Multifield quintessential inflation and Swampland constraints in the IDM
We investigate quintessential inflation in the Inert Doublet Model coupled to a light quintessence field through an exponential interaction. In the Einstein frame, the model forms a noncanonical two-field system with a curved field-space geometry and a Starobinsky-like inflationary plateau. We solve the covariant background and perturbation equations and perform a parameter scan of the exponential slope and the number of inflationary e-folds. The scalar amplitude fixes the inflationary normalization independently at each scan point, rather than selecting a particular value of the quintessence coupling. We find that cumulative entropy-to-curvature transfer significantly modifies the scalar spectrum, while the tensor-to-scalar ratio remains compatible with current CMB limits. The scalar spectral index provides the strongest sensitivity to the exponential coupling. Covariant Swampland diagnostics nevertheless reveal a persistent tension with a strong order-unity de Sitter bound.