If you want to do some research on the subject, you're looking for violations of homogeneity, as implied by the Lambda-CDM model of the universe. The lambda in this case is the cosmological constant. You'll need to read up on that too.
The shortest, simplest way I can think to explain it is that we expect the universe to look alike, anywhere we look. Think of it like a biopsy - we assume that anywhere we look should be much like anywhere else, because there's no reason to think any area of the universe has special conditions where physics plays by different rules.
That sets up some implications around what we think the universe should look like, at different scales. However, we recently have been running into structures which are bigger than we'd expect.
Where we get into the maths is to do with the value of the cosmological constant. We currently think it's positive, because the universe is expanding, and its rate of expansion is accelerating. To look into the maths for this, have a Google around the maths behind the accelerating expansion of the universe.
The shortest, simplest way I can think to explain it is that we expect the universe to look alike, anywhere we look. Think of it like a biopsy - we assume that anywhere we look should be much like anywhere else, because there's no reason to think any area of the universe has special conditions where physics plays by different rules.
That sets up some implications around what we think the universe should look like, at different scales. However, we recently have been running into structures which are bigger than we'd expect.
Where we get into the maths is to do with the value of the cosmological constant. We currently think it's positive, because the universe is expanding, and its rate of expansion is accelerating. To look into the maths for this, have a Google around the maths behind the accelerating expansion of the universe.