General Relativistic Time Dilation
One of the implications of General Relativity is that the nearer a clock is to a "gravitational body" (planet or star) the slower it runs. This may seem counter-intuitive, but when you take the law of conservation of energy into consideration, you realize that this has to be true.
If you throw a ball straight upward, it loses velocity as it moves up. Since velocity is related to kinetic energy,
The ball also loses kinetic energy as it moves upward. If it did not, it would not slow down, stop its ascent, and fall back to Earth.
.It is known that matter can be converted into energy in the form of light. If matter (here, a ball) loses energy as it moves away from the Earth, and if matter can be converted into light, then shouldn’t light lose energy as it moves away from the Earth? If this were not true, and the light lost no energy, you could devise an energy-producing system, in which matter would be converted into light at the Earth’s surface, with the light then re-converted into matter somewhere above. The energy of the falling matter could be utilized again and again as the matter fell back to the Earth’s surface, where it could again be re-converted to light. (remember that light, unlike the ball, does not fall back to Earth. This system, which would have no energy input, would continue producing energy, operating forever.
Such a system does not, and cannot exist, because it violates the principle of Conservation of Energy
. Light must lose energy as it moves away from the earth, or any other gravitational body, and its loss of kinetic energy is permanent. The following diagram illustrates this principle:The energy of light is given by the equation: energy = Planck’s constant x light frequency, or,
Planck’s constant doesn’t change under any known circumstances, so for light to lose energy, it must lose frequency. So, if you are high above the Earth and see light that was produced at the surface of the Earth, the light that you see will have a slightly lower frequency than will be seen by someone on the ground. Everything with a frequency that you see below you (the light itself or a clock the light is coming from) appears slower than it appears to someone at the surface of the earth, because the frequency is lower.
Conversely, light gains energy as it moves toward a gravitational field , just as the ball gains kinetic energy as it falls, so if you shine a light down toward the Earth, it will arrive with a slightly higher frequency than the frequency you measure when you produce it.
As a consequence of all this, when you are high above the Earth, you will see activities happening on the ground in slightly slow motion, while someone on the ground will see your activities in slightly fast motion. So, bizarre as it seems, time moves slower near a gravitational body, even though no one on gravitational body will notice it himself.
Using the principle of Conservation of Energy, it is possible to calculate how much slower time moves at the surface of the Earth than, say, 10,000 meters above it. This can be done by showing the loss of energy ( and consequently, frequency) of a photon produced at the Earth’s surface, moving away from the Earth. For this example, let’s use the photon created when an electron and a proton combine to form a hydrogen atom. The energy of the photon produced when this combination occurs is 13.5 volts, or
. Since energy and matter can be converted from one to the other, this photon has a (very small) mass equivalent that we will call "M". From , we have:
Now, the kinetic energy loss of something moving away from a gravitational field is
where is the mass of the planet or star producing the gravitational field, r is the distance to the center of the star or planet, is the mass of the object moving away from the star or planet, and G is the Universal Gravitational Constant ( ). To find the energy loss of the photon , it is only necessary to plug numbers into the equation in two sets of circumstances:The mass of the earth is
. The radius of the Earth is .In the following two equations, since the numerators are identical, and since the denominators differ by exactly 10,000 meters, all terms can be treated as if they had an infinite number of significant figures.
=
=
The difference in energy is
.
Since the energy of a photon is proportional to its frequency,
This factor represents how much slower time passes at the Earth’s surface than it does 10,000 meters above it. In terms of actual measured time, this amounts to
So, a clock at the Earth’s surface should be slower by one second every 29,100 years than a clock 10,000 meters above it.
Content of this paper may be freely used so long as credit is given to the author, Brian Stedjee
First publication date: October, 2003