Prof. Mel Ulmer DEPT OF PHYSICS & ASTRONOMY

19
Prof. Mel Ulmer DEPT OF PHYSICS & ASTRONOMY http://www.astro.edu/astro/faculty/ulmer/ a01_fall2002.html No discussion section meetings this week Next week begin observing, no signups necessary

description

Prof. Mel Ulmer DEPT OF PHYSICS & ASTRONOMY. Next week begin observing, no signups necessary. http://www.astro.edu/astro/faculty/ulmer/a01_fall2002.html. No discussion section meetings this week. Big Bang Myth. - PowerPoint PPT Presentation

Transcript of Prof. Mel Ulmer DEPT OF PHYSICS & ASTRONOMY

Page 1: Prof. Mel Ulmer DEPT OF PHYSICS               &      ASTRONOMY

Prof. Mel Ulmer

DEPT OF PHYSICS

&

ASTRONOMY

http://www.astro.edu/astro/faculty/ulmer/a01_fall2002.html

No discussion section meetings this week

Next week begin observing, no signups necessary

Page 2: Prof. Mel Ulmer DEPT OF PHYSICS               &      ASTRONOMY

Big Bang Myth

• 15 billion years ago universe was hot and dense and expanding

• It cooled and got less dense until it got to about 3000 K [273 K = 0 Celsius]• Then the gas became transparent = emits light

• We see this light today as the Cosmic Microwave Background (CMB) = really cold = 3 K

Page 3: Prof. Mel Ulmer DEPT OF PHYSICS               &      ASTRONOMY

Brick Wall, 15 billion lt yrs

Page 4: Prof. Mel Ulmer DEPT OF PHYSICS               &      ASTRONOMY

Basic Concepts• Space and time are interrelated

• Far away = look back in time. =>

• Brick wall about 15 billion light years away from us =>

• far away means looking at younger universe

• Brick wall = 500,000 to 1 million years old.

• The further away, more rapid expansion

• = The larger the shift to the red

• “redshift” = 1+z =>

Page 5: Prof. Mel Ulmer DEPT OF PHYSICS               &      ASTRONOMY

Big Bang Myth Details

• Seeing to the brick wall rushing away from us so it has a“redshift” of 1+z =1000 and T=T_o(1+z)

• T=temp of brick wall, T_o=Observed today

Page 6: Prof. Mel Ulmer DEPT OF PHYSICS               &      ASTRONOMY

• Look far away, we see universe when it was denser!

•Too dense to see through

• The brick wall concept… we see back until the universe is too dense for light to penetrate!

• Far away means long ago and high velocity of recession goes with z and redshift

• Long ago means the universe was hot and dense then

•But hot then but looks cold now

Page 7: Prof. Mel Ulmer DEPT OF PHYSICS               &      ASTRONOMY

• Key concepts:

•Expansion, distance, and “time travel” are all related

•Far way = long ago = objects moving away from us faster the further away they are.

•Long ago means (in our Myth) hot and dense

•Today means old and “sparse”

•At Brick Wall density = about 10-21 g/cm3)

• Today, density = about 10-30 g/cm3

Page 8: Prof. Mel Ulmer DEPT OF PHYSICS               &      ASTRONOMY

Brick Wall Facts:

•If Brick Wall density much less than air (about a billion, billion times less, why can’t we see through it?)

• Because it is about 1,000 light years thick and physics (deferred to later in the course)

Page 9: Prof. Mel Ulmer DEPT OF PHYSICS               &      ASTRONOMY

•Brick Wall (a.k.a. the CMB) was found to be too smooth to be explained by ordinary matter. Why? (again more deferred to later)

• Ordinary matter affects light with electrons (think electricity, radio, TV etc).

• If we assume initial lumps made of of enough ordinary matter to make clusters, CBM would have been lumpier

Page 10: Prof. Mel Ulmer DEPT OF PHYSICS               &      ASTRONOMY

• How much?

•About 10-100 times too much!

• “Simple” calculation to “see this”:

• Go backwards in time.

• Clusters don’t contract (aren’t expanding now, this is reverse)

•Universe does get more dense take ratio of densities cluster [lump] to average = about 5/10,000 = 500/1,000,000 versus observed smoothness to 50/1,000,000

Page 11: Prof. Mel Ulmer DEPT OF PHYSICS               &      ASTRONOMY

Model Universe Based on GR• Model is that we live on a 4-dimensional surface

• The more matter, the more tightly curved the surface:

• Works “locally,” and for the entire universe =>

• Concept of curvature of Universe

• It is related to the “mass density of the universe

Page 12: Prof. Mel Ulmer DEPT OF PHYSICS               &      ASTRONOMY

• Curvature (k)

• k = +1, closed (balloon)

• k = 0 flat (sheet)

• k= -1 open (saddle)

Page 13: Prof. Mel Ulmer DEPT OF PHYSICS               &      ASTRONOMY

k=-1

k=0

k=+1

Page 14: Prof. Mel Ulmer DEPT OF PHYSICS               &      ASTRONOMY

GR Concepts, Cont.

> 1; k =+1

0=1 ; k = 0

0<1 ; k =-1

•Additional concept: “density parameter = 0; the

subscript 0 means “today”

• stands for a ratio of the density of the universe to some “critical value” (later)

and k are intimately related:

Page 15: Prof. Mel Ulmer DEPT OF PHYSICS               &      ASTRONOMY

•Basic Holy grails of our Myth:

k and 0

• Other one, does universe expand forever or not?

• knowledge of value of 0 ALONE used to guarantee we could predict the future

• “Ain’t necessarily so”!!!

Page 16: Prof. Mel Ulmer DEPT OF PHYSICS               &      ASTRONOMY

complex case is ( greater than 0 )

value k value surface future

Greater than 1 +1 closed expand forever#

1 0 flat expand forever

Less than 1 -1 open expand forever

#unless m > 3, just barely positive = 0.01

Page 17: Prof. Mel Ulmer DEPT OF PHYSICS               &      ASTRONOMY

• Because of dark energy!

• Energy and mass are equivalent through E = Mc2

•Dark Energy contributes to

but

• Dark Energy can act as a pressure to push the universe apart more strongly than the Dark Energy mass pulls things in

Page 18: Prof. Mel Ulmer DEPT OF PHYSICS               &      ASTRONOMY

Basic Concepts Cont.•Additional holy grail: amount of Dark Energy =>•We need to know

• (Dark Energy mass ratio),

• m (total matter [= “stuff”] ratio),

• Total gives us k

• Generally, positive means will expand forever.

Page 19: Prof. Mel Ulmer DEPT OF PHYSICS               &      ASTRONOMY

Bottom Line:

= 0.7, m = 0.3, k= ?

0

Why do we believe this?

Observations plus “faith” in GR