The general expression for the Laplace operator ($\nabla^2 \phi$) on a scalar field $\phi$ in curvilinear coordinates is derived to be $\nabla^2 \phi=\frac{1}{\sqrt{g}} \partial_a\left(\sqrt{g} g^{a b} \partial_b \phi\right)$. This formula is established by starting with the definition of the Laplacian as the divergence of the gradient, $\nabla \cdot(\nabla \phi)$, and then utilizing the crucial tensor identity $\Gamma_{a b}^b=\partial_a \ln (\sqrt{g})$, which links the contracted Christoffel symbols to the partial derivative of the local volume factor ( $\sqrt{g}$ ). The identity allows the two components of the divergence (the partial derivative and the Christoffel symbol term) to be combined via the reverse product rule, demonstrating how the $\sqrt{g}$ factor is necessary to properly account for the expansion or contraction of the coordinate grid lines in the generalized space.

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✍️Mathematical Proof

$\complement\cdots$Counselor

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  1. Laplacian as Divergence of Gradient:

    The Laplace operator ( $\nabla^2 \phi$ ) acting on a scalar field $\phi$ is fundamentally defined as the divergence of the gradient ( $\nabla \cdot(\nabla \phi)$ ). This is the starting point for its coordinate-free definition.

  2. General Coordinate Expression:

In arbitrary curvilinear coordinates, the Laplace operator is expressed by the concise and powerful formula:

$$ \nabla^2 \phi=\frac{1}{\sqrt{g}} \partial_a\left(\sqrt{g} g^{a b} \partial_b \phi\right) $$

This formula is valid in any coordinate system (orthogonal or not), including Cartesian, cylindrical, spherical, and general Riemannian spaces.

  1. The Role of the Metric Determinant ( $\sqrt{g}$ ):

The term $\sqrt{ g }$ (the square root of the metric determinant) represents the Jacobian of the coordinate transformation and accounts for the local volume element in the curvilinear space. Its presence ensures the divergence operation correctly accounts for the expansion and contraction of the coordinate grid lines.

  1. Connection to Christoffel Symbols:

    The identity $\Gamma_{a b}^b=\partial_a \ln (\sqrt{g})$ is crucial. It shows that the contracted Christoffel symbols, which generally relate to the "curvature" or "non-flatness" of the coordinate system, are directly linked to the change in the local volume element. This link allows the complex terms involving Christoffel symbols in the covariant derivative (divergence) to be neatly reexpressed using the partial derivatives of $\sqrt{ g }$.

  2. Covariant Derivative Implication:

The derivation works by showing that the terms from the partial derivative and the Christoffel symbols in the divergence formula,

$$ \nabla^2 \phi=\partial_a\left(V^a\right)+\Gamma_{a b}^a V^b $$

can be combined using the reverse product rule because the Christoffel term is exactly what's needed to complete the total partial derivative of the weighted vector field $\sqrt{g} V^a$.

$$ \sqrt{g}(\nabla \cdot V )=\partial_a\left(\sqrt{g} V^a\right) $$

This is the core identity for the divergence of a contravariant vector in general coordinates.

✍️Mathematical Proof

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  1. Derivation of Tensor Transformation Properties for Mixed Tensors
  2. The Polar Tensor Basis in Cartesian Form
  3. Verifying the Rank Two Zero Tensor
  4. Tensor Analysis of Electric Susceptibility in Anisotropic Media
  5. Analysis of Ohm's Law in an Anisotropic Medium
  6. Verifying Tensor Transformations
  7. Proof of Coordinate Independence of Tensor Contraction
  8. Proof of a Tensor's Invariance Property
  9. Proving Symmetry of a Rank-2 Tensor
  10. Tensor Symmetrization and Anti-Symmetrization Properties
  11. Symmetric and Antisymmetric Tensor Contractions
  12. The Uniqueness of the Zero Tensor under Specific Symmetry Constraints
  13. Counting Independent Tensor Components Based on Symmetry
  14. Transformation of the Inverse Metric Tensor
  15. Finding the Covariant Components of a Magnetic Field
  16. Covariant Nature of the Gradient
  17. Christoffel Symbol Transformation Rule Derivation
  18. Contraction of the Christoffel Symbols and the Metric Determinant
  19. Divergence of an Antisymmetric Tensor in Terms of the Metric Determinant
  20. Calculation of the Metric Tensor and Christoffel Symbols in Spherical Coordinates
  21. Christoffel Symbols for Cylindrical Coordinates
  22. Finding Arc Length and Curve Length in Spherical Coordinates
  23. Solving for Metric Tensors and Christoffel Symbols
  24. Metric Tensor and Line Element in Non-Orthogonal Coordinates
  25. Tensor vs. Non-Tensor Transformation of Derivatives
  26. Verification of Covariant Derivative Identities
  27. Divergence in Spherical Coordinates Derivation and Verification
  28. Laplace Operator Derivation and Verification in Cylindrical Coordinates
  29. Divergence of Tangent Basis Vectors in Curvilinear Coordinates
  30. Derivation of the Laplacian Operator in General Curvilinear Coordinates
  31. Verification of Tensor Density Operations
  32. Verification of the Product Rule for Jacobian Determinants and Tensor Density Transformation
  33. Metric Determinant and Cross Product in Scaled Coordinates
  34. Vanishing Divergence of the Levi-Civita Tensor
  35. Curl and Vector Cross-Product Identity in General Coordinates
  36. Curl of the Dual Basis in Cylindrical and Spherical Coordinates
  37. Proof of Covariant Index Anti-Symmetrisation
  38. Affine Transformations and the Orthogonality of Cartesian Rotations
  39. Fluid Mechanics Integrals for Mass and Motion
  40. Volume Elements in Non-Cartesian Coordinates (Jacobian Method)
  41. Young's Modulus and Poisson's Ratio in Terms of Bulk and Shear Moduli
  42. Tensor Analysis of the Magnetic Stress Tensor
  43. Surface Force for Two Equal Charges
  44. Total Electromagnetic Force in a Source-Free Static Volume
  45. Proof of the Rotational Identity
  46. Finding the Generalized Inertia Tensor for the Coupled Mass System
  47. Tensor Form of the Centrifugal Force in Rotating Frames
  48. Derivation and Calculation of the Gravitational Tidal Tensor
  49. Conversion of Total Magnetic Force to a Surface Integral via the Maxwell Stress Tensor
  50. Verifying the Inhomogeneous Maxwell's Equations in Spacetime </aside>