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| subject: | Universe - UFO\U6.txt |
[video: animation showing clouds of protons moving through the ring)
For years, scientists had been accelerating protons in the giant CERN
ring, and colliding them with stationary targets.
[video: anti-proton collector ring] But now, for the first time,
anti-protons, rare particles identical to protons, but with opposite
charge, were manufactured and stored in this anti-matter collector.
Then the anti-protons were injected into the main ring, hurtling in
the opposite direction as the protons. When matter meets anti-matter,
the result is mutual annihilation.
The impact between a single proton and anti-proton releases, for
a tiny fraction of a second, more energy than the electrical output
of all the power plants in the world. Subatomic particles come
reeling out of that tiny explosion, and are captured in the onion skin
layers of this giant particle detector .
[video: CERN personnel studying particle tracings and other data on
display screens.] On the 28th of May, 1983, traces of a Z particle
were detected in the debris emitted by a proton-antiproton collision.
The electroweak unified theory had been confirmed.
Carlo Rubbia of CERN shared the 1984 Nobel Prize in physics for having
conceived of the idea of colliding matter with antimatter.
*****
CARLO RUBBIA: What we are really doing here, we are making little
bangs. We are concentrating, in a very small volume of space, for a
very short period of time, enough energy, density, so that we can
revive--or replace, so to speak--on a very modest scale, what was really
the state of affairs of the universe as a whole.
The major progress in science has been made, I believe, by Galileo
Galilei when he brought the experimental science to its right level of
importance. And I still believe that to a greater extent, our scientific
progress is made through experimental science. It's not because I am an
experimental scientist. [It's] just because I believe that there is
always the final verdict, the final guidance, which comes from the
physical phenomenon.
*****
TIMOTHY FERRIS: With electroweak theory a successor scientists went on to
compose the so-called grand unified theories. These theories say that
at still higher energy levels, three of the four forces might function
as a single force. And here again, it's theorized that an exotic particle
would do the work of unification. It's called the X particle.
[video: animation of particles] As we watch, a gluon, carrier of the
strong force, strikes an X particle, and is transformed into a photon,
the carrier of electromagnetism. Alternately, a gluon striking an X can
be transformed into a weak boson, carrier of the weak force.
[video: the "virtual sea," a computer-animated representation of
virtual particles appearing out of a vacuum] Particles of energy
live on borrowed time. They gather themselves up from the stray energy
in a vacuum, then ebb back into nonexistence. The grand unified theories
make the startling prediction that not just energy but matter may be
temporary. They say that protons, the particles that form the heart of
every atom in the universe, are not permanent, as had been thought,
but are destined to decay.
[voice over video, Venice, Italy, spires rising from the mist)
The grand unified theories paint in deepened colors the old lesson that
birth implies death. It's the latest chapter in a scientific saga that
began here in Venice 375 years ago.
[Ferris at Piazza San Marco] On August the 25th, 1609, Galileo led
a procession of Venetian senators across the square and up to the top
of that tower for their first look through his first telescope.
Galileo was teaching just up the river at the University of Padua at
the time. He was a respected teacher. Students flocked to his classes.
He'd written a couple of good books. But his contract was about to
expire, he never made enough money to get by, and he needed something
to help his career. He found it. It was the telescope.
[voice over video of Galileo's telescope] The senators were
impressed. They granted Galileo tenure, gave him a promotion, and
they commissioned telescopes for sighting ships at sea. But Galileo
trained his telescopes on the sky.
[video: Galileo's drawings] He saw that the moon has mountains
as rugged as the Apennines, and that other planets have moons, and
that the Milky Way runs deep with pasture lands of stars. And these
sights helped to convince him that the heavens are as substantial
and changeable as the Earth.
Galileo's observations provided evidence that the stars and planets
are worlds like ours, made of the same elements and functioning in
accordance with the same physical laws. They drew together the
realms of the large and small, and married the Earth to the universe.
[video: canals of Venice] The Venetians understood that nothing
on Earth lasts forever. They were citizens of a republic literally
raised upon shifting sands and supported by the risky business of
ocean-going trade. But they thought that the stars, at least, were
immutable.
Galileo's work changed that. By introducing into science the idea
that the Earth is part of the universe, he set the stage for the
subsequent discovery that even stars live and die. Since Galileo's
day, telescopes have looked out into space to scales Galileo never
dreamed of, and particle accelerators have looked just as far into
the world of the small. And everywhere, they have found change. If
the grand unified theories are right, not even atoms last forever.
[video: Venice flooded] The city where Galileo glimpsed signs
of the mortality of the heavens is itself in peril. Venice is
sinking, its streets flooding with every winter's storm. The city
cannot last forever, but it has company in that. Neither, it seems,
can the sun, nor the stars, nor the atoms they are made of.
[video: a mine in the mountains] Kamioka, Japan. Here, in a lead
mine, an experiment is underway to learn whether protons are mortal.
To minimize interference by high energy particles coming from space,
the experiment is conducted nearly two miles underground. The unified
theories predict that the average proton will last many billions of
years. But by assembling an enormous quantity of protons, scientists
can test the theories in the course of a year or two of careful
observation. And that's what's being done here.
continued...
--- FMail 1.22
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