Question regarding tensors derive acceleration in polar form

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SUMMARY

The discussion centers on deriving acceleration components in polar coordinates using tensors, specifically from Rindler's "Introduction to Special Relativity." The participants confirm that the components of a vector A^i in polar coordinates are \dot{r} and r\dot{\theta}. They also address the transformation of vector B^i, leading to the components \ddot{r} - r(\ddot{\theta})^2 and \ddot{\theta} + 2\dot{r}\dot{\theta}/r. The definition of contravariant tensors is utilized to facilitate these transformations, highlighting the importance of understanding tensor behavior under coordinate transformations.

PREREQUISITES
  • Understanding of contravariant tensors and their transformations
  • Familiarity with polar and Cartesian coordinate systems
  • Basic knowledge of calculus, particularly derivatives and second derivatives
  • Experience with Rindler's "Introduction to Special Relativity" or similar texts
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  • Study the properties of contravariant tensors in detail
  • Learn how to perform coordinate transformations between Cartesian and polar coordinates
  • Explore the application of tensors in classical mechanics and relativity
  • Practice deriving acceleration formulas in various coordinate systems
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I'm having trouble with this question. It's from Rindler's Introduction to Special Relativity which I'm going through myself. I'm just starting to learn about tensors.

<<<<i) A vector [tex]A^i[/tex] has components [tex]\dot{x}, \dot{y}[/tex] in rectangular Cartesian coordinates; what are its components in polar coordinates?>>>>

This part I believe I know. The components are [tex]\dot{r}, r\dot{\theta}[/tex]. The first component is the [tex]a_r[/tex] component and the second is the [tex]a_{\theta}[/tex] component.

<<<<ii) A vector [tex]B^i[/tex] has components [tex]\ddot{x}, \ddot{y}[/tex] in rectangular Cartesian coordinates; prove, directly from A.3 that its components in polar coordinates are [tex]\ddot{r}-r{(\ddot{\theta})}^2, \ddot{\theta}+2\dot{r}\dot{\theta}/r[/tex]>>>>

This is what A.3 says:
<<<<An object having components [tex]A^{ij...n}[/tex] in the [tex]x^i[/tex] system of coordinates and [tex]A^{i'j'...n'}[/tex] in the [tex]x^{i'}[/tex] system is said to behave as a contravariant tensor under the transformation [tex]\{x^i\}->\{x^{i'}\}[/tex] if [tex]A^{i'j'...n'}=A^{ij...n}{p_i}^{i'}{p_j}^{j'}...{p_n}^{n'}[/tex]>>>>

I'm not sure how this is to be done. The [tex]a_{\theta}[/tex] coordinate in part ii) seems to be divided by r. I don't know if this is a mistake in the book or there is some reason for it.

How do I use the definition of contravariant tensors to derive the formula for acceleration in polar coordinates? I really have no clue. I can derive the formula just using derivatives, but I don't see how to use tensors to derive it.

Thanks a bunch for your help!
 
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[tex]A' ^{i}=\frac{\partial x' ^{i}}{\partial x^{j}} A^{j}[/tex] (1)

For

[tex]A^{j}=\left(\dot{x},\dot{y}\right)[/tex] (2)

So

[tex]A'^{1}=\frac{\partial\rho}{\partial x} \dot{x}+\frac{\partial\rho}{\partial y} \dot{y} =\cos\phi \ \left(\dot{\rho}\cos\phi-\rho\dot{\phi}\sin\phi\right)+\sin\phi \ \left(\dot{\rho}\sin\phi+\rho\dot{\phi}\cos\phi\right)=\dot{\rho}[/tex]

This is for the first comp of the transformed velocity.

U do the other "3" (one for velocity & 2 for acceleration).

Daniel.
 
Cool! Thanks a bunch dexter! :biggrin:
 

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