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Staticboson said:But isn't the notion of expansion the result of physical measurements?
The problem here is that in GR the laws of physics can be expressed in coordinate independent way. Let's take the solar system for example.
If you are navigating by the stars, then your navigational charts are by necessity drawn for the Earth's frame of reference. This involves complicated annual motions of the planets. And, the motions of the moons of Jupiter relative to Earth are even more complicated.
If, however, you describe the solar system from the Sun's frame of reference, then everything simplifies. The planets move in ellipses about the Sun and the moons orbit their planets likewise.
Moreover, if you use Newton's law of gravitation, then you can explain the heliocentric solar system. It's tempting, therefore, to say that the solar system really is heliocentric in some absolute sense. However:
In GR, you can describe the solar system similarly in terms of the Schwarzschild coordinates for the spacetime geometry about a spherical star, like the Sun. But, in GR it is clear that your choice of Schwarzschild coordinates is arbitrary. The same spacetime geometry can be described in any other coordinate system and no system has absolute preference. If you wrote down what you know about the solar system, I'd bet most of those statements turn out to be coordinate dependent. E.g. that "the Earth spins on its axis" is a coordinate dependent statement.
In terms of Cosmology you have the same issue. Almost anything you want to say to describe the universe is coordinate dependent. Even the age of the universe is taken to mean in a reference frame where the CMB radiation is isotropic.
Likewise, that the universe is "expanding" is coordinate dependent. First, however, you would have to define "expanding" - which, in any case, is probably impossible in a coordinate independent way. If we go back to the solar system, we can decide that the heliocentric model is sufficiently useful that by convention we'll use it without excessive explanation each time. We might even call it the standard model of the solar system.
The expanding universe in the FLRW model is also sufficiently useful that Cosmologists will use it without unduly emphasising that it is, after all, only one of infinitely many coordinate-dependent descriptions of the universe. And, indeed, this has become something of the de facto standard model.
But, being the standard model is not the same as being absolutely real in some sense.