  In this work, we discuss the de Sitter swampland conjectures in the context
of the generalized Chaplygin-inspired inflationary model. We demonstrate that
these conjectures can be satisfied, but only in the region of the parameter
space far away from the General Relativity limit. The cosmic microwave
background data had already been found to restrict the allowed inflationary
potentials of this model. Our results impose a further limitation on the
possible potentials.
