Chapter 22- Makeup of the Universe Flashcards
what does “the universe was very dense and hot” mean
that the universe was full of particles and radiation
cosmic microwave background
- electromagnetic radiation as a remnant from an early stage of the universe in Big Bang cosmology
- evidence of BBT
what does it mean that we needed to wait of universe to become transparent
-the time of Recombination: the universe cooled enough for neutral atoms to form
ho long did we wait for the microwave background to start
380,000 years
cosmological redshift
-photons were stretched
isotropic
same in all directions
we know that cosmic microwave background is isotropic, so what can we infer
that Big Bang evidence is everywhere in the sky
closed (sphered) universe geometry
- positive curvature
- mass density exceeds critical limit
flat universe geometry
- zero curvature
- mass density equals critical limit
open universe geometry
- negative curvature
- mass density less than critical limit
what suggests that the universe is flat
angular separation of temp fluctuations
what are the two problems with our universe
1) isotropy problem
2) Flatness problem
what is the isotropy problem within the universe
- the uniform appearance of cosmic microwave background creates a problem
- how did all parts of the observable universe achieve a common temp
- to have a common temp things have to touch and some parts of the universe are just now coming in contact
what is the flatness problem within the universe
- if the density is greater than 1 then the universe would end in a Big Crunch
- if the density is less than 1 then the universe wouldn’t have enough matter to form
- how did the density magically equal one
inflation in the universe
universe expands by rapid factor (faster than the speed of light)