|
May 29, 2000 -- What do you think of when you hear
the word "antimatter?" Something exotic, something
unreal? Something about your Chief Engineer not being able to
keep the containment fields up during battle?
Well,
to a few NASA and university researchers, antimatter may just
be the future of human space travel. When it comes to packing
a punch, antimatter/matter reactions can't be beat. When a particle
and its antiparticle meet, they annihilate each other and their
entire mass is converted into pure energy.
Right: An artist's concept of a robotic antimatter-powered
probe sailing past planets in an imaginary nearby solar system.
Credit: Laboratory for Energetic Particle Science at Pennsylvania
State University.
Many physics textbooks describe matter as something "that
takes up space and has mass." Every physical object that
you've ever seen consists of matter. So if everything you know
is made of matter, then what's antimatter? Let's go back to the
1930s to find an answer.
In 1928, the British physicist Paul A.M. Dirac (1902-1984)
formulated a theory for the motion of electrons in electric and
magnetic fields. Such theories had been formulated before, but
what was unique about Dirac's was that his included the effects
of Einstein's Special Theory of Relativity. Dirac's equations
worked exceptionally well, describing many attributes of electron
motion that previous equations could not.
But his theory also led to a surprising prediction that
the electron must have an "antiparticle," having the
same mass but a positive electrical charge (the opposite of a
normal electron's negative charge). In 1932 Carl Anderson observed
this new particle experimentally and it was named the "positron."
This was the first known example of antimatter. In 1955 the antiproton
was produced at the Berkeley Bevatron, and in 1995 scientists
created the first anti-hydrogen atom at the CERN research facility
in Europe by combining the anti-proton with a positron (the normal
hydrogen atom consists of one proton and one electron). But when
these antihydrogen atoms are produced, they are traveling at
nearly the speed of light and don't last too long (40 nanoseconds
is typical).
Dirac's equations predicted that all
of the fundamental particles in nature must have a corresponding
"antiparticle." In each case, the masses of the particle
and antiparticle are identical, and other properties are nearly
identical. But in all cases, the mathematical signs of some property
are reversed. Antiprotons, for example, have the same mass as
a proton but the opposite electric charge. Since Dirac's time,
scores of these particle-antiparticle pairings have been observed.
Even particles that have no electrical charge, such as the neutron,
have antiparticles. These have other properties with a sign (such
as magnetic moment) that can be reversed.
Right:
A Penning trap is tested at Penn State University. Penning traps
use a combination of low temperatures and electromagnetic fields
to store antimatter. While the traps can only store incredibly
small quantities, the traps will help in developing the technologies
needed for advanced propulsion concepts. Credit: Laboratory for
Energetic Particle Science at Pennsylvania State University.
Interestingly, there is no real difference between particles
and antiparticles in particle physics theories. They are equivalent.
Most theoreticians believe that at the time of the Big Bang antiparticles
and particles were created in almost equal numbers. But why,
then, is antimatter so rare today?
The tentative answer (and it is tentative, since this question
is a topic of on-going research) is in the word almost.
Present theory suggests that if particles outnumbered antiparticles
in the Big Bang by as little as one part in 100 million, then
the present universe could be explained by those extra particles
that were not annihilated by an antiparticle counterpart. Other
theories suggest that even if identical amounts of antimatter
and matter were created in the Big Bang, the physics of antimatter
and matter are slightly different. This hypothesized difference
would favor residual matter after all original antimatter had
been annihilated.
So that's what antimatter is. Are we sure that there is no
antimatter left in the universe?
Dr. Charles Meegan, an astrophysicist at the Marshall Space
Flight Center, noted that orbiting gamma-ray observatories have
measured the sky in the range of energies that would have detected
the telltale signature of antimatter annihilation.
"None
of the instruments flown to date have uncovered evidence for
vast amounts of antimatter in the universe," says Meegan.
There is evidence that very energetic reactions are taking place
in isolated spots -- in
the cores of some galaxies and quasars, for example -- that
create antimatter which then annihilates. But this is not thought
to be residual antimatter left over from the Big Bang.
Above: Astronomers have discovered evidence for antimatter
near the center of our Milky Way galaxy by observing photons
with an energy of 511 keV -- the energy created when a positron
and an electron collide and annihilate. This image shows contours
of 511 keV radiation detected by NASA's Compton Gamma Ray Observatory
overlaid on an optical picture of the Galactic center. The vertical
structure is a jet of mutually-annihilating electrons and positrons.
[more information from Northwestern
University and NASA
HQ] Image Credit: Ron Murphy (Naval Research Laboratory)
.
On Earth all antimatter that exists is counted in individual
atoms. Low energy positrons are routinely used in a medical imaging
technique called Positron Emission Tomography as well as studies
of important materials used in electronics circuits. These positrons
are the result of the natural decay of radioactive isotopes.
While useful in medical and materials research applications,
there are not enough of these anti-electrons to provide a useful
form of rocket fuel. High-energy antimatter particles are only
produced in relatively large numbers at a few of the world's
largest particle accelerators. The current worldwide production
rate of antimatter is on the order of 1 to 10 nanograms (billionths
of a gram!) per year.
Right: This artist's concept of an antimatter-powered
rocket ship looks like a big space-borne linear accelerator.
Credit: Laboratory for Energetic Particle Science at Pennsylvania
State University.
How can antimatter help human exploration of space? The answer
lies in Einstein's famous equation E=mc2. When antimatter
annihilates normal matter, all the mass is converted to energy.
The energy output per unit particle vastly exceeds the efficiency
of chemical reactions such as burning hydrogen and oxygen in
the Space Shuttle main engines.
In Part 2 of this story, coming soon, we'll explain why some
rocket scientists think that antimatter is the ultimate fuel
and why nature may not cooperate!
What is
matter? Our ideas about matter have changed drastically in the
past 2500 years!
600 BC
- Thales of Miletus noticed that rubbing amber with fur caused
it to attract small bits of hair and other light objects. He
suggested that a mysterious force came from the amber.
460 BC - Democritus, from Greece, developed the concept
of dividing matter into smaller and smaller pieces until you
could divide it no more. He called these smallest pieces atoms.
Aristotle considered the idea of atoms to be worthless.
1687 AD - Sir Isaac Newton used arguments based upon the
theory of atoms to explain the gas laws.
1803 - John Dalton, English chemist, formulated his theory
that all matter consists of atoms, that chemical reactions result
from the union and separation of these atoms and that atoms have
characteristic properties.
1897 - English physicist, J.J. Thompson discovered the
electron and proposed a model of matter similar to "raisins
in a pudding."
1911
- Ernest Rutherford bombarded gold foil with helium nuclei (alpha
particles) and noticed that most go through the gold unchanged.
But some deflect into all directions and some even bounce back
in the direction they came. He concluded that matter is mostly
empty space and consists of a small positively charged center
surrounded by negatively charged particles.
1912 - Neils Bohr suggested that the electrons orbiting
the nucleus of atoms can only have certain discrete energies
and that each element had different electron energies.
1924 - Louis deBroglie, from France, suggested that matter,
like light, consisted of waves not particles.
1925 - Austrian physicist Erwin Schrodinger formed a model
of a complete atom as interacting waves. The particles became
like vibrations on a violin string, only they were closed in
circles.
1926
- German physicist Werner Heisenberg formulated his "uncertainty
principle" which says that you cannot know the position
and momentum of a particle simultaneously. The better you know
one, the worse you know the other. Atoms were now visualized
as a nucleus surrounded by a cloud of electron waves.
1960 - Murray Gel-Mann, American physicist, proposed that
protons and other basic particles in the atom consist of even
more fundamental particles he called quarks.
|
|