  Current observations do not rule out the possibility that the Universe might
end up in an abrupt event. Different such scenarios may be explored through
suitable parameterizations of the dark energy and then confronted to
cosmological background data. Here we parameterize a pseudorip scenario using a
particular sigmoid function and carry an in-depth multifaceted examination of
its evolutionary features and statistical performance. This depiction of a non
violent final fate of our cosmos seems to be arguably statistically favoured
over the consensus {\Lambda}CDM model according to some Bayesian
discriminators.
