Abstract:
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.
