\begin{document}$ H_0 $\end{document} data from SH0ES. For the νAxi-EDE model, we obtain \begin{document}$\sum m_{\nu,\mathrm{NH}}$\end{document} < 0.152 eV and \begin{document}$\sum m_{\nu,\mathrm{IH}}$\end{document} < 0.178 eV, whereas for the νAdS-EDE model, we find \begin{document}$\sum m_{\nu,\mathrm{NH}}$\end{document} < 0.135 eV and \begin{document}$\sum m_{\nu,\mathrm{IH}} $\end{document} < 0.167 eV. Our results exhibit a preference for NH in both the νAxi-EDE and νAdS-EDE models."> Cosmological constraints on neutrino mass within consistent cosmological models -
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