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According to the Boshongo people of central
Africa, in the beginning, there was only darkness, water, and the great
god Bumba. One day Bumba, in pain from a stomach ache, vomited up the
sun. The sun dried up some of the water, leaving land. Still in pain,
Bumba vomited up the moon, the stars, and then some animals. The
leopard, the crocodile, the turtle, and finally, man. This creation myth, like many others, tries to answer the questions we
all ask. Why are we here? Where did we come from? The answer generally
given was that humans were of comparatively recent origin, because it
must have been obvious, even at early times, that the human race was
improving in knowledge and technology. So it can't have been around that
long, or it would have progressed even more. For example, according to
Bishop Usher, the Book of Genesis placed the creation of the world at 9
in the morning on October the 27th, 4,004 BC. On the other hand, the
physical surroundings, like mountains and rivers, change very little in a
human lifetime. They were therefore thought to be a constant
background, and either to have existed forever as an empty landscape, or
to have been created at the same time as the humans. Not everyone,
however, was happy with the idea that the universe had a beginning. For example, Aristotle, the most famous of the Greek philosophers,
believed the universe had existed forever. Something eternal is more
perfect than something created. He suggested the reason we see progress
was that floods, or other natural disasters, had repeatedly set
civilization back to the beginning. The motivation for believing in an
eternal universe was the desire to avoid invoking divine intervention to
create the universe and set it going. Conversely, those who believed
the universe had a beginning, used it as an argument for the existence
of God as the first cause, or prime mover, of the universe.
If
one believed that the universe had a beginning, the obvious question was
what happened before the beginning? What was God doing before He made
the world? Was He preparing Hell for people who asked such questions?
The problem of whether or not the universe had a beginning was a great
concern to the German philosopher, Immanuel Kant. He felt there were
logical contradictions, or antimonies, either way. If the universe had a
beginning, why did it wait an infinite time before it began? He called
that the thesis. On the other hand, if the universe had existed for
ever, why did it take an infinite time to reach the present stage? He
called that the antithesis. Both the thesis and the antithesis depended
on Kant's assumption, along with almost everyone else, that time was
Absolute. That is to say, it went from the infinite past to the infinite
future, independently of any universe that might or might not exist in
this background. This is still the picture in the mind of many
scientists today.
However in 1915, Einstein introduced his
revolutionary General Theory of Relativity. In this, space and time were
no longer Absolute, no longer a fixed background to events. Instead,
they were dynamical quantities that were shaped by the matter and energy
in the universe. They were defined only within the universe, so it made
no sense to talk of a time before the universe began. It would be like
asking for a point south of the South Pole. It is not defined. If the
universe was essentially unchanging in time, as was generally assumed
before the 1920s, there would be no reason that time should not be
defined arbitrarily far back. Any so-called beginning of the universe
would be artificial, in the sense that one could extend the history back
to earlier times. Thus it might be that the universe was created last
year, but with all the memories and physical evidence, to look like it
was much older. This raises deep philosophical questions about the
meaning of existence. I shall deal with these by adopting what is
called, the positivist approach. In this, the idea is that we interpret
the input from our senses in terms of a model we make of the world. One
can not ask whether the model represents reality, only whether it works.
A model is a good model if first it interprets a wide range of
observations, in terms of a simple and elegant model. And second, if the
model makes definite predictions that can be tested and possibly
falsified by observation. In terms of the positivist approach, one can compare two models of the
universe. One in which the universe was created last year and one in
which the universe existed much longer. The Model in which the universe
existed for longer than a year can explain things like identical twins
that have a common cause more than a year ago. On the other hand, the
model in which the universe was created last year cannot explain such
events. So the first model is better. One can not ask whether the
universe really existed before a year ago or just appeared to. In the
positivist approach, they are the same. In an unchanging universe, there
would be no natural starting point. The situation changed radically
however, when Edwin Hubble began to make observations with the hundred
inch telescope on Mount Wilson, in the 1920s.
Hubble found that
stars are not uniformly distributed throughout space, but are gathered
together in vast collections called galaxies. By measuring the light
from galaxies, Hubble could determine their velocities. He was expecting
that as many galaxies would be moving towards us as were moving away.
This is what one would have in a universe that was unchanging with time.
But to his surprise, Hubble found that nearly all the galaxies were
moving away from us. Moreover, the further galaxies were from us, the
faster they were moving away. The universe was not unchanging with time
as everyone had thought previously. It was expanding. The distance
between distant galaxies was increasing with time.
The expansion
of the universe was one of the most important intellectual discoveries
of the 20th century, or of any century. It transformed the debate about
whether the universe had a beginning. If galaxies are moving apart now,
they must have been closer together in the past. If their speed had been
constant, they would all have been on top of one another about 15
billion years ago. Was this the beginning of the universe? Many
scientists were still unhappy with the universe having a beginning
because it seemed to imply that physics broke down. One would have to
invoke an outside agency, which for convenience, one can call God, to
determine how the universe began. They therefore advanced theories in
which the universe was expanding at the present time, but didn't have a
beginning. One was the Steady State theory, proposed by Bondi, Gold, and
Hoyle in 1948. In the Steady State theory, as galaxies moved apart, the idea was that
new galaxies would form from matter that was supposed to be continually
being created throughout space. The universe would have existed for ever
and would have looked the same at all times. This last property had the
great virtue, from a positivist point of view, of being a definite
prediction that could be tested by observation. The Cambridge radio
astronomy group, under Martin Ryle, did a survey of weak radio sources
in the early 1960s. These were distributed fairly uniformly across the
sky, indicating that most of the sources lay outside our galaxy. The
weaker sources would be further away, on average. The Steady State
theory predicted the shape of the graph of the number of sources against
source strength. But the observations showed more faint sources than
predicted, indicating that the density sources were higher in the past.
This was contrary to the basic assumption of the Steady State theory,
that everything was constant in time. For this, and other reasons, the
Steady State theory was abandoned.
Another attempt to avoid the
universe having a beginning was the suggestion that there was a previous
contracting phase, but because of rotation and local irregularities,
the matter would not all fall to the same point. Instead, different
parts of the matter would miss each other, and the universe would expand
again with the density remaining finite. Two Russians, Lifshitz and
Khalatnikov, actually claimed to have proved, that a general contraction
without exact symmetry would always lead to a bounce with the density
remaining finite. This result was very convenient for Marxist Leninist
dialectical materialism, because it avoided awkward questions about the
creation of the universe. It therefore became an article of faith for
Soviet scientists.
When Lifshitz and Khalatnikov published their
claim, I was a 21 year old research student looking for something to
complete my PhD thesis. I didn't believe their so-called proof, and set
out with Roger Penrose to develop new mathematical techniques to study
the question. We showed that the universe couldn't bounce. If Einstein's
General Theory of Relativity is correct, there will be a singularity, a
point of infinite density and spacetime curvature, where time has a
beginning. Observational evidence to confirm the idea that the universe
had a very dense beginning came in October 1965, a few months after my
first singularity result, with the discovery of a faint background of
microwaves throughout space. These microwaves are the same as those in
your microwave oven, but very much less powerful. They would heat your
pizza only to minus 271 point 3 degrees centigrade, not much good for
defrosting the pizza, let alone cooking it. You can actually observe
these microwaves yourself. Set your television to an empty channel. A
few percent of the snow you see on the screen will be caused by this
background of microwaves. The only reasonable interpretation of the
background is that it is radiation left over from an early very hot and
dense state. As the universe expanded, the radiation would have cooled
until it is just the faint remnant we observe today. Although the singularity theorems of Penrose and myself, predicted that
the universe had a beginning, they didn't say how it had begun. The
equations of General Relativity would break down at the singularity.
Thus Einstein's theory cannot predict how the universe will begin, but
only how it will evolve once it has begun. There are two attitudes one
can take to the results of Penrose and myself. One is to that God chose
how the universe began for reasons we could not understand. This was the
view of Pope John Paul. At a conference on cosmology in the Vatican,
the Pope told the delegates that it was OK to study the universe after
it began, but they should not inquire into the beginning itself, because
that was the moment of creation, and the work of God. I was glad he
didn't realize I had presented a paper at the conference suggesting how
the universe began. I didn't fancy the thought of being handed over to
the Inquisition, like Galileo.
The other interpretation of our
results, which is favored by most scientists, is that it indicates that
the General Theory of Relativity breaks down in the very strong
gravitational fields in the early universe. It has to be replaced by a
more complete theory. One would expect this anyway, because General
Relativity does not take account of the small scale structure of matter,
which is governed by quantum theory. This does not matter normally,
because the scale of the universe is enormous compared to the
microscopic scales of quantum theory. But when the universe is the
Planck size, a billion trillion trillionth of a centimeter, the two
scales are the same, and quantum theory has to be taken into account.
In
order to understand the Origin of the universe, we need to combine the
General Theory of Relativity with quantum theory. The best way of doing
so seems to be to use Feynman's idea of a sum over histories. Richard
Feynman was a colorful character, who played the bongo drums in a strip
joint in Pasadena, and was a brilliant physicist at the California
Institute of Technology. He proposed that a system got from a state A,
to a state B, by every possible path or history. Each path or history
has a certain amplitude or intensity, and the probability of the system
going from A- to B, is given by adding up the amplitudes for each path.
There will be a history in which the moon is made of blue cheese, but
the amplitude is low, which is bad news for mice. The probability for a state of the universe at the present time is given
by adding up the amplitudes for all the histories that end with that
state. But how did the histories start? This is the Origin question in
another guise. Does it require a Creator to decree how the universe
began? Or is the initial state of the universe, determined by a law of
science? In fact, this question would arise even if the histories of the
universe went back to the infinite past. But it is more immediate if
the universe began only 15 billion years ago. The problem of what
happens at the beginning of time is a bit like the question of what
happened at the edge of the world, when people thought the world was
flat. Is the world a flat plate with the sea pouring over the edge? I
have tested this experimentally. I have been round the world, and I have
not fallen off. As we all know, the problem of what happens at the edge
of the world was solved when people realized that the world was not a
flat plate, but a curved surface. Time however, seemed to be different.
It appeared to be separate from space, and to be like a model railway
track. If it had a beginning, there would have to be someone to set the
trains going. Einstein's General Theory of Relativity unified time and
space as spacetime, but time was still different from space and was like
a corridor, which either had a beginning and end, or went on forever.
However, when one combines General Relativity with Quantum Theory, Jim
Hartle and I realized that time can behave like another direction in
space under extreme conditions. This means one can get rid of the
problem of time having a beginning, in a similar way in which we got rid
of the edge of the world. Suppose the beginning of the universe was
like the South Pole of the earth, with degrees of latitude playing the
role of time. The universe would start as a point at the South Pole. As
one moves north, the circles of constant latitude, representing the size
of the universe, would expand. To ask what happened before the
beginning of the universe would become a meaningless question, because
there is nothing south of the South Pole.
Time, as measured in
degrees of latitude, would have a beginning at the South Pole, but the
South Pole is much like any other point, at least so I have been told. I
have been to Antarctica, but not to the South Pole. The same laws of
Nature hold at the South Pole as in other places. This would remove the
age-old objection to the universe having a beginning; that it would be a
place where the normal laws broke down. The beginning of the universe
would be governed by the laws of science. The picture Jim Hartle and I
developed of the spontaneous quantum creation of the universe would be a
bit like the formation of bubbles of steam in boiling water.
The
idea is that the most probable histories of the universe would be like
the surfaces of the bubbles. Many small bubbles would appear, and then
disappear again. These would correspond to mini universes that would
expand but would collapse again while still of microscopic size. They
are possible alternative universes but they are not of much interest
since they do not last long enough to develop galaxies and stars, let
alone intelligent life. A few of the little bubbles, however, grow to a
certain size at which they are safe from recollapse. They will continue
to expand at an ever increasing rate, and will form the bubbles we see.
They will correspond to universes that would start off expanding at an
ever increasing rate. This is called inflation, like the way prices go
up every year. The world record for inflation was in Germany after the First World War.
Prices rose by a factor of ten million in a period of 18 months. But
that was nothing compared to inflation in the early universe. The
universe expanded by a factor of million trillion trillion in a tiny
fraction of a second. Unlike inflation in prices, inflation in the early
universe was a very good thing. It produced a very large and uniform
universe, just as we observe. However, it would not be completely
uniform. In the sum over histories, histories that are very slightly
irregular will have almost as high probabilities as the completely
uniform and regular history. The theory therefore predicts that the
early universe is likely to be slightly non-uniform. These
irregularities would produce small variations in the intensity of the
microwave background from different directions. The microwave background
has been observed by the Map satellite, and was found to have exactly
the kind of variations predicted. So we know we are on the right lines.
The
irregularities in the early universe will mean that some regions will
have slightly higher density than others. The gravitational attraction
of the extra density will slow the expansion of the region, and can
eventually cause the region to collapse to form galaxies and stars. So
look well at the map of the microwave sky. It is the blue print for all
the structure in the universe. We are the product of quantum
fluctuations in the very early universe. God really does play dice.
We
have made tremendous progress in cosmology in the last hundred years.
The General Theory of Relativity and the discovery of the expansion of
the universe shattered the old picture of an ever existing and ever
lasting universe. Instead, general relativity predicted that the
universe, and time itself, would begin in the big bang. It also
predicted that time would come to an end in black holes. The discovery
of the cosmic microwave background and observations of black holes
support these conclusions. This is a profound change in our picture of
the universe and of reality itself. Although the General Theory of
Relativity predicted that the universe must have come from a period of
high curvature in the past, it could not predict how the universe would
emerge from the big bang. Thus general relativity on its own cannot
answer the central question in cosmology: Why is the universe the way it
is? However, if general relativity is combined with quantum theory, it
may be possible to predict how the universe would start. It would
initially expand at an ever increasing rate. During this so called inflationary period, the marriage of the two
theories predicted that small fluctuations would develop and lead to the
formation of galaxies, stars, and all the other structure in the
universe. This is confirmed by observations of small non uniformities in
the cosmic microwave background, with exactly the predicted properties.
So it seems we are on our way to understanding the origin of the
universe, though much more work will be needed. A new window on the very
early universe will be opened when we can detect gravitational waves by
accurately measuring the distances between space craft. Gravitational
waves propagate freely to us from earliest times, unimpeded by any
intervening material. By contrast, light is scattered many times by free
electrons. The scattering goes on until the electrons freeze out, after
300,000 years.
Despite having had some great successes, not
everything is solved. We do not yet have a good theoretical
understanding of the observations that the expansion of the universe is
accelerating again, after a long period of slowing down. Without such an
understanding, we cannot be sure of the future of the universe. Will it
continue to expand forever? Is inflation a law of Nature? Or will the
universe eventually collapse again? New observational results and
theoretical advances are coming in rapidly. Cosmology is a very exciting
and active subject. We are getting close to answering the age old
questions. Why are we here? Where did we come from?
Thank you for listening to me. |
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of Stephen Hawking. You may not reproduce, edit or distribute this
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