S-dual quintessence, the Swampland, and the DESI DR2 results

We propose a dark energy model in which a quintessence field ϕ rolls near the vicinity of a local maximum of its potential characterized by the simplest S self-dual form $V\left(\varphi \right)=\Lambda \mathrm{sech}(\sqrt{2}\varphi /M_p)$, where $M_p$ is the reduced Planck mass and $\Lambda \sim {10}^{-120}{M}_p^4$ is the cosmological constant. We confront the model with Swampland ideas and show that the S-dual potential is consistent with the distance conjecture, the de Sitter conjecture, and the trans-Planckian censorship conjecture. We also examine the compatibility of this phenomenological model with the intriguing DESI DR2 results and show that the shape of the S-dual potential is almost indistinguishable from the axion-like potential, $V\left(\varphi \right)=m_a^2{f}_a^2[1+\cos (\varphi /f_a\left)\right]$, with $m_a$ and $f_a$ parameters fitted by the DESI Collaboration to accommodate the DR2 data. The self-dual potential has the advantage that one starts at the self-dual point and this is a theoretical motivation, because as the universe cools off the $Z_2$ symmetry gets broken leading to a natural rolling away from the symmetric point.