In this work we study the possibility to detect the gravitational waves generated by a secluded self-interacting dark sector. “Secluded” means that the dark sector has almost no portal to the visible sector and thus its entropy is conserved by itself, and “self-interacting” means that dark matter in this model has a significant interaction to itself, making it consistent with the small-scale structure observations. A spontaneously broken $U(1)’$ is introduced for the interactions in the dark sector, and nearly massless dark radiation is also introduced to avoid the over-closure problem. Through a parameter space scan, we find that this model is highly constrained by the currently observed effective number of neutrinos ($N_{text{eff}}$) and the large-scale structure observable Lyman-$alpha$. Together, these two constraints exclude a large parameter space that is favored by future gravitational-wave detectors, but there is still a small portion of the model parameter space that can be detected by SKA.arXiv:2502.04108v3 Announce Type: replace-cross
Abstract: In this work we study the possibility to detect the gravitational waves generated by a secluded self-interacting dark sector. “Secluded” means that the dark sector has almost no portal to the visible sector and thus its entropy is conserved by itself, and “self-interacting” means that dark matter in this model has a significant interaction to itself, making it consistent with the small-scale structure observations. A spontaneously broken $U(1)’$ is introduced for the interactions in the dark sector, and nearly massless dark radiation is also introduced to avoid the over-closure problem. Through a parameter space scan, we find that this model is highly constrained by the currently observed effective number of neutrinos ($N_{text{eff}}$) and the large-scale structure observable Lyman-$alpha$. Together, these two constraints exclude a large parameter space that is favored by future gravitational-wave detectors, but there is still a small portion of the model parameter space that can be detected by SKA.