Does Empty Space Reflect Einstein's 4D Space-Time Curvature?

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Discussion Overview

The discussion centers around the nature of empty space in relation to Einstein's 4D space-time curvature, particularly how regions of space that are mostly empty can still exhibit curvature according to general relativity (GR). Participants explore theoretical implications, the conditions for black hole formation, and the interpretation of density in relation to curvature.

Discussion Character

  • Debate/contested
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • Some participants suggest that while most of space is empty, it can still be described as 4D Minkowski space when viewed closely, but larger scales may not appear flat.
  • There is a contention regarding how a void in 4D space can be bent by a small amount of matter, with some arguing that neutron stars and black holes play a significant role in the universe's curvature.
  • Others assert that the average density of a region is more important than whether space is empty, and that black holes can form from various materials, not just dense ones.
  • Several participants express disagreement about the necessity of high density for black hole formation, with some arguing that a large enough mass, regardless of density, can lead to black hole formation.
  • Discussions include interpretations of the Schwarzschild radius and its implications for black hole formation, with conflicting views on the role of density versus mass.
  • Some participants emphasize that empty space can still be curved, referencing solutions to Einstein's equations that allow for curved empty spacetimes.

Areas of Agreement / Disagreement

Participants generally disagree on the relationship between density and curvature, as well as the conditions necessary for black hole formation. Multiple competing views remain unresolved throughout the discussion.

Contextual Notes

Limitations include varying interpretations of general relativity, the definitions of density and curvature, and the mathematical implications of the Schwarzschild radius. The discussion does not resolve these complexities.

delplace
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As you know 99.9999 % of our world is empty. Does this empty space correspond to Einstein 4D space-time.
 
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Well any well-behaved region of space, viewed close up enough, looks like 4D minkowski space. However, even though such a vast majority of space is devoid of matter, as a general rule space does not look flat on larger scales.
 
well, you point out my problem, how a void 4D space (according to GR) can be bent by few matter ? the only way I can understand it is in neutron stars because they are a "big neutron" without void. Does it mean in a rough approximation that universe curvature is due do neutron stars and black holes ?
 
1. It is not important if space is empty or not. What is important is average density
2. The interesting property of GR is that if (in abstract static universe) you make a bigger and bigger ball of something, you eventually end with a black hole. So you can make a BH of water, air or even interstellar gas. So BH does not need to be 'dense'
 
Sorry but I don't agree
1. I would like to understand how something empty can be bent. Think 99.9999999% empty !
2. I know that BH formation need an enormous density and not only a big size !

Kindly :-)
 
delplace said:
Sorry but I don't agree
1. I would like to understand how something empty can be bent. Think 99.9999999% empty !

It's also 0.000...001% bent.
 
yes :-)
 
delplace said:
Sorry but I don't agree
1. I would like to understand how something empty can be bent. Think 99.9999999% empty !
2. I know that BH formation need an enormous density and not only a big size !

Kindly :-)

2. No
Only stellar size BH have high density
Check the formula for Scharshield radius:

http://en.wikipedia.org/wiki/Black_hole

r = 2GM/c^2

It is proportional to the mass! While when density is the same, mass is proportional to r^3
 
Your interpretation of Schwartzhield formula is wrong. This equation give the radius where a star of mass M will be dense enough to produce a black hole ! BH formation is only a question of density.
 
  • #10
absolutely wrong.

for a given density p the mass M in a sphere of radius r is

M = 4/3 * pi * p * r^3

S. radius for the given M is

r = 2GM/c^2

hence

r = 1/sqrt( 8/3*pi* p )

So if your material is not dense enough, you just need to take more material.
 
Last edited:
  • #11
in fact you don't need any formulas to understand that.
Take Earth for example, it has r=6300km and Rsh=0.5cm
Add more and more material to Earth.

when you double r, the total mass increases as r^3
For 'earth' of r=10*6300km Rsh=0.5cm*1000=5m

Sooner or later schwarshield raduis 'catches up' with an actual one.

The same is applicable to the whole Universe - in that case it becomes closed (unless it is expanding)
 
  • #12
you forget a G in your last equation (not important). More important is the interpretation of S. formula. The physical meaning is : if you take a planet of mass M and volume V; you will obtain a BH if you decrease the volume until you reach a density M/V sufficiently high. The radius will be the S. radius. Of course you will obtain the same result by increasing M but it is not possible because you can not add more matter.
 
  • #13
delplace said:
1. I would like to understand how something empty can be bent. Think 99.9999999% empty !

First of all, spacetime is not "bent", it is curved. Secondly, what exactly is your objection to spacetime being mostly empty? General relativity even allows empty spacetimes that are curved (for example Schwartzschild solution).


delplace said:
2. I know that BH formation need an enormous density and not only a big size !
This is simply not correct, and trivially so. It would be a good idea to accept it. If I take a large enough batch of interstellar dust, to an outside observer the cloud will look like a black hole, and all the dust will collapse to the center in finite proper time. For any given (assume constant) density [tex]\rho[/tex], an event horizon will form if the radius of the cloud is [tex]r \gtrsim M_p / \sqrt{\rho}[/tex].
 
  • #14
GR equation is for me clear : space-time is "curved" by energy (tensor in the right hand of GR equation).

Hawking think we could obtain BH in the LHC. It is not in agreement with your proposal.
 
  • #15
delplace said:
you forget a G in your last equation (not important). More important is the interpretation of S. formula. The physical meaning is : if you take a planet of mass M and volume V; you will obtain a BH if you decrease the volume until you reach a density M/V sufficiently high. The radius will be the S. radius. Of course you will obtain the same result by increasing M but it is not possible because you can not add more matter.

For a given planet - yes, because we fix M.
But the BH formation is not caused by HIGH DENSITY - as I showed, you can create a BH from cotton wool
 
  • #16
I don't think that even if you take a lot of cotton wool :-) but I respect your way of thinking

best regards
 
  • #17
delplace said:
GR equation is for me clear : space-time is "curved" by energy (tensor in the right hand of GR equation).

... and what exactly makes you think an empty spacetime is not curved? As you may know, Einstein equation is a partial differential equation of the metric, and PDE's can certainly have nontrivial solutions even with no source term...

delplace said:
Hawking think we could obtain BH in the LHC. It is not in agreement with your proposal.
I am sure you don't mind explaining this claim in detail.
 
  • #18
yes, PDE's can be solved with no source term. But Einstein introduce one Tij. And my physical approach let me think that you need Energy to obtain deformations and then movement. For me GR equation describe the non steady state evolution of univers.

I could explain in details ! :-)
 
  • #19
It can be curved in a region with no source term though. A universe filled with a single star is still curved throughout, so it shouldn't be troubling to think that one with billions has some curvature too.
 

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