Evicting Einstein
Evicting Einstein
A physics experiment on the drawing board for the
International Space Station could help find the grand unifying "Theory
of Everything."
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March 26, 2004: Sooner or later, the reign of Einstein, like the reign of Newton before him, will come to an end. An upheaval in the world of physics that will overthrow our notions of basic reality is inevitable, most scientists believe, and currently a horse race is underway between a handful of theories competing to be the successor to the throne.
In
the running are such mind-bending ideas as an 11-dimensional universe,
universal "constants" (such as the strength of gravity) that vary
over space and time and only remain truly fixed in an unseen 5th dimension,
infinitesimal vibrating strings as the fundamental constituents of
reality, and a fabric of space and time that's not smooth and continuous,
as Einstein believed, but divided into discrete, indivisible chunks
of vanishingly small size. Experiment will ultimately determine which
triumphs.
Right:
According to Einstein's theory of general relativity, the sun's gravity
causes starlight to bend, shifting the apparent position of stars
in the sky.
A new concept for an experiment to test the predictions of Einstein's
relativity more precisely than ever before is being developed by scientists
at NASA's Jet Propulsion Laboratory (JPL). Their mission, which effectively
uses our solar system as a giant laboratory, would help narrow the
field of vying theories and bring us one step closer to the next revolution
in physics.
A House Divided
|
But the two theories are like different languages, and no one is yet sure how to translate between them. Relativity explains gravity and motion by uniting space and time into a 4-dimensional, dynamic, elastic fabric of reality called space-time, which is bent and warped by the energy it contains. (Mass is one form of energy, so it creates gravity by warping space-time.) Quantum mechanics, on the other hand, assumes that space and time form a flat, immutable "stage" on which the drama of several families of particles unfolds. These particles can move both forward and backward in time (something relativity doesn't allow), and the interactions between these particles explain the basic forces of nature -- with the glaring exception of gravity.
Left:
Astronomers use the light-bending properties of gravity to view very
distant galaxies--such as the arc shapes in this image--in a technique
called "gravitational lensing." [More]
The stalemate between these two theories has gone on for decades.
Most scientists assume that somehow, eventually, a unifying theory
will be developed that subsumes the two, showing how the truths they
each contain can fit neatly within a single, all-encompassing framework
of reality. Such a "Theory of Everything" would profoundly affect
our knowledge of the birth, evolution, and eventual fate of the universe.
Slava Turyshev, a scientist at JPL, and his colleagues have thought
of a way to use the International Space Station (ISS) and two mini-satellites
orbiting on the far side of the sun to test the theory of relativity
with unprecedented accuracy. Their concept, developed in part through
funding from NASA's Office of Biological and Physical Research, would
be so sensitive that it could reveal flaws in Einstein's theory, thus
providing the first hard data needed to distinguish which of the competing
Theories of Everything agree with reality and which are merely fancy
chalk-work.
The experiment, called Laser Astrometric Test Of Relativity (LATOR),
would look at how the sun's gravity deflects beams of laser light
emitted by the two mini-satellites. Gravity bends the path of light
because it warps the space through which the light is passing. The
standard analogy for this warping of space-time by gravity is to imagine
space as a flat sheet of rubber that stretches under the weight of
objects like the sun. The depression in the sheet would cause an object
(even a no-mass particle of light) passing nearby the sun to turn
slightly as it went by.
In
fact, it was by measuring the bending of starlight by the sun during
a solar eclipse in 1919 that Sir Arthur Eddington first tested Einstein's
theory of general relativity. In cosmic terms, the sun's gravity is
fairly weak; the path of a beam of light skimming the edge of the
sun would only be bent by about 1.75 arcseconds (an arcsecond is 1/3600
of a degree). Within the limits of accuracy of his measuring equipment,
Eddington showed that starlight did indeed bend by this amount --
and in doing so effectively impeached Newton.
LATOR would measure this deflection with a billion (109) times the precision
of Eddington's experiment and 30,000 times the precision of the current
record-holder: a serendipitous measurement using signals from the
Cassini spacecraft on its way to explore Saturn.
Above: The curvature of space due to the sun's mass caused signals from the Cassini probe to curve on their way to Earth. [More]
"I think [LATOR] would be quite an important advance for fundamental physics," says Clifford Will, a professor of physics at Washington University who has made major contributions to post-Newtonian physics and is not directly involved with LATOR. "We should continue to try to press for more accuracy in testing general relativity, simply because any kind of deviation would mean that there's new physics that we were not aware of before."
Solar laboratory
The experiment would work like this: Two small satellites, each about
one meter wide, would be launched into an orbit circling the sun at
roughly the same distance as Earth. This pair of mini-satellites would
orbit more slowly than Earth does, so about 17 months after launch,
the mini-satellites and Earth would be on opposite sides of the sun.
Even though the two satellites would be about 5 million km apart,
the angle between them as viewed from Earth would be tiny, only about
1 degree. Together, the two satellites and Earth would form a skinny
triangle, with laser beams along its sides, and one of those beams
passing close to the sun.
Above: A schematic diagram of the proposed LATOR mission.
Turyshev plans to measure the angle between the two satellites using an interferometer mounted on the ISS. An interferometer is a device that catches and combines beams of light. By measuring how waves of light from the two mini-satellites "interfere" with each other, the interferometer can measure the angle between the satellites with extraordinary precision: about 10 billionths of an arcsecond, or 0.01 µas (micro-arcseconds). When the precision of the other parts of the LATOR design are considered, this gives an overall accuracy for measuring how much gravity bends the laser beam of about 0.02 µas for a single measurement.
"Using the ISS gives us a few advantages," Turyshev explains. "For one, it's above the distortions of Earth's atmosphere, and it's also large enough to let us place the two lenses of the interferometer far apart (one lens on each end of the solar panel truss), which improves the resolution and accuracy of the results."
Left:
The interferometer will be mounted to the solar-panel truss
of the ISS, which automatically rotates to continuously face the sun.
Image courtesy Slava Turyshev.
The 0.02 µas accuracy of LATOR is good enough to reveal deviations
from Einstein's relativity predicted by the aspiring Theories of Everything,
which range from roughly 0.5 to 35 µas. Agreement with LATOR's
measurements would be a major boost for any of these theories. But
if no deviation from Einstein is found even by LATOR, most of the
current contenders--along with their 11 dimensions, pixellated space,
and inconstant constants--will suffer a fatal blow and "pass on" to
that great dusty library stack in the sky.
Because the mission requires only existing technologies, Turyshev
says LATOR could be ready to fly as soon as 2009 or 2010. So it may
not be too long before the stalemate in physics is broken and a new
theory of gravity, space, and time takes the throne.
Web Links
NASA's Office of Biological and Physical Research (OBPR) supports studies like Turyshev's for the benefit of humans in space and on Earth
Laser Astrometric Test Of Relativity (LATOR) -- technical paper by Turyshev and colleagues about the LATOR concept
Many of the candidates
for a "Theory of Everything" predict the existence of a
scalar field
that permeates the universe. Einstein first proposed such a field
when he introduced a cosmological
constant into his equations for gravity. He later changed his
mind and removed this
term, but recently the idea has garnered renewed interest among
physicists. Such a term could account for the surprising discovery
that the expansion of the universe is actually accelerating, not slowing
down as physicists previously thought. Like the famous Michelson-Morley
experiment in 1887 that sought to detect the existence of the
"aether", LATOR will be able to determine whether the scalar
field exists -- a finding that will be pivotal in the search for a
Theory of Everything.
Einstein's Relativity and Everyday Life -- Physicist Clifford Will explains how the Global Positioning System depends on the theory of relativity.
The Theory of Everything -- article about the search for a theory to unify relativity with quantum mechanics, by physicist Michio Kaku
A Pop Quiz for Einstein -- (Science@NASA) The Gravity Probe B mi will test two important aspects of Einstein's theory of General Relativity.
The Elegant Universe -- Watch a 3 hour series from PBS's Nova about the quest to find a unifying Theory of Everything
"Laser Astrometric Test of Relativity (LATOR) Mission Studies" is just one of many fundamental physics research grants recently awarded by NASA's Office of Biological and Physical Sciences.
General Relativity -- Introduction to general relativity, from the Wikipedia
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