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Towards a Relativistic Theory of Gravity

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Theory of Gravitational Interactions

Part of the book series: Undergraduate Lecture Notes in Physics ((ULNP))

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Abstract

The need for a relativistic generalization of Newton’s theory of gravity is phenomenologically motivated, and a possible generalization based on the introduction of a space–time metric more general than the Minkowski one is suggested. The crucial role of the equivalence principle is discussed, and shown to provide strong support to the choice of a Riemannian geometric structure.

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Notes

  1. 1.

    As we shall see in Chap. 10, the perihelion precession predicted by general relativity is approximately six times larger that the special-relativistic result (2.11), and is thus in good agreement with the astronomical observations.

References

  1. Kolb, E.W., Turner, M.S.: The Early Universe. Addison–Wesley, Redwood City (1990)

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  2. Rindler, W.: Essential Relativity. Springer, Berlin (1977)

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Gasperini, M. (2013). Towards a Relativistic Theory of Gravity. In: Theory of Gravitational Interactions. Undergraduate Lecture Notes in Physics. Springer, Milano. https://doi.org/10.1007/978-88-470-2691-9_2

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