Patchy Kinetic Sunyaev-Zel'dovich Effect with Controlled Reionization History and Morphology
arXiv:2203.04337 · doi:10.3847/1538-4357/ac8481
Abstract
Using the novel semi-numerical code for reionization AMBER, we model the patchy kinetic Sunyaev-Zel'dovich (kSZ) effect by directly specifying the reionization history with the redshift midpoint , duration , and asymmetry . We further control the ionizing sources and radiation through the minimum halo mass and the radiation mean free path . AMBER reproduces the free electron number density and the patchy kSZ power spectrum of radiation-hydrodynamic simulations at the target resolution () with matched reionization parameters. With a suite of simulations using AMBER, we first constrain the redshift midpoint using the Planck2018 Thomson optical depth result (95\% CL). Then, assuming , we find that the amplitude of scales linearly with the duration of reionization , and is consistent with the upper limit from the South Pole Telescope (SPT) results up to ( encloses to ionization). Moreover, a shorter can lead to a lower and a flatter slope in the scaling relation, thereby affecting the constraints on at . Allowing and to vary simultaneously, we get spectra consistent with the SPT result ( CL) up to (but is needed to ensure an end of reionization before ). We show that constraints on the asymmetry require measurement accuracy at multipoles other than . Finally, we find that the amplitude and shape of the kSZ spectrum are only weakly sensitive to under a fixed reionization history and radiation mean-free path.
20 pages, 17 Figures; comments welcome