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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

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. - PowerPoint PPT Presentation

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Page 1: 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

Page 2: Announcements

Expansion of the Universe and Curved Spacetime

• Expansion of the Universe

• Geometry

• Non-Euclidean geometry

• Geometry of the Universe

Page 3: Announcements

Hubble expansion v = H0d

Page 4: Announcements

Expansion of the Universe

Page 5: Announcements

Motion at constant velocity

0

0.5

1

1.5

2

2.5

3

3.5

0 1 2 3 4 5 6

Time [s]

Dis

tan

ce [

cm]

distance = velocity time velocity = 0.5 cm/s

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

Page 6: Announcements

Receding galaxy

01

23

45

67

8

0 2 4 6 8 10 12 14

Time [Gyr]

Dis

tan

ce [

Mp

c]

When were galaxies in the same place?

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

= 13.8 Gyr ago

Velocity =

= 500 km/s

= 0.508 Mpc/Gyr

Page 7: Announcements

Hubble expansion v = H0d

Time = distance/velocity

= d/H0d

= 1/H0

= 1/(71 km/s/Mpc)

= 13.8 Gyr

Page 8: Announcements

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

1. most of the galaxies approaching her.2. the same Hubble’s law that we see.3. about equal numbers of red and blue shifted

galaxies.4. everything rushing away from a point near

the Milky Way galaxy.

Page 9: Announcements

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

Page 10: Announcements

Geometry

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

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

Page 11: Announcements

Geometry in flat space

• Circumference = 2 radius

= 3.1415926… 2 = 6.28…

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

Page 12: Announcements

Non-Euclidean Geometry

• How about in a curved space?

• Do demo 8C10.50

Page 13: Announcements

Geometry in positively curved space

• Circumference < 2 radius

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

Page 14: Announcements

Properties of positively curved space• Finite

• Unbounded

• No center

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

Page 15: Announcements

Geometry in negatively curved space

• Circumference > 2 radius

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

Page 16: Announcements

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.