Confusion over Einstein summation convention and metric tensors.

Lyalpha
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My understanding of the Einstein Summation convention is that you sum over the repeated indices. But when I look at the metric tensor for a flat space I know that

g^{λ}_{λ} = 1

But the summation convention makes me think that it should equal the trace of the matrix g_{μσ}. So it should be the number of dimensions of the space?
 
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g_{\alpha}^{\; \alpha} = N where N is the dimension of the space. Why do you think it's 1?
 
A^{\nu} = g^{μ \nu}A_{μ}

A_{μ} = g_{μ\nu}A^{\nu}

A_{μ} = g_{μ\nu}g^{\nu\rho}A_{\rho}

g_{μ\nu}g^{\nu\rho} = g^{\rho}_{\mu}

g^{\rho}_{\mu} = 1 for μ = ρ

g^{\rho}_{\mu} = 0 for μ \neq ρ

taken from Dirac's book
 
Yes but g^{\rho}_{\mu} is not a summation. It simply indicates what the components are. So it's saying when \rho = \mu, the component is 1, else it is 0. However, g^{\rho}_{\rho} = \sum^{N}_{\alpha = 1} g_{\alpha}^{\alpha}.

It's like how sometimes people get confused with the delta function \delta_{ij}. In a 3-dimensional space, you can have \delta_{ij} = 1 if i=j, else it is 0. However, this is different from \delta_{ii} which is the actual summation which is equal to 3.
 
ok thanks
 
I asked the question because I'm getting g^{λ}_{λ} after some contractions of a certain curvature tensor. For Example I have a term g^{μ}_{σ} and I'm contracting the tensor by setting μ and σ to λ. The term will now equal the dimension D?
 
Yes it will equal D if you're contracting the metric in the way you asked. This is true only for the metric, however.
 
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Not in general. If g_{\mu \nu } = \delta _{\mu \nu } on the n - manifold in question then g^{\lambda }_{\lambda } = \delta ^{\lambda }_{\lambda } = n. But this doesn't have to be true for arbitrary metrics on their respective manifolds.
 
WannabeNewton said:
Not in general. If g_{\mu \nu } = \delta _{\mu \nu } on the n - manifold in question then g^{\lambda }_{\lambda } = \delta ^{\lambda }_{\lambda } = n. But this doesn't have to be true for arbitrary metrics on their respective manifolds.

No, in general (at least in GR, I don't know about some really weird cases or w/e),

g^\mu_\nu=\delta^\mu_\nu

This is because the contravariant metric must be the inverse of the covariant metric. The two must be inverses of each other or else you won't get the same vector back if you lower it's indices and then raise them.

The trace of the Kronecker delta is obviously the dimension, and therefore so is the trace of the (1,1) form of the metric.
 
  • #10
WannabeNewton said:
Not in general. If g_{\mu \nu } = \delta _{\mu \nu } on the n - manifold in question then g^{\lambda }_{\lambda } = \delta ^{\lambda }_{\lambda } = n. But this doesn't have to be true for arbitrary metrics on their respective manifolds.

No, in general it is true if g_{ab} and g^{ab} are inverses of each other. Remember, g_{a}^{a} = \sum_{i,j=1}^N g_{ij}g^{ij} =N
 
  • #11
Well it still isn't true in general because what if g isn't diagonal. But yeah I get your point if g is diagonal.
 
  • #12
Lyalpha said:
But when I look at the metric tensor for a flat space I know that

g^{λ}_{λ} = 1

ORLY? Where did you see that?
 
  • #13
WannabeNewton said:
What if g is non - diagonal?

This is in general, the metric does not need to be diagonal since g_{ab} and g^{ab} by definition are inverses of each other. If g^{ab} is the inverse of g_{ab}, then by definition, g_a^b = \sum_{i=1}^n g_{ai}g^{ib} = \delta_{ab}. Remember, this g_a^b component is a n-term summation and the inverse metric must be defined so this is true.
 
  • #14
But what if it's the fundamental metric tensor? Where g_{00} is -1 and the rest are 1? Would I get D-2 ?
 
  • #15
WannabeNewton said:
Well it still isn't true in general because what if g isn't diagonal. But yeah I get your point if g is diagonal.

Here:

A_\mu=g_{\mu\nu}A^\nu

A^\mu=g^{\mu\nu}A_\nu

Which implies:

A^\mu=g^{\mu\nu}g_{\nu\tau}A^\tau

If it is true that A^\mu=\delta^\mu_\tau A^\tau

Then it must be that:

g^{\mu\nu}g_{\nu\tau}=g^\mu_\tau=\delta^\mu_\tau
 
  • #16
Lyalpha said:
But what if it's the fundamental metric tensor? Where g_{00} is -1 and the rest are 1? Would I get D-2 ?

No, you can only trace the (1,1) form of the metric. You can't trace the purely covariant metric. the (1,1) form of the metric, almost by definition, MUST be diag(1,1,1,1...). See my proof above.
 
  • #17
Pengwuino said:
This is in general, the metric does not need to be diagonal since g_{ab} and g^{ab} by definition are inverses of each other.

So you're telling me that for the metric g_{\mu \nu } = \begin{pmatrix}<br /> 1 + 4c^{2}p^{2} &amp; 2cp\\ <br /> 2cp &amp; 1<br /> \end{pmatrix} that g_{\mu \nu }g^{\mu \nu } = 2 (c = const.).
 
  • #18
WannabeNewton said:
So you're telling me that for the metric g_{\mu \nu } = \begin{pmatrix}<br /> 1 + 4c^{2}p^{2} &amp; 2cp\\ <br /> 2cp &amp; 1<br /> \end{pmatrix} that g_{\mu \nu }g^{\mu \nu } = 2 (c = const.).

Yes. And this is because the inverse metric must be defined such that it is true. The inverse for that metric won't just look like 1 over the components of the metric because that does not satisfy g_{am}g^{mb} = \delta_{ab}
 
  • #19
Yes, WannabeNewton, see my previous proof...why does this bother you?
 
  • #20
yeah my bad forgot to include 2g_{12}g^{12} lol
 
  • #21
I'm starting with a conformally flat space with the interval ds^{2} = e^{2φ} η_{ab} dx^{a} dx^{b} , where \eta_{ab} is a fundamental metric tensor of D-dimensional flat space. I'm trying to find the usual stuff (Christoffel symbols, curvature tensor, ricci tensor, curvature scalar). When it comes to contracting the curvature tensor I get a few \eta^{c}_{c} terms. What would they be in the case I described?
 
  • #22
Lyalpha said:
I'm starting with a conformally flat space with the interval ds^{2} = e^{2φ} η_{ab} dx^{a} dx^{b} , where \eta_{ab} is a fundamental metric tensor of D-dimensional flat space. I'm trying to find the usual stuff (Christoffel symbols, curvature tensor, ricci tensor, curvature scalar). When it comes to contracting the curvature tensor I get a few \eta^{c}_{c} terms. What would they be in the case I described?

It's D. You know what the components of the metric and inverse metric are for such a simple case. Do the actual summation for even D = 2 and you'll see \eta_n^{\; n} = D
 
  • #23
But isn't \eta^{n}_{n} equal to \eta^{0}_{0} + \eta^{1}_{1} + \eta^{2}_{2} + ... + \eta^{D}_{D} where \eta^{0}_{0} = -1 and \eta^{1}_{1}, \eta^{2}_{2}, \eta^{D}_{D} are 1?
 
  • #24
Lyalpha said:
But isn't \eta^{n}_{n} equal to \eta^{0}_{0} + \eta^{1}_{1} + \eta^{2}_{2} + ... + \eta^{D}_{D} where \eta^{0}_{0} = -1 and \eta^{1}_{1}, \eta^{2}_{2}, \eta^{D}_{D} are 1?

No \eta_{00} = -1 but \eta_0^0 = 1. \eta_0^0 = \sum_{i=0}^D \eta_{0i}\eta^{i0} = 1
 
  • #25
Lyalpha said:
But what if it's the fundamental metric tensor? Where g_{00} is -1 and the rest are 1? Would I get D-2 ?

Careful with the negative signs. -12+12+12+12=4=D
 
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