General Relativity: Contracting Indices

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In summary,The two equations that the author was discussing are:$$ -\frac{1}{2}( {\Gamma}^{\sigma}_{\sigma}+{{\Gamma}^{\sigma}_{\sigma\rho}} ) \mathrm{g}^{\mu\nu} &=0,\tag1 \\ \mathrm{g}^{[\mu\nu]}_{,\nu} -\frac{1}{2}( {\Gamma}^{\r
  • #1
direct99
9
0
Hello,

I was reading a book about general relativity and I came across these two equations

$$ \begin{align}
\mathrm{g}^{\mu\nu}_{,\rho}+
\mathrm{g}^{\sigma\nu}{\Gamma}^{\mu}_{\sigma\rho}+
\mathrm{g}^{\mu\sigma}{\Gamma}^{\nu}_{\rho\sigma}
-\frac{1}{2}(
{\Gamma}^{\sigma}_{\sigma}+{{\Gamma}^{\sigma}_{\sigma\rho}}
)
\mathrm{g}^{\mu\nu}
&=0,
\tag1
\\
\mathrm{g}^{[\mu\nu]}_{,\nu}
-\frac{1}{2}(
{\Gamma}^{\rho}_{\rho\nu}+{\Gamma}^{\rho}_{\nu\rho}
)
\mathrm{g}^{(\mu\nu)}
&=0,
\tag2
\end{align}
$$

and it says that by contracting equation (1) once with respect to ($\mu,\rho$), then with respect to ($\nu,\rho$), then subtracting the resulting equations we can get equation (2), however I can't see how that's possible.
Also, This connection is not symmetric with respect to the lower Indices
 
Last edited:
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  • #2
It breaks down into two parts, one part for the terms with only the derivatives of the metric, and one for the terms that involve the metric contracted with the Christoffel symbols. I did the first part and it worked out. Want to try that part and post what you get? Then we could move on to the second part. Remember that when an index is summed over, you're free to rename it to whatever you like.
 
  • #3
Well, when contracting with respect to μ and ρ I get:
$$
-\frac{1}{2} g^{\rho \nu } {\Gamma} _{a\rho}^{a}-\frac{1}{2} g^{\rho
\nu} \Gamma _{\rho a}^{a}+g^{a\nu} \Gamma _{a\rho}^{\rho}+g^{\rho a} \Gamma _{\rho a}^{\nu}+g_{,\rho}^{\rho\nu}=0
$$
and when contracting with respect to nu and ρ I get:
$$
-\frac{1}{2} g^{\mu \rho } \Gamma _{a\rho}^a-\frac{1}{2} g^{\mu
\rho} \Gamma _{\rho a}^a+g_{}^{a\rho } \Gamma _{a\rho}^{\mu }+g^{\mu a} \Gamma _{\rho a}^{\rho
}+g_{,\rho }^{\mu \rho }=0
$$
when subtracting these two equations I get:
$$
\frac{1}{2} g_{}^{\mu \rho } \Gamma _{a\rho }^a-\frac{1}{2} g_{}^{\rho
\nu } \Gamma _{a\rho }^a+\frac{1}{2} g_{}^{\mu \rho } \Gamma
_{\rho a}^a-\frac{1}{2} g_{}^{\rho \nu } \Gamma _{\rho
a}^a+g_{}^{a\nu } \Gamma _{a\rho }^{\rho
}-g_{}^{a\rho } \Gamma _{a\rho }^{\mu }-g_{}^{\mu a}
\Gamma _{\rho a}^{\rho }+g_{}^{\rho a} \Gamma _{\rho
a}^{\nu }-g_{,\rho }^{\mu \rho }+g_{,\rho }^{\rho \nu }=0
$$
I can't see how this is equal to equation (2).
 
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  • #4
How to get equation (2) from

$$
\frac{1}{2} g_{}^{\mu \rho } \Gamma _{a\rho }^a-\frac{1}{2} g_{}^{\rho
\nu } \Gamma _{a\rho }^a+\frac{1}{2} g_{}^{\mu \rho } \Gamma
_{\rho a}^a-\frac{1}{2} g_{}^{\rho \nu } \Gamma _{\rho
a}^a+g_{}^{a\nu } \Gamma _{a\rho }^{\rho
}-g_{}^{a\rho } \Gamma _{a\rho }^{\mu }-g_{}^{\mu a}
\Gamma _{\rho a}^{\rho }+g_{}^{\rho a} \Gamma _{\rho
a}^{\nu }-g_{,\rho }^{\mu \rho }+g_{,\rho }^{\rho \nu }=0
$$
 
  • #5
For now let's concentrate on the terms that have derivatives of the metric in them. The way you've done it, you end up with something ungrammatical. In your expression

$$
-g_{,\rho }^{\mu \rho }+g_{,\rho }^{\rho \nu }=0
$$

you have a term with an upper μ index and a term with an upper ν index. You can't add terms that are written in this way. This tells you that you should rename your ρ indices before doing the subtraction.
 
  • #6
bcrowell said:
For now let's concentrate on the terms that have derivatives of the metric in them. The way you've done it, you end up with something ungrammatical. In your expression

$$
-g_{,\rho }^{\mu \rho }+g_{,\rho }^{\rho \nu }=0
$$

you have a term with an upper μ index and a term with an upper ν index. You can't add terms that are written in this way. This tells you that you should rename your ρ indices before doing the subtraction.

so are you saying that

$$
-g_{,\rho }^{\mu \rho }+g_{,\rho }^{\rho \nu }=0
$$
should be something like
$$
-g_{,\sigma }^{\mu \sigma }+g_{,\rho }^{\rho \nu }=0
$$
If so does this mean that its equivalent to
$$
g_{,\nu }^{[\mu \nu ]}=0
$$
 
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Related to General Relativity: Contracting Indices

1. What is General Relativity?

General Relativity is a theory of gravitation that was developed by Albert Einstein in the early 20th century. It explains the relationship between matter and space-time and describes how objects with mass interact with each other.

2. What are contracting indices in General Relativity?

Contracting indices refer to the mathematical operation of contracting or summing over repeated indices in an equation. In General Relativity, this operation is used to simplify and solve equations involving the curvature of space-time.

3. How do contracting indices relate to the principle of equivalence?

The principle of equivalence states that the effects of gravity and acceleration are indistinguishable. Contracting indices in General Relativity help to show how the curvature of space-time, which is caused by massive objects, can also account for the effects of gravity.

4. What is the significance of contracting indices in General Relativity?

Contracting indices are an essential aspect of General Relativity as they allow for the development of equations that accurately describe the behavior of matter and energy in a curved space-time. They also help to simplify complex equations and make them easier to solve.

5. Are there any real-world applications of contracting indices in General Relativity?

Yes, contracting indices are used extensively in the field of cosmology to study the structure and evolution of the universe. They are also used in the development of technologies such as GPS, which rely on the principles of General Relativity for accurate positioning and timekeeping.

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