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The Birth of the Big Bang

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A Student's Guide Through the Great Physics Texts

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Abstract

In Chap. I of his book, The Primeval Atom, Lemaître suggested that our universe is not a flat, Euclidean space (as one might presume), but rather an elliptical, non-Euclidean space. Indeed, the nebulae which populate our universe bend space in their vicinity, according to Einstein’s theory of general relativity, allowing its edges to meet up—just like the opposite edges of a mercator projection map meet up to form a single meridian. In this sense, both the surface of the earth and the space of the universe are finite yet unbounded. Now, in Chap. IV Lemaître turns to the question of cosmogony: how did the world begin? Before providing his own hypothesis, Lemaître reviews the cosmogonic theories of Buffon, Kant and Laplace. Which (if any) of these theories of cosmogony do you find most compelling? Why?

The evolution of the world does not depend solely upon the law of universal attraction.

—Georges Lemaître

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Notes

  1. 1.

    Lecture given at La Société Royale Belge des Ingénieurs et Industriaux, at Brussels, January 10, 1945, and published in Ciel et Terre, March–April, 1945.

  2. 2.

    We quote according to: The History and Theory of the Earth, translated by William Smellie, member of the Antiquarian & Royal Societies of Edinburgh, published by W. Clowes, London.

  3. 3.

    For a more detailed discussion of mass-energy equivalence see Chap. 32 of volume II, and especially Ex. 32.1.

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Correspondence to Kerry Kuehn .

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Kuehn, K. (2015). The Birth of the Big Bang. In: A Student's Guide Through the Great Physics Texts. Undergraduate Lecture Notes in Physics. Springer, New York, NY. https://doi.org/10.1007/978-1-4939-1360-2_28

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  • DOI: https://doi.org/10.1007/978-1-4939-1360-2_28

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  • Online ISBN: 978-1-4939-1360-2

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