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11 - The Big Bang's cosmic echo

Published online by Cambridge University Press:  05 December 2015

David J. Eicher
Affiliation:
Editor-in-Chief, Astronomy magazine
Alex Filippenko
Affiliation:
University of California, Berkeley
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Summary

Few things have polarized the astronomy enthusiast community like the Big Bang Theory. Despite overwhelming evidence for the Big Bang origin of the cosmos, a select group of amateur astronomers resists accepting it, although this strange phenomenon has dimmed somewhat as more and more evidence for the Big Bang has piled up.

The basis for the logic behind the Big Bang is simple. In the 1910s and 1920s, Vesto M. Slipher, Edwin Hubble, and others discovered initial evidence for the expansion of the universe – everything appears to be expanding away from everything else on large scales. Running the history of the universe backwards, then, naturally brings all of this expanding material together into a very small initial space.

The initial, primeval, incredibly dense state, in which all matter and energy were compressed almost unbelievably and then expanded as space-time rushed outward, is now familiar as the Big Bang. But such was not always the case. In 1922, Russian physicist Alexander Friedmann (1888–1925) led the charge with an idea that perhaps the universe had an initial singular state of extraordinarily high density. Five years later the Belgian priest‒astronomer Georges Lemaître (1894–1966) published a milestone paper suggesting a dense origin of the cosmos and a “primeval atom.” Lemaître believed the dense early universe was akin to a huge radioactive atomic nucleus. Because Lemaître was a priest, some cosmologists were initially skeptical of his notions.

In the late 1940s, the adventurous English cosmologist Fred Hoyle (1915–2001) proposed a major alternative to what was shaping up as the Big Bang. Calling it the steady-state theory, Hoyle and his colleagues, Thomas Gold (1920–2004) and Hermann Bondi (1919–2005), suggested that matter is created continuously as the universe expands, allowing the cosmos to be homogeneous (alike everywhere) and isotropic (uniform in all orientations) in space and time. Hoyle, in fact, appeared on BBC Radio in 1949, arguing against the Big Bang Theory, and using the term “big bang” for the first time, derisively (or perhaps jokingly). To his utter horror, the term stuck and was used by the Big Bang's proponents.

The uncertainty over differing cosmological models lingered for a variety of reasons. Working against the Big Bang was the fact that the Hubble Time, an indicating figure of the age of the universe, seemed to be less than the age of Earth.

Type
Chapter
Information
The New Cosmos
Answering Astronomy's Big Questions
, pp. 145 - 156
Publisher: Cambridge University Press
Print publication year: 2015

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