Dark Energy Pressure: Exploring the Mystery

In summary, the Wikipedia article on dark energy says that dark energy would need to have a strong negative pressure in order to remain in equilibrium.
  • #1
Rasalhague
1,387
2
The Wikipedia article on dark energy says "dark energy would need to have a strong negative pressure". In what sense can energy "have" pressure?

Is it that the value of the metric tensor field at an event, when multiplied by the cosmological constant, is a tensor in some way analogous to the stress-energy tensor, with components corresponding to energy-density, momentum density and stress? Is this effectively the stress-energy tensor of some, as yet, unidentified matter? If so, why does it play a different role in the equation to the stress-energy tensor of dark matter, which I'm guessing (rightly or wrongly) is subsumed into the regular stress-energy tensor. When Wikipedia: Dark energy says, "In the standard model of cosmology, dark energy currently accounts for 73% of the total mass-energy of the universe", what is the relationship of pressure to this figure of 73%?
 
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  • #2
The dark energy looks like this in terms of SETs. Isotropic negative pressure.

[tex]G_{\mu\nu}=\kappa \left[ \begin{array}{cccc}
\mu c^2& 0 & 0 & 0 \\\
0 &0 &0 & 0 \\\
0 &0 &0 & 0 \\\
0 & 0 & 0 & 0\end{array} \right]-
\left[ \begin{array}{cccc}
\Lambda g_{00} & 0 & 0 & 0 \\\
0 &\Lambda g_{11} & 0 & 0 \\\
0 & 0 &\Lambda g_{22} & 0 \\\
0 & 0 & 0 & \Lambda g_{33}\end{array} \right]
[/tex]
 
  • #3
What does [itex]\mu[/itex] stand for in the time-time component of [itex]\text{diag}(\mu c^2,0,0,0) = T_{\mu\nu}[/itex]? Is the name pressure only given to the spatial diagonal components of the second term? If this is a tensor equation, could we chose coordinates in which the second term on the right, by analogy with the stress-energy tensor, would have off-diagonal space-space components (dark stress)? Does the name dark energy refer to [itex]\Lambda g_{00}[/itex], or to the whole of the second term on the right, or to or [itex]\mu c^2[/itex], or to the whole expression? Does the name dark energy refer to a quantity defined only in a particular conventional coordinate system, or does it refer to a particular component of a tensor, regardless of what value that component takes in a given coordinate system?
 
  • #4
The first term is the SET of the gravitating matter in its rest-frame. The second term is energy/pressure caused by [itex]\Lambda[/itex]. The SET of a perfect fluid is

[tex]
T_{\mu\nu}=(\mu+p)U_\mu U_\nu + pg_{\mu\nu}
[/tex]

with Um=0, m= 1,2,3 and U0 <> 0, it reduces to something like my first expression. So the cosmological constant is claimed to be energy/pressure ( I've dropped a factor of c2 somewhere...)

This is informative,

http://en.wikipedia.org/wiki/Fluid_solution
 
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  • #5
Do "gravitating matter" and "perfect fluid" here both refer to the source of the acceleration in the expansion of the universe, commonly called dark energy?

And do I understand you correctly that [itex]\Lambda g_{\mu\nu}[/itex] is just the [itex]p g_{\mu\nu}[/itex] term of the SET for this exotic perfect fluid?
 
  • #6
Are you referring to this theory: Dark fluid?
 

Related to Dark Energy Pressure: Exploring the Mystery

1. What is dark energy pressure?

Dark energy pressure is a theoretical concept used to describe the mysterious force that is believed to be causing the universe to expand at an accelerating rate. It is believed to make up about 68% of the total energy of the universe.

2. How is dark energy pressure different from dark energy?

Dark energy pressure is a characteristic of dark energy, which is the overall term used to describe the unknown energy that is causing the expansion of the universe. Dark energy pressure refers specifically to the pressure exerted by this energy, while dark energy encompasses all aspects of this unknown force.

3. What evidence do we have for the existence of dark energy pressure?

There is currently no direct evidence for dark energy pressure, as it is a theoretical concept. However, the expansion of the universe at an accelerating rate and other phenomena such as the cosmic microwave background radiation support the existence of dark energy and its associated pressure.

4. How is dark energy pressure related to the concept of a cosmological constant?

The cosmological constant is a term used in Einstein's theory of general relativity to represent a constant energy density that exists throughout space. It is often used interchangeably with dark energy, as it is believed to be the energy responsible for the expansion of the universe. Dark energy pressure is a component of this overall energy, with the cosmological constant representing its density.

5. Can we manipulate or control dark energy pressure?

Currently, we do not have the technology or understanding to manipulate or control dark energy pressure. However, ongoing research and advancements in our understanding of this mysterious force may lead to potential applications in the future.

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