Error in Concepts: Intro to Mechanics Kolenkow & Kleppner

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SUMMARY

The discussion centers on the treatment of spacetime curves in "Mechanics" by Kolenkow & Kleppner, specifically questioning whether these curves can be accurately represented as parabolas. It is established that while every differentiable curve can be approximated as a parabola to second order, the actual curve in this context is a hyperbola. The derivation presented is valid as an approximation, utilizing the Schwarzschild solution to analyze wave emission and reception in a gravitational field. The conclusion emphasizes the importance of careful interpretation of results, particularly regarding redshift in light emitted from a gravitational source.

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  • Understanding of differentiable curves and their properties
  • Familiarity with the Schwarzschild solution in general relativity
  • Knowledge of wave mechanics and frequency ratios
  • Basic concepts of redshift and gravitational effects on light
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  • Learn about differentiable curves and their approximations in mathematical physics
  • Explore the concept of redshift and its applications in astrophysics
  • Review the treatment of special relativity in classical mechanics texts, particularly Kolenkow & Kleppner
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Physics students, educators, and researchers interested in general relativity, wave mechanics, and the nuances of classical mechanics as presented in Kolenkow & Kleppner's work.

Ramanathan k s
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TL;DR
While reading "The Equivalence Principle and the Gravitational Red Shift" in the book (Introduction to Mechanic by Kolenkow & Kleppner) I'm having doubts about how they arrived at the result gL/(c^2).
They are treating the spacetime curve as a parabola, but is it a parabola?
And I think there is some serious conceptual error in the analysis.
please help me
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Ramanathan k s said:
They are treating the spacetime curve as a parabola, but is it a parabola?
Every differentiable curve is a parabola to 2nd order about any given point.
 
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Dale said:
Every differentiable curve is a parabola to 2nd order about any given point.
But what will be the actual curve in this case?
 
Ramanathan k s said:
But what will be the actual curve in this case?
It is actually a hyperbola. However, that does not make the derivation wrong. It just makes the derivation a derivation to 2nd order. This is not a "conceptual error", it is a valid approximation.
 
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It's still a somewhat hand-waving argument, but it's correct given the approximations made.

A simple argument is to use the exact Schwarzschild solution, of which we only need
$$\mathrm{d} s^2=(1-2m/r) c^2 \mathrm{d} t^2 + \ldots$$
Now a wave is emitted from a source at rest at ##r=r_0##. The time it takes from one maximum of the wave to the next is
$$\frac{2 \pi}{\omega_{\text{em}}} = \mathrm{d} \tau (r_0)=\sqrt{1-2m/r_0} \mathrm{d} t_{\text{em}}.$$
Then it's received by an observer at rest at ##r_0+h##, and there
$$\frac{2 \pi}{\omega_{\text{obs}}}=\mathrm{d} \tau (r_0+h) = \sqrt{1-2m/(r_0+h)} \mathrm{d} t_{\text{obs}}.$$
Now ##\mathrm{d} t_{\text{obs}}=\mathrm{d} t_{\text{em}}##, from which
$$\frac{\omega_{\text{obs}}}{\omega_{\text{em}}}=\sqrt{\frac{1-2m/r_0}{1-2m/(r_0+h)}} \simeq 1-\frac{m h}{(r_0-2m)r_0}.$$
Now ##m=G M/c^2=R_{\text{S}}/2## is half the Schwarzschild radius. For ##r_0 \gg R_{\text{S}}##, where the Newtonian limit is valid, we have
$$\frac{\omega_{\text{obs}}}{\omega_{\text{em}}}=1-\frac{m h}{r_0^2}=1-\frac{G M/(c^2 r_0^2)} h =1-\frac{g h}{c^2}.$$
 
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vanhees71 said:
It's still a somewhat hand-waving argument, but it's correct given the approximations made.

A simple argument is to use the exact Schwarzschild solution, of which we only need
$$\mathrm{d} s^2=(1-2m/r) c^2 \mathrm{d} t^2 + \ldots$$
Now a wave is emitted from a source at rest at ##r=r_0##. The time it takes from one maximum of the wave to the next is
$$\frac{2 \pi}{\omega_{\text{em}}} = \mathrm{d} \tau (r_0)=\sqrt{1-2m/r_0} \mathrm{d} t_{\text{em}}.$$
Then it's received by an observer at rest at ##r_0+h##, and there
$$\frac{2 \pi}{\omega_{\text{obs}}}=\mathrm{d} \tau (r_0+h) = \sqrt{1-2m/(r_0+h)} \mathrm{d} t_{\text{obs}}.$$
Now ##\mathrm{d} t_{\text{obs}}=\mathrm{d} t_{\text{em}}##, from which
$$\frac{\omega_{\text{obs}}}{\omega_{\text{em}}}=\sqrt{\frac{1-2m/r_0}{1-2m/(r_0+h)}} \simeq 1-\frac{m h}{(r_0-2m)r_0}.$$
Now ##m=G M/c^2=R_{\text{S}}/2## is half the Schwarzschild radius. For ##r_0 \gg R_{\text{S}}##, where the Newtonian limit is valid, we have
$$\frac{\omega_{\text{obs}}}{\omega_{\text{em}}}=1-\frac{m h}{r_0^2}=1-\frac{G M/(c^2 r_0^2)} h =1-\frac{g h}{c^2}.$$
actually the result is $$\ 1+\frac{g h}{c^2}.$$
 
Ramanathan k s said:
actually the result is ## 1+\frac{g h}{c^2}##
Can’t be, the ratio of frequencies has to be less than one for upwards-moving light to be redshifted.
 
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I think my sign is correct, because for ##h>0## there must be red shift, because the "naive photon" looses energy moving "upwards".
 
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