What is the relationship between expansion and curvature?

Click For Summary

Discussion Overview

The discussion explores the relationship between the expansion of the universe and its curvature, touching on concepts from cosmology and general relativity. Participants examine how the density of matter and dark energy influences both the expansion rate and the geometric shape of the universe, considering implications for different models of cosmic evolution.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • Some participants propose that the expansion of the universe is influenced by a balance between the attractive force of matter and the repulsive force of dark energy, with density playing a crucial role.
  • Others argue that the curvature of the universe is determined by the average density of matter, suggesting that more mass leads to greater curvature.
  • A participant questions the assertion that a universe expanding forever must be negatively curved, suggesting that a flat universe could also expand indefinitely.
  • Some contributions reference the Lambda-CDM model to illustrate the relationship between curvature and expansion, noting that observational data supports a flat universe that can still expand forever.
  • One participant discusses the Ricci curvature scalar, indicating that expansion can be understood as a manifestation of space-time curvature, with specific mathematical relationships outlined.
  • Another participant mentions the Milne universe as an exception where expansion occurs without curvature, highlighting the complexity of the relationship between expansion and curvature.

Areas of Agreement / Disagreement

Participants express differing views on the relationship between expansion and curvature, with no consensus reached on whether a universe that expands forever must be negatively curved or if a flat universe can also exhibit perpetual expansion.

Contextual Notes

Some statements rely on assumptions about the distribution of matter and the nature of dark energy, and the discussion includes references to specific models and mathematical formulations that may not be universally accepted.

RogerWaters
Messages
19
Reaction score
2
TL;DR
Untangling the effects of mass on the expansion and the curvature of the universe
Physics novice here reading pop sci cosmology. Please bear with me.

Premise 1: Whether or not expansion is slowing down or speeding up depends on a battle between two phenomena: the attractive gravitational pull of matter and the repulsive gravitational push of dark energy. What counts in this contest is the density of each. (Also, the density of matter decreases as the universe expands because the volume of space increases). Basically: More mass, less/slower expansion.

Premise 2: The spatial curvature of the universe is related to general relativity, which describes how spacetime is curved and bent by mass and energy. If all forms of dark energy are ignored, then the curvature of the universe can be determined by measuring the average density of matter within it, assuming that all matter is evenly distributed. The distribution of mass in the universe determines the curvature of space in Einstein's theory. Basically: More mass (per unit of space), more curvature.

To my mind this means that the expansion and the shape of the universe are intrinsically linked? On first thought, this seemed strange to me as surely the universe could be expanding regardless of whether it is positive curved, negatively curved, or flat.

Question time:

1. How are expansion and curvature related? This article states:

"If the actual density of the universe is less than the critical density, then there is not enough matter to stop the expansion of the universe, and it will expand forever. The resulting shape is curved like the surface of a saddle. This is known as an open universe."

2. But why should a universe that expands forever be negatively curved like a saddle? Why can't a flat universe continually expand?

Thanks.
 
Last edited:
Space news on Phys.org
RogerWaters said:
But why should a universe that expands forever be negatively curved like a saddle? Why can't a flat universe continually expand?
It can.
cerndar2_9-03.jpg

This image shows the Lambda-CDM model. As you can see, the dividing lines for open/flat and expand forever/recollapse are very different. The statement is particular for a Universe containing only matter.

Edit: Note that the observational data (implications are shown as coloured regions) suggest that we are firmly inside the expand forever regime while still being compatible with a flat universe.
 
  • Like
Likes   Reactions: RogerWaters
RogerWaters said:
Physics novice here reading pop sci cosmology.
You should not be trying to learn actual science from pop science sources.
 
RogerWaters said:
1. How are expansion and curvature related? This article states:
:welcome:

That article is a good example of why we are not keen on popular science sources. It may be unfair to say so, but it appears the author is writing about something that she herself does not fully understand.

The Wikipedia pages are considerably better, although still not considered a valid source for discussion here.

https://en.wikipedia.org/wiki/Expansion_of_the_universe

https://en.wikipedia.org/wiki/Ultimate_fate_of_the_universe
 
Orodruin said:
It can.
View attachment 293296
This image shows the Lambda-CDM model. As you can see, the dividing lines for open/flat and expand forever/recollapse are very different. The statement is particular for a Universe containing only matter.

Edit: Note that the observational data (implications are shown as coloured regions) suggest that we are firmly inside the expand forever regime while still being compatible with a flat universe.
Thanks for this - what's the source out of interest?
 
  • Like
Likes   Reactions: RogerWaters
RogerWaters said:
Summary:: Untangling the effects of mass on the expansion and the curvature of the universe

Physics novice here reading pop sci cosmology. Please bear with me.

Premise 1: Whether or not expansion is slowing down or speeding up depends on a battle between two phenomena: the attractive gravitational pull of matter and the repulsive gravitational push of dark energy. What counts in this contest is the density of each. (Also, the density of matter decreases as the universe expands because the volume of space increases). Basically: More mass, less/slower expansion.

Premise 2: The spatial curvature of the universe is related to general relativity, which describes how spacetime is curved and bent by mass and energy. If all forms of dark energy are ignored, then the curvature of the universe can be determined by measuring the average density of matter within it, assuming that all matter is evenly distributed. The distribution of mass in the universe determines the curvature of space in Einstein's theory. Basically: More mass (per unit of space), more curvature.

To my mind this means that the expansion and the shape of the universe are intrinsically linked? On first thought, this seemed strange to me as surely the universe could be expanding regardless of whether it is positive curved, negatively curved, or flat.

Question time:

1. How are expansion and curvature related? This article states:

"If the actual density of the universe is less than the critical density, then there is not enough matter to stop the expansion of the universe, and it will expand forever. The resulting shape is curved like the surface of a saddle. This is known as an open universe."

2. But why should a universe that expands forever be negatively curved like a saddle? Why can't a flat universe continually expand?

Thanks.
The expansion is a manifestation of space-time curvature.

If you calculate the Ricci curvature scalar for a uniform, expanding universe, you get a result which is just a function of the expansion and the spatial curvature:

$$R = 6 \left( \dot{H} + 2 H^2 + {k \over a^2}\right)$$

So you have terms for the rate of expansion ##H##, its time derivative ##\dot{H}##, and the spatial curvature ##k##. You can literally understand the expansion as being space-time curvature.

Edit: I'm really not sure why the forum isn't picking up the LaTeX in this post, but hopefully it's still legible.
 
kimbyd said:
I'm really not sure why the forum isn't picking up the LaTeX in this post
It looks OK to me. You might need to reload the page and/or log out of PF and log back in again, and/or clear cookies.
 
kimbyd said:
Edit: I'm really not sure why the forum isn't picking up the LaTeX in this post, but hopefully it's still legible.
It's a known problem. If you are the first to use Latex in a thread (except in the OP), then it does not render until you refresh the page.
 
  • Informative
Likes   Reactions: hmmm27
  • #10
kimbyd said:
The expansion is a manifestation of space-time curvature.

If you calculate the Ricci curvature scalar for a uniform, expanding universe, you get a result which is just a function of the expansion and the spatial curvature:

$$R = 6 \left( \dot{H} + 2 H^2 + {k \over a^2}\right)$$

So you have terms for the rate of expansion ##H##, its time derivative ##\dot{H}##, and the spatial curvature ##k##. You can literally understand the expansion as being space-time curvature.

Edit: I'm really not sure why the forum isn't picking up the LaTeX in this post, but hopefully it's still legible.
Well, there is the well known exception of the limit of a universe without mass, which still has expansion but no curvature (Milne universe). It is just Minkowski spacetime in funny coordinates. However, it has all the major features of realistic cosmologies - arbitrarily large superluminal recession rates, cosmological redshift, etc.

Noting that H(t) and a(t) are related (##H(t)=a'(t)/a(t)##) , if a(t) is taken to be simply t, then H(t) is required to be 1/t, and taking k=-1, R vanishes. k=-1 implies the spatial slices are hyperbolic.
 
  • #11
PeroK said:
It's a known problem. If you are the first to use Latex in a thread (except in the OP), then it does not render until you refresh the page.
Ahhh, I did not know this! Thanks!
 
  • #12
I think that, at the end, it is absolutely necessary to understand what "space" is or what "space-time" is, and we need to stop the abuse of terminology like "matter curve spacetime" or "space is expanding" or "spacetime is expanding" or things like that.
 
  • #13
pabloweigandt said:
I think that, at the end, it is absolutely necessary to understand what "space" is or what "space-time" is, and we need to stop the abuse of terminology like "matter curve spacetime" or "space is expanding" or "spacetime is expanding" or things like that.
:welcome:
 
  • #14
pabloweigandt said:
I think that, at the end, it is absolutely necessary to understand what "space" is or what "space-time" is, and we need to stop the abuse of terminology like "matter curve spacetime" or "space is expanding" or "spacetime is expanding" or things like that.
"Matter curves spacetime" doesn't seem to me to be a terrible abuse. Strictly it's the stress-energy associated with the matter (and, indeed, other things like radiation) that is the source term for curvature, but I don't really see the issue. "Space is expanding" is kind of an abuse, yes, in that it's more like that later surfaces of constant cosmological time have increased scale factors compared to earlier ones, but that's a lot harder to say. And "spacetime is expanding" isn't an abuse of terminology, it's just wrong.
 
  • #15
"Space is expanding" will mean that I know what space is. And that there is no difference between two galaxies that are getting apart at superluminal speeds (if it is true that I can use the term "speed" or "velocity" in this case) and two cars moving apart each other.
 
  • #16
pabloweigandt said:
"Space is expanding" will mean that I know what space is. And that there is no difference between two galaxies that are getting apart at superluminal speeds (if it is true that I can use the term "speed" or "velocity" in this case) and two cars moving apart each other.
In any case, this is what's called "hijacking" a thread.
 
  • Like
Likes   Reactions: RogerWaters
  • #17
Ok. I am new to this. I found the definition of "hijacking". You are right and I am so sorry. I would be grateful If anyone can tell me where to post this kind of topics.
 
  • Like
Likes   Reactions: PeroK
  • #18
Go to the front page (physicsforums.com), scroll down until you find the Cosmology forum, click on that, and then click "Post thread". Do make sure you've read the posting guidelines.
 
  • #19
pabloweigandt said:
Ok. I am new to this. I found the definition of "hijacking". You are right and I am so sorry. I would be grateful If anyone can tell me where to post this kind of topics.
This is a "B" level thread, which suggests that the OP (original poster) is not a university student. The answers to his question were at a level that hopefully he could understand.

The thread is nearly a month old and the OP has not responded in some time.
 
  • #20
pabloweigandt said:
"Space is expanding" will mean that I know what space is.
And in the case where that term is used, FRW spacetimes, there is a definition of "space" that is picked out by the symmetries of the spacetime (namely, the spacelike surfaces that are orthogonal to the comoving worldlines).

pabloweigandt said:
And that there is no difference between two galaxies that are getting apart at superluminal speeds (if it is true that I can use the term "speed" or "velocity" in this case) and two cars moving apart each other.
No. There is a difference. In a curved spacetime, there is no such thing as a well-defined "relative speed" for objects that are separated by significant distances. That issue doesn't arise for two cars near each other on Earth, but it does for galaxies distant from each other in the universe. It is not true that you can use the term "speed" or "velocity" in the latter case with their usual meanings. Nor do you need to to give a well-defined meaning to "space is expanding".

pabloweigandt said:
I would be grateful If anyone can tell me where to post this kind of topics.
Before starting a new thread, I would suggest taking some time to learn what cosmologists actually mean by "space is expanding" as a description of our universe. If you have questions about what you read, as @Ibix has said, you can start a new thread in the Cosmology forum (the forum this thread is in). His advice about reading the posting guidelines first is also good.
 
  • #21
PeroK said:
The thread is nearly a month old and the OP has not responded in some time.
And that being the case, this thread is now closed.
 

Similar threads

  • · Replies 3 ·
Replies
3
Views
3K
  • · Replies 54 ·
2
Replies
54
Views
5K
  • · Replies 2 ·
Replies
2
Views
2K
Replies
18
Views
1K
  • · Replies 9 ·
Replies
9
Views
3K
  • · Replies 19 ·
Replies
19
Views
3K
  • · Replies 4 ·
Replies
4
Views
801
  • · Replies 6 ·
Replies
6
Views
2K
  • · Replies 37 ·
2
Replies
37
Views
6K
  • · Replies 13 ·
Replies
13
Views
3K