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Origin of Universe • Universe…all the space, time, energy and matter that exists • Because things are so far from Earth, and light takes so long to travel to us, when we look in the sky, we look into the past • Most of space is empty … um … space Early thoughts • Steady State Theory: everything is now as it always has been and nothing will ever change…stars, planets, galaxies are the same as they always have been and will never change • The Scientific Theory at turn of last century (1900’s) Early thoughts • Einstein…1916…theory of general relativity redefines gravity and space to space/time – Implies that universe must be moving (not static/unchanging), but doesn’t say expanding or contracting • Lemaitre…1927…says universe should be expanding (observed red shift) and therefore once had a beginning • People ignored Lemaitre in favor of Einstein until… Edwin Hubble, 1929 • Noticed that light from stars is shifted towards red end of spectrum • Means they’re moving away from us • More it’s shifted, faster they’re moving •Opposite is blue shift (means it’s moving towards us) Edwin Hubble, 1929 • Hubble noticed that most galaxies are moving away from us and the farther they are, the faster they’re moving • If go backwards, means everything was in a small point and exploded and is moving from that point out. • Was called Big Bang to make fun of it and the name stuck! Big Bang Theory • EVERYTHING (space, time, matter, energy) was in one small point (singularity) that “blew up” and is still moving outwards today • Not really an explosion, so much as a very rapid expansion…like blowing up a balloon • About 13.7 billion years ago • Microwave radiation detected in the 1960’s supports this theory. It’s left over energy from the Big Bang Penzias and Wilson • In addition to Hubble’s evidence • 1960’s discovered microwave radiation all throughout the universe, but couldn’t explain where it came from • Only possible source is it’s left over from Big Bang • Later shown not to be “evenly spread” WMAP…background radiation Other evidence • First elements to form should be simplest….Hydrogen and Helium, and that’s what most of the universe is (>99%)! • Other heavier elements made by stars (fusion up to Iron) and supernovas (other heavier elements) • Called nucleosynthesis Timeline • Inflationary period: – Rapid expansion, temperature billions of degrees…way too hot even for atoms to exist! • 10-43 sec after – .00000000000000000000000000000000000000 00001 seconds – 4 forces separate (electromagnetism, gravity, weak nuclear, strong nuclear) – Rules of physics we know now start to work Timeline • 10-35 seconds after – Protons and neutrons form – .00000000000000000000000000000000001 • 10-1 seconds after – Electrons form – .01 sec. • 3 minutes after – 1st atomic nuclei form Temperature down to 1 billion degrees • 300,000 years after – First atoms (H and He) – Light shines for first time (CMBR) What’s next? • Amount of mass will decide what’s going to happen to the universe: – May continue expanding forever – May continue expanding and then stop at some size – May expand to a point and then collapse and explode again • Hard to measure amt. to of mass. We see the effects (gravity) of some matter we can’t see, so we call it dark matter (e.g. WIMPs) What’s next? • Galaxies don’t seem to be slowing down (so Big Crunch is doubtful, or we’re still in a period of expansion) • Open universe: idea that not enough matter to keep it all together, and things keep expanding (like molecules from open jar) • Closed universe: idea that enough mass to pull everything back in to Big Crunch • Flat universe….expands to certain size and stops • Oscillating Universe: Bang, Crunch, Bang, Crunch forever and ever