We investigate the validity of cosmological models with an oscillating scale
factor in relation to late-time cosmological observations. We show that these
models not only meet the required late time observational constraints but can
also alleviate the Hubble tension. As a generic feature of the model, the
Hubble parameter increases near the current epoch due to its cyclical nature
exhibiting the phantom nature allowing to address the said issue related to
late time acceleration.
