Chapter 23 In the Beginning…..

 

When did it all start?  About 13.7 billion years ago

Extrapolating the Hubble Constant backwards (allowing for acceleration)

Also get the temperature and density

 

The theory that describes the physics is called the Big Bang

         This is NOT an explosion!!

 

Outline of the events:

The early universe

 

Grand Unified Theory  GUT  All the forces were the same when the energy is high

Inflation - a sudden expansion of spacetime  about 1050 

         It flattens our piece of the universe.

 

Evidence

 

Cosmic Microwave Background

         Transition at 380,000 years

         What we see the CMB sky   ‘zoom’     b

 

H He abundance in Population II stars

         Number of neutrons sets amount of H vs. He

         Baryonic matter only about 4%

 

 

Persistent problems

         Why is the universe so smooth?  [ to about .01%]

         Where did the small fluctuations come from?

         Why is the universe so close to the critical density

 

Solved by Inflation

         Current parts of CMB  used to be much closer

         Inflation flattens spacetime

 

Why not perfectly flat?

         Quantum fluctuations get ‘inflated’ to be the current size of the lumps

 

If all this happened we should see the lumps in the CMB and their size should tell us what the density was at that time. (Was it the critical density?)

         WMAP Sky and results  (higher resolution made it possible)

 

According to WMAP:

         The geometry is flat

         Baryonic matter is 4.4%

         Total matter is 27%

         Flatness implies dark energy makes up other 73%

         Universe age is 13.7 billion years

 

 

The Future

         An accelerating universe runs down

         If protons decay all ordinary matter falls apart

         Eventually even black holes evaporate so only particles and photons exist