Monday, November 12, 2007 Vilenkin Chs: 1-3.

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Presentation transcript:

Monday, November 12, 2007 Vilenkin Chs: 1-3

Agenda Announce: Handback/discuss tests Chs. 1-3 No Class on Thursday Read Chs 4-6 Handback/discuss tests Chs. 1-3

Vilenkin’s Many Worlds in One Cosmology—study of the large scale structure of the Universe What constitutes “large scale”? How is this different than material in Thorne’s book? Ford’s book? How are all three books similar?

The Big Bang (Theory) Features of the theory Universe has been expanding from some smaller region (not into anything!) Was very hot and cools as it expands Primordial nucleosynthesis

Big Bang Evidence #1 Hubble’s observation of the expansion of galaxies Why not stars? Are we at the center? What’s expanding?

Big Bang Evidence #2 CMBR—Cosmic Microwave Background Radiation Hugely isotropic radiation associated with the Universe (what does this mean?) Indicative of a very cold temperature of the Universe of 2.73 Kelvin (how so?)

If you’re still not convinced… All the astrophysics we do which relies on Big Bang…..Works! That’s what we said about relativity and quantum mechanics Again, it’s not that we wish to brainwash you…we’d desperately want to find stuff that does not work!

What Banged? The big bang theory doesn’t attempt to explain what banged, how, or why Free to insert God, philosophy, etc here Not particularly clear how far science, even in principle, take us

Guth’s Proposal Substance w/ special properties Causes gravity to be repulsive (not a new force) Density always remains the same Doesn’t decrease w/ expansion Increasing strength with increasing volume Energy comes from increasingly negative gravitational energy Termed Inflation

Inflation Universe began Expanded very quickly for a short time very small Chunk of this “repulsive gravity stuff” Expanded very quickly for a short time Repulsive stuff decayed away producing lots of hot particles Universe continued expanding (not so fast) and cooling and that’s what we observe now

Einstein & Cosmology Study a very simple Universe Homogenous—unform density Isotropic—looks same in all directions Static (why?)—doesn’t change in time No solution for such assumptions Stuff wants to attract other stuff Decides his equations must be changed…

Einstein’s Biggest Blunder How could he change equations? Needed to maintain “reference frame invariance” Constant speed of light Only freedom was to introduce cosmological constant Energy of empty space Strange stuff: Negative pressure (tension)

Nature of Vacuum Energy Constant (in space and time) energy density and tension Can’t see effect of tension or energy density because it’s everywhere Except for its gravitational effect Tension so great overcomes its energy density to produce “anti-gravity” Can produce a static universe where vacuum energy balances attraction of the rest of the Universe

Friedmann’s Universe(s) Assume: Homogenous Isotropic Closed (but not static) Universe expands (bigger sphere) Then contracts (smaller sphere) Big Bang and Big Crunch are singular

Do you prefer eternal Universe or singular beginning? The problem with an eternal universe: Eventual heat death…everything reaches same temperature (thermal equilibrium) Entropy increases in a closed system (2nd law) So if Universe has existed forever, then we should be in state of maximum entropy…we don’t so Universe not eternal The problem with a 13.7 billion year old Universe: Why did it start then? How was it homogenous and isotropic? etc

The Competitor: The Steady State Theory Universe remains essentially the same (steady state) Universe expands (as per Hubble) Matter continually gets created in voids left by expansion Failure of energy conservation comparably to creation of Universe at Big Bang However, observations show differences long ago…universe didn’t look same billions of years ago