The Birth of the Universe

1. The Birth of the Universe

2. Hubble Expansion and the Big Bang The fact that more distant galaxies are moving away from us more rapidly indicates that the universe is expanding. This implies that the universe was born in a huge explosion, or Big Bang.

3. Testing the Big Bang: Has the universe changed? If the Big Bang theory is correct, then the universe was very different in the past. We can test this prediction with images of the faintest and most distant galaxies, and hence looking back in time to when the universe was much younger. To detect very distant galaxies, Hubble stared at small patch of sky for an entire week. This image, known as the Hubble Deep Field, shows that galaxies were smaller and more irregular in the past than they are today.

5. Testing the Big Bang: Do we see an afterglow? Another prediction of the Big Bang theory is that the universe was very hot immediately after it was born. As a result, the universe would have glowed at short wavelengths (gamma rays). Because of the expansion of the universe, the light produced after the Big Bang should be redshifted over time, and should now appear at radio wavelengths (or more specifically, microwave wavelengths).

6. Prediction vs. Observation The Big Bang afterglow was predicted in 1948, and it was detected with a radio telescope in 1965 (resulting in a Nobel Prize). This confirmed the Big Bang theory. This afterglow is called the Cosmic Microwave Background (CMB). It appears across the entire sky in every direction, and its spectrum is equivalent to a blackbody with a temperature of 3 degrees above absolute zero.

7. The Expansion of Space The galaxies are not flying apart into the universe. The universe itself is expanding. The galaxies are simply riding along as the fabric of space expands.

8. The Expansion of Space The expansion of the universe also causes light to get stretched to longer wavelengths, or redshifted. So the redshifts that we measure for galaxies are not really due to their velocities away from us, but instead result from the expansion of the space itself.

9. The Expansion of Space Given that space is distorted by the presence of matter (and energy), it is natural that space experiences expansion along with the matter and energy.

10. No Center or Edge in the Universe As an analogy, imagine a 2-D universe on the surface of a sphere. Now let the sphere expand. The surface area of the sphere increases (like the volume of space in our 3-D universe), and yet there isn’t a location on that surface that is the center of the expansion, and that surface does not have an edge. Because space is expanding along with the mass and energy, the universe does not have a center or an edge.

12. The Age of the Universe We can estimate the age of the universe from its rate of expansion, which is measured in the Hubble Law. If the universe expanded at a constant rate since the Big Bang, then the age of the universe would D/Vfor any point along the Hubble Law, which produces an age of about 13 billion years. According to the Big Bang theory, the universe has not existed forever, and instead has a finite age. V D

13. The Age of the Universe The gravity from the matter in the universe should slow the expansion of the universe over time. So the universe must have expanded faster in the past than it does now. As a result, the true age of the universe should be less than D/V, or <13 billion years. In other words, because it expanded faster in the past, the universe reached its current size more quickly than if it had been expanding at a constant rate. Big Bang expansion gravity

14. The Age of the Universe But stars in some globular clusters are at least 13 billion years old. How can some stars be older than the universe? The solution to this puzzle wasn’t found until the 1990’s, and is explained in the next lecture.

15. The Size of the Universe The observable universe consists of the portion of the universe that is close enough so that light from it has had enough time to reach us since the Universe was born. This region is a sphere centered on the Earth, and its boundary is called the light horizon.

16. The Size of the Universe The microwave background radiation that we see today was produced shortly after the Big Bang by material that was only 36 million light years from our position in the universe, and yet it took 13 billion years to arrive at our location because of the expansion of the universe. 36 million light years after Big Bang: our location Now: CMB seen today 46 billion light years The matter that produced the microwave photons that we see today is now 46 billion lyrs away, probably in the form of a galaxy. So the current diameter of the observable universe is 92 billion lyrs.

17. Inflation But how can 2 points in the universe be separated by 92 billion light years when the universe is only about 13 billion years old? The universe has expanded faster than the speed of light! Nothing in the universe can move faster than light, but the universe itself is not restricted to this speed limit as it expands. The most rapid expansion occurred right after the Big Bang in a period called inflation. In a tiny fraction of a second, the universe grew from the size of an atom to 1 billion light years across!

18. Beyond the Observable Universe Because the universe has expanded faster than the speed of light, some areas of the universe have been pulled beyond our light horizon, and are outside of our observable universe.

19. Beyond the Observable Universe If we wait long enough, light will eventually reach us from some of the areas currently outside of our observable universe. But other areas are too far away for their light to ever catch up and reach us as the universe expands. Those areas will always remain outside of our observable universe. Theories of inflation suggest that the true size of the universe may be 1026 times larger than our observable universe, or 1037 light years! And it’s still expanding, so it will grow even larger!

20. History of the Universe • For the first split second after the Big Bang, the universe contained only energy in the form of radiation. • 10-43-10-35 seconds after Big Bang: inflation • 10-35 seconds: some of the radiation converts to elementary particles (quarks) • 0.00001 seconds: protons and neutrons form • 3 minutes: fusion of hydrogen to helium ends • 400,000 years: the microwave background that we see today is produced Timeline of Universe

21. The Microwave Background By the time the universe reached an age of 400,000 years, it had expanded enough so that photons of light could travel large distances without scattering. In other words, the universe was now transparent to light. So the microwave background shows us the appearance of the universe 400,000 years after the Big Bang.

22. Formation of Structures Over time, very small ripples appeared in the dark matter. Gravity caused these ripples to collapse and grow to become dense clumps. The gravity of the dark matter clumps then attracted normal matter. The resulting clumps of normal matter eventually became clusters of galaxies.

23. Formation of Galaxies We see the clumps of normal matter that eventually became galaxy clusters in the map of the microwave background.

25. The Fate of the Universe Will the Universe expand forever? Or will it stop expanding and collapse (a Big Crunch)?