Diffuse cosmic-ray (left) and neutrino (right) spectra from a population of jetted TDEs obtained for an injection of 70% Si and 30% Fe, with spectral index α = 1.5, ξ_CRf_s = 2.6 × 10⁻³ and source evolution derived in this work, with maximum bolometric luminosity in the population L_max = 6.8 × 10⁴⁶ erg s⁻¹ (in the medium state). Left: total spectrum (black) and its composition. We superimposed data from the Auger experiment (black dots, The Pierre Auger Collaboration 2015) and from the Telescope Array experiment (gray dots, Fukushima 2015) for which only statistical uncertainties are shown. Right: diffuse neutrino flux for three flavors (black), the diffuse neutrino flux measured by the IceCube experiment (IceCube Collaboration 2017), and the projected limits for GRAND (GRAND Collaboration 2020), ARA/ARIANNA (Allison et al. 2015; Barwick et al. 2015), and POEMMA (Neronov et al. 2017).