The early universe was remarkably smooth. In a universe governed by gravity, that smooth beginning represents an unusually ordered state from which stars, galaxies, and usable energy could later develop.
Why did the universe begin in such an unusually ordered state?
The early universe was hot and filled with matter and radiation, but it was also remarkably smooth. Matter was spread almost evenly through space.
That may sound like disorder. When gravity is important, however, a smooth distribution of matter represents a special low-entropy condition. Gravity later caused matter to gather into stars, galaxies, and eventually black holes.
Entropy is often described as a measure of disorder, although the scientific concept is more precise than that simple description. Physical systems tend to move toward states of higher entropy.
The early universe presents an important puzzle because the universe had to begin far from its eventual maximum-entropy state. Its smooth distribution of matter provided enormous opportunity for later change as gravity formed increasingly complex structures.
A low-entropy beginning helps explain why useful energy differences exist at all. Stars can shine, planets can receive energy, and physical processes can occur because the universe did not begin in complete equilibrium.
The early universe was extremely smooth compared with the clumpy universe of stars, galaxies, and black holes that developed later. In gravitational systems, this corresponds to low gravitational entropy.
The total entropy of the universe has increased with time.
Cosmologists have proposed several ways of understanding the special early state, including inflationary models and broader ideas about the initial conditions of the cosmos.
There is no generally accepted final explanation for why the universe began with the particular low-entropy conditions needed for the thermodynamic history we observe.
The early universe was highly uniform. For a gravitating system, this smooth state corresponds to low gravitational entropy. Cosmic entropy has increased as structure has formed.
The low-entropy beginning is relevant to design because it concerns not simply the laws of physics but the starting condition of the universe. A law can describe how a system changes without necessarily explaining why the system began in a very special state.
The low initial entropy of the universe is a genuine foundational question in cosmology. We should avoid attaching a dramatic probability to that state unless the assumptions behind such a calculation are made clear.