Gradient in general co-ordinates

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SUMMARY

The discussion focuses on the expression of the gradient in a general coordinate system, specifically referencing the definitions provided in "A First Course in Continuum Mechanics" by Gonzalez and Stuart. The gradient is defined as grad phi(x) = (partial d phi by d xi)(x) ei, where {ei} represents an arbitrary frame. The user seeks clarification on how this definition relates to the presence of the 1/r term in cylindrical coordinates, which is essential for understanding the transformation between coordinate systems and its implications for deformation gradients.

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  • Understanding of general coordinate systems in vector calculus
  • Familiarity with the concepts of covariant and contravariant basis vectors
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Homework Statement



I know that for a general co-ordinate system, the gradient can be expressed as it is at the bottom of this page:

http://en.wikipedia.org/wiki/Orthogo...ree_dimensions

However, the book I am working from (A First Course in Continuum Mechanics by Gonzalez and Stuart) defines it as:

"Let {ei} be an arbitrary frame. Then grad phi(x)= (partial d phi by d xi)(x) ei where (x1,x2,x3) are the coordinates of x in ei"

I don't understand how this relates to the actual definition, for example given the definition in my book, how do I show that the gradient in cylindricals contains a 1/r in front of the unit theta term?

I presume that these ei are completely general so they are not unit vectors?

I need to understand this notation properly so I can apply it to deformation gradients etc



Homework Equations





The Attempt at a Solution



From reading http://en.wikipedia.org/wiki/Curvilinear_coordinates where the same formula as the book is given, I presume it has something to do with covariant and contravariant basis but this isn't really mentioned in the book.
 
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A circular arc, from point (r, \theta) to (r, \theta+ d\theta) will have length rd\theta. A vector, in the \theta direction, at the point with coordinates (r, \theta_0) will, similarly, have length given by r d\theta. The "1/r" is required to remove the dependence on r.
 
How would I know, merely from the definition in the book that I need that, for example if we were dealing with some totally arbitrary coordinates? (I completely understand why it is there in this case and know how to derive it)
 

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