It is always a mystery about how the universe began, whether if and when
it will end. Astronomers construct hypotheses called cosmological models
that try to find the answer. There are two types of models: Big Bang and
Steady State. However, through many observational evidences, the Big Bang
theory can best explain the creation of the universe.
The
Big Bang
model
postulates that about 15 to 20 billion years ago, the universe violently
exploded into being, in an event called the Big Bang. Before the Big Bang,
all of the matter and radiation of our present universe were packed together
in the primeval fireball--an extremely hot dense state from which the
universe rapidly expanded.1 The Big Bang was the start of time and space.
The matter and radiation of that early stage rapidly expanded and cooled.
Several million years later, it condensed into galaxies. The universe has
continued to expand, and the galaxies have continued moving away from each
other ever since. Today the universe is still expanding, as astronomers
have observed.
The Steady State model says that the universe does not
evolve or change in time. There was no beginning in the past, nor will
there be change in the future. This model assumes the perfect cosmological
principle. This principle says that the universe is the same everywhere on
the large scale, at all times.2 It maintains the same average density of
matter forever. There are observational evidences found that can prove the
Big Bang model is more reasonable than the Steady State model. First,
the redshifts of distant galaxies. Redshift is a Doppler effect which states
that if a galaxy is moving away, the spectral line of that galaxy observed
will have a shift to the red end. The faster the galaxy moves, the more
shift it has. If the galaxy is moving closer, the spectral line will show a
blue shift. If the galaxy is not moving, there is no shift at all.
However, as astronomers observed, the more distance a galaxy is located
from Earth, the more redshift it shows on the spectrum. This means the
further a galaxy is, the faster it moves. Therefore, the universe is
expanding, and the Big Bang model seems more reasonable than the Steady
State model. The second observational evidence is the radiation produced
by the Big Bang. The Big Bang model predicts that the universe should
still be filled with a small remnant of radiation left over from the
original violent explosion of the primeval fireball in the past. The
primeval fireball would have sent strong shortwave radiation in all
directions into space. In time, that radiation would spread out, cool, and
fill the expanding universe uniformly. By now it would strike Earth as
microwave radiation. In 1965 physicists Arno Penzias and Robert Wilson
detected microwave radiation coming equally from all directions in the
sky, day and night, all year.3 And so it appears that astronomers have
detected the fireball radiation that was produced by the Big Bang. This
casts serious doubt on the Steady State model. The Steady State could not
explain the existence of this radiation, so the model cannot best explain
the beginning of the universe.
Since the Big Bang model is the better
model, the existence and the future of the universe can also be explained.
Around 15 to 20 billion years ago, time began. The points that were to
become the universe exploded in the primeval fireball called the Big
Bang. The exact nature of this explosion may never be known. However, recent
theoretical breakthroughs, based on the principles of quantum theory, have
suggested that space, and the matter within it, masks an infinitesimal realm
of utter chaos, where events happen randomly, in a state called quantum
weirdness.4
Before the universe began, this chaos was all there was. At
some time, a portion of this randomness happened to form a bubble, with
a temperature in excess of 10 to the power of 34 degrees Kelvin. Being that
hot, naturally it expanded. For an extremely brief and short period,
billionths of billionths of a second, it inflated. At the end of the period
of inflation, the universe may have a diameter of a few centimetres. The
temperature had cooled enough for particles of matter and antimatter to
form, and they instantly destroy each other, producing fire and a thin haze
of matter-apparently because slightly more matter than antimatter was
formed.5 The fireball, and the smoke of its burning, was the universe at an
age of trillionth of a second.
The temperature of the expanding fireball
dropped rapidly, cooling to a few billion degrees in few minutes. Matter
continued to condense out of energy, first protons and neutrons, then
electrons, and finally neutrinos. After about an hour, the temperature had
dropped below a billion degrees, and protons and neutrons combined and
formed hydrogen, deuterium, helium. In a billion years, this cloud of
energy, atoms, and neutrinos had cooled enough for galaxies to form. The
expanding cloud cooled still further until today, its temperature is a
couple of degrees above absolute zero.
In the future, the universe may
end up in two possible situations. From the initial Big Bang, the universe
attained a speed of expansion. If that speed is greater than the universe's
own escape velocity, then the universe will not stop its expansion. Such
a universe is said to be open. If the velocity of expansion is slower than
the escape velocity, the universe will eventually reach the limit of its
outward thrust, just like a ball thrown in the air comes to the top of its
arc, slows, stops, and starts to fall. The crash of the long fall may be the
Big Bang to the beginning of another universe, as the fireball formed at
the end of the contraction leaps outward in another great expansion.6 Such a
universe is said to be closed, and pulsating.
If the universe has
achieved escape velocity, it will continue to expand forever. The stars will
redden and die, the universe will be like a limitless empty haze, expanding
infinitely into the darkness. This space will become even emptier, as
the fundamental particles of matter age, and decay through time. As the
years stretch on into infinity, nothing will remain. A few primitive atoms
such as positrons and electrons will be orbiting each other at distances of
hundreds of astronomical units.7 These particles will spiral slowly toward
each other until touching, and they will vanish in the last flash of
light. After all, the Big Bang model is only an assumption. No one knows for
sure that exactly how the universe began and how it will end. However, the
Big Bang model is the most logical and reasonable theory to explain the
universe in modern science.
BIBLIOGRAPHY
Boslough, John. Stephen
Hawking's Universe. New York: Cambridge University Press, 1980.
Caes, J. Charles. Cosmology, The Search For The Order Of The
Universe. USA: Tab Books Inc., 1986.
Gribbin, John. In Search Of The
Big Bang. New York: Bantam Books, 1986.
Holt, Terry. The Universe
Next Door. New York: Charles Scribner's Sons, 1985.
Kaufmann, J.
William III. Astronomy: The Structure Of The Universe. New York: Macmillan
Publishing Co., Inc., 1977.
Mache, L. Dinah. Astronomy. New York: John
Wiley & Sons, Inc., 1987.
Silk, Joseph. The Big Bang. New York:
W.H. Freeman and Company, 1989.
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