The Big Bang theory says that the entire universe was created in
a tremendous
explosion about 15 billion years ago. The enormity of this event
is hard to
grasp and it seems natural to ask ourselves 'What was it like then?'
and 'What
happened before the Big Bang?'. To try to answer these queries,
lets take a
brief journey backwards in time.
By 700.000 years, the universe is awash with the fireball radiation
that keeps
all matter at a temperature of 4.000 degrees. Because of this, darkness
is
completely absent since every point in the sky glows with the brilliance
of the
sun. No stars, planets or even dust grains exist, just a hot dense
plasma of
electrons, protons and helium nuclei. By 3 minutes, we see helium
form from the
fusion of hydrogen atoms while the universe seeths at a temperature
of nearly
1 billion degrees. The average density of matter is that of lead.
By 1 second,
the Lepton Era ends and the ratio of neutrons to protons has become
fixed at 1
neutron for every 5 protons. The temperature is now 5 billion degrees
everywhere. At about .0001 second, we watch as the Quark Era ends
and the
temperature of the fireball radiation rises to an incredable 1 trillion
degrees. Quarks, for the first time, can combine in groups of two
and three to
become neutrons, protons and other types of heavy particles. The
universe is
now packed with matter as densly as the nucleus of an atom. A mountain
like Mt.
Everest could be squeezed into a volume no greater than the size
of a golf
ball!
By 1 billionth of a second, the temperature is 1 thousand trillion
degrees and
we see the electromagnetic and weak forces merge into one force.
The density
of the universe has increased to the point where the entire earth
could be
contained in a thimble. Quarks and anti-quarks are no longer confined
inside
of particles like neutrons and protons but are now part of a superheated
plasma
of unbound particles. As the remaining history of the universe unfolds,
a long
period seems to pass when nothing really new happens. Then, at a
time 10(-35)
second after the Big Bang, a spectac ular change in the size of
the universe
occurs. This is the GUT Era when the strong nuclear force becomes
distinguishable from the weak and electromagnetic forces. The temperature
is an
incredable 10 thousand trillion trillion degrees and the density
of matter has
sored to nearly 10(75) gm/cm3. This number is so enormous that even
our
analogies are almost beyond comprehension. At these densities, the
entire Milky
Way galaxy could easily be stuffed into a volume no larger than
a single
hydrogen atom! Electrons and quarks together with their anti-particles,
were
the major constituents of matter and very massive particles called
Leptoquark
Bosons caused the quarks to decay into electrons and vice versa.
If we now move
forward in time we would witness the vacuum of space undergoing
a 'phase
transition' from a higher energy state to a lower energy state.
This is
analogous to a ball rolling down the side of a mountain and coming
to rest in
the lowest valley. As the universe 'rolls down hill' it begins a
brief but
stupendous period of expansion. The universe swells to billions
of times its
former size in almost no time at all.
In addition to this, a slight excess of matter over anti-matter appears
becaus
of the decay of massive particles called X Higgs Bosons. As we continue
to
watch the universe age, the remaining pairs of particles and anti-particles
find themselves and vanish in a tremendous burst of annihilation.
From this
paroxysm, the bulk of the fireball radiation that we now observe
is born.
The GUT Era is the last stop in our fanciful journey through time.
If we had
asked what it was like before the GUT Era, we would immediately
have entered a
vast no mans land where few indisputable facts would serve to gui
de us. What
does seem clear is that gravity is destined to grow in importance,
eventually
becoming the dominant force acting between parti cles, even at the
microscopic
level.
G R A V I T Y
According to theories developed since the 1930's, what we call a
'force' is
actually a collective phenomenon caused by the exchange of innumerable,
force-carrying particles called gauge bosons. The electromagnetic
force, which
causes like charges to attract and dissimilar ones to repel, is
transmitted by
gauge bosons called photons, the strong force that binds nucleii
together is
transmitted by gluons and the weak force which causes particles
to decay is
transmitted by the, recently discovered, W and Z Intermediate Vector
Bosons. In
an analogous way, physicists believe that gravity is transmitted
by particles
called Gravitons. If gravity really does have such a quantum property,
its
effects should appear once quarks and electrons can be forced to
within 10(-33)
centimeter of one another, a distance called the Planck length.
To acheive
these conditions, quarks and electrons will have to be collided
at energies of
10(19) GeV. An accelerator patterned after the 2-mile, Stanford
Linear
Accelerator would have to be 1 light-year in length to push particles
to these
incredable energies! Fortunatly, what humans find impossible to
do, Nature with
its infinite resources finds less difficult. Before the universe
was 10(-43)
second old, matter routinely experienced collisions at these energies.
This
period is what we call the Planck Era.
THROUGH A LOOKING GLASS, DARKLEY
Since our technology will not allow us to physically reproduce the
conditions
during these ancient times, we must use our mathematical theories
of how matter
behaves to mentally explore what the universe was like then. We
know that the
appearence of the universe before 10(-43) second can only be adequatly
described by modifying the Big Bang theory because this theory is,
in turn,
based on the General Theory of Relativity. General Relativity tells
us how
gravity operates on the macroscopic scale of planets, stars and
galaxies. At
the Planck scale, we need to extend General Relativity so that it
includes not
only the macroscopic properties of gravity but also is microscopic
characteristics as well. The theory of 'Quantum Gravity' is still
far from
completion but physicists tend to agree that, at the very least,
Quantum
Gravity must combine the conceptual elements of the two great theories
of
modern physics: General Relativity and Quantum Mechanics.
In the language of General Relativity, gravity is a consequence of
the
deformati on of space caused by the presence of matter and energy.
Gravity is
just another name for the amount of curvature in the geometry of
3-dimensional
space. In Quantum Gravity theory, gravity is produced by massless
gravitons so
that gravitons now represent individual packages of curved space
that travel
through space at the speed of light.
The appearence and dissappearence of innumerable gravitons gives
the geometry
of space a very lumpy and dynamic appearance. John Wheeler at Princeton
University thinks of this as a foamy, sub-structure to space where
the geometry
of space twists and contorts so that far flung regions of space
may suddenly
find themselves connected by 'wormholes' which constantly appear
and dissappear
within 10(-43) seconds. Even as you are reading this article, this
frenetic
activity is occurring in the hyper-microscopic domain, 100 billion
billion
times smaller than the nucleus of an atom. For a comparison, the
size of the
sun and the size of a single atom stand in about this same proportion.
Although
Quantum Gravity effects are completely undetectable today at the
atomic and
nuclear scale, during the Planck Era, macroscopic and microscopic
worlds merged
and the Quantum Gravity of the microcosm suddenly became the Quantum
Cosmology
of the macrocosm!
QUANTUM COSMOLOGY
As we approach the end of the Planck Era, the random appearance and
dissappearance of innumerable gravitons will eventually force us
to give up the
concept of a specific geometry to 3-dimensional space. Instead,
the geometry at
a given moment will have to be thought of as an average over all
3-dimensional
space geometries that are possible. Once again, the reason for this
is that
particles are squeezed so closely together that we can now see individual
gravitons moving around in the space between them causing space
to become
curved. We can no longer get away with saying that the space between
two
quarks, for example, is flat. This is what we mean when we say that
the
gravitational force between them is insignificant when compared
to the other
three forces of Nature.
To make matters much worse, not only will Quantum Gravity not allow
us to
calculate the exact 3-dimensional geometry to space but, at the
Planck scale,
it will not allow us to simultaneously determine its exact geometry
and precise
rate of change in time. What this means is that we may never be
able to
calculate with any certainty exactly what the history of the universe
was like
before 10-43 second. Today, the large-scale geometry of space is
one of three
possible types: flat and infinite, negatively curved and infinite
or positively
curved and finite. During the Planck Era, the 'large-scale' geometry
was
contorted by wormholes and and infinite number of possibilities
were possible.
To probe the history of the universe then would be like trying to
trace your
ancestral roots if every human being on earth had a possibility
of being one of
your parents. Now try to trace your family tree back a few generations!
The
farther back in time you go, the greater are the number of possible
ancestors
you could have had. An entirely new conception of what we mea n
by 'a history
for the universe' will have to be developed. Even the concepts of
space and
time will have to be completely re-evaluated in the face of the
qua ntum
fluctuations of spacetime at the Planck Era!
THE BIRTH OF THE UNIVERSE
The picture that seems to emerge from using our sketchy outline of
what Quantum
Gravity theory might look like is that as we approach the Planck
Era, gravitons
are exchanged between quarks and electrons with increasingly higher
energy and
in greater number. By the time we reach the end of the Planck Era
at 10(-43)
second, gravitons will begin to carry as much energy as the other
force
carriers (Gluons, IVBs and Photons). At still earlier times, a period
of
complet e symmetry and unification between all the natural forces
will ensue.
Only one super-unified force exists here (gravity) and only one
kind of
particle dominates the activity of this age (Gravitons).
During the early 70's, the Russian physicists Ya. Zel'dovitch and
A.
Starobinski of the USSR Academy of Science proposed that the rapidly
changing
geometry of space during the Planck Era may actually have created
all the
matter, anti-matter and radiation that existed soon after Creation.
In their
picture of Creation, the rapidly changing geometry of space created
particles
and anti-particles with masses of 10(19) GeV. This production of
matter and
anti-matter removed energy from the enormous fluctuations occuring
in the
geometry of space and eventually succeeded in damping them out altogether
by
the end of the Planck Era. They also found that the rate of particle
creation
increased as more and more particles were created.
Several recent studies by Physicists Edward Tryon of Hunter College,
R. Brout,
F. Englert and E. Gunzig of the University of Brussels and david
Atkatz and
Heinz Pagels of the Rockefeller University have shed additional
light on what
Creation may have been like. Imagine if you can, nothing at all!
This is the
primordial vacuum of space. There is complete darkness here, no
light yet
exists. The number of dimensions to space was probably not the normal
3 that we
are so accustomed to but may have been as high as 11 according to
Supergravity
theory! In this infinite emptiness, random fluctuations occurred
that ever so
slightly changed the energy of the vacuum at various points in space.
Eventually, one of these fluctuations attained a critical energy
and began to
grow. As it grew, very massive particles called leptoquarks and
anti-leptoquarks were created, causing the expansion to accelerate.
This is
much like a ball rolling down a hill that moves slowly at first
and then gains
momentum. The expansion of the proto-universe, in turn, caused still
more
leptoquarks to be created. This furious cycle continued until, at
long last,
the leptoquarks decayed into quarks, leptons (electrons, muons etc)
and their
anti-particles and the universe emerged from the Planck Era. Particle
creation
stopped once the fluctuations in the geometry of space subsided.
So, we are left with the remarkable possibility that, in the beginning,
there
ex isted quite literally, nothing at all and from it emerged nearly
all of the
matter and radiation that we now see. This process has been described
by the
physicist Frank Wilczyk at the University of California, Santa Barbara
by
saying, " The reason that there is something instead of nothing
is that
nothing is unstable". A ball sitting on the summit of a steep hill
needs but
the slightest tap to set it in motion. A random fluctuation in space
was
apparently all that was required to unleash the incredable latent
energy of
the vacuum, thus creating matter and energy and an expanding universe
from
'nothing at all'.
The universe did not spring into being instantaneously but was created
a little
bit at a time in a 'bootstrap' process. Once a few particles were
created by
quantum fluctuations of the empty vacuum, it became easier for a
few more to
appear and so, in a rapidly escalating process, the universe gushed
forth from
nothingness.
How long did this take? The primordial vacuum could have existed
for an
eternity before the particular fluctuation that gave rise to our
universe
happened. Physicist Edward Tryon expresses this best by saying that
" Our
universe is simply one of those things that happens from time to
time".
The principles of Quantum Gravity may ultimatly force us to reconsider
questions like 'What happened before the Big Bang?' because they
imply the
existence of something (time) that may not have any meaning at all.
These
questions may be as empty of meaning as an explorer on the north
pole asking,
'Which way is North?'. Only the complete theory of Quantum Gravity
may tell us
how to ask the right questions!