Confusion over Einstein summation convention and metric tensors.

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Discussion Overview

The discussion revolves around the Einstein summation convention and its application to metric tensors in various contexts, including flat spaces and curvature tensors. Participants explore the implications of the convention on the trace of the metric tensor and the conditions under which certain identities hold true.

Discussion Character

  • Debate/contested
  • Technical explanation
  • Mathematical reasoning

Main Points Raised

  • Some participants assert that the Einstein summation convention implies summing over repeated indices, leading to confusion regarding the trace of the metric tensor.
  • One participant claims that for a flat space, the trace of the metric tensor should equal the number of dimensions, while another argues it equals 1.
  • Participants discuss the implications of contracting the metric tensor and how it relates to the dimension of the space.
  • There are claims that the trace of the Kronecker delta equals the dimension, suggesting that similar reasoning applies to the metric tensor.
  • Some participants emphasize that the relationship between covariant and contravariant metrics does not necessarily hold for non-diagonal metrics.
  • Concerns are raised about the validity of certain assumptions when dealing with fundamental metric tensors that have mixed signs.
  • One participant mentions a specific example of a conformally flat space and queries about the resulting terms when contracting the curvature tensor.
  • Discussions include the need to carefully consider the signs and values of components in the metric tensor when calculating traces.

Areas of Agreement / Disagreement

Participants express differing views on the implications of the Einstein summation convention and the properties of metric tensors. There is no consensus on whether the trace of the metric tensor equals the dimension of the space in all cases, and discussions remain unresolved regarding the conditions under which specific identities hold.

Contextual Notes

Participants highlight that the behavior of the metric tensor can vary significantly based on its structure (diagonal vs. non-diagonal) and the specific definitions used in different contexts. There are unresolved mathematical steps and assumptions regarding the properties of the metric tensor and its components.

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.
 
Last edited:
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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