Is the Geometry of the Universe Determined by Its Density?

  • Context: Graduate 
  • Thread starter Thread starter Lapidus
  • Start date Start date
  • Tags Tags
    Density Geometry
Click For Summary

Discussion Overview

The discussion revolves around the relationship between the density of the universe and its geometry, specifically focusing on how the curvature parameter k in the Friedmann equation is influenced by the universe's density. Participants explore theoretical implications, model assumptions, and the dynamics of curvature over time.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • Some participants assert that the geometry of the universe is determined by its density, with k in the R-W metric being a function of this density.
  • Others question how the curvature parameter k is determined, noting that the scale factor is the only dynamical element in the Friedmann equation.
  • A participant mentions that model universes in textbooks assume a curvature type and then add energy components, raising questions about whether curvature is an external parameter or intrinsic to the model.
  • It is noted that the global curvature of the universe is contingent upon whether the density is above, below, or equal to the critical density.
  • Some participants refer to Ryden's cosmology book, which discusses various models and how different components influence the universe's geometry.
  • A later reply suggests that while density changes over time, the curvature parameter k is fixed at the universe's inception and is not influenced by dynamics.

Areas of Agreement / Disagreement

Participants generally agree that density plays a crucial role in determining the geometry of the universe, but there are competing views regarding the nature of the curvature parameter k and its dependence on initial conditions versus dynamical factors.

Contextual Notes

There are unresolved questions regarding the assumptions made in model universes and the implications of density changes over time on the curvature parameter k.

Lapidus
Messages
344
Reaction score
12
Just for clarity, the geometry of the universe is completely determined by the stuff that the universe contains. The parameter k in the R-W metric and in the Friedmann equation *is determined* by the density.

The curvature/ geometry of the universe is not independent of the density.

Correct or not?

Thank you!
 
Space news on Phys.org
Thanks!

But how is the sign of the curvature parameter k determined? As I understand, only the scale factor is dynamical in the Friedmann equation. So if our universe is sphere or a saddle, the curvature of the universe in our observable part could have been flatten out if the scale factor accelerated fast enough.

Also, there seems to be model universes in the textbooks (like in Ryden or in Carroll), where they assume a curvature of a universe (open/flat/closed) and then add energy components (matter/radiation/vaccum constant) to the model. Unfortunately, they nowhere say clearly if the curvature is a parameter outside of the model (the Friedmann equation) or not.So again my question: what physics determine if the universe is open, flat or closed?

Addendum: I just read in some notes that k never changes and that density, though it depends on time, always remains in whichever regime it starts with ( larger than one, equal to one, smaller than one).

So can we say then that k is given and can only be determined by measurement?
 
Last edited:
The global curvature of the universe (whether k is positive, negative, or zero) depends on whether the density of the universe is greater than, less than, or equal to the critical density, \rho_c = \frac{3H^2}{8\pi G}.
 
Ryden's Introduction in cosmology book has a variety of models. Single and multi-component
universes. She adds components to arrive at her benchmark model. If you work through each model it becomes clear how each component influences the universe. Bapowell has already answered how K is determined. That is also shown in Ryden's book.
 
Thanks again!

After reading some more I came to understand that the universe is "born" with a certain amount of matter, radiation, vacuum energy and with or without a certain curvature.

The density changes, but depending on the value of k, which is given when the universe comes into existence, the density remains larger than one, one or smaller than one.

So k is indeed not determined by any dynamics, but a given constant given at the start of a universe.
 

Similar threads

  • · Replies 9 ·
Replies
9
Views
3K
  • · Replies 2 ·
Replies
2
Views
3K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 7 ·
Replies
7
Views
3K
  • · Replies 6 ·
Replies
6
Views
2K
  • · Replies 27 ·
Replies
27
Views
6K
  • · Replies 6 ·
Replies
6
Views
2K
  • · Replies 7 ·
Replies
7
Views
5K
  • · Replies 9 ·
Replies
9
Views
3K
  • · Replies 3 ·
Replies
3
Views
2K