Components of Einstein's Equations in 4 dimensions

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Discussion Overview

The discussion centers around the interpretation of the independent equations in Einstein's equations within the context of four-dimensional spacetime. Participants explore the implications of these equations, their physical representation, and the degrees of freedom associated with the metric tensor.

Discussion Character

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

Main Points Raised

  • One participant cites Sean M. Carroll's notes, explaining that Einstein's equations can be viewed as second-order differential equations for the metric tensor field, leading to ten equations but only six independent ones due to constraints from the Bianchi identity.
  • Another participant expresses confusion regarding the physical representation of the six independent equations, initially associating them with spatial and temporal coordinates.
  • A participant clarifies that the indices in the equations correspond to 16 components, which are reduced to six independent equations after accounting for constraints.
  • There is a suggestion that the six equations may describe the time evolution of the spatial portions of the metric, referred to as "propagating the 3-metric."
  • One participant discusses the degrees of freedom in General Relativity (GR), suggesting that the number can be derived from the components of the metric tensor and various constraints, leading to a total of two degrees of freedom.
  • Another participant notes that understanding degrees of freedom may not yield a unique interpretation, comparing it to different ways of defining a point in space.
  • There is a proposal that exploring the corresponding question for Maxwell's equations might provide useful physical insight.
  • A later reply indicates that one participant is beginning to grasp the concepts discussed, suggesting a progression in understanding.

Areas of Agreement / Disagreement

Participants express varying levels of understanding regarding the physical implications of the six independent equations, with some seeking clarification while others provide insights. No consensus is reached on a definitive interpretation of these equations.

Contextual Notes

Participants highlight the complexity of interpreting the degrees of freedom and the physical meaning of the equations, indicating that the discussion may involve assumptions and definitions that are not fully resolved.

Airsteve0
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In this excerpt from the notes of Sean M. Carrol, he says:

"Einstein’s equations may be thought of as second-order differential equations for the
metric tensor field gμν. There are ten independent equations (since both sides are symmetric
two-index tensors), which seems to be exactly right for the ten unknown functions of the
metric components. However, the Bianchi identity ∇μGμν = 0 represents four constraints on
the functions Rμν, so there are only six truly independent equations in (4.52). In fact this is
appropriate, since if a metric is a solution to Einstein’s equation in one coordinate system
xμ it should also be a solution in any other coordinate system xμ′ . This means that there are
four unphysical degrees of freedom in gμν (represented by the four functions xμ′ (xμ)), and
we should expect that Einstein’s equations only constrain the six coordinate-independent
degrees of freedom."


R_{\mu\nu}-\frac{1}{2}Rg_{\mu\nu}=8\piGT_{\mu\nu} (Eq. 4.52)

I am confused as to what the 6 independent equations represent. I'm getting lost on thinking that these equations represent 3 spatial coordinates and 1 time coordinate but then what do the other 2 components represent (obviously my understanding is flawed). Any clarification would be greatly appreciated, thanks.
 
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Airsteve0 said:
I'm getting lost on thinking that these equations represent 3 spatial coordinates and 1 time coordinate but then what do the other 2 components represent (obviously my understanding is flawed). Any clarification would be greatly appreciated, thanks.

The indices mu and nu *each* take on 4 values, so it's 16 equations, not 4, until you start subtracting out the ones that aren't independent.
 
Ok, so once you get down to the 6 which are independent, what do these represent physically?
 
I've read that these 6 equations "propagate the 3-metric", if this is correct does this mean they describe time evolution of the spatial portions of the metric?
 
Somehow related, IIRC the nr of DOF of GR is 2 and can be obtained in Lagrange formulation as 16 components of metric tensor - 6 because of symmetry of the tensor - 4 from the metricity condition (\nabla_{\mu} g^{\mu\nu} = 0) - 4 from the Noether identities (\nabla_{\mu} G^{\mu\nu} = 0) = 2, with G the Einstein tensor. In the Hamiltonian formulation, it's 16-6-8 first class constraints = 2.
Going into quantum mechanics, this 2 are two possible eigenvalues of the 3rd component of the helicity operator, namely -2 and +2.
 
thank you for the reply but I feel this is slightly more advanced than what I was looking for in my last question; I am more so looking for an understanding of what the 6 equations physically represent.
 
Think about it, what do the Newton's equations represent ? It's the same for the EFE, they are PDE's whose solutions are the components of the metric tensor of the 4D spacetime in the canonical basis.
 
Airsteve0 said:
thank you for the reply but I feel this is slightly more advanced than what I was looking for in my last question; I am more so looking for an understanding of what the 6 equations physically represent.

When you count degrees of freedom, you don't necessarily get a unique interpretation. For example, I could define a point in space using (x,y,z), or by giving latitude, longitude, and height above sea level.

So the best we can hope for here is at least one story that successfully accounts for why we have a certain number of d.f.

For physical insight, maybe it would be helpful if we could work out the answer to the corresponding question for Maxwell's equations.
 
I think I am starting to understand, thank you bcrowell and dextercioby.
 

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