Abstract
There are two complementary ways to use Einstein’s equations:
After choosing a momentum–energy tensor on the basis of some physical assumptions, we can try to determine the solutions of Einstein’s equations corresponding to that momentum–energy tensor. For example, if the momentum–energy tensor of a perfect fluid is chosen and a spherically symmetric solution is searched for, then a reasonable stellar model is obtained.
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Notes
- 1.
See [92].
- 2.
A polynomial P of degree m is called homogeneous if \(P(\lambda x_{1}, \ldots , \lambda x_{n})=\lambda ^{m}P(x_{1}, \ldots , x_{n})\) for all \(\lambda \in \mathbb {C}\). Every polynomial P can be written as \(P=P_{0}+P_{1}\), where \(P_{0}\) is homogeneous of degree m and the degree of \(P_{1}\) is less than m. The polynomial \(P_{0}\) is called the principal part of P.
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Romano, A., Mango Furnari, M. (2019). Cauchy’s Problem for Einstein’s Equations. In: The Physical and Mathematical Foundations of the Theory of Relativity. Birkhäuser, Cham. https://doi.org/10.1007/978-3-030-27237-1_13
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DOI: https://doi.org/10.1007/978-3-030-27237-1_13
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