Stephen and, since 1979, he has held

Stephen J. Hawking by Rachel Finck
Stephen Hawking was born in January of 1942 in Oxford, England. He grew
up near London and was educated at Oxford, from which he received his BA in 1962,
and Cambridge, where he received his doctorate in theoretical physics. Stephen
Hawking is a brilliant and highly productive researcher, and, since 1979, he has
held the Lucasian professorship in mathematics at Cambridge, the very chair once
held by Isaac Newton. Although still relatively young, Hawking is already being
compared to such great intellects as Newton and Albert Einstein. Yet it should
be noted that since the early 1960s he has been the victim of a progressive and
incurable motorneurone disease, ALS, that now confines him to a wheelchair.

This affliction prevents Hawking from reading, writing, or calculating in a
direct and simple way. The bulk of his work, involving studying, publishing,
lecturing, and worldwide travel, is carried on with the help of colleagues,
friends, and his wife. Of his illness, Hawking has said that it has enhanced
his career by giving him the freedom to think about physics and the Universe.

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Stephen Hawking has written many essays involving the unified theory,
which is a theory summarizing the entire of the physical world; a theory that
would stand as a complete, consistent theory of the physical interactions that
would describe all possible observations. Our attempts at modeling physical
reality normally consists of two parts: a) A set of local laws that are obeyed
by the various physical quantities, formulated in terms of differential
equations, and b) Sets of boundary conditions that tell us the state of some
regions of the universe at a certain time and what effects propagate into it
subsequently from the rest of the universe. Presently, physicist are still
trying to unify two separate theories to describe everything in the universe.

The two theories are the general theory of relativity and quantum mechanics.

Albert Einstein formulated the general theory of relativity almost
single-handedly in 1915. First, in 1905, he developed the special theory of
relativity, which deals with the concept of people measuring different time
intervals, while moving at different speeds, yet measuring the same speed for
the speed of light, regardless of velocity. In 1915, he developed the general
theory of relativity. This theory dealt with the concept of gravity as a
distortion of space-time, and not just a force within it.

Einstein’s original equations predicted that the universe was either
expanding or contracting. Einstein’s equations showed that mass and energy are
always positive, which is why gravity always attracts bodies toward each other.

Space-time is curved back onto itself like the surface of the earth. It was
then theorized that what if matter could curve a region in on itself so much
that it could cut itself off from the rest of the universe. The region would
become what is known as a black hole. Nothing could escape it, although objects
could fall in. To get out, the objects would have to move faster than the speed
of light, and this was not allowed by the general theory of relativity. In 1965,
Hawking along with Roger Penrose proved a number of theorems that showed the
fact that space-time was curved in on itself so that there would be
singularities where space-time had a beginning or an end.

“The fact that Einstein’s general theory of relativity turned out to
predict singularities led to a crisis in physics. (Hawking)” The equations of
general relativity cannot be defined as a singularity. This means that general
relativity cannot predict how the universe should begin at the big bang. Thus,
it is not a complete theory. It must be paired with quantum mechanics.

In 1905, the photoelectric effect was written about by Einstein, which
he theorized could be explain if light came not in continuously variable amounts,
but in packets of a certain size. A few years earlier, the idea of energy in
quanta had been introduced by Max Planck.

The full implications of the photoelectric effect were not realized
until 1925, when Werner Heisenberg pointed out that it made it impossible to
measure the position of a particle exactly. To see where a particle is, you
have to shine a light on it. As Einstein showed, you had to use at least one
quanta of light. This whole packet of light would disturb the particle and
cause it to move at some speed in some direction different than its state before
the light was shined. In this way, it was theorized that the more accurately
you want to measure the position of the particle, the greater the energy packet
you would have to use and thus the more you would disturb the particle. This
dilemma is called the Heisenberg uncertainty principle.

Einstein’s general theory of relativity is a classic theory because it
does not take into account the uncertainty principle. One therefore has to find
a new theory that combines general relativity and the uncertainty principle. In
most situations, the difference between the general relativity theory and the
new theory is very small. However, the singularity theorems that Hawking proved
show that space-time will become highly curved on very small scales. The
effects of the uncertainty principle will then become very important.

The problems that Einstein had with quantum mechanics is that he used
the commonsense notion that a particle has a definite history. And that a
particle has a definite location. But, it must be taken into account that a
particle has an infinite set of histories. A famous thought experiment called
Shroedinger’s cat helps to illustrate this concept. Let’s say that a cat is
placed in a sealed box and a gun is pointed at it. The gun will only go off if
a radioactive nucleus decays. There is exactly a 50% chance of this happening.

Later on, before the box is opened, there are two possibilities of what happened
to the cat: the gun did not go off, and the cat is alive, or the gun did go off,
and the cat is dead. Before the box is opened, the cat is both alive and dead
at the same time. The cat has two separate histories.

Another way to think of this was put forth by a physicist Richard
Feynman. He contributed that a system didn’t just have a single history in
space-time, but it had every possible history. “Consider, for example, a
particle at point A at a certain time. Normally, one would assume that the
particle would move in a straight line away from A. However, according to the
sum over histories, it can move on any path that starts at A. (Hawking)” It’s
like what happens when you place a drop of ink on blotting paper, and it
diffuses along every path away from its point of origin.

In 1973, Stephen Hawking began investigating what effect the uncertainty
principle would have on a particle in the curved space-time near a black hole.

He found that the black hole would not be completely black. The uncertainty
principle would allow particles to leak out of the black hole at a steady rate.

Although, the discovery came as a complete surprise, “It ought to have been
obvious. The Feynman sum over histories says that particles can take any path
through space-time. Thus it is possible for a particle to travel faster than
light. (Hawking)”
In 1983, Stephen Hawking proposed that the sum of histories for the
universe should not be taken over histories in real time. Rather, it should be
taken over histories in imaginary time that were closed in on themselves, like
the surface of the earth. Because these histories didn’t have any singularities
or any beginning or end, what happened to them would be determined entirely by
the laws of physics. This means, what happened in imaginary time could be
calculated. “And if you know the history of the universe in imaginary time, you
can calculate how it behaves in real time. In this way, you could hope to get a
complete unified theory, one that would predict everything in the universe.

Imaginary time is a concept that Hawking has made a particular advance
in as a physicist. It seems obvious that the universe has a unique history, yet
since the discovery of quantum mechanics, we have to consider the universe as
having every possible history. To grasp the concept of imaginary time, think of
real time as horizontal line. Early times are on the left, and late times are
on the right. Then think of lines going 90 from the horizontal line of real
time. These lines, which are at right angles to real time, represent imaginary
time. The importance of imaginary time lies in the fact that the universe is
curved in on itself, leading to singularities. At the singularities, the
equations of physics cannot be defines, thus one cannot predict what will happen.

But the imaginary time direction is at right angles to real time. This means
that it behaves in a similar way to the three directions that correspond to
moving in space. Then, the curvature of space can lead to the three directions
and the imaginary time direction meeting up around the back. These would form a
closed surface, like the surface of the earth. Stephen Hawking as a physicist
has many much progress in the use of imaginary time in the way the field of
physics thinks.


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