Find infinitesimal displacement in any coordinate system

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SUMMARY

The discussion focuses on finding infinitesimal displacement in various coordinate systems, specifically highlighting spherical coordinates. The transformation equations for spherical coordinates are provided: x = ρ sinθ cosφ, y = ρ sinθ sinφ, and z = ρ cosθ. The infinitesimal displacement is expressed as dℓ = drâ + r dθâ + r sinθ dφâ. The general formula for infinitesimal displacement in any coordinate system is dℝ = ∂ℝ/∂qj dqj, where the sum is over j. For further reading, the book "Mathematical Methods for Physics and Engineering" by Riley & Hobson is recommended, particularly chapters 10 and 26.

PREREQUISITES
  • Understanding of spherical coordinates and their transformations
  • Familiarity with vector calculus
  • Knowledge of differential geometry concepts
  • Basic proficiency in mathematical notation and summation conventions
NEXT STEPS
  • Study the transformation of coordinates in different systems, including cylindrical and polar coordinates
  • Learn about the applications of infinitesimal displacements in physics and engineering
  • Explore differential geometry, focusing on Riemannian manifolds
  • Read "Mathematical Methods for Physics and Engineering" by Riley & Hobson, especially chapters 10 and 26
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Students and professionals in physics, engineering, and mathematics, particularly those interested in vector calculus and coordinate transformations.

Msilva
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I am wondering how can I find the infinitesimal displacement in any coordinate system. For example, in spherical coordinates we have the folow relations:
x = \, \rho sin\theta cos\phi
y = \, \rho sin\theta sin\phi
z = \, \rho cos\theta

And we have that d\vec l = dr\hat r +rd\theta\hat \theta + r sin\theta d\phi \hat \phi
How do I found this for any system? What book has this explanation? I am not finding.
 
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In general the infinitesimal displacement given in some coordinates q_i is d\vec r=\frac{\partial \vec r}{\partial q_j}dq_j (sum over j), so if you have a vector given in cartesian coordinates, and know how to transform those to the new coordinates, you can use the above formula. For more info, I'd suggest Riley & Hobson, chapters 10 and 26.

Note: this works fine in Euclidean space \mathbb R^n, but for an arbitrary Riemannian manifold I'm not so sure.
 
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