The Problem of Measurement:
* No Absolute Frame of Reference: We don't have a fixed, external point from which to measure the universe's rotation. All measurements are relative to our own frame of reference (Earth, Milky Way, etc.).
* Cosmic Microwave Background (CMB): The CMB is the faint afterglow of the Big Bang. It shows tiny temperature fluctuations that *could* be interpreted as evidence of rotation, but the signal is extremely weak and disputed.
Arguments for Zero Angular Momentum:
* The Big Bang Model: The prevailing model suggests the universe began in a very hot, dense state with a near-uniform distribution of matter. This makes it statistically improbable that the universe started with a significant net angular momentum.
* Conservation of Angular Momentum: A fundamental principle in physics states that the total angular momentum of a closed system remains constant. If the universe began with negligible angular momentum, it should still be close to zero today.
Arguments for Non-Zero Angular Momentum:
* The CMB Anisotropy: While the CMB is incredibly uniform, there are tiny temperature fluctuations. Some physicists argue these fluctuations could be caused by a slight rotation of the universe.
* Large-Scale Structure: The distribution of galaxies and other cosmic structures isn't perfectly uniform. Some argue this suggests the universe may have a slight, non-uniform rotation.
In Conclusion:
The question of the universe's total angular velocity remains an active area of research. While the evidence points toward a near-zero angular momentum, the lack of a definitive frame of reference and the complexity of cosmic observations make it difficult to definitively conclude.
It's important to note: Even if the universe has a tiny, non-zero angular momentum, it wouldn't be noticeable on local scales. We wouldn't feel any "spinning" effect.