  We investigate a new possible solution to the Hubble constant tension. we
propose a simple resolution to the problem assuming that a first-order phase
transition related to H0 transition occurred in the early Universe. The early
evolution of the Universe is a result of hybrid inflation that has lasted for a
specific period until symmetry breaking takes place. Fitting our model to
measurements from Planck and SH0ES data provides a key explanation of
discrepancies of H0 measurements. The quantum fluctuations calculated in this
model have significant results on the reheating parameters Nre and Tre.
Therefore, new constraints must be taken into consideration to fit these
parameters to recent results.
