First algebraic Bianchi identity of Riemann tensor (cyclic relation)

In summary, the conversation discusses the difficulty in finding a proof for $R_{a[bcd]}=0$ using the symmetries of $R_{ab(cd)]}=R_{(ab)cd}=0$ and $R_{[ab][cd]}=0$. The conversation concludes that the proof likely involves one of the symmetries mentioned and the second covariant Bianchi identity. However, there is also a more high-brow approach using the Jacobi identity and acting on an arbitrary scalar field or vector field. This method also requires the definition of the Riemann tensor.
  • #1
binbagsss
1,254
11
I am guessing that:

$R_{a[bcd]}=0$

can not be derived from the symmetries of

$R_{ab(cd)]}=R_{(ab)cd}=0$

$R_{[ab][cd]}=0$ ?Sorry when I search the proof for it I can not find much, it tends to come up with the covariant Bianchi instead.

I am guessing it will need one of the symmetries above (at least) and the second covariant Bianchi identity to prove it?

Thanks
 
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  • #2
* one of the symmetries above (at least) and either the second second Bianchi identity/ def of the Riemann tensor- basically will need involvement of the metric to prove? Thanks.
 
  • #3
binbagsss said:
$$R_{a[bcd]}=0$$ [...]
Sorry when I search the proof for it I can not find much, it tends to come up with the covariant Bianchi instead.

I am guessing it will need one of the symmetries above (at least) and the second covariant Bianchi identity to prove it?
It's easy to prove by brute force, using just the skewsymmetry on the last 2 indices, since the latter means that ##R_{a[bcd]}=0## can be re-written as $$R^a_{~bcd} + R^a_{~cdb} + R^a_{~dbc} = 0 ~.$$ Then just write out the LHS in full. It's not that hard. You'll find that everything cancels to zero, provided ##\Gamma## is symmetric in its lower indices.
 
  • #4
strangerep said:
It's easy to prove by brute force... provided ##\Gamma## is symmetric in its lower indices.
that's what I meant. So yeh it does need the definition of the tensor. that's all I was looking for, thanks.
 
  • #5
binbagsss said:
that's what I meant. So yeh it does need the definition of the tensor. that's all I was looking for, thanks.
What tensor? It doesn't need the definition of the metric tensor.
 
  • #6
strangerep said:
What tensor? It doesn't need the definition of the metric tensor.
the Riemann as a function of the metric/connection I meant.
 
  • #7
binbagsss said:
the Riemann as a function of the metric/connection I meant.
Oh, I see.

There is a more high-brow way to derive the identity. Start from the Jacobi identity $$[A,[B,C]] + [B,[C,A]] +[C,[A,B]] ~=~ 0 ~,$$and replace the A,B,C with ##\nabla## operators, e.g., ##\nabla_a##, etc. Then let the LHS act on an arbitrary scalar field ##\phi##. You'll get terms like a commutator acting on ##\nabla_? \phi##, and ##\nabla_? \phi## can be treated as a covector. So that gives you 3 terms involving the Riemann tensor. The other terms have ##[\nabla_a, \nabla_b] \phi## but these just involve the torsion, hence they vanish in a torsionless theory. That should give you the 1st Bianchi identity.

The 2nd Bianchi identity can be derived in a similar way, by acting with the Jacobi identity on an arbitrary vector field ##V^\alpha## instead the scalar field ##\phi##.
 
  • #8
strangerep said:
Oh, I see.

There is a more high-brow way to derive the identity. Start from the Jacobi identity $$[A,[B,C]] + [B,[C,A]] +[C,[A,B]] ~=~ 0 ~,$$and replace the A,B,C with ##\nabla## operators, e.g., ##\nabla_a##, etc. Then let the LHS act on an arbitrary scalar field ##\phi##.
which uses the definition of the Riemann tensor. my question was answered, as I said.
 

What is the first algebraic Bianchi identity of Riemann tensor?

The first algebraic Bianchi identity of Riemann tensor, also known as the cyclic relation, is a mathematical expression that relates the components of the Riemann tensor, which is a geometric object used to describe the curvature of a manifold in differential geometry.

Why is the first algebraic Bianchi identity important?

The first algebraic Bianchi identity is important because it is a fundamental property of the Riemann tensor that allows us to understand the geometric properties of a manifold, such as its curvature and topology. It is also used in various mathematical and physical applications, such as in general relativity and differential geometry.

How is the first algebraic Bianchi identity derived?

The first algebraic Bianchi identity can be derived from the definition of the Riemann tensor and the properties of covariant derivatives. It is a consequence of the symmetry and antisymmetry properties of the Riemann tensor, and it is also related to the commutator of covariant derivatives.

What is the physical interpretation of the first algebraic Bianchi identity?

The first algebraic Bianchi identity has a physical interpretation as a conservation law for the Riemann tensor. It states that the sum of the cyclic permutations of the covariant derivatives of the Riemann tensor is equal to zero, which means that the Riemann tensor is conserved under certain transformations.

How is the first algebraic Bianchi identity used in general relativity?

In general relativity, the first algebraic Bianchi identity is used to simplify the Einstein field equations, which describe the relationship between the curvature of spacetime and the distribution of matter and energy. It also allows us to derive other important equations, such as the contracted Bianchi identities and the Ricci identities.

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