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Time Travel Research Center
© 2005 Cetin BAL - GSM:+90 05366063183 - Turkey / Denizli
The Observable Universe
Contents
The Observable Universe
Big Bang Theory
Dark Energy, Dark Matter
Parallel Universes, Multiverse - the Unobservable Universe
Footnotes
References
Index
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The observable universe is the space around us bounded
by the observable horizon - the distance to which light can have
traveled since the universe originated. This space is huge but finite
with a radius of 1028 cm. There are definite total numbers of
everything: about 1011 galaxies, 1021 stars, 1078
atoms, 1088 photons. There is a hierarchy of structure:
Everything is composed of smaller things and is a part of something
larger as shown in Figure 02-01 and
Figure
15-01. The character of structures with different scale changes
according to the interplay of various physical forces. Quantum phenomena
control the small scales, while gravity dominates on large scales, and
both come into play at the beginning of the universe. On each scale of
size there is a corresponding scale of time: processes tend to happen
quickly on small scales and slowly on large scales. |
Figure 02-01 The Observable Universe
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Big Bang Theory
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In 1922 Alexander Friedmann predicted the Big Bang cosmology, which portrays the
universe as expanding space from a point where the matter-energy density
was extremely high. The expansion can be visualized by a two dimensional
analogy as shown in Figure 02-02. As the balloon expands, all the points
on the surface recede from each other, and the wavelength on the surface
is stretched. It is similar to the shift to longer wavelength when the
source and receiver are moving away from each other. |
Figure 02-02 Cosmic Expansion
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This phenomenon is called red shift
of the spectrum because in visible light the shift to longer wavelength is
toward the red colour. It plays a prominent role in discovering the cosmic
expansion through the detection of the spectral line shift from distant
galaxies.
This simple picture of expanding universe with all the galaxies flying
away from each other remained unchanged until 1980s when the Inflation
Theory
was introduced to resolve a number of discrepancies. The rapid expansion
occurred at the interval between 10-35 sec and 10-33
sec. It predicts a much smaller universe near the origin of the Big Bang
such that the matter-energy within can be mixed evenly as reflected in the
CMBR mapping. It also predicts that the geometry of
the Universe is flat. Events before the
inflation is essentially unknown. It is subjected to a lot of speculations.
For example, it is suggested that space-time may be created from vacuum
fluctuation - the quantum foam; and that the four fundamental forces may be unified to
just one kind (as envisioned by the
theory of
superstrings). Baryongenesis (generation of quarks and anti-quarks which
has a baryon number of 1/3 or -1/3) happened in an epoch before inflation,
when a imbalance between matter and anti-matter was established by a quantum
process called CP violation. Quarks and anti-quarks combined to form baryons and mesons at
10-5 sec. Nucleosynthesis started at about 3 min. During this
epoch the light chemical elements were produced from protons and neutrons.
The universe was still opaque up to 380,000 years when neutral atoms started
to form and the radiation was able to escape as shown by the CMBR. This
epoch is called decoupling to indicate that matter and radiation are
separated. From then on matter had a chance to condense into stars and
galaxies and evolved to the present-day universe. Figure 02-03 shows the
history of the universe according to the Big Bang Theory.
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Supplement to the legend of Figure
02-03:
The quark (q), electron (e), and neutrino (n) are the fundamental
particles. The corresponding anti-particle is labeled with a bar on top.
The gluon (g) is the boson mediating the strong interaction between
quarks. The vector bosons W and Z mediate the weak interaction between
electrons/neutrinos and the quarks. The photon (wavy line) mediates the
electromagnetic interaction between charged particles. One quark and one
anti-quark combine to form a meson. Three quarks combine to form a
baryon (proton, neutron, etc.). Protons and neutrons combine to form
nucleus (ion). Nucleus and electrons combine to form atom. The muon (m)
and tau (t) are the 2nd and 3rd generation of the lepton family, the 1st
generation is the electron. (See more about elementary particles in
Topic-15.)
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Figure 02-03 History of the Universe
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There are scales for the time t (in second), temperature T (in oK)
and energy E (in Gev) at the bottom of Figure 02-03. These variables are
related by the simple mathematical formulas:
E(Gev) = 10-3 / t1/2(sec), and E(Gev) = 10-13
x T(oK)
There is no such simple formula for the size of the observable universe and
these variables. Its relationship with time can be plotted in a
graph.
Table 02-01 depicts the sequence of events after the Big Bang in time order.
The relics and observables are physical facts, while the interpretations of
the events are mostly theories or conjestures.
Era |
Time |
Size
(observable) |
Energy or
Temperature |
Relics & Observables |
Events |
Planck era |
< 10-43 sec |
< 10-33 cm |
> 1019 Gev |
4-dimensional spacetime;
cosmic expension |
Smallest unit
of space-time started to expand |
GUT era |
< 10-36 sec |
< 10-25 cm |
> 1016 Gev |
Super-heavy particles; fundamental interactions |
Separation of spacetime and mass;
gravit-ational,
strong, and electroweak forces |
Inflation |
< 10-34 sec |
< 1 cm + (unob-
servable extent) |
> 1014 Gev |
Observable universe;
large scale structures |
Unstable vacuum;
quantum fluctuations |
Electro-weak era |
< 10-10 sec |
< 1012 cm |
> 100 Gev |
Radiation; excess of matter over antimatter;
separation of force and matter fields |
Radiation released in reheating; baryon-antibaryon
asymmetry; separation of weak and electromagnetic forces, origin of mass |
Strong era |
< 10-4 sec |
< 1016 cm |
> 200 Mev |
Exotic forms of dark matter |
Formation of hadrons from quarks including neutrons
and protons |
Weak decoupling |
< 1 sec |
< 1018 cm |
> 1 Mev |
Hydrogen nuclei domination |
Neutrinos decouple, neutron/proton ratio fixed |
e-e+ Annihilation |
< 5 sec |
< 1019 cm |
> 0.5 Mev |
Photons hotter than neutrinos today |
Electron heat dumped into photons |
Nucleo-synthesis |
< 100 sec |
< 1020 cm |
> 100 Kev |
Light element abendances: D, He, Li |
Nuclear reactions freeze out, stable nuclei form |
Spectral decoupling |
< 106 sec |
< 1022 cm |
> 500 ev |
Blackbody background radiation |
End of efficient photon production |
Matter ~ radiation |
< 104 yrs |
< 1024 cm |
> 3 ev |
Mass density fluctuations |
Matter density ~ radiation density |
Recom-bination |
< 0.3 My |
< 1025 cm |
> 3000 K |
CMBR |
e- and p+ recombine into H
atoms, universe transparent to light |
Dark ages |
< 1 Gy |
< 1027 cm |
> 20 K |
First stars, heavy elements |
mass fluctuations grow, first small objects coalesce,
reionization |
Galaxy formation |
< 2 Gy |
< 2x1027 cm |
> 10 K |
Stars, quasars, galaxies |
Collapse to galactic system |
Bright ages |
< 13 Gy |
< 1028 cm |
> 3 K |
Milk Way
and Solar System |
Gas consumed into stars, remnants, planets |
Present era |
~ 13.7 Gy |
~ 1028 cm |
~ 2.73 K |
Supercluster |
Large scale gravitational instability |
Table 02-01 A History of Cosmic Expansion
In an effect to learn more about the processes occurred in the early
universe, which was associated with very high energy as shown in Table
02-01. Particle Physicists have been simulating the condition in the
laboratory with high energy particle accelerators (see the entries in top
left of Figure 02-03). In collaborating with the theory of elementary
particles, experiments are developed to investigate the creation of
fundamental particles, and their properties. A list of the major
accelerators in the world is shown in
Table
15-01.
It seems that the Big Bang Theory has been validated conclusively with
all these supporting evidences. However, recent observations in the last few
years reveal that there is something amiss. It is noticed that even though
there is not enough mass to hold the stars, galaxies and galaxy clusters in
place, they are still moving around and would not disperse. It looks as if
there is some kind of invisible force (gravity from the dark matter) to hold
them together. The situation is similar to a puppet show, where the audience
can safely assume that someone behind is manipulating the movements.
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The second problem is related to the use of
the Type Ia supernovae as "standard candles" to measure the distance of
remote objects. The measurements imply that the cosmic expansion is
accelerating. It is proposed that there is some kind of repulsive "dark
energy" to induce the acceleration. Figure 02-10a shows the proportion
of the various matter-energy components in the Universe. Most of the
matter-energy content is in the form of "dark energy". The
composition of the Universe is listed in Table
02-02 below. |
Figure 02-10a Energy-Matter in the Universe
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Acceleration of the cosmic expansion is placed on a firmer footing when
it is observed in 2003 that the CMBR becomes slightly hotter after going
through a galaxy, which forms a gravitational (potential) well. Dark energy,
being gravitationally repulsive, makes a gravitational well shallower as a
photon passes through, so the photon exits with slightly more energy than it
had when it entered.
Material |
Representative Particles |
Particle Mass or Energy (ev) |
No. of Particles in Observed Universe |
Probable Contribution to Mass of Universe |
Sample Evidence |
Ordinary (baryonic) matter |
Protons, electrons |
106 to 109 |
1078 |
5% |
Direct observation, inference from element abundances |
Radiation |
photons |
10-4 |
1087 |
0.005% |
Microwave telescope observations |
Hot dark matter |
Neutrinos |
< 1 |
1087 |
0.3% |
Neutrino measurements, cosmic structure |
Cold dark matter |
Supersymmetric particles? |
1011 |
1077 |
25% |
Inference from galaxy dynamics |
Dark energy |
Scalar particles? |
10-33 |
10118 |
70% |
Supernova observations of accellerated cosmic
expansion |
Table 02-02 Composition of the Universe
The nature of both the "dark matter" and "dark energy" is still the
subject of intense research observationally and theoretically. Some of the
suggestions are listed below:
- Cosmological constant - Eistein had introduced a term with the
cosmological constant in the gravitational field equation to keep a static
universe from collapsing. This additional repulsive force is no longer
necessary when the cosmic expansion became apparent. It has become
fashionable again with the new discovery of cosmic acceleration. It is
very tempting to identify the cosmological constant with the vacuum energy
of the various quantum fields. However, the simplest versions of quantum
theory predict far too much energy. One explanation involves the
cancellation of all these fields (of vacuum energy) to almost zero,
leaving only a residual trace corresponding to the observed dark energy.
- Quintessence - This hypothetical form of dark energy permeates all
space. Like inflation, quintessence is thought to have somehow originated
when the universe was just 10-35 sec old. It is driven by a
scalar field whose energy varies gradually. The difference is the energy
and time scale: inflation occurred quickly at very high energies, whereas
the scalar field responsible for quintessence operates at much lower
energies over a much longer time frame.
- Neutrino -
It is a reasonable candidate for dark matter because of its unreactive
nature. Theoretical calculations indicate that there should be as many as
100 million neutrinos for every atom in the universe. However, the recent
estimates of neutrino mass is so slight that it could account for only
about 0.1 - 7 per cent of the mass of the universe.
- WIMP - Many new particles with heavy mass appear in the
supersymmetry formulation. These are referred to as weakly interacting
massive particles, or WIMPs. For example, the photino (the fermionic
partner of photon) has a mass about 10 to 100 times that of the proton.
Most of these electrically neutral particles would, like neutrino, go
straight through Earth. On rare occasion, however, one might interact with
an atom in the material they pass through. So far, the only claimed
detection of a dark matter particle (by an Italian team in 2000) has been
strongly disputed.
- Nonluminous matter - Ordinary hidden matter consists of atoms that
emit little or no light. It includes a host of celestial objects such as
planets, dark gas clouds, brown dwarfs, neutron stars, and black holes.
The Massive Compact Halo Objects Project (MACHO) has been looking for them
in the halo of the Milky Way. A search for microlensing has turned up four
candidates toward the Large Magellanic Cloud and 45 toward the Galactic
Bulge.
- Minimal model - Since we don't feel the effect of dark energy and dark
matter around us except through the gravitational influence on large scale,
a model has been constructed with no noticeable interactions between each
other or with ordinary matter. It fits the observational data such as the
high-redshift supernovae, the microwave background radiation, the
distribution of large-scale structure, and the dynamic of celestial
objects very well. The dominance of dark energy and dark matter over
ordinary matter indicates that human beings are extremely unimportant in
the grand scheme of the universe as suggested in a 1985 movie called "Insignificance''
in which Einstein and Monroe explores relativity and our place in the
universe.
- Future of the universe - It seems that the effect of dark energy
became dominant only recently about 8 x 109 years after the Big
Bang. If the acceleration presists in the future, it will impose a horizon
surrounding a galaxy like the Milkyway - a distance beyond which light
cannot reach us. Figure 02-10b depicts the sequence of events for the
future of the universe with cosmic acceleration according to a computer
simulation (click image to obtain larger view). The model assumes that the
dark energy permeating the vacuum has a positive, constant value - similar
to the cosmological constant, as Einstein once posited.
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Figure 02-10b Future of the Universe
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The subject of parallel universes used to belong to the realm of science
fictions. The idea is familiar on some TV shows such as "Star Trek'', which portrays other worlds that are almost like our own, except
... there is a slight difference. Then some cosmologists propose that our
Universe might be just one of many in an ever-multiplying network of
parallel universes, which they call the
multiverse.
Recent observational data open up the possibility that it is conceivable
scientifically with some imaginative inferences.
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Figure 02-11 shows recent astronomical observations,
which tend to support the hypothesis. The diagram on the left
illustrates the WMAP measurement of the
fluctuations in the CMBR temperature. The strongest fluctuations are
just over half a degree across, which indicates that space is very large
or infinite. In addition, the diagram on the right illustrates the
measurements of matter density from WMAP and 2dF Galaxy Redshift Surveyc.
They are consistent with uniform distribution of matter on large scales.
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Figure 02-11 Universe, Flat and Uniform
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These observational data support the inflation theory,
which suggests that the universe underwent an exponential expansion at
10-35 sec after the Big Bang. The universe became so large
that it looks flat within our event horizon, and in addition, the
contents in the universe were mixed uniformly as witnessed by the CMBR.
Our universe with a size of about 1026 meters (as limited
by the event horizon) is just a speck in comparison to this vast expand.
The number of ways to arrange matter in the space outside our universe
is enormous and each one would have its own event horizon (size); these
are the parallel universes. Statistically, an arrangement similar to
ours is bound to happen given enough space. Thus there would be
universes identical to ours somewhere. However, we cannot communicate
with any of these parallel universes because the speed of light is
finite.
This conclusion is derived from elementary probability and does not
assume speculative modern physics, merely that space is infinite (or at
least sufficiently large) in size and almost uniformly filled with
matter, as observations indicate. In infinite space, even the most
unlikely events must take place somewhere. |
Figure 02-12 Parallel Universes
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There are even more exotic scenarios about multiverse:
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- Our universe and contiguous regions of space is a bubble embedded
in an even vaster but mostly empty volume. Other bubbles exist out
there, disconnected from ours. They nucleate like raindrops in a cloud.
During nucleation, each one may acquire different strength of the
forces, and may emerge with different spatial and temporal dimensions.
It all depends on the outcome of symmetry breaking. The anthropic
principle dictates that we see the universe the way it is because if
it were different we would not be here to observe it (see Figure 02-13
and Topic 15).
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Figure 02-13 Anthropic Principle
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- In quantum mechanics the superposition of quantum states suddenly
"collapsed" into a definite quantum state when we make a measurement.
For example, measurement of the spin state for a
spinning
particle would yield either 1 or 0; it would not be any value in
between. Generalization of this concept to the macroscopic world
suggests that one classical reality would gradually split into
superpostions of many as shown in Figure 02-14. Observation
experiences one of the splittings by a decoherent process, which
mimics wavefunction collapse. The classical states (no weird happening
such as being in two different places at once) are observed because
they are in the most robust states.
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Figure 02-14 Quantum Worlds
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aSince the inflation has generated a much
bigger universe than we can see, the visible universe becomes flat to our
perception just like the flat Earth in local view. This implies parallel
lines will never meet no matter how far they are extended, and the familiar
scenery of galaxies and galaxy clusters would extend infinitely far beyond
our cosmic horizon.
bThe first peak (the whole curve) of the power spectrum moves
from left to right with increasing radius of space.
cThe 2dF redshift survey uses the two-degree field spectroscopic facility on
the Anglo-Australian Telescope to measure the redshifts of 250,000 galaxies.
- Big Bang Tour (animation) --
http://superstringtheory.com/cosmo/cosmo3.html
- Cosmology (lecture notes) --
http://blueox.uoregon.edu/~jimbrau/astr123
- Inflation --
http://www.ucolick.org/~patrik/ay5/notes/lecture15.pdf
- CMBR Spectrum --
http://archive.ncsa.uiuc.edu/Cyberia/Cosmos/Footprints.html
- CMBR Fluctuations --
http://pancake.uchicago.edu/~carroll/ourpreposterous/img19.htm
- CMBR Polarization --
http://www-news.uchicago.edu/releases/02/020918.carlstrom.shtml
- CMBR Polarization, DASI home page --
http://astro.uchicago.edu/dasi/
- CMBR Power Spectrum --
http://www.livingreviews.org/Articles/Volume1/1998-11jones/node2.html
- CMBR Power Spectrum (animation) --
http://background.uchicago.edu/~whu/intermediate/gravity.html
- Wilkinson Microwave Anisotropy Probe (WMAP), Home Page --
http://map.gsfc.nasa.gov/
- Dark Energy, Dark Matter --
http://hitoshi.berkeley.edu/290E/
- Parallel Universes, Multiverse --
http://www.hep.upenn.edu/~max/multiverse.html
Anthropic Principle
Aristotle and Plato
Big Bang Theory
Black-body radiation
CMBR fluctuations
CMBR polarization
CMBR power spectrum
CMBR spectrum
Composition of the Universe
Dark energy, dark matter
Decoupling epoch
Future of the Universe
History of the Universe
Hubble's law
Hubble's constant
Hubble deep fields |
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Hubble's space telescope
Inflation Theory
Loop quantum gravity
Milky Way
Multiverse
Nucleosynthesis
Observable universe
Olber's paradox
Parallel Universes
Polarization
Quantum Foam
Quantum worlds
Red shift
Standard Candle
Supernova type Ia
Wilkinson Microwave Anisotropy Probe (WMAP)
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