Albert Einstein's theory of relativity, which includes the famous equation E=mc^2, was not developed with the intention of getting as far away from Newton's theory of gravity and force as possible. Einstein's theories were formulated as a result of his deep curiosity and quest for understanding the fundamental nature of space, time, and the behavior of objects in the universe.
Einstein's theory of general relativity, which introduced the concept of "curved" space, was an attempt to provide a more comprehensive understanding of gravity. In this theory, he proposed that the presence of mass and energy curves the fabric of spacetime, and objects move along the curves created by this curvature. This was a departure from Newton's concept of gravity as a force acting at a distance.
Regarding time dilation, Einstein's theory of special relativity, published in 1905, introduced the concept that time can appear to pass at different rates for observers in relative motion. This theory revolutionized our understanding of space, time, and motion and was not primarily aimed at rejecting Newton's ideas but rather at reconciling the discrepancies between classical physics and the observed behavior of light.
It is important to note that Einstein's work built upon and expanded existing scientific knowledge, including Newtonian physics. Newton's laws of motion and universal gravitation are still valid and highly accurate within their applicable domains, which typically include everyday situations on Earth. Einstein's theories are more comprehensive and accurate in extreme conditions involving high speeds, strong gravitational fields, and situations on cosmological scales.
In summary, while Einstein's theories represent significant advancements in our understanding of the universe, they were not developed with the sole purpose of distancing themselves from Newton's theories. Instead, they emerged from Einstein's deep exploration of the fundamental nature of space, time, and the behavior of matter and energy.