Beginnings of Cosmology
Humans have always held ideas about how the universe originated. But it wasnt until advances in the 20th century, including Albert Einsteins theories of relativity, that astronomers could really form educated ideas about how the universe formed.
Alexander Friedmann, a Russian physicist, was the first to realize that applying the rules of relativity across large scales described a universe that changed over time. With a mathematical approach, he showed the universe could have started small before expanding over enormous distances and, in some cases, eventually collapsing back in on itself.
Observations carried outby Lowell Observatorys V.M. Slipher and, later, Edwin Hubble, showed that the universe was in fact expanding. And this helped confirm these initial ideas of the Big Bang. Two years later, the Belgian physicist Georges Lematre published a paper describing how the expanding universe had started as a tiny, hot, dense speck, which he called the primeval atom. Ordained as a Catholic priest, Lematre reported the finding as a happy coincidence of cosmology and theology in an early draft of the paper, though the comment was removed for the final publication of the paper.
Two decades later, George Gamow would develop theories on the fallout of a hot-birthed universe namely, how it would create neutrons and protons and published a popular book on the subject. It even caught the eye of Pope Pius XII, who was taken by the parallels between the scripture of Genesis and the scientific theory.
Unlike the church, Einstein wasnt initially happy with the idea of a changing universe, preferring one invariable on large scales. British astronomer Fred Hoyle wasnt happy, either. Along with two other scientists, he developed a counter-theory the steady state model. The steady state model suggested that the universe had no beginning and had always been expanding. To explain why the universe looks identical in all directions, it proposed tiny traces of matter, too small to be experimentally measured, were continually being created.
This model initially garnered support of around half of the scientific community albeit one that was very small at the time and became the Big Bang theorys biggest rival.
This [debate between theories] was not in the mainstream of physics research, says David Kaiser, science historian and physics professor at MIT. Basically no one paid attention or very little attention, even among professional physicists and astronomers.
But as evidence started gathering, that would change.
Observations of distant ultra-bright galaxies in the 1950s suggested the universe was changing, and measurements of the helium content in the universe didnt match the steady state models predictions. In 1964, the monumental discovery of the cosmic microwave background radiation direct evidence of a young, hot universe would deal the final deathblow to the steady state model.
It really seems to suggest the universe had very different conditions in early times than today, Kaiser says. And that was just not what the steady state model suggests.
In an ironic twist, Hoyle used the term Big Bang in an attempt to dismiss the theory in a BBC interview. Though his own theory would be largely lost to history, the irreverent name would stick.
To his death, Hoyle would never submit to the Big Bang theory. A small subset of cosmologists still work on resurrecting a steady state model; but, on the whole, the community overwhelmingly supports the Big Bang theory.
There are a couple of other puzzles, so cosmologists don't think we're done, but theyre now kind of patching or filling in some holes to the original Big Bang models certainly not replacing it, Kaiser says.
Continue reading here:
The Steady State: When astronomers tried to overthrow the Big Bang - Astronomy Magazine
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