  The James Webb Space Telescope (JWST) has made startling discoveries
regarding the early universe. It has revealed galaxies as soon as 300 million
years after the Big Bang, challenging current galaxy formation models.
Additionally, it has identified massive, bright galaxies in the young universe,
contradicting the standard {\Lambda}CDM model's age estimate of 13.8 Gyr. This
prompts a reevaluation of galaxy formation and cosmological models. There is a
strong tension between JWST high-redshift galaxy observations and Planck Cosmic
Microwave Background (CMB) satellite measurements. Even alternative
cosmological models, including those incorporating dark matter baryon
interaction, f(R) gravity, and dynamical dark have failed to resolve this
tension. One possible solution is that the Universe's age exceeds predictions
by the {\Lambda}CDM model. The study challenges this by introducing a method
based on blue straggler stars (BSs) within GCs, comparing ages with other
models. The ages obtained are compared with those of different models to
certify that they are equally valid. These values are comparable within the
error ranges except for the clusters: NGC104, NGC 5634, IC 4499, NGC 6273 and
NGC 4833, finding their respective ages to be between 14.7 and 21.6 Gyr,
surpassing the commonly accepted age of the Universe. These results inferred an
age for the Universe of around 26 Gyr, close to 26.7 Gyr. This value aligns
with that suggested by the cosmological model named Covarying Coupling
Constants + TL (CCC+TL). Such a value is consistent with early universe
observations from the James Webb Space Telescope (JWST). The results of the
present paper reinforce the advocating for a critical review of models
encompassing dark mass, dark energy, and the dynamics of the Universe,
particularly in explaining the presence of primitive massive galaxies, very old
GCs, and very old and poor metallic stars.
