Recovering Forces from Christoffel Symbols: A Derivation

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SUMMARY

This discussion focuses on deriving forces from Christoffel symbols, particularly under the assumption of a Cartesian coordinate system (t,x,y,z) and specific "flatness" conditions. The key finding is that for the transformation of Christoffel symbols to yield a rank 1 vector, most symbols must be zero or small, specifically \(\Gamma^x{}_{tt}\), \(\Gamma^y{}_{tt}\), and \(\Gamma^z{}_{tt}\) can be nonzero. The discussion highlights the limitations of time transformations in inertial frames and emphasizes the need for Lorentz transformations to validate the use of forces in relativistic contexts.

PREREQUISITES
  • Understanding of Christoffel symbols and their properties
  • Familiarity with tensor transformation laws
  • Knowledge of inertial frames and coordinate systems
  • Basic principles of relativistic physics, including Lorentz transformations
NEXT STEPS
  • Study the properties and applications of Christoffel symbols in differential geometry
  • Learn about tensor transformation laws in detail
  • Explore the implications of Lorentz transformations on force calculations
  • Investigate the use of forces in polar coordinates and their derivations
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Physicists, mathematicians, and students studying general relativity or differential geometry, particularly those interested in the relationship between forces and Christoffel symbols.

pervect
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I don't think I've ever seen this discussed in a textbook, this is an attempt to throw some light on the connection between Christoffel symbols and forces.

In particular I want to derive the later as an approximation of the former, with some limitations on choices of coordinate systems (inertial frames).

I'll start off with assuming a cartesian coordinate system (t,x,y,z).
Next, we will add some "flatness" assumptions. Basically, to reduce the rank 3 Christoffel symbols to a rank 1 vector, we need the majority of them to be zero, or at least "small".

\Gamma^x{}_{tt}, \Gamma^y{}_{tt}, and \Gamma^z{}_{tt}[/tex] can be nonzero, the rest must be &quot;small&quot;.<br /> <br /> We will assume this to be the case, and check to see if it&#039;s sufficient for starters.<br /> <br /> Now that we have the right rank, we still need to worry about the fact that Christoffel symbols aren&#039;t tensors. So we take a close look at the transformation law:<br /> <br /> Wiki <a href="http://en.wikipedia.org/w/index.php?title=Christoffel_symbols&amp;oldid=551829920" target="_blank" class="link link--external" rel="nofollow ugc noopener">http://en.wikipedia.org/w/index.php?title=Christoffel_symbols&amp;oldid=551829920</a><br /> <br /> writes this as:<br /> <br /> \overline{\Gamma^k{}_{ij}} =&lt;br /&gt; \frac{\partial x^p}{\partial y^i}\,&lt;br /&gt; \frac{\partial x^q}{\partial y^j}\,&lt;br /&gt; \Gamma^r{}_{pq}\,&lt;br /&gt; \frac{\partial y^k}{\partial x^r}&lt;br /&gt; + &lt;br /&gt; \frac{\partial y^k}{\partial x^m}\, &lt;br /&gt; \frac{\partial^2 x^m}{\partial y^i \partial y^j}<br /> <br /> We can substitute in \partial y^i = \partial y^j = \partial t, since i and j must be equal to the index of t (usually zero) by our assumption.<br /> <br /> \overline{\Gamma^k{}_{ij}} =&lt;br /&gt; \frac{\partial x^p}{\partial t}\,&lt;br /&gt; \frac{\partial x^q}{\partial t}\,&lt;br /&gt; \Gamma^r{}_{pq}\,&lt;br /&gt; \frac{\partial y^k}{\partial x^r}&lt;br /&gt; + &lt;br /&gt; \frac{\partial y^k}{\partial x^m}\, &lt;br /&gt; \frac{\partial^2 x^m}{\partial t^2}<br /> <br /> We see that we need \frac{\partial^2 x^m}{\partial t^2} to be zero - this is true if we transform between inertial frames.<br /> <br /> This then leaves us with basically the basic tensor transformation law, except that forces transform quadratically with time.<br /> <br /> This is a bit troublesome, apparently we can&#039;t do arbitrary time transformations t-&gt;t&#039; if we wish to use forces. This makes sense, though, intiutively - it means as part of choosing an &quot;inertial frame&quot; we&#039;re stucking with choosing a regularly ticking clock if we wish to use forces. Then this factor becomes a simple scale factor.<br /> <br /> I think that&#039;s pretty much the basics, though due to the limitations on time transformation, some extra attention should be paid to Lorentz transforms to demonstrate why four-fources work relativistically.<br /> <br /> I feel there are some things lacking in this approach - it doesn&#039;t quite demonstrate that Lorentz transforms work, nor does it demonstrate, really, why you can use forces in polar coordinates. But I think it&#039;s a start.<br /> <br /> If anyone has seen anything similar to this in the literature, I&#039;d be interested in hearing about it.
 

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