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Mini review of where we

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Therefore a major goal of some people is to go out and measure these quantities ... Electrons and protons are free of each other in a weird' state we call a 'plasma. ... – PowerPoint PPT presentation

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Title: Mini review of where we


1
Mini review of where weve come from CMB, SNe
Ia, And Clusters tell us the universe is mostly
dark energy and will expand forever. Plus that we
need CDM Escape Equation and adiabatic expansion
show how why we want to measure H, Wm, WL, plus
how k, R, t, etc are all related. Didnt derive
how t depends on Wm, WL, etc, did argue by units
that 1/H gives approximate age
2
Defined de-acceleration parameter as W/2 for L
0, matter dominated era, but a different
physical concept. Showed static universe
naturally requires dark energy. This gives a
negative pressure for positive matter and k 1.
We can see from dU -pdV this causes
expansion From de-acceleration definition and
that q Wm/2-WL for measured values of WL and Wm
we can see the universe is accelerating today
3
  • Big Bang pretty good
  • BB was invented to explain several things
  • We know we need more (CDM and L) but
  • Theres more
  • Inflation is needed ( maybe, you be the judge)

4
Classical BB was based on laboratory (confirmed)
physics. Do next. We can use R(t) and t versus
1z and T T0(1z), I never proved in detail
comes from radiation density (rr) proportional to
T4 and rr goes as rr0(R(t0)/R(t))4 Also use r
ro(R(t0)/R(t))3, for matter
5
  • First a review of what BB does explain
  • And how
  • We will put in detail!
  • Logical progression from the escape equation math

6
The Big Bang Explains
  • Why the sky is dark at night (Olbers paradox).
  • Why the Universe is old.
  • Why the Universe is mainly hydrogen and helium.
  • The existence of the CMB.
  • That the Universe is expanding.

7
Olbers Pardox
  • If the Universe were infinite
  • AND UNEVOLVING
  • uniform in density of stars (or galaxies)
  • then we would be burned to crisp.
  • From simple geometry
  • The apparent brightness of objects falls off as
    one over the distance squared.

8
Olbers Pardox, cont.
  • Number of objects per unit volume in a shell at a
    distance goes as the distance squared.
  • Exactly cancels the one over distance squared
    dimming of an individual star or galaxy.
  • The sum of all the brightness adds to infinity if
    the Universe is static, un-evolving, uniform in
    density, and infinite.

9
Olbers Pardox, cont.
  • The BB defeats Olbers Paradox by
  • Expanding universe
  • Star formation had a beginning.
  • Stars to evolve.
  • Expansion is not necessary, however, only that
    stars live for a finite time is.

10
  • The BB says the Universe expands
  • And we observe expansion
  • Our models with the escape equation give
    expansion
  • The observation of distant objects plus (time it
    takes light to travel implies a large age)
  • The CMB (universe has been cooling) fits with
    expansion model and observations
  • Model says the Universe is about 15 billion years
    old.

11
BB Explains Hydrogen Heliumso called BB
Nucleo-synthesis
  • The Big Bang starts the Universe off with a hot
    big bang!
  • The initial universe was then hot and dense in
    the first 3 minutes (or so) to burn (fuse)
    hydrogen into helium.
  • Expansion prevented heavier elements from being
    formed in any significant quantities.

12
  • Universe in first 3 minutes not too hot to break
    up He and not too cold or under dense to fuse H
    into He.
  • Works if we start at 1 second with a reasonably
    high T (about 1 million K).
  • We can estimate this T and density (r) by
    extrapolating back from the brick wall
  • know T, r, 1z of brick wall when becomes
    transparent from simple atomic physics

13
  • 1z R(t0)/R(t)
  • t AR(t)2 A constant
  • applies in radiation dominated era
  • about 100,000 years before brick wall becomes
    transparent.
  • know t, know T at brick wall transparent
  • Extrapolate back to t 1 second
  • using T T0(1z) gt at 1 second
  • T 1 million K , OK!

14
  • We also know the physics of radiation , matter
    etc. well enough to do this back to 1 second, at
    least. See the book, page 376, figure 13.7
  • Key players are protons, neutrons, electrons
    and neutrinos.
  • Neutrons decay into protons, electrons, and
    neutrinos.
  • the reverse can happen as long as the temperature
    and density are high enough.

15
  • gt density and temperature fall and a
    significant number of free neutrons have
    decayed, the fusion process halts.
  • Half of all of free neutrons will decay in about
    10.6 minutes
  • Net effect is that after about 3 minutes process
    stops
  • The higher the density, the higher the
    probability the neutrons and protons will join up
    and eventually make He.

16
  • An intermediate step join of proton to neutron
    deuterium D.
  • The simple process is then p n gt D
  • D p gt light He (with only 1 neutron) written
    3He.
  • 3He 3He gt 4He (ordinary, super stable helium)
    stuff
  • The denser the material, the more D is burned
    into He at faster rate than D is made.

17
Baryonic matter
18
gt Higher He/H tracks with lower D/H
19
The Net Result cont.
gt A measure of the ratio of He/H and or D/H is
the most direct method we have of determining Wb.
  • gt A measure of the ratio of He/H and or D/H is
    the most direct method we have of determining
    Wb.
  • Therefore a major goal of some people is to go
    out and measure these quantities while others
    make sure the theory is correct.

20
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21
  • Neutrinos are so penetrating that
  • IF we could detect them
  • we could see back to about the 1st second
  • Very exciting

22
  • The BB model then starts out hot and dense to
    explain He/H and D/H.
  • The Universe expands and cools until the brick
    wall becomes transparent.
  • gt What is the brick wall made of and how to we
    predict transparency?
  • The brick wall is mainly hydrogen gas but before
    it becomes transparent, the hydrogen is nearly
    totally ionized.
  • Electrons and protons are free of each other in a
    weird state we call a plasma.

23
The CMB more details now
  • As the Universe expands,
  • Both the hydrogen gas and the photon gas cool.
  • If hot enough, the photons can separate
    electrons from protons that might have joined
    together to make ordinary hydrogen gas.
  • And at the same time electrons are very efficient
    at absorbing or scattering photons.
  • So the photons cant travel far and we have
    brick wall.

24
The CMB more details now
  • Eventually, however, the gases (photons,
    electrons, and protons) cool so much
  • that the photons dont have enough energy to free
    bound (to protons)
  • not enough to even to excite the atom by being
    absorbed. (Nature has conspired so that
    electrons can only circle the proton in certain
    specific orbits and if there isnt enough energy
    for an orbital transfer, the photon cant be
    absorbed be the atom.)

25
The CMB more details now
  • So gases cool down to point where hydrogen
    becomes atomic hydrogen and the gas suddenly
    becomes transparent. The photon gas then streams
    away on its own to reach us today as the CMB.

26
The BB doesnt really say why started out hot or
expanding but
  • The model is consistent with this much of the
    data.
  • Using only laboratory physics
  • We already know some problems smoothness of
    CMB, CMB fine structure, SNe Ia, and clusters.
    But some say we need more gt enter Inflation
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