Clearing Up Confusion: G_{\mu\nu} Explained

  • Thread starter John_Doe
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So, the result is a matrix with elements of the form g_{\alpha\beta}g^{\gamma\delta} and the indices are completely free indices.
  • #1
John_Doe
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Dumb question, but...

[itex]G_{\mu\nu}=R_{\mu\nu}-\frac{1}{2} g_{\mu\nu}R[/itex]

Since

[itex]R=g^{\mu\nu}R_{\mu\nu}[/itex]

and

[itex]g^{\mu\nu}g_{\mu\nu}=1[/itex]

it would appear that

[itex]
G_{\mu\nu}
=R_{\mu\nu}-\frac{1}{2} g_{\mu\nu}g^{\alpha\beta}R_{\alpha\beta}
=R_{\mu\nu}-\frac{1}{2} g_{\mu\nu}g^{\mu\beta}g_{\mu\beta}g^{\alpha\beta}R_{\alpha\beta}
=R_{\mu\nu}-\frac{1}{2} \delta^{\beta}_{\nu}\delta^{\alpha}_{\mu}R_{\alpha\beta}
=R_{\mu\nu}-\frac{1}{2} R_{\mu\nu}
=\frac{1}{2} R_{\mu\nu}
[/itex]

which cannot be correct. I would be very grateful if someone could clear this up for me. Thank you in advance.
 
Last edited:
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  • #2
John_Doe said:
[itex]
G_{\mu\nu}=R_{\mu\nu}-\frac{1}{2} g_{\mu\nu}g^{\alpha\beta}R_{\alpha\beta}
R_{\mu\nu}-\frac{1}{2} g_{\mu\nu}g^{\mu\beta}g_{\mu\beta}g^{\alpha\beta}R_{\alpha\beta}
[/itex]

your [tex]\mu \nu[/tex] indices don't match on both side of equation.. check that first and foremost
btw, don't mix fixed indices [tex]\mu \nu[/tex] with the summation indices.
 
Last edited:
  • #3
Yeah - there should be an = there so that it's
[itex]G_{\mu\nu}
=R_{\mu\nu}-\frac{1}{2} g_{\mu\nu}g^{\alpha\beta}R_{\alpha\beta}
=R_{\mu\nu}-\frac{1}{2} g_{\mu\nu}g^{\mu\beta}g_{\mu\beta}g^{\alpha\beta}R _{\alpha\beta}[/itex]
Then the metric tensors contract, yielding the kronecker deltas. I'm not sure where the mistake is.
 
Last edited:
  • #4
[itex]g^{\mu\nu}g_{\mu\nu}=1[/itex] No. It equals 4. Assuming you are in dimension 4. It's a trace.
 
  • #5
John_Doe said:
Yeah - there should be an = there so that it's
[itex]G_{\mu\nu}
=R_{\mu\nu}-\frac{1}{2} g_{\mu\nu}g^{\alpha\beta}R_{\alpha\beta}
=R_{\mu\nu}-\frac{1}{2} g_{\mu\nu}g^{\mu\beta}g_{\mu\beta}g^{\alpha\beta}R _{\alpha\beta}[/itex]
Then the metric tensors contract, yielding the kronecker deltas. I'm not sure where the mistake is.

in the second step you are contracting [tex]\mu[/tex] (confusing choice of symbol) with the wrong metric tensor, note as I pointed out before [tex]\mu, \nu[/tex] are not summation indices. If in doubt always put back in the summation signs and write things out in components.
 
  • #6
Thank you very much, except now I seem to have

[tex]g_{\mu\alpha}g^{\mu\beta}=\delta_{\alpha}^{\beta}=\left\{\begin{array}{cc}1,&\mbox{ if }
\alpha=\beta\\0, & \mbox{ if } \alpha\neq\beta\end{array}\right.[/tex]

but also

[tex]g_{\mu\nu}g^{\mu\nu}=4[/tex]

Marginal confusion there... and I also don't quite understand why it matters which tensors the contraction is done on, other than you get the wrong answer.

All help is appreciated, thank you.
 
  • #7
[tex]g_{\mu\alpha}g^{\mu\beta}=\delta_{\alpha}^{\beta}= \left\{\begin{array}{cc}1,&\mbox{ if }\alpha=\beta\\0, & \mbox{ if } \alpha\neq\beta\end{array}\right.[/tex]
is wrong. As Dick pointed out, for any tensor [itex]A^{ij}[/itex], [itex]A_{ij}A^{ij}[/itex] is the trace of A.
 
  • #8
I'm sorry, but you've lost me there. It's not equal to [tex]\delta_{\alpha}^{\beta}[/tex]?

I thought that [tex]g^{\mu\nu}[/tex] was defined as the inverse of the [tex]g_{\mu\nu}[/tex]. After all, [tex]g^{\mu\nu}=\frac{G(\mu,\nu)}{g}[/tex] if [tex]G(\mu,\nu)[/tex] denotes the cofactors of [tex]g_{\mu\nu}[/tex] and [tex]g = |g_{\mu\nu}|[/tex].

Edit:
Taking into account corrections,
[itex]
G_{\mu\nu}
=R_{\mu\nu}-\frac{1}{2} g_{\mu\nu}g^{\alpha\beta}R_{\alpha\beta}
=R_{\mu\nu}-\frac{1}{8} g_{\mu\nu}g^{\mu\beta}g_{\mu\beta}g^{\alpha\beta}R _{\alpha\beta}
=R_{\mu\nu}-\frac{1}{8} \delta^{\beta}_{\nu}\delta^{\alpha}_{\mu}R_{\alpha \beta}
=R_{\mu\nu}-\frac{1}{8} R_{\mu\nu}
=\frac{7}{8} R_{\mu\nu}
[/itex]
 
Last edited:
  • #9
It's still not okay. You must not use the same index both as "dummy index" and as summation index, and here i mean "\mu" and must not use the same index twice as a summation index, and here i mean "\beta".
 
  • #10
[itex]
G_{\mu\nu}
=R_{\mu\nu}-\frac{1}{2} g_{\mu\nu}g^{\alpha\beta}R_{\alpha\beta}
=R_{\mu\nu}-\frac{1}{8} g_{\mu\nu}g^{\sigma\tau}g_{\sigma\tau}g^{\alpha\beta}R _{\alpha\beta}
[/itex]

So all the working here is now correct, even if it doesn't help in the slightest? That's a good thing. Thank you all very much.
 
  • #11
Yes, it's now correct. But it doesn't say very much, just 4*(1/8)=1/2. What were you trying to prove to begin with?
 
  • #12
No, it just seemed to me at first, by eye, that the equation should simpllify, which is obviously wrong. It's not supposed to say much now - I'm just insterested in the fact that all the working is now correct.

Except, one last thing: what if I have

[tex]g_{\alpha\beta}g^{\gamma\delta}[/tex]

and each of the indices does not appear anywhere else in the equation? Shouldn't [itex]\alpha=\gamma[/itex] and [itex]\beta=\delta[/itex]?
 
  • #13
No, why would they they have to be like that ? Notice it's just a tensor product. 2 2-nd rank tensors multiplied yeilding a (2,2) 4-th rank tensor.
 

1. What is G_{\mu\nu}?

G_{\mu\nu} is the Einstein tensor, which is used in Einstein's field equations to describe the curvature of spacetime in general relativity. It is a mathematical object that represents the relationship between matter and energy and the geometry of the universe.

2. How is G_{\mu\nu} related to gravity?

G_{\mu\nu} is a key component in Einstein's field equations, which describe how matter and energy influence the curvature of spacetime. This curvature is what we experience as gravity.

3. What do the indices in G_{\mu\nu} represent?

The indices in G_{\mu\nu} represent the four dimensions of spacetime - three spatial dimensions (x, y, z) and one temporal dimension (t). The Greek letters μ and ν are used to denote these dimensions.

4. How is G_{\mu\nu} calculated?

G_{\mu\nu} is calculated using a mathematical formula that involves the energy and momentum of matter and the curvature of spacetime. It is a complex calculation that requires advanced mathematical techniques and is used in theoretical physics and cosmology.

5. Why is understanding G_{\mu\nu} important?

Understanding G_{\mu\nu} is important because it is a fundamental concept in general relativity, which is a key theory in modern physics. It helps us understand the relationship between matter, energy, and the geometry of the universe, and has implications for our understanding of gravity and the behavior of the universe on a large scale.

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