How Does Dark Energy Exhibit Negative Pressure in Cosmology?

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Discussion Overview

The discussion revolves around the concept of dark energy and its characterization as having negative pressure within the framework of cosmology. Participants explore the relationship between dark energy, the stress-energy tensor, and the implications of these concepts for the expansion of the universe.

Discussion Character

  • Technical explanation
  • Conceptual clarification
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • One participant questions how energy can exhibit pressure, suggesting a possible analogy between the metric tensor field and the stress-energy tensor.
  • Another participant presents a mathematical representation of dark energy in terms of the stress-energy tensor, indicating isotropic negative pressure.
  • A participant seeks clarification on the meaning of the variable \mu in the context of the stress-energy tensor and questions the definition of pressure in this framework.
  • Discussion includes the distinction between the stress-energy tensor of gravitating matter and the contribution of the cosmological constant to energy and pressure.
  • There is a query about whether "gravitating matter" and "perfect fluid" refer to the same source of cosmic acceleration attributed to dark energy.
  • A participant introduces the concept of "dark fluid" as a potential theory related to the discussion.

Areas of Agreement / Disagreement

Participants express varying interpretations of the relationship between dark energy, pressure, and the stress-energy tensor, indicating that multiple competing views remain without consensus on these definitions and relationships.

Contextual Notes

Participants highlight the complexity of defining dark energy and its properties, including the dependence on coordinate systems and the interpretation of tensor components, which remain unresolved.

Rasalhague
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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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The dark energy looks like this in terms of SETs. Isotropic negative pressure.

[tex]G_{\mu\nu}=\kappa \left[ \begin{array}{cccc}<br /> \mu c^2& 0 & 0 & 0 \\\<br /> 0 &0 &0 & 0 \\\<br /> 0 &0 &0 & 0 \\\<br /> 0 & 0 & 0 & 0\end{array} \right]-<br /> \left[ \begin{array}{cccc}<br /> \Lambda g_{00} & 0 & 0 & 0 \\\<br /> 0 &\Lambda g_{11} & 0 & 0 \\\<br /> 0 & 0 &\Lambda g_{22} & 0 \\\<br /> 0 & 0 & 0 & \Lambda g_{33}\end{array} \right][/tex]
 
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?
 
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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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?
 
Are you referring to this theory: Dark fluid?
 

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