Young_and_Hot_Big bang

When the Universe Was Young and Hot : 

f Don Lincoln, Fermilab f When the Universe Was Young and Hot Don LincolnFermilabf

Hubble Telescope : 

f Don Lincoln, Fermilab f Hubble Telescope This image is taken of galaxies that are billions of light-years away. Light takes a very long time to travel to Earth. Consequently, this photograph is of the conditions that existed billions of years ago, just a billion years or so after the big bang. Astronomers have thus created a time machine of sorts.

Ancient Greek Cosmology : 

f Don Lincoln, Fermilab f Ancient Greek Cosmology In the beginning there was an empty darkness. The only thing in this void was Nyx (Chaos), a bird with black wings. With the wind she laid a golden egg and for ages she sat upon this egg. Finally life began to stir in the egg and out of it rose Eros, the god of love. One half of the shell rose into the air and became the sky and the other became the Earth. Eros named the sky Uranus and the Earth he named Gaia. Then Eros made them fall in love.

Familiar Cosmology : 

f Don Lincoln, Fermilab f Familiar Cosmology In the beginning God created the heaven and the earth. And the earth was without form, and void; and darkness was upon the face of the deep. And the Spirit of God moved upon the face of the waters.

Modern Cosmology : 

f Don Lincoln, Fermilab f Modern Cosmology Approximately 15 billion years ago, all of the matter in the universe was concentrated at a single point A cataclysmic explosion (of biblical proportions perhaps?) called the Big Bang caused the matter to fly apart. In the intervening years, the universe has been expanding, cooling as it goes.

Consequences of the Big Bang : 

f Don Lincoln, Fermilab f Consequences of the Big Bang If the universe did come into existence through a cataclysmic explosion, there should be some evidence. Three forms which I will discuss are: The universe should be expanding The universe should have a measurable temperature. The mix of the elements should be known.

Doppler Effect : 

f Don Lincoln, Fermilab f Doppler Effect The Doppler effect says that things moving away from you look redder than they would if they weren’t moving. Things moving towards you look more blue.

Edwin Hubble : 

f Don Lincoln, Fermilab f Edwin Hubble Using the Doppler effect, Edwin Hubble discovered that objects that were further away move away faster (and, hence, were redder) than nearer objects. This discovery showed that the universe was expanding and still provides one of the best measurements of the age of the universe.

Black Body Radiator : 

f Don Lincoln, Fermilab f Black Body Radiator Universe A black body radiator is one which absorbs all light which is incident on it. Such a body can also emit light, if sufficiently hot. The universe should thus have a temperature and an ‘afterglow’.

Afterglow From the Big Bang : 

f Don Lincoln, Fermilab f Afterglow From the Big Bang In 1964, while working at Bell Labs, Penzias and Wilson discovered a radio hiss that they couldn’t make go away. They had (by accident!) discovered the remnant ‘echo’ of the Big Bang The universe was shown to have a temperature of 2.726K (-450 °F)

Cosmic Background Explorer : 

f Don Lincoln, Fermilab f Cosmic Background Explorer In 1992, COBE announced a measurement that showed that the background radiation was not quite uniform (although nearly so) This measurement records information approximately 300,000 years after the Big Bang

Goldilocks Effect : 

f Don Lincoln, Fermilab f Goldilocks Effect These three plots show three different effects, each 10% less than the one larger than it. You can see how seeing a small effect first requires removing the bigger one. Full, 10%, and 1% 10% and 1% 1% Full only 10% only

Helium Abundance in the Universe : 

f Don Lincoln, Fermilab f Helium Abundance in the Universe At the late time (as we shall see) of 3 minutes in the history of the universe, atomic nuclei were created. Big Bang theory predicts that the relative abundances of hydrogen and helium were: Hydrogen 76% Helium 24% Lithium 1 part per 1010 Due to nuclear fusion in stars since the Big Bang, current abundances: Hydrogen 73% Helium 26% Everything else 1%

Summary of Cosmologic Measurements : 

f Don Lincoln, Fermilab f Summary of Cosmologic Measurements The Big Bang theory is consistent with observations. Specifically Hubble Telescope can view the universe ~1,000,000,000 years after the Big Bang The COBE satellite can view the universe ~300,000 years after the Big Bang The Hydrogen/Helium ratio can view the universe ~3 minutes after the Big Bang

What’s so interesting about that?All the interesting stuff is overby three minutes.The universe was in a retirement home by then. : 

f Don Lincoln, Fermilab f What’s so interesting about that?All the interesting stuff is overby three minutes.The universe was in a retirement home by then.

The really interesting question is:What happened when the universe was young and hot? : 

f Don Lincoln, Fermilab f The really interesting question is:What happened when the universe was young and hot?

History of the Universe : 

f Don Lincoln, Fermilab f History of the Universe In the beginning, the universe was really, really, hot. Consequently, things looked very different in the beginning.

Consider an Ice Cube : 

f Don Lincoln, Fermilab f Consider an Ice Cube Heat it and it Melts Boils Turns to steam H2O breaks up into hydrogen and oxygen atoms The electrons get ripped off the atoms and electrons and atomic nuclei scurry around Atomic nuclei get broken up into protons and neutrons Protons and neutrons get ripped apart into particles called quarks.

The Big Question : 

f Don Lincoln, Fermilab f The Big Question How do you get something as hot as it was during the Big Bang? Smash stuff together!! Hot!

Slide 20: 

f Don Lincoln, Fermilab f E = m c2 Energy is Matter Matter is Energy Lots of energy makes lots of matter and vice versa!!!!!!

Slide 21: 

f Don Lincoln, Fermilab f