Titlebook: Beyond Einstein Gravity; The Minimal Geometri Jorge Ovalle,Roberto Casadio Book 2020 The Author(s), under exclusive license to Springer Nat

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書目名稱Beyond Einstein Gravity讀者反饋學(xué)科排名

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International Handbook of Universities 2019, black holes and gravitational waves—just to mention some of the most remarkable ones, have given it the honours which deserves as one of the fundamental theories of Physics (for a recent review on experimental tests of GR see?[.] and references therein).

干旱

International Handbook of Universities 2019it works the way it does was not yet explained. This is precisely the objective of this final chapter. We will see that the MGD scheme has to do with the decoupling of the gravitational sources in the Einstein field equations?[., .], something which is not trivial, given the complexity and non-linearity of that system of equations.

多產(chǎn)子

The Minimal Geometric Deformation,, black holes and gravitational waves—just to mention some of the most remarkable ones, have given it the honours which deserves as one of the fundamental theories of Physics (for a recent review on experimental tests of GR see?[.] and references therein).

學(xué)術(shù)討論會(huì)

Gravitational Decoupling,it works the way it does was not yet explained. This is precisely the objective of this final chapter. We will see that the MGD scheme has to do with the decoupling of the gravitational sources in the Einstein field equations?[., .], something which is not trivial, given the complexity and non-linearity of that system of equations.

Needlework

Book 2020dictions of four-dimensional General Relativity, a model known as the Brane world; secondly, it explains, step-by-step, a new technique called .Minimal Geometric Deformation., which was introduced for the purpose of solving the correspondingly modified Einstein field equations. This method gave rise

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Stellar Distributions,n-locality makes the BW equations an open system. As we have seen in the previous chapter, the non-locality derives from the projection of the bulk Weyl tensor onto the brane, and this leads to a very complicated system of equations which are particularly difficult to study for non-uniform matter distributions.

reserve

2191-5423 gly modified Einstein field equations. This method gave rise to the .Gravitational Decoupling in General Relativity., which is widely used to solve the Einstein field equations in various contexts. .978-3-030-39492-9978-3-030-39493-6Series ISSN 2191-5423 Series E-ISSN 2191-5431

過度

Book 2020l Geometric Deformation., which was introduced for the purpose of solving the correspondingly modified Einstein field equations. This method gave rise to the .Gravitational Decoupling in General Relativity., which is widely used to solve the Einstein field equations in various contexts. .

磨坊

International Handbook of Universities 2019n-locality makes the BW equations an open system. As we have seen in the previous chapter, the non-locality derives from the projection of the bulk Weyl tensor onto the brane, and this leads to a very complicated system of equations which are particularly difficult to study for non-uniform matter distributions.