What is the canonical form of the metric?

In summary, the canonical form of the metric, as described by Sean M Carroll in his book "Spacetime and Geometry: An Introduction to General Relativity", is a diagonal matrix with ±1 in each component, representing a non-degenerate metric. This form has the same range of indices as any other form and is commonly used in physics even if it technically represents a pseudo-metric.
  • #1
George Keeling
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I am reading Spacetime and Geometry : An Introduction to General Relativity – by Sean M Carroll and he writes:
Quote: A useful characterisation of the metric is obtained by putting ##g_{\mu\nu}## into its canonical form. In this form the metric components become $$ g_{\mu\nu} = \rm{diag} (-1, -1,...-1,+1,+1, ... +1,0,0, ... ,0) $$where "diag" means a diagonal matrix with the given elements. End quote.

Wikipedia tells me to "Write ## \rm{diag} (a_1, ..., a_n)## for a diagonal matrix whose diagonal entries starting in the upper left corner are ##a_1, ..., a_n##." So Carroll's expression seems to imply a diagonal matrix with with a minimum size 9x9 and one extra row and column wherever one of his .'s takes a value. Or something like $$\begin{pmatrix}
-1 & 0 & 0 & 0 & 0 & 0 & 0 & 0 & . & 0 \\
0 & -1 & 0 & 0 & 0 & 0 & 0 & 0 & . & 0 \\
. & . & . \\
0 & 0 & 0 & 0 & -1& 0 & 0 & 0 & . & 0 \\
0 & 0 & 0 & 0 & 0 & 1 & 0 & 0 & . & 0 \\
. & . & .
\end{pmatrix}$$ In general Carroll does not assume that ##\mu,\nu## have a range such as 1,2,3 or 0,1,2,3 until he gets to examples which are much simpler.

I don't think my interpretation is correct. Can anybody cast any light for me?
 
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  • #2
He means exactly the same thing as the wiki article.
 
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  • #3
George Keeling said:
So Carroll's expression seems to imply a diagonal matrix with with a minimum size 9x9 and one extra row and column wherever one of his .'s takes a value.
No, this is not what is intended. Each set of numbers (-1,1,0) can correspond to any quantity of that number. For a non-degenerate metric there would be no zeros and for an actual metric (defined as positive definite) there would be only ones. For a Lorentzian metric (one time-like direction), there would be one -1 and the rest of the diagonals would be 1.
 
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  • #4
The canonical form of the metric has the same range of indices as any other form - four for relativity. Carroll is using ##-1,\ldots,-1## to mean "some number, possibly zero, possibly more, of -1s". In relativity the canonical form of the metric has three -1s, one +1, and no zeros (though sign conventions do vary!).
 
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  • #5
I like #3 and #4 so I get $$
\begin{pmatrix}
-1 & 0 & 0 & 0 \\
0 & 1 & 0 & 0 \\
0 & 0 & 1 & 0 \\
0 & 0 & 0 & 1
\end{pmatrix} $$ perhaps Carroll would have been clearer had he written $$ g_{\mu\nu} = \rm{diag} (-1, 0,1,...-1, 0,1, ... -1, 0,1, ... ,-1, 0,1) $$ Thanks!
 
  • #6
That would have been wrong and very unclear.
 
  • #7
Does this work?
As a matrix, a non-degenerate metric in canonical form is diagonal with ±1 in each component.
 
  • #8
George Keeling said:
Does this work?
As a matrix, a non-degenerate metric in canonical form is diagonal with ±1 in each component.
Technically, that would be a pseudo-metric unless you have +1 in all diagonals, but in physics we just call it metric anyway.
 
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  • #9
This
$$
\begin{pmatrix}
-1 & 0 & 0 & 0 \\
0 & 1 & 0 & 0 \\
0 & 0 & 1 & 0 \\
0 & 0 & 0 & 1
\end{pmatrix} $$
and this
$$ g_{\mu\nu} = \rm{diag} (-1, 1, 1,1) $$
are the same.
 
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1. What is the canonical form of the metric?

The canonical form of the metric is a specific mathematical representation of the metric tensor, which describes the geometry of space and time in the theory of general relativity. It is expressed as a diagonal matrix with coefficients that depend on the coordinates used to describe the space-time. It is also known as the Minkowski metric or the flat metric.

2. Why is the canonical form of the metric important?

The canonical form of the metric is important because it simplifies the calculations and equations used in general relativity. It allows for a clearer understanding of the geometry of space and time and makes it easier to solve problems and make predictions based on the theory.

3. How is the canonical form of the metric derived?

The canonical form of the metric is derived using the principle of covariance, which states that the laws of physics should be the same for all observers regardless of their frame of reference. By applying this principle to the equations of general relativity, the metric can be transformed into a simpler, diagonal form.

4. Can the canonical form of the metric be changed?

Yes, the canonical form of the metric can be changed by using different coordinate systems or by introducing additional terms to the metric tensor. However, the transformed metric must still satisfy the principles of general relativity and accurately describe the geometry of space and time.

5. How does the canonical form of the metric differ from the Euclidean metric?

The canonical form of the metric differs from the Euclidean metric in that it takes into account the curvature of space and time caused by the presence of massive objects. The Euclidean metric assumes a flat, non-curved space and time, while the canonical form of the metric allows for the effects of gravity to be included in the equations of general relativity.

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