Ranku
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Cosmological constant dark energy has equation of state parameter = -1. What is the equation of state parameter of gravitational energy?
The discussion revolves around the concept of the equation of state parameter for gravitational energy in the context of General Relativity, particularly in comparison to the equation of state parameter for dark energy, which is known to be -1. Participants explore whether a similar parameter can be defined for gravitational energy and how it relates to pressure and energy density.
Participants do not reach a consensus on whether an equation of state parameter for gravitational energy can be defined or how it would relate to dark energy. Multiple competing views remain regarding the implications of introducing new quantities and the nature of gravitational energy.
The discussion highlights limitations in defining gravitational energy within the framework of General Relativity and the complexities introduced by curved spacetime. There are unresolved questions about the mathematical formulation and the physical implications of proposed concepts.
There isn't one. In the standard formulation of General Relativity, there is no such thing as gravitational energy.Ranku said:Cosmological constant dark energy has equation of state parameter = -1. What is the equation of state parameter of gravitational energy?
Chalnoth said:There isn't one. In the standard formulation of General Relativity, there is no such thing as gravitational energy.
No, I don't think so.Ranku said:Since dark energy density is related to negative pressure, is there no way to construct a relation between 'positive pressure' and 'gravitational energy density', even though gravitational energy does not occur in general relativity?
Chalnoth said:No, I don't think so.
One way you could do it, though, is through the conservation of the stress-energy tensor. The stress-energy tensor is a 2nd-rank tensor (sort of like a matrix) that includes components such as energy, momentum, pressure, and shear (shear includes things like twisting forces). This tensor is always conserved in a very particular way: its so-called covariant derivative is zero.
If you examine this conservation law in flat space-time, you get an energy transport equation: the time rate of change of energy in a region of space is equal to the flow of energy into/out of that region.
However, in curved space-time things get a little bit more complicated. What you could do is make up a new "total energy density" which is always conserved: as in the flat space-time example, the total energy density within a region of space-time only changes if it flows from one place to another. You could do this by adding an extra term to the equations that exactly cancels the extra terms you get from curved space-time, and call this your gravitational potential energy.
Hmm, that's not what I was talking about. The basic idea is this. If we have massless particles in flat space-time, we can write energy conservation as:AWA said:Would't that leave you with a completely new stress-energy tensor with two components(simplifying a lot): one negative "dark" energy (pressure) and one "gravitational" positive energy pressure?
Er, dark energy must have a positive energy density to produce an accelerated expansion.AWA said:It's interesting, if a bit radical. In the past there have been attempts along those lines with negative and positive gravity or with inertia versus gravity(de Sitter) but they were all turned down because they seemed to bring up unphysical concepts like "negative energy".Since 1998 with the accelerated expansion surprise and "dark energy" there is more going in that direction.
No, the tensor remains exactly the same. This would just be a way of talking about gravitational potential energy.AWA said:Ok, and wouldn't adding that new made up quantity change anything in the tensor,at least conceptually?