The question "how can the Universe be larger than its age in light-years?" arises from a common confusion between the age of the Universe expressed in light-years (which corresponds to a distance traveled by light in a certain time) and the actual size or observable extent of the Universe, which is much larger.
The current age of the Universe is estimated to be about 13.8 billion years. One might intuitively think that nothing could have traveled farther than 13.8 billion light-years since the light travels at a finite speed and nothing can exceed it (according to special relativity). But this intuition does not take into account the Expansion of Space.
The Universe is not a static space in which galaxies simply move like projectiles. It is space itself that expands over time, according to general relativity. This phenomenon is modeled by the Friedmann–Lemaître–Robertson–Walker (FLRW) equations.
Due to this expansion, the light we receive today, which has traveled for 13.8 billion years, comes from objects that are now much farther away than 13.8 billion light-years.
Calculations based on cosmological models give a radius of the observable Universe of about 46.5 billion light-years, or a diameter of 93 billion light-years. This does not mean that light has traveled faster than c, but rather that the fabric of space on which it moves has stretched during its journey.
Alice and Bob start from a point on the balloon, each walking at 1 km/h in opposite directions. The balloon stretches as they walk. After 1 hour, normally, they should be 2 km apart. But if the balloon has doubled in size during this time, they will actually be 4 km apart! Yet, neither has exceeded the speed of 1 km/h relative to the surface of the balloon.
Concrete example: A galaxy located 1 million light-years away 13.8 billion years ago is today about 1.1 billion light-years away!
\[ds^2 = -c^2 \, dt^2 + a(t)^2 \left[ \frac{dr^2}{1 - k r^2} + r^2 \, d\Omega^2 \right]\]
The proper distance at a given moment is then: \(D(t) = a(t) \cdot r\)
At the present moment \( t_0 \), we conventionally set \( a(t_0) = 1 \). The comoving radial coordinate of the cosmological horizon (limit of the observable Universe) is approximately:
\[ r \approx 14.4 \, \text{Gpc} = 14.4 \times 10^9 \, \text{pc} \]
We can then calculate the current proper distance:
\[ D(t_0) = a(t_0) \cdot r = 1 \times 14.4 \, \text{Gpc} = 14.4 \, \text{Gpc} \]
This corresponds to approximately \( 46.5 \) billion light-years (since \( 1 \, \text{Gpc} \approx 3.26 \) billion light-years).
Thus, although the Universe is only \( 13.8 \) billion years old, the size of the observable Universe is approximately:
\[ D(t_0) \approx 46.5 \, \text{billion light-years} \]
Special relativity forbids an object from moving through space faster than light. But the expansion of space is not a movement through space; it is the evolution of the very fabric of spacetime. This expansion can "separate" two galaxies at an apparent speed greater than c, without contradicting relativistic principles.