A New Perspective on Dark Matter and Cosmic Inflation

The Big Bang is a cosmic event in which the collision and subsequent explosion of masses and particles give rise to an enormous cloud that expands far from the central point. This vast cloud eventually forms nebulae, which act as the cradle for future stars.

Following the end of cosmic inflation, particles begin to cluster together due to gravitational and magnetic forces. Over time, these clusters grow into larger celestial bodies such as moons, planets, and stars.

During the early inflationary phase, when the universe primarily consisted of gas and tiny particles, each particle remained suspended in space, unaffected by any dominant gravitational pull. Inflation involved both linear and rotational motion, yet no central force influenced these particles. Gradually, as they drifted in the vast expanse, they began merging to form larger astronomical structures.

In galactic systems containing a central black hole, this black hole exerts a gravitational pull on free-floating particles that are otherwise unaffected by external forces. With minimal effort, the black hole captures and holds these particles—including stars, planets, and moons—within its orbit, shaping the structure of the galaxy.

So if we consider the particles existing in the universe during the inflationary period, these are the same objects that later form stars or moons. In fact, one could argue that dark matter originates from particles that remained suspended in space during the inflationary period.