EINSTEINSCHE FELDGLEICHUNGEN PDF

Wir wollen Einstein zu ehren einen von ihm vorgeschlagenen Weg gehen, um zu den Feldgleichungen zu gelangen. Das Potential in der AR ist der Metriktensor. Die Christoffelsymbole befinden sich schon sehr dicht am Ziel, jedoch sind sie nur von erster Ordnung, d. Nur leider beinhaltet dieser neue Tensor keine zweiten Ableitungen des Metriktensors.

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These equations, together with the geodesic equation[7] which dictates how freely-falling matter moves through space-time, form the core of the mathematical formulation of general relativity. Volume 13 Issue 12 Decpp. Volume 58 Issue 12 Decpp. This work may also be in the public domain in countries and areas with longer native copyright terms that apply the rule of the shorter term to foreign works.

Although the Einstein feldgleichungeh equations were initially formulated in the context of a four-dimensional theory, some theorists have explored their consequences in n dimensions.

Volume 51 Issue 12 Decpp. Volume 70 Issue 12 Decpp. Background Principle of relativity Galilean relativity Galilean transformation Special relativity Doubly special relativity.

Views Read Edit View history. International Journal of Theoretical Physics. Volume 7 Issue 12 Decpp. This will reduce to its Newtonian counterpart, provided. Volume 32 Issue 12 Decpp. Eine der Feldgleichungen kann sofort integriert werden. Here you can find all Crossref-listed publications in which this article is cited. Volume 26 Issue 12 Decpp. Volume 46 Issue 12 Decpp. Feldgleivhungen theory Kaluza—Klein Quantum gravity.

Each tensor has 10 independent components. However, approximations are usually made in these cases. One might think that EFE are non-polynomial since feldglsichungen contain the inverse of the metric tensor.

Volume 54 Issue 12 Decpp. With his field equations Einstein ensured that general relativity is consistent with this eijsteinsche condition. Volume 4 Issue 9 Seppp. Applying these simplifying assumptions to the spatial components of the geodesic equation gives. Wikibooks has a book on the topic of: The nonlinearity of the EFE distinguishes general relativity from many other fundamental physical theories.

Volume 37 Issue 12 Decpp. Einstein, AlbertQuantentheorie des einatomigen idealen Gases, 2. Further simplification is achieved in approximating the actual spacetime as flat spacetime with a small deviation, leading to the linearized EFE. When do Projections Commute? Einstein thought of the cosmological constant as an independent parameter, but its term in the field equation can also be moved algebraically to the other side, written as part of the stress—energy tensor:.

Volume 68 Issue 12 Decpp. De Gruyter Online Google Scholar. Volume 18 Issue 12 Decpp. In general relativity, these equations are replaced by the Einstein field equations in the trace-reversed form. Phenomena Gravitoelectromagnetism Kepler problem Gravity Gravitational field Gravity well Gravitational lensing Gravitational waves Gravitational redshift Redshift Blueshift Time dilation Gravitational time dilation Shapiro time delay Gravitational potential Gravitational compression Gravitational collapse Frame-dragging Geodetic effect Gravitational singularity Event horizon Naked singularity Black hole White hole.

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Volume 48 Issue 12 Decpp. General relativity Special relativity Doubly special relativity. This effort was unsuccessful because:. Volume 22 Issue 12 Decpp.

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