Solving the Critical Radius for Relativity: Find krE!

In summary, Special Relativity states that a clock orbiting Earth will tick slower than one on the surface of Earth, while General Relativity states that a clock will tick faster the further it is from a mass. However, there is a critical radius where these two effects cancel out. This can be determined using the time dilation factor for an object on the surface of Earth and an object in orbit at a certain radius. The radius can be represented as rc=krE, where k is a number to be determined and rE is the radius of the Earth.
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n1caboose
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Special Relativity states that a clock orbiting Earth will tick slower than one on the surface of Earth. General Relativity states the opposite - a clock will tick faster the further it is from a mass. Is there then a critical radius where these two effects cancel out? Ignore the rotation of Earth for this problem. State the radius in terms of rc=krE, where k is the number to be determined and where rE is the radius of the Earth.

-This was the extra credit problem on my Relativity final which I really wish I could have solved. Anybody want to take a shot at it?
 
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n1caboose said:
Special Relativity states that a clock orbiting Earth will tick slower than one on the surface of Earth. General Relativity states the opposite - a clock will tick faster the further it is from a mass. Is there then a critical radius where these two effects cancel out?

Yes. If you want to take a second stab at it, consider the following:

An object on the surface of the Earth, ignoring the Earth's rotation, will have a "time dilation factor" of

[tex]\sqrt{1 - \frac{2GM}{c^2 r_E}}[/tex]

An object in orbit about the Earth at some radius r will have a "time dilation factor" of

[tex]\sqrt{1 - \frac{2GM}{c^2 r} - \frac{v^2}{c^2}}[/tex]

where v is the orbital velocity at radius r. (Can you see how to get this result?) These two facts are enough to get the answer you seek.
 

Related to Solving the Critical Radius for Relativity: Find krE!

1. What is the critical radius in relativity?

The critical radius in relativity refers to the distance from a massive object at which gravity becomes so strong that even light cannot escape. This is also known as the event horizon.

2. How is the critical radius calculated?

The critical radius is calculated using the equation krE = 2GM/c^2, where k is a constant, rE is the event horizon radius, G is the gravitational constant, and c is the speed of light.

3. Why is solving the critical radius important in relativity?

Solving the critical radius is important in relativity because it helps us understand the behavior of massive objects in the universe, such as black holes. It also plays a crucial role in understanding the nature of gravity and its effects on space and time.

4. What are the applications of the critical radius in relativity?

The critical radius has several applications in relativity, including predicting the behavior of black holes, understanding the formation of galaxies and other celestial bodies, and studying the effects of gravity on light and other particles.

5. Are there any limitations to using the critical radius in relativity?

Yes, there are some limitations to using the critical radius in relativity. For example, it only applies to non-rotating, spherically symmetric objects and does not take into account quantum effects. It also assumes a vacuum environment and does not account for the presence of matter or other forces.

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