Covariant Derivatives & Christoffel Symbols Flashcards

(38 cards)

1
Q

What is a covariant derivative?

A

A derivative that accounts for curvature and preserves tensor transformation properties.

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2
Q

Why is the partial derivative not suitable in curved spacetime?

A

Because it does not transform covariantly under coordinate changes.

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3
Q

What does ∇_μ V^ν mean?

A

The covariant derivative of the vector V^ν with respect to x^μ.

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4
Q

What is the formula for the covariant derivative of a vector?

A

∇_μ V^ν = ∂μ V^ν + Γ^ν{μλ} V^λ.

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5
Q

What is the formula for the covariant derivative of a covector?

A

∇_μ V_ν = ∂μ V_ν - Γ^λ{μν} V_λ.

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6
Q

What is the general rule for covariant derivatives?

A

Add Γ for each upper index, subtract for each lower index.

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7
Q

What are Christoffel symbols?

A

Connection coefficients used in defining the covariant derivative.

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8
Q

Are Christoffel symbols tensors?

A

No, they do not transform like tensors.

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9
Q

What is the formula for Christoffel symbols?

A

Γ^λ_{μν} = 1/2 g^{λρ}(∂μ g{νρ} + ∂ν g{μρ} - ∂ρ g{μν}).

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10
Q

What is the symmetry of the Christoffel symbols?

A

Γ^λ_{μν} = Γ^λ_{νμ} — symmetric in lower indices.

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11
Q

What does ∇μ g{αβ} = 0 mean?

A

Metric compatibility — the metric is preserved under parallel transport.

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12
Q

What is parallel transport?

A

Moving a vector along a curve while keeping it ‘parallel’ using the connection.

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13
Q

What happens to a vector under parallel transport around a closed loop?

A

It may change direction due to curvature (encoded in Riemann tensor).

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14
Q

What is torsion in connections?

A

The antisymmetric part of the connection: Γ^λ_{μν} ≠ Γ^λ_{νμ} implies torsion.

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15
Q

Does the Levi-Civita connection have torsion?

A

No, it is torsion-free and metric-compatible.

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16
Q

How do you compute Γ in practice?

A

From the metric using Γ^λ_{μν} = 1/2 g^{λρ}(∂μ g{νρ} + ∂ν g{μρ} - ∂ρ g{μν}).

17
Q

What is ∇_μ T^ν_λ?

A

μ T^ν_λ + Γ^ν{μρ}T^ρ_λ - Γ^ρ_{μλ}T^ν_ρ

18
Q

What does ∇_μ δ^ν_λ equal?

A

Zero, since the Kronecker delta is constant.

19
Q

Why is ∇_μ g^{νλ} = 0?

A

Follows from metric compatibility and the inverse metric relation.

20
Q

Can ∇_μ of a scalar differ from ∂_μ?

A

No, ∇_μ φ = ∂_μ φ for any scalar φ.

21
Q

How does curvature appear in derivatives?

A

In second derivatives — via the Riemann tensor when commuting derivatives.

22
Q

What is the product rule for ∇_μ?

A

It satisfies the Leibniz rule: ∇_μ (AB) = (∇_μ A)B + A(∇_μ B).

23
Q

How do Christoffel symbols behave under coordinate change?

A

They transform with an inhomogeneous term — not tensorially.

24
Q

What is a geodesic equation in terms of Christoffel symbols?

A

d²x^λ/dλ² + Γ^λ_{μν} dx^μ/dλ dx^ν/dλ = 0.

25
How do covariant derivatives help define curvature?
Curvature measures the non-commutativity of covariant derivatives.
26
What is ∇_λ T^{μν}?
∂_λ T^{μν} + Γ^μ_{λρ} T^{ρν} + Γ^ν_{λρ} T^{μρ}.
27
What is the physical role of the covariant derivative?
It ensures the derivative of a tensor remains a tensor.
28
How is a covariant derivative visualized?
As a limit of parallel transport differences along a curve.
29
Why do we subtract Γ for lower indices?
Because lowering an index corresponds to using the metric, which introduces a minus sign.
30
How is covariant differentiation related to parallel transport?
Covariant derivative vanishes along a vector's own direction if it is parallel transported.
31
What does ∇_μ A_ν = 0 mean?
The vector A_ν is constant along x^μ in a covariant sense.
32
Can you define divergence with ∇?
Yes, ∇_μ V^μ is the covariant divergence of the vector field.
33
Why is the connection symmetric in the Levi-Civita case?
Because it is derived from a symmetric metric and is torsion-free.
34
What is the effect of curvature on parallel transport?
Vectors change direction when moved around a loop in curved spacetime.
35
What is the condition for a vector field to be Killing?
∇_μ ξ_ν + ∇_ν ξ_μ = 0
36
What is a Killing vector?
A vector field whose flow preserves the metric — indicates a symmetry.
37
Why is ∇ used instead of ∂ in GR?
Because spacetime is curved and we need derivatives that respect curvature.
38
What is the covariant Laplacian?
□φ = ∇_μ ∇^μ φ — the d'Alembertian operator in curved spacetime.