Why wasn't the Big Bang an isotropic explosion?

Click For Summary

Discussion Overview

The discussion revolves around the nature of the Big Bang and whether it can be considered an isotropic event. Participants explore concepts related to the homogeneity of space and time, the implications of quantum fluctuations, and the formation of structures in the universe. The conversation touches on theoretical aspects of cosmology, including gravitational stability and the geometry of the universe.

Discussion Character

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

Main Points Raised

  • Some participants suggest that the Big Bang should be isotropic if space and time are assumed to be homogeneous and infinite in every direction.
  • Others argue that while isotropy is a common assumption, quantum fluctuations introduce deviations, leading to inhomogeneities in the early universe.
  • It is proposed that gravitational equilibrium of an isotropic distribution of matter is unstable, leading to clustering of matter due to slight imbalances.
  • A participant questions how stars and galaxies formed if the expansion is isotropic, suggesting that a homogenous gravitational field should prevent clustering.
  • Some participants discuss the implications of the universe's geometry, noting that while space can be finite, it may not have an edge, similar to the surface of a sphere.
  • There is mention of inflation theory as a mechanism that could explain the flatness and isotropy of the early universe, although this is not universally accepted.

Areas of Agreement / Disagreement

Participants express differing views on the isotropy of the Big Bang and the implications of gravitational stability. There is no consensus on whether the early universe was truly isotropic or how to reconcile observations with theoretical models.

Contextual Notes

Participants note that while isotropy is observed on large scales today, extrapolating this back to the early universe is complicated by instabilities. The discussion includes references to models of the universe that may or may not support finite spacetime, highlighting the complexity of the topic.

randybryan
Messages
51
Reaction score
0
I'm sure I'm making a plethora of naive assumptions in this question, but I was just thinking that the Big Bang, or the birth of our universe should logically be isotropic if space and time is assumed to be homogenous and infinite in every direction.
 
Space news on Phys.org
Isotropic up to quantum fluctuations. Yes, that is the usual assumption (and observations agree very well with that). Note that the big bang was not an "explosion" in space. Space itself expanded (and continues to expand).
Space does not have to be infinite, but it is probably without a boundary. This is not a contradiction, see the surface of Earth for example: finite area, but no boundary.
 
Thanks for the reply. I did actually think explosion was a poor lexical choice, so thanks for correcting me. How were stars and galaxies formed then if the expansion is isotropic? Is this explained by quantum fluctuation alone?, there should surely be a homogenous gravitational field, which would mean matter shouldn't cluster? My knowledge of cosmology, as you can probably tell, is very limited.
 
Gravitational equilibrium of an isotropic distribution of matter is unstable; Newton understood this and so proposed an infinite distribution of stars.

This the slightest imbalance, anywhere, or at anytime will start the gravitational agglomeration of matter.

But such a slight imbalance at any time during the Big Bang, early or late, will result in inhomogeneity at some level - this is where detailed models must be compared to observational evidence in order to refine our understanding.
 
  • Like
Likes   Reactions: 1 person
How come gravitational equilibrium of an isotropic distribution is unstable? Is there a good book you would recommend reading? I don't know if I'm verging on some seriously difficult physics here...
 
"Philosophiæ Naturalis Principia Mathematica" by Isaac Newton - if you read Latin!
http://en.wikipedia.org/wiki/Philosophiæ_Naturalis_Principia_Mathematica

But the argument is simple:

One object alone exerts gravity on nothing but itself.

Two objects exert gravity on each other, and are attracted. If they were originally still they will collide; if they had their own motions they will follow a conic section: parabolic (a bullet), hyperbolic (some comets), elliptical (planets)

What if you arrange 3 in a line? Then maybe you can cancel the net gravity on the middle one, but the other two are still going to move.

Keep adding one more, and every arrangement is unstable.

In the limit you can generate an infinite array - like a giant salt crystal, but with stars instead of atoms of Cl and Na - with an equal number of stationary attractors in each direction.

But once the perfect alignment is broken, you will have worlds in collision!
 
The basic idea is quantum fluctuations resulted in slightly overdense regions in the early universe. These over dense regions show up as temperature fluctuations in the CMB. So, thanks to quantum fluctuations, the universe was never truly homogenous.
 
Awesome. Thanks for the reply. Definitely going to read up on some cosmology
 
mfb said:
Isotropic up to quantum fluctuations. Yes, that is the usual assumption (and observations agree very well with that). Note that the big bang was not an "explosion" in space. Space itself expanded (and continues to expand).
Space does not have to be infinite, but it is probably without a boundary. This is not a contradiction, see the surface of Earth for example: finite area, but no boundary.

sooo if you get to the edge of the universe you go to the beginning?
 
  • #10
There is no "edge of the universe".
 
  • #11
I thought space-time was finite:confused:
 
  • #12
The surface area of a sphere is finite ... but there is no edge.
 
  • #13
Superposed_Cat said:
I thought space-time was finite:confused:

In what sense?

There are models of the universe for which space finite, but I know of no seriously considered models of the universe for which spacetime is finite. In fact, all spacetimes that satisfy a certain finiteness condition have closed timelike curves.
 
  • #14
randybryan said:
I'm sure I'm making a plethora of naive assumptions in this question, but I was just thinking that the Big Bang, or the birth of our universe should logically be isotropic if space and time is assumed to be homogenous and infinite in every direction.
It's the other way around: isotropy implies homogeneity (the easy example is a homogeneous electric field pointing in a given direction: it's uniform but not isotropic). While we happen to observe that isotropy holds on relatively large scales today, we can't easily extrapolate that back to the early universe, for reasons of instability mentioned above. To get around these, one must fine tune the initial curvature of the universe to an immense degree. The idea that the very early universe emerging from the big bang was flat and isotropic is therefore by no means a natural proposal. Inflation, a period of accelerated expansion in the very early universe, can be invoked to dynamically push the universe to flatness and isotropy.
 

Similar threads

  • · Replies 9 ·
Replies
9
Views
3K
  • · Replies 20 ·
Replies
20
Views
3K
  • · Replies 8 ·
Replies
8
Views
3K
  • · Replies 13 ·
Replies
13
Views
5K
  • · Replies 25 ·
Replies
25
Views
4K
  • · Replies 1 ·
Replies
1
Views
3K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 43 ·
2
Replies
43
Views
5K
  • · Replies 6 ·
Replies
6
Views
3K
  • · Replies 33 ·
2
Replies
33
Views
4K