The Big Bang Theory

Galaxies: islands of stars making up the universe

Edwin Hubble First to realize that galaxies lie

outside the Milky Way …

… by measuring their distances using Cepheid variables as ‘standard candles’

Edwin P. Hubble (1889-1953) was trained as a lawyer, before boredom made him turn to astronomy instead

Cepheid variables oscillate in brightness with a regular period that depends on their luminosity. By measuring this period, they can be used as standard candles.

Cosmic Speedometer

When a galaxy is receding, light waves travelling to us are red-shifted

Hubble measured the spectrum of these galaxies and found the spectral lines to be red-shifted

The faster the recession, the greater the red-shift

Hubble’s Law

Hubble noticed a correlation between the distance of the galaxies and the speed at which they are moving away from us

Hubble constant graph

Expansion of the Universe

… ‘winding’ backwards, the universe must have had a beginning

Georges Lemaître (1894-1966) was a Belgian Catholic priest who was fond of saying there is no conflict between science and religion

Georges Lemaître

Proposed that the universe began with the explosion of a ‘primeval atom’

His model was improved by George Gamow and others, who proposed that elements were forged during this hot and dense stage

Known as the Big Bang theory today; coined by Fred Hoyle who proposed a rival theory ...

Steady State Model

Universe is expanding, but maintainsa constant average density

Matter is continually being created in the voids to form new stars, galaxies

Universe has no beginning and no end

But disproved with the discovery of …

Cosmic Microwave Background (CMB)

Background radiation from the sky that is isotropic (same strength in all directions)

Corresponds to a temperatureof just 2.7 Kelvins

Identified as the radiation left over from the Big Bang explosion

Arno Penzias (right) and Robert Wilson of Bell Laboratories, next to the horn antenna with which they discovered the CMB in 1965

Cosmic Background Explorer (COBE)

The COBE was the world’s most sensitive thermometer, built to probe the heat radiation left over from the Big Bang. In 1992, it detected fluctuations of just a few millionths of a degree in the CMB.

CMB Maps by COBE of the Entire Sky

1) This dipole signal is due to the motion of the Earth through space. The CMB is blue-shifted in the direction of Earth’s motion, and red-shifted in the opposite direction

2) After the dipole signal has been subtractedout, we are left with a hot central bandrunning across the sky, which is due to ourown Milky Way

3) The final CMB map is obtained after both the dipole and galaxy signals have been removed. The resultis a map of regions that are a few millionths of a degree hotter (pink) or colder (blue) than average

These tiny fluctuations have evolved into clusters of galaxies today

Tests of the Big Bang Theory

Expansion of the universe

Cosmic microwave background

Relative abundances

of hydrogen,

deuterium, helium

and lithium

Obtaining the Age of the Universe

Extrapolate the current expansion rate (Hubble constant) back to the Big Bang

– 10 to 20 billion years old

Look for the oldest stars (in globular clusters)

– 11 to 18 billion years old

Best current estimate is 13.4 ± 1.6 billion years

M10 Globular Cluster

Problems with the Big Bang Theory

Flatness problem

– why is the geometry of universe so

close to being flat?

Horizon problem

– why is the universe so isotropic?

Smoothness problem

– why is the universe so

– homogeneous?

Why does the universe appear so uniformeven on opposite sides of the sky, whichcould never have been in causal contactwith each other?

Alan Guth: Inflation

Lasted between 10-35 and 10-32

seconds after the Big Bang

Universe expanded by a factor of

1050, from smaller than an atom to

bigger than a galaxy

It was driven by vast amounts of energy released when a ‘symmetry breaking’ phase transition occurred

Alan Guth of MIT was only 32 when he developed the theory of inflation in 1979

Inflation to the Rescue

Flatness problem

Horizon and smoothness problems

In each successive frame, the sphere is inflated by a factor of three. By the fourth frame, it looks like a flat plane. Thus, inflation drives the geometry of the universe toward flatness

Without inflation, the universe today would consist of a patchwork of different regions. Instead, it is very uniform

Inflation had the effect of expanding a small region to a very large one. Since we are inside such a region, our neighborhood appears uniform

Summary: Timeline of the Universe

Timeline of the Universe 2

Possible Fates of the Universe

Will the Universe Recollapse?

Gravitational pull of the galaxies on each other

is slowing down the rate of expansion

Required density for the universe to recollapse is 4.5 x 10-30 g/cm3

Observed density of luminous material (stars, galaxies) is about 3 x 10-31 g/cm3

Dark Matter

But there may be about 10 times this amount in the form of ‘dark matter’

So the universe is very close to the threshold for recollapse! (This is related to the flatness problem)

Measurements of the velocities of stars ina galaxy show that there must be morematter in the galaxy than is apparent.This ‘dark matter’ is known to form aninvisible halo around the galaxy

Possible forms of dark matter

If the universe recollapses ...

If the universe expands forever ...

“Some say the world will end in fire, others say in ice.” – Robert Frost

Your Research Presentation

Groups must do more extensive research into the following topics:

1) Red Shift/Doppler Effect

2) Cosmic Microwave Background Radiation

3) Inflation

4) Steady State Model

5) Cepheid Variables and Hubble Constant

6) Fates of the Universe

Project RequirementsThursday Meet in Computer Lab 322

1) 8 Minute (minimum) Power Point Presentation• Each Group Member must speak• Each slide must be labeled by the creator of the

slide

2) Each group must create one paper poster summarizing their topic

3) Draft slides (one per student) due Thursday, September 15th (50 classwork points)

4) 2nd Draft Slides due Tuesday, September 20th

(50 classwork points)

5) Presentations next Thursday, SEPTEMBER 22nd (100 project points)