• Corpus ID: 119144820

Revisiting the Schwarzschild and the Hilbert-Droste Solutions of Einstein Equation and the Maximal Extension of the Latter

@article{Mol2014RevisitingTS,
  title={Revisiting the Schwarzschild and the Hilbert-Droste Solutions of Einstein Equation and the Maximal Extension of the Latter},
  author={Igor Mol},
  journal={arXiv: Mathematical Physics},
  year={2014}
}
  • I. Mol
  • Published 10 March 2014
  • Mathematics
  • arXiv: Mathematical Physics
In this pedagogical note, the differences between the Schwarzschild and the Hilbert-Droste solutions of Einstein equation are scrutinized through a rigorous mathematical approach, based on the idea of warped product of manifolds. It will be shown that those solutions are indeed different because the topologies of the manifolds corresponding to them are different. After establishing this fact beyond any doubt, the maximal extension of the Hilbert-Droste solution (the Kruskal-Szekeres spacetime… 

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References

SHOWING 1-10 OF 41 REFERENCES

David Hilbert and the origin of the "Schwarzschild solution"

The very early dismissal of Schwarzschild's original solution and manifold, and the rise, under Schwarzschild's name, of the inequivalent solution and manifold found instead by Hilbert, are

Completion and Embedding of the Schwarzschild Solution

An analytic manifold is found, the most important properties of which are that it is complete and that it contains the manifold of the Schwarzschild line element. It is thus the complete analytic

Regular coordinate systems for Schwarzschild and other spherical spacetimes

The continuation of the Schwarzschild metric across the event horizon is a well-understood problem discussed in most textbooks on general relativity. Among the most popular coordinate systems that

The Schwarzschild metric: It's the coordinates, stupid!

Every general relativity textbook emphasizes that coordinates have no physical meaning. Nevertheless, a coordinate choice must be made in order to carry out real calculations, and that choice can

The Large Scale Structure of Space-Time

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.

The Particle Problem in the General Theory of Relativity

The writers investigate the possibility of an atomistic theory of matter and electricity which, while excluding singularities of the field, makes use of no other variables than the g&„of the general

Uber das Gravitationsfeld eines Massenpunktes nach der Einstenschen Theorie

Schwarzschild's solution of Einstein's field equations in vacuum can be written in many different forms. Unfortunately Schwarzschild's own original form is less nice looking and simple than that

The Schwarzschild solution: corrections to the editorial note

Explanatory Note The editorial note on the Schwarzschild paper published in our journalGeneralRelativity andGravitation [16b]mayhave been an acceptable description of the perception of the

Past-Future Asymmetry of the Gravitational Field of a Point Particle

The analytic extension of the Schwarzschild exterior solution is given in a closed form valid throughout empty space-time and possessing no irregularities except that at the origin. The gravitational

“Golden Oldie”: On the Gravitational Field of a Mass Point According to Einstein's Theory

where (1) ds = √6gμνdxμdxν μ, ν = 1, 2, 3, 4, where the gμν stand for functions of the variables x , and in the variation the variables x must be kept fixed at the beginning and at the end of the