rasp said:
What is the working explanation for the expansion of cosmological space? Surely, it can not be as simple as "distance increases between objects when they move away from each other"?
The common literature speaks about the "stretching of space". This seems to imply a metric for space that is changing, and it's why I thought there had to be a relativistic effect to explain the change, i.e. every interval of space stretches from some measure to some new measure.
Fundamentally GR does not deal with a metric on space, but a metric on spacetime, which gives some notion of the "length" of arbitrary paths in spacetime, like the time along the timelike worldlines of actual objects, or the distance along spacelike paths (which cannot represent the path of any actual object because they'd represent an object moving faster than light in a local sense--each point on a spacelike path would lie outside the future
light cone of other nearby points on the path). The
Einstein field equations describe the relationship between the metric of spacetime and the distribution of matter and energy--how matter/energy curve spacetime. The field equations just describe the local relationship, so what physicists in GR look for are entire global "solutions" that satisfy the field equations everywhere.
In the case of cosmology, the simplest solutions for a universe filled with matter are different cases of the
Friedmann–Lemaître–Robertson–Walker metric (FLRW metric for short). Again, these are entire 4D curved spacetimes, not descriptions of space expanding over time. But 4D curved spacetime can be sliced up into a series of 3D sections, something known as a "foliation". It's hard to visualize slicing up a 4D surface, but we can drop the number of spatial dimensions from 3 to 1 and then visualize a curved spacetime surface as a curved 2D surface where one dimension is space and one is time. Then the spacetime corresponding to an "expanding universe" could be something like the surface of a cone or an American football, and the foliation could consist of slicing it into circular cross-sections, with each cross-section further from the tip being larger than cross-sections closer to the tip (in the case of a football, the largest cross-section would be at the center and then cross-sections closer to the tip on the other side would get smaller again, analogous to a universe that expands from a Big Bang, reaches a maximum size, and shrinks again until it collapses in a Big Crunch, which is what you get if you plug a sufficiently high matter density into the FLRW metric). One point to realize is that for a given curved spacetime surface, the foliation is not unique--just as you can slice a cone into cross sections at different angles to get different-looking
conic sections, so you can slice a 4D spacetime into a series of 3D cross-sections at different "angles" too and get different-looking spatial slices. So, in a given spacetime there is no unique truth about how space is changing over time, it depends on how you define "simultaneity" (which events at different points are defined to have happened at the same time-coordinate).
But with the FLRW spacetimes, there is a particularly simple type of foliation that cosmologists tend to use, one in which the 3D slices are what's called "hypersurfaces of homogeneity"--the 3D slices are chosen such that the matter in each slice is distributed in a perfectly uniform way, with a uniform density at every point. With such a foliation the distance between an arbitrary pair of particles of matter does continually increase over time (I believe you could define this distance in any given 3D slice in terms the shortest spacelike path between particles that is confined to that slice), and the local density of matter continually decreases. So, this is basically where the notion of the "expansion of space" comes from. But this idea isn't really fundamental, what's fundamental is that these are curved 4D spacetime solutions which satisfy the Einstein field equations at every point. For some criticisms of the whole language of "expanding space", see
this paper which was discussed on
this thread, along with
this paper as well.
rasp said:
Does the changing speed of light in a cosmological setting imply changes to a basic metric of space and time? Or is the changing speed of light fully explained by identifying the geodesic path that light takes through a gravitationally induced curved spacetime?
Again, GR only says that light moves at c in a local sense, in the locally inertial frame of an observer right next to the light at any given point on its worldline. Even in flat SR spacetime there is no requirement that light move at c in a non-inertial coordinate system (and all global coordinate systems in curved spacetime will be non-inertial), so this doesn't really depend in any specific way on the metric. It might even be possible to find a coordinate system in a FLRW spacetime where light
does continue to have a coordinate speed of c everywhere, just as you can do with Kruskal-Szekeres coordinates in the curved spacetime around a nonrotating black hole (which I discussed on
this recent thread).