Announcements
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Announcements. Scores from the fourth exam are available on WebCT. Final exam is Monday, May 9, at 7:30 am. Students with last names A-K go to 225 CB. Students with last names L-Z go to 300 CB. All students must bring their ID. Iowa Book and Supply will buy back textbooks and PRS units.

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Announcements

Announcements

  • Scores from the fourth exam are available on WebCT.

  • Final exam is Monday, May 9, at 7:30 am.

    • Students with last names A-K go to 225 CB.

    • Students with last names L-Z go to 300 CB.

    • All students must bring their ID.

  • Iowa Book and Supply will buy back textbooks and PRS units


Expansion of the universe and curved spacetime

Expansion of the Universe and Curved Spacetime

  • Expansion of the Universe

  • Geometry

  • Non-Euclidean geometry

  • Geometry of the Universe


Hubble expansion v h 0 d

Hubble expansion v = H0d


Expansion of the universe

Expansion of the Universe


Motion at constant velocity

Motion at constant velocity

distance = velocity  time velocity = 0.5 cm/s

time = distance / velocity = 3 cm/(0.5 cm/s) = 6 s


Receding galaxy

Receding galaxy

Velocity =

= 500 km/s

= 0.508 Mpc/Gyr

When were galaxies in the same place?

time = distance / velocity = 7 Mpc/(0.508 Mpc/Gyr)

= 13.8 Gyr ago


Hubble expansion v h 0 d1

Hubble expansion v = H0d

Time = distance/velocity

= d/H0d

= 1/H0

= 1/(71 km/s/Mpc)

= 13.8 Gyr


Announcements 3307051

An observer at a distance of 3 billion light years from us looking in our general direction would see

  • most of the galaxies approaching her.

  • the same Hubble’s law that we see.

  • about equal numbers of red and blue shifted galaxies.

  • everything rushing away from a point near the Milky Way galaxy.


Two dimensional geometry

Two dimensional geometry

  • Only two directions: up/down and left/right

    : north/south and east/west

  • All motion of particles, light confined to two dimensions

  • Examples: black board, piece of paper, surface of sphere, surface of donut, surface of saddle


Geometry

Geometry

  • How are the diameter and circumference of a circle related?

  • What is the sum of all of the angles in a triangle?


Geometry in flat space

Geometry in flat space

  • Circumference = 2  radius

     = 3.1415926… 2 = 6.28…

  • The sum of the angles in a triangle is 180º


Non euclidean geometry

Non-Euclidean Geometry

  • How about in a curved space?

  • Do demo 8C10.50


Geometry in positively curved space

Geometry in positively curved space

  • Circumference < 2  radius

  • The sum of the angles in a triangle > 180º


Properties of positively curved space

Properties of positively curved space

  • Finite

  • Unbounded

  • No center

How do the properties of positively curved space differ from flat space?


Geometry in negatively curved space

Geometry in negatively curved space

  • Circumference > 2  radius

  • The sum of the angles in a triangle < 180º


Review questions

Review questions

  • Suppose it was discovered that the Hubble constant is twice the value that it is currently thought to be, how would this change our estimate of the age of the Universe?

  • Compare a flat universe with a positively curved universe as to whether they are finite, bounded, and have a center.


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