Deriving Geodetic Line by Einstein: Clarifying Difficulties

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SUMMARY

The discussion focuses on the derivation of the geodetic line as presented in Albert Einstein's "The Foundation of the General Theory of Relativity." The key equation, δ∫_P^{P'}ds=0, is transformed into a parametric form, ∫_{λ1}^{λ2}δwdλ=0, where w^2=g_{μν}(dx_μ/dλ)(dx_ν/dλ). The participant seeks clarification on the transition represented by δ and its implications for the integral, particularly how δ interacts with the integral sign. The conversation emphasizes the importance of understanding the parametrization via λ and the nature of the variations involved in the derivation.

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  • Understanding of general relativity concepts, particularly geodesics
  • Familiarity with calculus of variations
  • Knowledge of differential geometry and tensor notation
  • Basic grasp of parametric equations and their applications
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Students and researchers in physics, particularly those specializing in general relativity, differential geometry, and mathematical physics. This discussion is beneficial for anyone seeking to deepen their understanding of geodesic equations and their derivations.

sujoykroy
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I was reading "The foundation of the general theory of relativity" by Albert Einstein. I faced some difficulty to understand his derivation of "geodetic line", stated in "The equation of the geodetic line. The motion of particle" headed section. I will try to describe my problem clearly and in short.

Einstein first stated that along geodetic line \int ds is stationary, which means equation of geodetic should be,
δ\int_P^{P'}ds=0​
between two points P and P' of four dimensional continuum, where ds means linear element. Solving this variation equation would give 4 new differential equations describing the geodetic line. This is clear and simple and no difficulty arises here.

However, then he replaced this equation with a parametric version,..

\int_{λ1}^{λ2}δwdλ=0
where, w^2=g_{μν}\frac{dx_μ}{dλ}\frac{dx_ν}{dλ}​

Einstein, described λ as follows,

Let λ be a function of the co-ordinates x_ν, and let this define a family of surfaces which intersect the required geodetic line as well as all the lines in immediate proximity to it which are drawn through the points P and P'.

Thus, lines, joining P and P', seems to become function of this new "family of surfaces" λ, as mentioned by him in this way,
Any such line may then be supposed to be given by expressing its co-ordinates x_ν as functions of λ.

Upto this point, things are not yet quite that difficult, although some elaboration of λ would be useful. But next he reinterpret δ as follows,
Let the symbol δ indicate the transition from a point of the required geodetic to the point corresponding to the same λ on a neighbouring line.

My question is what is this transition? Is it change of line-length? Moreover, how the δ sign will cross the integral ∫ sign, as it happened in the 2nd, replaced, equation, involving λs? although, i guess, knowing the meaning of δ and transition will answer the 2nd question.

I have stressed my brain neurons quite a bit to understand what this transition means and run through some pages of calculus of variations, but still it is hiding at large from me. An enlightenment from you will re-energize my brain cells.
 
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Okay, a parametrized path connecting points P and P' gives 4 functions of the parameter, \lambda: x^0(\lambda), x^1(\lambda), x^2(\lambda), x^3(\lambda). The meaning of lambda is just that it is a real number indicating how far along the path. So lambda is just a real number that increases continuously from P to P'. It doesn't actually matter, but for concreteness, let's assume that at P, lambda = 0, and at P', lambda = 1.

Now to vary the path x^\mu(\lambda), you replace x^\mu(\lambda) by a shifted value:x'^\mu(\lambda) = x^\mu(\lambda) + \delta x^\mu(\lambda). (Where \mu runs over the four coordinate indices). \delta x^\mu(\lambda) is just another function of \lambda, but since the shifted path has to start at P, and has to end at P', we have to have \delta x^\mu(0) = \delta x^\mu(1) = 0. Other than that, \delta x^\mu is an arbitrary function, except that it is assumed to be small. (The shifted path is not much different from the original path).

Then using x'^\mu instead of x^\mu, we can compute a shifted value for w = \sqrt{g_{\mu \nu} \frac{dx^\mu}{d\lambda} \frac{dx^\nu}{d\lambda}}. Call this shifted value w'. Then \delta w = w' - w (only keeping the lowest-order terms in \delta x^\mu).
 
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As far as my little brain progressed, i figured out as follows.
Since the equation δ\int_P^{P'}ds=0 is evaluated between two points of four coordinates continuum, to convert this into a well-known form of variation some parametrization was required and hence λ was introduced. Using λ, all those 4 coordinates are transformed into functions of λ. Much like, λ is acting like the independent variable. So, the former equation, first, transformed into this, -
δ\int_{λ1}^{λ2}\frac{ds}{dλ}dλ=0​
As i get to know from ancient book of Dionysius Lardner, (although one could have proved by himself), that, in variation equations interchanging of δ and ∫ does not alter the result. Hence, the last equation can surely be rewritten as
\int_{λ1}^{λ2}δ(\frac{ds}{dλ})dλ=0​

Lastly, Einstein did declared that
ds^2=\sum\limits_{τσ}g_{στ}dx_{σ}dx_{τ}​
or if following his notation system, it is
ds^2=g_{στ}dx_{σ}dx_{τ}​
.
From there we can put dλ into this equation and transform it into
({\frac{ds}{dλ}})^2=g_{στ}\frac{dx_{σ}}{dλ}\frac{dx_{τ}}{dλ}​
So, taking w={\frac{ds}{dλ}}, the final, previously troublesome, equation gets into the picture,
\int_{λ1}^{λ2}δwdλ=0​
 

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