"You can't make a man unsee what he has seen"
--Bertolt Bercht, The Life of Galileo
The history of the universe can be compared to a play in which the actors- matter and radiation, stars and galaxies - dance across the cosmic stage according to a script set by the laws of physics. The challenge for the cosmologist is to figure out the story line after arriving at the show 14 billion years too late, long past the crucial opening scenes.
Observations of nearby galaxies and stars provide an accurate picture of the present scene. By gathering light emitted long ago from more distant objects and applying the physical principles learned and tested on Earth, astronomers have been able to reconstruct more and more of what happened in the past. The epoch [ Act Two] which began just one-second after the big bang and continues to the present day, is the period of cosmic history that is best understood. During this nearly 14-billion-year span, the universe expanded more than a billion times in size, and the hot primordial gas that filled the infant universe cooled to less than a billionth of its initial temperature, condensing into structures of increasing mass and complexity, the first planets, stars, galaxies, galaxy clusters and super clusters.
One might imagine that, armed with this detailed knowledge of Act two, scientists could straightforwardly determine what happened before or what will happen next. The big surprise is that this is not the case. The inflationary and cyclic models both incorporate Act Two, but they sandwich it between completely different first and third acts. In the case of cyclic model, Act Three is not even the final act: the plot eventually leads to a new Act One, in which the story begins all over again. To appreciate how two radically different views of the history of the universe can both be consistent with the plethora of observations available today, one must first understand what is known and what is not known about the Act two.
--Bertolt Bercht, The Life of Galileo
The history of the universe can be compared to a play in which the actors- matter and radiation, stars and galaxies - dance across the cosmic stage according to a script set by the laws of physics. The challenge for the cosmologist is to figure out the story line after arriving at the show 14 billion years too late, long past the crucial opening scenes.
Observations of nearby galaxies and stars provide an accurate picture of the present scene. By gathering light emitted long ago from more distant objects and applying the physical principles learned and tested on Earth, astronomers have been able to reconstruct more and more of what happened in the past. The epoch [ Act Two] which began just one-second after the big bang and continues to the present day, is the period of cosmic history that is best understood. During this nearly 14-billion-year span, the universe expanded more than a billion times in size, and the hot primordial gas that filled the infant universe cooled to less than a billionth of its initial temperature, condensing into structures of increasing mass and complexity, the first planets, stars, galaxies, galaxy clusters and super clusters.
One might imagine that, armed with this detailed knowledge of Act two, scientists could straightforwardly determine what happened before or what will happen next. The big surprise is that this is not the case. The inflationary and cyclic models both incorporate Act Two, but they sandwich it between completely different first and third acts. In the case of cyclic model, Act Three is not even the final act: the plot eventually leads to a new Act One, in which the story begins all over again. To appreciate how two radically different views of the history of the universe can both be consistent with the plethora of observations available today, one must first understand what is known and what is not known about the Act two.