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| subject: | Universe - UFO\U7.TXT |
[video: inside the mine] A pit has been excavated, rigged with
sensitive detectors, and then filled with 660 tons of pure water.
If a proton in any one of the billions of water molecules in the tank
were to decay, it would send out a telltale flash of light. Computers
monitoring the flash of light would bring the news to waiting scientists.
If the results are positive, the experiment will confirm an unsettling
hypothesis: that all the matter in the universe is a passing fancy,
a stage in the ongoing dance of energy.
If electromagnetism and the weak force unite at high energies, and
the strong force joins with them at still higher energies, then might
not all the four forces ultimately be one? Some of the most inventive
minds in physics are at work trying to solve that riddle.
Stephen Hawking ranks among the world's leading physicists, despite
his having suffered, for more than 20 years, from a progressive disease
of the central nervous system that has left him paralyzed and almost
unable to speak.
Hawking holds Isaac Newton's old chair as Lucasian professor
of mathematics at Cambridge University. During a recent seminar at
Cal Tech, his words were interpreted by a former student, super-
symmetry physicist Nick Warner. Hawking's subject, the infancy
of the universe.
*****
[video: A California Institute of Technology classroom; Hawking
speaks, while Warner translates and draws equations and diagrams on the
board.]
NICK WARNER: [translating Hawking] The boundary conditions are that the
universe has no boundary. (Sounds rather Zen, doesn't it?) [laughter]
What Stephen means by this is that spacetime is some compact, four-
dimensional manifold... This is a general four manifold--some compact
four-manifold M with some metric on it, G Mu Nu, on the surface, and
also some matter fields, Phi, on the surface.
MURRAY GELL-MANN: [later in the conference] Do I understand, then,
that you want the mass of effective unification of a Yang-Mills or super
Yang-Mills theory to be this low, like 10 to the 14th? Or can that M be
something else?
NICK WARNER: [Translating Hawking] It may be something else.
MURRAYGELL-MANN But in any case, the M is the mass characteristic of
whatever physics is responsible for the transition?
NICK WARNER: [translating Hawking] It is a mass. It generates the
the inflation cosmological constant. Stephen wants just to add that
you can also explain-you can also explain the arrow of time from this.
He thinks that would take much more time than we have. That's all.
[applause]
*****
TIMOTHY FERRIS: No laboratory on Earth can produce the energy at which
the four forces would act as one. Only the fires of Genesis were hot
enough for that. The search for simplicity in the realm of the atom
draws us out into the realm of the galaxies, and back toward the
beginning of time.
(End of Part One)
THE
CREATION
OF THE
UNIVERSE
TIMOTHY FERRIS: [video: computer animation of the Milky Way galaxy,
wheeling in space.] We live in a major spiral galaxy that we call
the Milky Way. It's home to the sun and a few hundred billion other
stars.
The galaxy belongs, in turn, to a cluster of galaxies. Astronomers
call it the local group. And the local group is part of the Virgo
supercluster, an archipelago of galaxies stretching across one hundred
million light years of space.
[video: animated expansion of the Virgo Supercluster] The galaxies
are marching away from one another as the universe expands. In a
computer simulation based upon astronomical observations, we witness
something never before seen by human eyes, the predicted scattering of
the Virgo supercluster, by the expansion of the universe, over the
course of the next fifty billion years.
[video: stills of Einstein; then, footage of Einstein and Hubble
at Mt. Wilson Observatory] The expansion of the universe was
predicted by Einstein's general theory of relativity, published in
1915. But the idea seemed so outlandish that Einstein himself
rejected it.
He introduced an extraneous term into the field equations to try
to make his theoretical universe stand still. Later Einstein would
call this modification of the theory, "the worse blunder of my
career." Then, in 1929, the American astronomer Edwin Hubble,
without knowing of the relativity prediction, discovered that the
universe is indeed expanding. Einstein and Hubble met in California
in 1931, and celebrated Hubble's having found, at the telescope,
what the mind of Einstein had conceived.
Astronomer Allan Sandage, once Hubble's pupil, has devoted much
of his career to studying the expansion of the universe.
*****
ALLAN SANDAGE: It is not as if these galaxies are expanding into
a space that's already there. The view is that space itself is
expanding, carrying the galaxies with it. The expansion creates the
space. The crucial analogy, first made by Eddington as long ago as
1930, just one year after Hubble had announced the expansion, was
you can conceptualize the thing as the two dimensional analog, by
the surface of a balloon.
You paint dots on the surface of a balloon and you blow it up.
You put yourself on any dot. You seem to be the center, and all the
other dots move away from you. Now, take the air out of the balloon,
and look what the dots do. All the dots come toward every other dot,
and if you could take all of the air out of a perfect balloon, the
surface itself would go to zero; all the dots would be back at one
place at one time. Every place is the center of the expansion.
When you talk about this, the question that always comes, well,
can you find the center of the expansion? Every place is the center
of the expansion. There is no center to the beginning. Everything
was back at one place, and every place and every time was identical,
in the beginning.
*****
continued...
--- FMail 1.22
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