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The Observable Universe and Beyond


Contents

The Observable Universe
Big Bang Theory
CMBR (Cosmic Microwave Background Radiation) Spectrum
CMBR Fluctuations
CMBR Polarization
CMBR Power Spectrum
Wilkinson Microwave Anisotropy Probe (WMAP)
Dark Matter
Dark Energy
Parallel Universes, Multiverse - the Unobservable Universe
Quantum Cosmology and Pre-Big Bang Theories
Footnotes
References
Index

The Observable Universe

The observable universe is the space around us bounded by the event 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
Cosmos Inflation composed of smaller things and is a part of something larger as shown in Figure 02-01a (See also "Map of the Universe" for a different perspective) 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

Figure 02-01a The Observable Universe [view large image]

Figure 02-01b Inflationary Cosmology [view large image]

scale of time: processes tend to happen quickly on small scales and slowly on large scales.

Note that according to inflationary cosmology, the entire universe is much bigger than the observable one (see Figure 02-01b, not to scale), and the confine of observable universe depends on the location. Observers living in the Andromeda galaxy and beyond have their own observable universes that are different from but overlap with ours.

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Big Bang Theory1,2

cosmic expansion 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. 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.

Figure 02-02 Cosmic Expansion
[view large image]

Note that contrary to the balloon analogy, it is the space itself that is expanding. It needs neither a center to expand away from nor empty space on the ouside to expand into.

This simple picture of expanding universe with all the galaxies flying away from each other remained unchanged until the 1980s when the Inflation Theory3 was introduced to resolve a number of discrepancies. The rapid expansion occurred at the interval between 10-35 sec and 10-32 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 flata. 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 grand unified theories). 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 02-03a shows the history of the universe according to the Big Bang Theory. Table 02-01 summarizes the major events during the course of the cosmic history.

cosmology Supplement to the legend of Figure 02-03a:
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.)

Figure 02-03a History of the Universe [view large image]

Cosmic Expansion There are scales for the time t (in second), temperature T (in oK) and energy
E (in Gev) of the photon gas at the bottom of Figure 02-03a. These variables are related by the simple mathematical formulas:

For the earlier relativistic matter dominated era: E(Gev) = 2.76x10-3 / t1/2(sec) --- (1) where the proportional constant is calibrated with the Planck scale of
E(Gev) = 1.2x1019 Gev at 5.4x10-44sec.

Figure 02-03b Cosmic Expansion [view large image]

For the non-relativistic matter dominated era: E(Gev) = 156x10-3 / t2/3(sec) --- (2)
where the proportional constant is calibrated with the CMBR temperature of 2.73oK at the present age of 13.7x109years.
According to Eqs.(1) and (2), the energy of radiation and matter became equal at about 1000 years after the Big Bang.

The energy and temperature are related by the formula:    E(Gev) = 10-13 x T(oK) ----- (3)

There is no such simple formula for the size R of the early universe and time until 10-32 sec at the end of the inflation. Their relationship during the earlier epoch can be obtained from a graph (Figure 02-03b, the numerical values are not reliable as the precise numbers are highly uncertain caused by missing details in the Grand Unified Theories). For the later period, a mathematical formula for the size and time can be found from the standard model curve on the same graph:

log[R(cm)] = 0.5036 x log[t(sec)] + 19.12 ----- (4)

where the constants are estimated by fitting two points on the straight line - one with the size of 1000 cm for the end of the inflation at 10-32sec, the other with the size of about 1028cm for the present age of 13.7x109years. Eq.(4) implies a relativistic matter dominated cosmological model with R ~ 1019x t1/2; because in the logarithmic scale, more than 90% of the graph is related to the relativistic matter dominated era. It also equates the distance to the cosmic horizon (in the present) to be the size of the universe, which in general are not equal.

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 conjectures.

Era Time Size Energy or
Temperature
Relics & Observables Events
Planck era < 10-43 sec < 10-50 cm > 1019 Gev 4-dimensional spacetime;
cosmic expansion
Smallest unit of space-time started to expand; all forces united into one
GUT era < 10-35 sec < 10-47 cm > 1014 Gev Super-heavy particles; fundamental interactions Separation of spacetime and matter; gravitational, strong, and electroweak forces
Inflation < 10-32 sec < 1000 cm > 1013 Gev Observable universe;
large scale structures
Unstable vacuum;
quantum fluctuations
Electro-weak era < 10-10 sec < 1014 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 < 1017 cm > 200 Mev Exotic forms of dark matter Formation of hadrons from quarks including neutrons and protons
Weak decoupling < 1 sec < 1019 cm > 3 Mev Hydrogen nuclei domination Neutrinos decouple, neutron/proton ratio fixed
e-e+ Annihilation < 5 sec < 3x1019 cm > 1 Mev Photons hotter than neutrinos today Electron heat dumped into photons
Nucleo-synthesis < 100 sec < 1020 cm > 200 Kev Light element abendances: D, He, Li Nuclear reactions freeze out, stable nuclei form
Spectral decoupling < 106 sec < 1022 cm > 3 Kev Blackbody background radiation End of efficient photon production
Matter ~ radiation < 104 yrs < 8x1024 cm > 3 ev Mass density fluctuations Matter density ~ radiation density
Recom-bination < 0.4 My < 5x1025 cm > 3000oK CMBR e- and p+ recombine into H atoms, universe transparent to light
Dark ages < 1 Gy < 3x1027 cm > 15oK First stars, heavy elements mass fluctuations grow, first small objects coalesce, reionization
Galaxy formation < 2 Gy < 4x1027 cm > 10oK Stars, quasars, galaxies Collapse to galactic systems
Bright ages < 13 Gy < 9.7x1027 cm > 2.8oK Milky Way and Solar System Gas consumed into stars, remnants, planets
Present era ~ 13.7 Gy ~ 1028 cm ~ 2.73oK 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 02-03a). 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.

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CMBR (Cosmic Microwave Background Radiation) Spectrum4

CMBR Spectrum It was discovered in 1965 that there is a feeble microwave radiation emanating uniformly from all directions in the sky. It contributes about one percent to the static on a television screen that is not tuned to a local channel. This is the cosmic microwave background radiation (CMBR). The CMBR spectrum is identical to a blackbody radiation of 2.726oK as shown in Figure 02-04. The solid line represents the blackbody radiation spectrum that has been computed from theory. The data being represented by various symbols are collected from various measurements. The agreement between observation and theory is remarkable.

Figure 02-04 CMBR Spectrum [view large image]

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CMBR Fluctuations5

CMBR1

The all sky maps in Figure 02-05 shows the three views of CMBR (in false colours) with increasing sensitivity (in temperature variation). To a first approximation the sky is uniform (top). At a sensitivity level of 1 part in 1000, it reveals a shift in wavelength to blue and red (middle) . The pattern is caused by the motion of the earth relative to the frame of the CMBR. When this shift is subtracted off, fluctuations are visible at a sensitivity level of 1 part in 100000 (bottom). The red band in the middle is the emission from the Milky Way.

Figure 02-06 shows the final view after all the corrections have been applied. The slight variation in temperature then takes on a blotchy appearance with each patch a little above or below the average temperature of 2.726oK.

All the above-mentioned observations can be interpreted in a consistent way by the Big Bang Theory. According to this theory the CMBR was emitted about 380000 yr. after the Big Bang when neutral atoms (such as the hydrogen atoms) started to form. As the neutral atoms interact much less to the radiation, they became free and escaped the fireball at a blackbody temperature of about 4000 oK. It takes about 14 billion years to reach us and has since been cooled down to 2.726 oK by the cosmic expansion.

Figure 02-05 The Three Views of CMBR

CMBR2 The patchy features in Figure 02-06 are related to the fluctuations occurred close to the beginning of the universe. The CMBR is the furthest astronomical phenomenon that can be witnessed by any beings because the universe was opaque before this event. It is like looking up in a cloudy day when nothing can be seen beyond the cloud ceiling.

Figure 02-06 Cosmic Microwave Background Radiation

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CMBR Polarization6

CMBR polarization

Recently in 2002, the Degree Angular Scale Interferometer (DASI) has detected partial polarization of the CMBR at the sensitivity level of one part in a million. In Figure 02-07 the temperature fluctuations are represented by yellow for hotter, red for colder regions. Superimposed is the polarization measured by DASI7. The polari-zation at each point is represented by a black line, whose orientation and length correspond to the direction and amount of polarization, respectively. The magnitude of the polarization on small angular scales depends on the anisotropy being in place at recombination but on large angular scales, the polarization patterns were formed at the beginning of the reionization era, when the first starlight began ionizing the cold hydrogen that filled the universe after the Big Bang cooled. Measurement by WMAP indicates that the first stars were born about 100 to 400

Figure 02-07 CMBR Polarization
[view large image]

million years after the Big Bang. New polarization data (white bars in Figure 02-09a) from WMAP in 2006 provide further evidence that the first stars formed some 400 million years after the Big Bang, which was followed by a period of inflation.

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CMBR Power Spectrum8,9

power spectrum Theoretical physicists use the power spectrum plot to determine the cosmological parameters by the observational data. Essentially, the power spectrum is a plot of the amount of fluctuation against the angular (or linear) size. The fluctuation is the difference in the two measurements at the corresponding points. It can be the fluctuation of temperature or density or any other kind of measurable quantity. Figure 02-08 shows just one example with the WMAP observational data superimposed on a theoretical curve. The theoretical curve varies with several parameters such as the total cosmic density, the baryon density (luminous matter) and the Hubble's constant. The best fit model is the lambda cold dark matter model with an initial inflation, a period of galaxies formation induced by cold dark matter, and then the speedup of the cosmic expansion. However, none of the theoretical models based on inflation can account for the anomalous data in Figure 02-08 at large angular size. Double checking the instruments and analysing procedures also fails to explain the anomalies. More observations are needed to resolve the puzzle.

Figure 02-08 Power Specturm
[view large image]

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Wilkinson Microwave Anisotropy Probe (WMAP)10

CMBR, High Resolution The Wilkinson Microwave Anisotropy Probe (WMAP) team has released the first detailed full-sky map of the oldest light in the universe on February 11, 2003. Figure 02-09a shows the measurements with red indicates "warmer" and blue indicates "cooler" spots. The patterns in the map are tiny temperature differences within an extraordinarily evenly dispersed microwave radiation bathing the Universe, which now averages a frigid 2.73 degrees above absolute zero temperature. WMAP resolves the slight temperature fluctuations, which vary by only millionths of a degree. Analyses of this microwave radiation emitted only 380,000 years after the Big Bang

Figure 02-09a High Resolution CMBR
[view large image]

appear to define our universe more precisely than ever before. Measurements from WMAP resolve several
long-standing disagreements in cosmology rooted in less precise data. Specifically, present analyses of the WMAP all-sky image indicate that the universe is 13.7 billion years old (accurate to 1 percent), composed of 73 percent dark energy, 23 percent cold dark matter, and only 4 percent atoms, is currently expanding at the rate of 71 km/sec/Mpc (accurate to 5 percent), underwent episodes of rapid expansion called inflation, the geometry of the Universe is flat1, and will expand forever. The Wilkinson Microwave Anisotropy Probe was launched on June 30, 2001. It is designed to operate for four years.

Further analysis of the WMAP data in 2007 reveals two oddities:
WMAP Oddities 1. It has been deduced from the absence of radio sources that there is a big hole in the sky devoid of both normal and dark matter in the direction of the constellation Eridanus. Its size is nearly a billion light years across at a distance 6 - 10 billion light years away (40 times larger in volume than the previous record holder). The void coincides with an extra large cold spot in the WMAP map covering a few degrees of the sky (many times more than the full moon). The temperature of the void is

Figure 02-09b WMAP Oddities
[view large image]

between 20 and 45 % lower than the average. It is suggested that the discovery of the void ties in neatly with the WMAP cold spot and the existence of dark energy as the photons would lose energy passing through an empty space.
2. WMAP's temperature variations can be decomposed into set of patterns called multipoles. The lowest multipoles are the largest-area, continent- and ocean-size undulations on the temperature map. Higher multipoles are like successively smaller-area plateaus, mountains and hills (and trenches and valleys) inserted on top of the larger features. As shown in Figure 02-09b both the quadrupole and the octupole are aligned along an "axis" which standard cosmology cannot explain. This could happen by chance only about 0.1% of the time. Critics have considered a variety of possibilities. One explanation involves some kind of imperfection in WMAP's detector that introduces the patterns, but there is no evidence for this.

The Void A theory based on the multiverse aspect of the string theory claims that the dynamic effect of matter and gravity would have weeded out the majority of string vacuums, leaving only our patch and close neighbours in the string landscape. A calculation shows that interaction between neighbouring patches in early epoch would leave the universes in an entangled state linking them together even when their separation is space-like (meaning they cannot interact with each other in the usual way). It predicts that pushing and squeezing between the patches will produce voids on the scales of about 1/2 billion light year. The alignment in the lower multipoles is the byproduct of such interaction, which squeezes our universe on one side, perhaps shaped it like a pancake. This theory may point us to the first glance of another universe after all kinds of speculation in science fictions (Figure 02-09c).

Figure 02-09c The Void
[view large image]

The NASA/WMAP Science Team presents the cosmic microwave temperature fluctuations from the 5-year WMAP data
WMAP 2 Early Universe (Figure 02-09d) on March, 2008. The composition of the early universe has been measured from the data as shown in Fiugre 02-09e. It is obvious by comparing with the composition in the current epoch that it varies as the universe expands. It appears that the dark energy density does not decrease at all, so

Figure 02-09d WMAP 5-Year Data [large image]

Figure 02-09e Early Universe
[view large image]

it now dominates the universe even though it was a tiny fraction 13.7 billion years ago. Other major findings include:
  1. New evidence that a sea of cosmic neutrinos permeates the universe. Cosmic neutrinos existed in such huge numbers they affected the universe’s early development. That, in turn, influenced the microwaves that WMAP observes.
  2. The first stars took more than a half-billion years to create a cosmic fog. The data provide crucial new insights into the end of the "dark ages," when the first generation of stars began to shine. The glow from these stars created a thin fog of electrons in the surrounding gas that scatters microwaves.
  3. The new WMAP data places tight constraints on the theory of inflation. Some versions of the inflation theory now are eliminated. Others have picked up new support.

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Dark Matter11

Earth-Moon System 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. It is suggested that the mass of dark matter within the lunar orbit can be computed by subtracting the total mass (Earth + Dark Matter) within the lunar orbit from the mass of the Earth measured by a gravity-sensing satellite (Figure 02-10a). It turns out to be no more than 1.5x1015 kg or about one

Figure 02-10a Earth-Moon System [view large image]

billion times lower than the mass of the Earth. It means that the difference is too small to be measured by the 2008 technology. All that can be found is the upper bound, which is just another way of saying that there is no difference up to the current level of accuracy.

Dark Matter Distribution Figure 02-10b shows the large-scale distribution of dark matter mapped by the Hubble's Cosmic Evolution Survey in early 2007. Since light will follow the deformed path created by massive object, the quantity and location of the dark matter can be estimated by the amount of the bending. However, it should be cautioned that such image represents only a small facet of the whole picture. Just like representing the distortion of space-time as a piece of stretched rubber sheet, or the probability density of an electron (in the atom) by some foggy orbital, the dark matter distribution map does not include the other interesting properties such as its lack of interaction with other matter except via gravity.

Figure 02-10b Dark Matter Distribution [large image]

Note the increasing clumpiness from distant past to more recent epoch in the picture.


Dark Matter The map of dark matter forms a filamentous 'skeleton' upon which visible matter congregates, eventually producing stars and galaxies. Baryonic structures are expected to form only inside the dark-matter scaffold. But as shown in Figure 02-10c, the concentrations of dark matter (mapped in contours) usually - but not always - match up with normal matter (coloured). The discrepancies could be a simple error resulting from the way the observations were made. Alternatively it is suggested that dark matter, if the clump is small enough, could have any accumulating visible matter blown out of it by a high-energy phenomenon such as

Figure 02-10c Dark Matter and Baryonic Matter [view large image]

a quasar or a supernova, for example. The collision of two galaxies could also blow an amount of visible matter out as a faint satellite galaxy that has no associated dark matter.

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Dark Energy

The other problem with modern cosmology 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 as shown in Figure 02-10f, which shows that the supernova appears to be dimmer than expected from an uniformly expanding universe. It is proposed that
Supernova Ia dark energy there is some kind of repulsive "dark energy" to induce the acceleration. Figure 02-10g 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 02-10f Supernova Ia [view large image]

Figure 02-10g Energy-Matter in the Universe

New data in 2006 further refine the universe's contents to: 4% ordinary matter, 22% dark matter, and 74% dark energy.


Material Representative Particles Particle Mass or Energy (ev) No. of Particles in Observed Universe Probable Contribution to Mass of Universe Sample Evidence
Ordinary 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

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.

Dark Energy and Sound Wave Another method to verify the cosmic acceleration is by detecting the bunching intervals of the clusters of galaxies. Whereas Type Ia supernovae behave like standard candles, the spacing between clusters of galaxies acts like a standard ruler. The bunching was generated by the cosmic sound wave, which compressed matter to higher density at its peaks. According to different scenarios of cosmic expansion, the amount of stretching is different as shown in Figure 02-10h. In the primordial gas, the incoherent acoustic oscillations

Figure 02-10h Dark Energy and Sound Wave

created peaks at intervals of 436000 light years, today the spacing should be about 500 million light years depending on the kind of cosmic model.


Dark Energy and Galaxies Gradually, it dawns on some astronomers that dark energy could be responsible for turning off galaxy and star formation in the latter half of the cosmic history at redshift
z ~ 0.75
(~ 6.5 billion years since the Big Bang). The central piece of evidence is the rough coincidence in timing between the end of most galaxy and cluster formation and the onset of the domination of dark energy. Both happened when the universe was about half its present age. The influence of dark energy include stopping the merger of galaxies, sorting out the types of galaxies, lowering the rate of star formation, and preventing the growth of galaxy clusters (Figure 02-10i). Such idea has been confirmed in 2008 by NASA's Chandra X-ray Observatory. The X-ray results on the hot gas in dozens of

Figure 02-10i Galaxy Formation & Dark Energy

galaxy clusters some of which are relatively close and others are more than halfway across the universe reveal that accelerated expansion stifles the growth of galaxy clusters. It also tentatively identifies the cosmic constant as the dark energy.


The effect of dark energy became dominant only at an epoch 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 02-10n 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.

1
Future of the Universe 1 Future of the Universe 2 Future of the Universe 3

Figure 02-10n Future of the Universe

A study on the consequence of cosmic acceleration concludes that while most of the galaxies move away beyond the cosmic horizon, the local group of galaxies will collapse into a supergalaxy by gravitational attraction. Eventually, the
Future of the Universe a Future of the Universe b universe goes black when the last stars burn out. Future civilizations (if there is any left) will have a very different perspective of the universe. Our descendants will observe an island of stars (the supergalaxy) embedded in a vast emptiness. It will resemble the de Sitter universe originally envisioned by Einstein. Figure 02-10o shows the sequence of events according to an artist's rendition.

Figure 02-10o Future of the

Milkyway [large image 1, 2]

Since we don't feel the effect of dark energy and dark matter around us except through the gravitational influence on large
Insignificance scale, a model has been constructed with no other 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. But if 96% of the Universe is in the form of unseen substances, does this not mean that there is the possibility of hidden structure? Might the dark sector be a fascinating place, with its own intricate interactions — perhaps even a kind of intelligent life? Is there a 'dark light' that we do not see, radiating and absorbing in the dark Universe? Such possibility suggests that human beings are extremely unimportant in the

Figure 02-10p Insignificance [view large image]

grand scheme of the universe as portrayed in a 1985 movie called "Insignificance" in which Einstein and Monroe explores relativity and our place in the universe (Figure 02-10p).

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Parallel Universes, Multiverse - the Unobservable Universes12

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 creative imagination.

flat space Figure 02-11 shows recent astronomical observations, which tend to support the hypothesis. The diagram on the left illustrates the WMAP measurementb 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.

Figure 02-11 Universe, Flat & Uniform [view large image]

Parallel Universes 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)

Figure 02-12 Parallel Universes [view large image]

in size and almost uniformly filled with matter, as observations indicate. In infinite space, even the most unlikely events must take place somewhere.

Quantum Worlds
  • 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.

Figure 02-14 Quantum Worlds
[view large image]

Aristotle
  • The correspondence between mathematics and physics has been a source of debate that goes as far back as Aristotle and Plato. According to the Aristotelian paradigm, physical reality is fundamental and mathematical language is merely a useful tool. The Platonic argument considers the mathematical structure to be the true reality and observers only perceive it imperfectly. Thus a fundamental asymmetry appears to be built into the very heart of reality - why is only one of the many mathematical structures singled out to describe our universe? It is suggested that complete mathematical symmetry holds: that all mathematical structures exist physically as well. Every mathematical structure

Figure 02-15 Aristotele and Plato [view large image]

corresponds to a parallel universe. As a consequence, each universe is governed by its own fundamental laws of physics (see more in Topic 15). In Figure 02-15 Aristotle points down to the reality on earth while Plato points up to multiverse.
By 2006, the confluence of events has pushed many leading physicists toward the notion of a multiverse. These include: measurements that indicate the universe's expansion is accelerating; empirical tests that bolster the inflationary universe scenario; theories of eternal inflation (see below) that suggest an endless number of Big Bang; and developments in string theory that show how to design universes with widely different properties.
Eternal Inflation The theory of eternal inflation posits that the entire eternally inflating spacetime (false vacuum) originated as a minuscule closed multiverse. It tunneled, quantum-mechanically, out of nothing and immediately plunged into the never-ending inflation. Thus, the multiverse is eternal, but it did have a beginning. Inflation rapidly blows the universe up to an enormous size. It stopped where we are, producing our own island universe, and many others. But due to the peculiar structure of inflationary spacetime, it continues in other areas of the multiverse at large. The multiverse contains an unlimited number of island universes. We live in one of them, and our observable region is one of the infinite numbers of observable regions (at different locations) that it contains (see Figure 02-16). We may be able to travel to the other observable regions, but we are forever confined to our own island universe. Constants of nature that shape the character of our world take different values in other island universes. Most of these universes are drastically

Figure 02-16 Multiverse, Eternal Inflation [view large image]

different from ours, and only a tiny fraction of them are hospitable to life.


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Quantum Cosmology and Pre-Big Bang Theories

Quantum Cosmology According to the classical cosmology, the universe starts from a singularity state. It is obvious that the size of the universe would be very small during the initial expansion, and thus quantum effect must be taken into consideration. Unfortunately, a theory of quantum gravity is not available now. However, it

Figure 02-17 Quantum Cosmology
[view large image]

does not stop physicists from adding quantum effects into this early phase of the universe in an ad hoc fashion, some examples are listed in Table 02-03:

Ad Hoc Add On Quantum Effect Epoch To Explain
A Period of Inflation Quantum Field 10-35-10-32 sec after Big Bang The flatness of space and homogeneous appearance
Density fluctuations Uncertainty Principle When the universe is smaller than the size of an atom CMBR and large galactic structures
History of the universes Path integral From Big Bang to present Geometry of our universe
Probability of universes Schrodinger equation From Big Bang and beyond Our universe is most probable type
Origin of Big Bang Interactions of branes At the moment of Big Bang Cosmic Expansion
Pre-Big Bang Processes
(see below)
Wave propagation in theory of superstring Before the Big Bang Creation of our universe
LQG universe (see below) Loop quantum gravity Before the Big Bang Creation of our universe
Cyclic universe (see below) Theory of superstring Endless cycles Beginning of our universe

Table 02-03 Quantum Cosmology

*** Quantum Model
When talking about Big Bang, the inevitable question would be: "what went before it?" The common expectation is that the scientists will disguise their ignorance with some sort of excuses. Physicists in the 21th century is fast coming up with an
String Cosmology answer to such open-end interrogation. Figure 02-17 shows the progression of our understanding about the Big Bang. Figure 02-17(a) portrays our ignorance in classical cosmology. There is no further explanation when we encounter the singularity. Gradually, quantum standard cosmology suggests that the seed of the universe was tunneling through a high energy and high curvature region without

Figure 02-18 String Cosmology
[view large image]

specifying from what as shown in Figure 02-17(b). In quantum string cosmology (Figure 02-17(c)), the pre-big bang is identified with the string perturbative vacuum in the Superstring Theory as sketched qualitatively in Figure 02-18.
Evolution of H and G The models are constructed with a framework where the universe can be represented as a wave (the Wheeler-DeWitt wave function) propagating in an abstract, multidimensional space dubbed superspace (no connection with super-symmetry). The string perturbative vacuum is characterized by a nearly flat space-time geometry and the vanishingly small coupling of all interactions. Figure 02-19 shows the evolution of the curvature (represented by the Hubble parameter H) and the gravitational constant G (determined by the dilaton).

Figure 02-19 Evolution of H and G
[view large image]

Figure 02-18(a) is a schematic diagram to portray the transition as a quantum mechanical reflection of the wave function in a mini-superspace whose coordinates correspond to the dilation and to the spatial radius of the universe. The dilaton is a neutral scalar force field (or particle) associated with the duality transformation for the spatial radius (of the universe) R 1/R. The incident wave describes the initial evolution of the universe from the string perturbative vacuum towards the high curvature regime. Part of this incoming wave is not stopped by the barrier and is classically transmitted to the region of ever increasing dilaton, running towards the singularity. Another part is reflected to the region of decreasing dilaton and standard post-big bang evolution. This process is not very efficient as shown in Figure 02-17(c). The more efficient one is the "anti-tunneling" effect of the wave function, i.e., as the creation of pairs of universes from the string perturbative vacuum. The wave function is amplified during this process as shown in Figure 02-18(b).

*** Loop Quantum Model
The theory of "loop quantum gravity (LQG)" incorporates quantum effect into gravity by latticizing general relativity (GR) in a way similar to the "lattice theory in QFT" with the spacing between nodes replaced by the Planck area (~10-66cm2), i.e., the
LQG Cosmology links now represent units of area, and the nodes become quantized units of volume. A crucial difference in such formulation is that the lattice is not fixed, it evolves according to some rules. Thus, space-time is not a background scaffold anymore. Its application to cosmology reveals that the universe evolved from a pre-existing state toward very high density in a very small volume but then bounced back because repulsion is generated at such high density in LQG. It led to a "super-inflation" era, then the "inflation" era and the classical space-time afterward (Figure 02-20). It has been shown that super-inflation can produce the kind of quantum fluctuations in the fabric of space-time for the formation of galaxies and clusters of galaxies later. The period of inflation is still required to resolve the horizon and flatness problems. Since the

Figure 02-20 LQG Cosmology
[view large image]

repulsive dark energy has not been taken into consideration in the computation, it is not known if the pre-existing universe will really collapse as suggested in this model.

*** Brane Model
Cyclic Universe The theory of superstring admits up to seven extra spatial dimensions. The cyclic universe model represents our universe as a 3-dimensional brane moving in a 4-dimensional space. It interacts with another 3-dimensional brane via a spring-like force, which is identified with the dark energy. These two branes execute periodic motion as shown in Figure 02-21. The moment of collision is perceived by us as the Big Bang. We can never reach out to the extra dimension, only gravity and the dark energy can reside there. Figure 02-21 depicts the sequence of events during one cycle of the endless oscillations with a more detailed description in the followings:

Figure 02-21 Cyclic Universe [view large image]

  1. According to the cyclic universe model, the Big Bang is not the beginning of space or time. Instead, it is the moment when gravitational and other forms of energy are transformed into new matter and radiation and a new period of expansion and cooling begins.
  2. Hot, dense matter and radiation fills the universe immediately after the bang. The cosmic temperature reaches about 1027 oK. At this temperature, matter exists only in its elementary forms such as quarks, electrons, photons, and the like. However, the temperature remains modest compared to the 1032 oK or higher in the scenario for the usual Big Bang.
  3. During the following 9 billion years, the cosmos expands and cools. The elementary constituents clump into protons and neutrons, and eventually atoms, molecules, planet, stars, galaxies, clusters of galaxies, and superclusters. The blueprint had been laid down as tiny density variations (ripples) nearly the end of the previous cycle.
  4. Dark energy becomes dominant at this point. The repulsive nature of this substance causes the cosmic expansion to speed up as witnessed by present day astronomers.
  5. During the next trillion years, the accelerating expansion will continue and rapidly dilute the universe of the matter content and lumpy structures.
  6. The universe is restored to a simple, uniform, and pristine state, which is essentially similar to the prediction by the usual Big Bang theory.
  7. However in the cyclic universe model, dark energy is unstable. It will decay near the cycle's end into a form of extremely high-pressure energy that causes the universe to contract slowly.
  8. Space becomes increasingly smooth and flat as the contraction proceeds, while quantum effect produces random fluctuations seeding density variations over all the regions.
    This model provides answers to two annoying inquiries in cosmology:
  1. What went before the pre-big bang, before the pre-pre-big bang, ... ad infinitum -- There could be no beginning or end in a cyclic universe, which may exist forever.
  2. What is the 3 dimensional space expands into -- The usual explanation asserts that cosmic expansion is special, it doesn't expand into anything. Since the cyclic universe is a 3-D brane immersing in a 4-D space, the cosmic expansion in this model naturally expands into this 4-D bulk without invoking anything special.
Although the cyclic and inflationary theories explain equally well all the astronomical data, there are two tests that can distinguish them. Firstly, inflation in the usual Big Bang theory produces detectable gravitational waves. These wrinkle in space propagate through the universe and should produce a measurable polarization pattern in the CMBR. The gravitational waves in the cyclic model are far too weak to induce any change in the CMBR. Secondly, the inflationary picture predicts that the statistical distribution of temperature variations in CMBR should follow a bell curve, while the distribution has measurable deviation (from a bell curve) in the cyclic model. Observations in the next decade will be able to decide which one is correct. The first test may come very soon by ESA's Planck mission, scheduled for launch in 2009.

Planck Image, First The first image of a strip of the millimeter wavelength sky (Figure 02-22, from Planck in September 2009) shows that all systems are working well. Routine operations will continue for at least 15 months without a break. In this time, Planck will be able to gather data (at 9 different wavelengths) for two full independent all-sky maps. To fully exploit the high sensitivity of Planck, the data will require a great deal of delicate calibrations and careful analysis. It will keep cosmologists and astrophysicists busy for decades to come.

Figure 02-22 First Image from the Planck Satellite

See more in Pre-Big Bang models, and a pictorial depiction including multiverse.

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Footnotes

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.

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    References:

  1. Big Bang Tour (animation) -- http://superstringtheory.com/cosmo/cosmo3.html
  2. Cosmology (lecture notes) -- http://blueox.uoregon.edu/~jimbrau/astr123
  3. Inflation -- http://www.ucolick.org/~patrik/ay5/notes/lecture15.pdf
  4. CMBR Spectrum -- http://archive.ncsa.uiuc.edu/Cyberia/Cosmos/Footprints.html
  5. CMBR Fluctuations -- http://pancake.uchicago.edu/~carroll/ourpreposterous/img19.htm
  6. CMBR Polarization -- http://www-news.uchicago.edu/releases/02/020918.carlstrom.shtml
  7. CMBR Polarization, DASI home page -- http://astro.uchicago.edu/dasi/
  8. CMBR Power Spectrum -- http://www.livingreviews.org/Articles/Volume1/1998-11jones/node2.html
  9. CMBR Power Spectrum (animation) -- http://background.uchicago.edu/~whu/intermediate/gravity.html
  10. Wilkinson Microwave Anisotropy Probe (WMAP), Home Page -- http://map.gsfc.nasa.gov/
  11. Dark Energy, Dark Matter -- http://hitoshi.berkeley.edu/290E/
  12. Parallel Universes, Multiverse -- http://www.hep.upenn.edu/~max/multiverse.html

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Index

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 law
Hubble's constant
Hubble deep fields
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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