Pulsars hold a unique significance in astronomy, and studying their life cycle evolution offers a window into understanding the broader dynamics of their surrounding environments. This essay delves into the evolution of pulsars by analyzing data from 299 pulsar samples, which include recorded parameters such as period, period derivative, characteristic age, luminosity, spin-down energy loss rate, and surface magnetic flux density. Through plotting graphs of these parameters against each other, the essay aims to uncover the relationships between them and compare the findings with established theories. The results of the analysis reveal a consistent pattern in pulsar evolution. As pulsars evolve, both their period and period derivative decrease. This reduction in period and period derivative consequently leads to a decline in both magnetic flux density and spin-down energy loss rate. Notably, these two parameters exhibit an exponential decrease over the characteristic age of the pulsar. This study sheds light on the dynamic evolution of pulsars and emphasises the interconnection of various parameters that shape their evolutionary trajectories. By understanding the evolution of pulsars, we can gain valuable insights into the broader processes at work in their surrounding environments.