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Adrian Wagner

Gravity Waves  

Sir Isaac Newton viewed gravity as a force of attraction between two bodies that manifest itself via a gravitational field.   For 400 years, this description of gravity was left unchanged; it stood solid in the minds of physicists and in the explanations of their experimental observations.  Its was not until the end of the 19th century, that astronomers began to notice a slight differences in the calculated and observed orbit of Mercury, which could not be explained via Newton's gravitational laws.

By 1915, this error of observation had been mathematically rationalized, but it was only after building an entire new theory of gravity.  This theory is known as Einstein's General Theory of Relativity.

Einstein replaced Newton's gravitational force, with the idea that mass effected space and time itself by curving it.  According to the General Theory of relativity, it is this curvature that causes what can be observed as the force of gravity.

 

 

In the figure above, which represents the curvature of space-time by the large central white mass, it is the mass itself that is causing the curvature.  Any object placed near the mass will fall towards it, just as if it was being pulled towards it by a force.  Any object with perpendicular motion - relative to the line formed between its position and the center of the sphere - will, if moving at the right velocity, circle in orbit around the sphere.  Just as the earth revolves around the sun, a body in such a relationship to a central mass that is curving space and time, will orbit the central body.  According to General Relativity, it is not a force that acts upon the body.  Rather, the body in orbit feels no force at all.  It is space and time that is curved, such that the body, moving, unchanging in its movement, un-accelerated - can travel through this curved space as if it were unaffected by any force, and appear as if it were being accelerated by a force if it were indeed in flat space.  It is the very notion of a path that must be revisited.  A line that is straight in flat space is not so in curved space, such that the line formed by a body's trajectory can loop back upon itself as in an orbit.  This is the general premise of Einstein's theory.

            One of the outcomes of the theory of General Relativity is the prediction of Gravity Waves.  If a body with significant mass is at rest, it curves space and time around it as previously described.  If, however, the body moves suddenly, the curvature of space-time must also be altered around it.  Yet space-time can only experience change from the point of origin at the rate that it takes light to radiate from that origin.  In other words, nothing in the known universe can travel faster than light.  As such, the very fabric of space-time that makes up the universe can also not be effected by change - in this case the change of its curvature - at a speed faster than light.  So if gravity curves space and the curvature of space is altered by moving the gravitational 'source' that curves it, the change of this curvature travels across the fabric of space time at the speed of light, as a ripple travels across the surface of a pond.

 

 

These gravitational waves, Einstein predicted, "are produced when objects are accelerated, or when strong gravitational fields interact dynamically."

Gravitational waves cause a variable strain of space-time.  What this means is that as a gravitational wave passes a region of space, the wave changes the distance between points in that space.  The size of these changes is proportional to the distance between the points.  It is therefore possible to detect gravitational waves, given that one could detect minute changes distance.  However, the change of distance caused by a fairly large gravitational wave would alter the distance between the sun and the earth by less than the diameter of an atom.  Clearly detecting such an effect is a great challenge.

            To date, no one has observed a gravitational wave directly by such means.  However there is already strong evidence that they indeed do exist.  One of the outcomes of their prediction is that any source that emits gravitational waves looses energy as it produces them.

A strong candidate for the production of significantly high-energy gravitational waves is a pair of orbiting neutron stars and/or black holes.  Because of the high densities of these objects, they produce very powerful distortions in the curvature of space-time.  The interaction of these curvatures should produce high-intensity gravitational waves.  Consequently, the two orbiting pairs will emit energy, thus loosing the momentum necessary to maintain their orbits.  As the stars get closer together, the period of their orbit decreases according to Kepler's third law. 

This effect has been observed in the binary pulsar system PSR 1913+16 discovered in 1974.  This system consists of two massive objects, probably neutron stars, separated by a distance only a few times larger than the distance from the Earth to the moon.  As one of the stars emits radio signals, the period of its orbit can be determined by looking at the Doppler shifts in the signals frequency.  Indeed the pair is slowly spiraling inward, at a rate 99.5% of that predicted by the theory of General Relativity. 

This slowing of the orbital period is the strongest evidence found for the existence of gravity waves.  However, large and costly projects are underdevelopment to detect these waves directly.

As already noted, the presence of gravity waves changes the distances between points every so slightly.  If these changes in distance can be detected, the magnitude and frequency of these changes can shed light on the very ripples of space-time that pass through them.  In fact, if multiple detectors are set up in a three dimensional array, the shape and direction of these waves can be detected.  The value of such a systems come from the fact that gravitational waves, unlike electromagnetic ones, are not absorbed, deflected, not dispersed by matter.  They do not travel through space, but rather the are the fluctuations of space-time itself.  Therefore, they may one day allow us to pear into the center of object that are otherwise not transparent to electromagnetic waves.  We may be able to see the inside of a supernova.  We may be able to see the properties of a black hole.  We may even be able to see into the far reaches of time, in the early moments of the universe.  Such a devise "may be able to peer into the nursery of creation.  The earliest instant following the Big Bang - the Planck era - marked its passage by emitting gravitational waves."  After 300,000 years, the universe had cooled enough to allow atoms to form, thus becoming transparent to the microwave radiation that we can observe today.  But prior to this time, the history of the universe is hidden.  The detection of gravitational waves, which were able to stream freely as early as 10-43 seconds after the big bang, could enable us to hear "at last the hush of the universe's birth."

 

 

The above depicts how a gravitational wave detector would work.  The underlying principle is based on the fact that the distance between two bodies will change as a gravitational wave passes through them.  This change in distance, however, can be very difficult to detect. In fact, the changed effected by a fairly large gravitational wave on two large masses separated by 4km can be as little as the side of the nucleus of an atom.  Do be able to measure such distances, scientists propose to use laser light to bounce a beam back and forth between the two masses.  Any change in the distance should result in a noticeable change in the phase of the light, and bands of dark phase cancellations should appear.  Another challenge is isolating any seismic disturbances from the earth from these masses.  Elaborate spring dampening and active seismic cancellation systems are now in development.

If the detection of gravitational waves proves to one day be possible, it will in theory open up an entire new spectrum into the universe.  We will be able to see inside of otherwise mysterious object, and perhaps even pear into our universe's very origin.

 

 
 

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