On the history of the so-called Lense-Thirring effect

@article{Pfister2007OnTH,
  title={On the history of the so-called Lense-Thirring effect},
  author={Herbert Pfister},
  journal={General Relativity and Gravitation},
  year={2007},
  volume={39},
  pages={1735-1748}
}
  • H. Pfister
  • Published 26 September 2007
  • Physics
  • General Relativity and Gravitation
Some historical documents, especially the Einstein–Besso manuscript from 1913, an extensive notebook by H. Thirring from 1917, and the correspondence between Thirring and Einstein in the year 1917 reveal that most of the merit for the so-called Lense-Thirring effect of general relativity belongs to Einstein. Besides telling this “central story” of the effect, we give a short “prehistory”, with contributions by E. Mach, B. and I. Friedlaender, and A. Föppl, followed by the later history of the… 

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References

SHOWING 1-10 OF 56 REFERENCES

Mach's principle : from Newton's bucket to quantum gravity

This volume is a collection of scholarly articles on the Mach Principle, the impact that this theory has had since the end of the 19th century, and its role in helping Einstein formulate the doctrine

Cosmological gravitomagnetism and Mach's principle

The spin axes of gyroscopes experimentally define local nonrotating frames, i.e. the time evolution of axes of inertial frames. But what physical cause governs the time evolution of gyroscope axes?

The Large Scale Structure of Space-Time

TLDR
The theory of the causal structure of a general space-time is developed, and is used to study black holes and to prove a number of theorems establishing the inevitability of singualarities under certain conditions.

Einstein and the History of General Relativity

This book is a collection of essays by the authors and other people that deal with scientific opinions that led Einstein and his contemporaries to their views of general relativity. Some of the

XCVI. On the gravitational effects of distant rotating masses

Summary Thirring's calculation of the gravitational field near the centre of a rotating spherical shell is corrected and elaborated. First, an additional term, representing elastic stresses, is

MOTION OF A GYROSCOPE ACCORDING TO EINSTEIN'S THEORY OF GRAVITATION.

  • L. Schiff
  • Physics
    Proceedings of the National Academy of Sciences of the United States of America
  • 1960
TLDR
This section examines the experimental basis of Einstein's theory of gravitation, and the principle of equivalence, which is expressed in the following way: all observations made locally on a system in a static, uniform gravitational field in the absence of local background matter agree with corresponding observations made on the same system when it is subjected to an equivalent acceleration in the presence of the field.

Rotating masses and their effect on inertial frames.

An analysis is given of the stress-energy tensor and geometry produced by slowly rotating bodies. The geometrized mass $\frac{\mathrm{GM}}{{c}^{2}}$ of the body is allowed to be comparable to its

Induction of correct centrifugal force in a rotating mass shell

Mach's idea of relativity of rotation is confirmed for a shell-type model of the Universe by showing that flat geometry in rotating coordinates, realising correct Coriolis and centrifugal forces, can

Gravitation and Inertia

PrefaceChart of Main Topics1A First Tour12Einstein Geometrodynamics133Tests of Einstein Geometrodynamics874Cosmology, Standard Models, and Homogeneous Rotating Models1855The Initial-Value Problem in

Do Rotations Beyond the Cosmological Horizon Affect the Local Inertial Frame

If perturbations beyond the horizon have the velocities prescribed everywhere then the dragging of inertial frames near the origin is suppressed by an exponential factor. However if perturbations are
...