Find Einstein's GR Papers: Read His Own Words

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SUMMARY

This discussion centers on the quest for original texts of Albert Einstein's General Relativity (GR) papers, emphasizing the importance of studying his work in its original form. Participants highlight the limitations of relying solely on Einstein's writings due to advancements in GR over the past century. Key points include the distinction between general covariance and the absence of prior geometry in GR, as well as the equivalence principle's local applicability. Recommendations for further reading include works by Misner, Thorne, Wheeler, and Clifford Will's "Was Einstein Right?" to gain a comprehensive understanding of GR.

PREREQUISITES
  • Understanding of General Relativity concepts, including the equivalence principle.
  • Familiarity with Einstein's original papers on General Relativity.
  • Knowledge of modern interpretations of GR, including Mach's principle.
  • Basic grasp of the historical context of GR's development and its key figures.
NEXT STEPS
  • Read Einstein's "The Foundation of the General Theory of Relativity" for original insights.
  • Explore "Relativity: The Special and General Theory" by Einstein for foundational concepts.
  • Study "Relativity Simply Explained" by Gardner for a beginner-friendly overview of GR.
  • Investigate "Was Einstein Right?" by Clifford Will for a critical analysis of Einstein's theories.
USEFUL FOR

Students of physics, researchers in gravitational theory, and anyone interested in the historical and conceptual foundations of General Relativity will benefit from this discussion.

  • #31
atyy said:
We start with Newton's laws in an inertial frame. When we transform to a noninertial frame, we pick up "Christoffel symbols". If instead of defining "same form" without Christoffel symbols, we define it as including the Christoffel symbols, then Newton's laws are valid in any frame.

It is the same with special relativity, which is capable of handling accelerated frames (eg. Rindler coordinates).

I like http://arxiv.org/abs/gr-qc/0603087 .

But the moment you bring Christoffel symbols into the picture, don't you march away from Newtonian Physics to General Relativity by taking into account the effects of curvature? And all this has been done quite recently after GR was developed and not at the time of Newton.vCorrect me if I am wrong as I am quite new to General Relativity.
 
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  • #32
aashay said:
But the moment you bring Christoffel symbols into the picture, don't you march away from Newtonian Physics to General Relativity by taking into account the effects of curvature? And all this has been done quite recently after GR was developed and not at the time of Newton.vCorrect me if I am wrong as I am quite new to General Relativity.

http://www.mth.uct.ac.za/omei/gr/chap6/node4.html

You can have Christoffel symbols in flat space, eg. when you use polar coordinates.

The essential idea is that the Christoffel symbols are first derivatives of the metric, where the Riemann curvature tensor which indicates the difference between flatness and curvedness is made of second derivatives of the metric.

In GR, fake gravity (from acceleration) makes first derivatives of the metric, whereas true gravity (more properly, tidal gravity) is due to curvature. (I'm sure bcrowell is going to disagree with my terminology here!)
 
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