… but the equilibrium is unstable. in order to prevent the universe from either expanding or...

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Page 1: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field
Page 2: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field
Page 3: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field
Page 4: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field
Page 5: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field
Page 6: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field
Page 7: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field

… but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field that was called

The Cosmological Constant

in order to keep the universe static.

Page 8: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field
Page 9: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field
Page 10: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field
Page 11: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field
Page 12: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field
Page 13: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field
Page 14: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field

The Age of the Universe

No gravity: v = Hor to = r/v = Ho-1

Newtonian gravity for a flat universe:

½ mv2 - GmM/r = 0 v = dr/dt = (2GM/r)½

so we can integrate r½dr = (2GM)½dt to get

to = 2/3 (r3/2GM)½ = 2/3 (r/v) = 2/3 Ho-1

Ho = 73.8 ± 2.4 (km/s)/Mpc.

to = 13.7 billion years

Page 15: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field
Page 16: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field
Page 17: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field

Oscillations on many scales

Source: Wayne Hu: background.chicago.edu

Page 18: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field

Power Spectrum

cosmic variancelimited for l<354

S/N>1for l<658

Page 19: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field
Page 20: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field

Evidence for the Hot Big Bang

Abundances of the light elements

BBN measures the universe at approximately t = 200 s

Hubble flow

Ho measures the universe at approximately t = 1010 yrs

Cosmic microwave background radiation

CMB measure the universe at approximately t = 4 x105 yrs

Page 21: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field

Galactic Rotation Curves

For a star of mass m a distance r from the center of a galaxy, where the total mass interior to r is M(r):

mv2/r = GM(r)m/r2

so that we would expect

v= [GM(r)/r] ½ so that v should go like r -½

Page 22: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field
Page 23: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field
Page 24: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field
Page 25: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field
Page 26: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field
Page 27: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field
Page 28: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field
Page 29: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field

Size and Scale of the UniverseSize and Scale of the Universe

Image courtesy of The Cosmic Perspective by Bennett, Donahue, Schneider, & Voit; Addison Wesley, 2002

Page 30: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field

You Are Here

The Milky Way Galaxy is a giant disk of stars 160,000 light-years across and 1,000 light-years thick.

There are over 100 Billion stars in the Milky Way

The Spiral arms are only 5% more dense than average, and are the locations of new star formation

The Sun is located at the edge of a spiral arm, 30,000 light-years from

the center

It takes 250 Million years for the Sun to complete one orbit

The Milky Way GalaxyThe Milky Way Galaxy

Page 31: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field

The Local GroupThe Local Group

• Contains 3 large spiral galaxies--Milky Way, Andromeda (M31), and Triangulum (M33)—plus a few dozen dwarf galaxies with elliptical or irregular shapes.

• Gravitationally bound together—orbiting about a common center of mass

• Ellipsoidal in shape

• About 6.5 million light-years in diameter

Page 32: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field

The Local SuperclusterThe Local Supercluster

• A cluster of many groups and clusters of galaxies

• Largest cluster is the Virgo cluster containing over a thousand galaxies.

• Clusters and groups of galaxies are gravitationally bound together, however the clusters and groups spread away from each other as the Universe expands.

• The Local Supercluster gets bigger with time

• It has a flattened shape

• The Local Group is on the edge of the majority of galaxies

• The Local Supercluster is about 130 Million light-years across

Page 33: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field

The UniverseThe Universe1.

3 B

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• Surveys of galaxies reveal a web-like or honeycomb structure to the Universe

• Great walls and filaments of matter surrounding voids containing no galaxies

• Probably 100 Billion galaxies in the Universe

The plane of the Milky Way Galaxy obscures our view of what lies beyond. This creates the wedge-shaped gaps in all-sky galaxy surveys such as those shown here.

Page 34: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field

The UniverseThe Universe

Computer Simulation

The observable Universe is ~26

Billion light-years in diameter.

Page 35: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field

The UniverseThe Universe

Page 36: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field
Page 37: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field

The distance to the center of the Milky Way is about 104 pc, whereas the size of the solar system is about 10-4 pc. If the distance to the center of the Milky Way were scaled to the size of this room (10 meters), then on the same scale the solar system would be about the size of: 

A. An atom (10-10 m); B. A molecule of DNA (10-7 m); C. A pin head (10-3 m); D. A foot (10-1 m); E. You (1 meter).

Page 38: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field

Elements of an Interactive Classroom

• Feedback (Clicker questions)

• Peer education (Think pair share)• • Formative and summative assessment (JiTT)

• Inquiry based learning (workshop style classrooms)

• Web-based activities & resources (facebook, youtube, twitter & compadre)

• Visualizations (Phet Simulations, demos)

Page 39: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field

A "Hubble diagram" is a graph of:

A. Brightness versus wavelength or frequency; B. Luminosity versus temperature; C. Mass versus radius; D. Size versus time; E. Velocity versus distance.

Page 40: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field

What is the principal observational evidence that the age of the Universe is about 14 billion years?

A. The oldest rocks (carbonaceous chondrites) in the solar system indicate an age of 14 billion years; B. Radioactive decay of heavy elements created in the Big Bang indicates an age of 14 billion years; C. The main sequence turn-off point in the HR diagrams of globular clusters indicates ages of about 14 billion years; D. Light from the most distant galaxies and quasars appears to be about 14 billion years old; E. The reciprocal of Hubble's constant gives an estimate of the age of the Universe.

Page 41: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field

How can astronomers measure that a galaxy is rotating?

A. From the rotating motion of the galaxy on the sky; B. From its redshift; C. From the difference in the redshift of the galaxy from one side to the other; D. From the swept back appearance of its spiral arms; E. From Cepheid variables in the galaxy.

Page 42: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field

The distance to the center of the Milky Way is about 104 pc, whereas the size of the solar system is about 10-4 pc. If the distance to the center of the Milky Way were scaled to the size of this room (10 meters), then on the same scale the solar system would be about the size of: 

A. An atom (10-10 m); B. A molecule of DNA (10-7 m); C. A pin head (10-3 m); D. A foot (10-1 m); E. You (1 meter).

Page 43: … but the equilibrium is unstable. In order to prevent the universe from either expanding or contracting, Einstein introduced a scalar field

There was a revolution in cosmology, leading to the "Standard Model of Cosmology" (according to which the Universe contains 70% Dark Energy, 26% non-baryonic Dark Matter, 4% baryonic matter). What observational discovery caused the revolution?

A. The redshifts of galaxies showed that the Universe is expanding; B. The discovery of the Cosmic Microwave Background.C. The rotation of spiral galaxies showed the existence of Dark Matter; D. All of the above