Exploring Relativistic Motion: Insights from Special and General Relativity

In summary, rotational motion is different than linear motion in that linear motion causes us to feel dizzy, while rotational motion does not. However, there may be other differences between rotational and linear motion that are yet to be discovered.
  • #1
Naty1
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I've always found rotational motion a little weird...

The "odd" result is that a while a fixed linear force causes steady acceleration and an ever increasing speed with a fixed direction a fixed rotational force causes steady acceleration via a steady change in direction while speed remains constant. And that's because acceleration and velocity vectors are coincident in linear motion and offset 90 degrees with uniform rotational motion.

But as one "silly example" of how they may be different, linear acceleration doesn't make us dizzy and that might hint at some fundamental physical difference.

Are their any other, maybe unique, insights from special or general relativity regarding these two "types" of motion? For example the "equivalence principle" would seem to break down with rotational motion...since I think we'd sure know the difference versus gravitational effects.
 
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  • #2
Naty1 said:
I've always found rotational motion a little weird...

The "odd" result is that a while a fixed linear force causes steady acceleration and an ever increasing speed with a fixed direction a fixed rotational force causes steady acceleration via a steady change in direction while speed remains constant. And that's because acceleration and velocity vectors are coincident in linear motion and offset 90 degrees with uniform rotational motion.

But as one "silly example" of how they may be different, linear acceleration doesn't make us dizzy and that might hint at some fundamental physical difference.

Are their any other, maybe unique, insights from special or general relativity regarding these two "types" of motion? For example the "equivalence principle" would seem to break down with rotational motion...since I think we'd sure know the difference versus gravitational effects.

The gravitational effects of a moving or rotating body include "gravitomagnetism", which is equivalent to a rotating frame of reference and "frame-dragging" effects. "Gravitomagnetism" is related to the ordinary gravitational acceleration field in the same way that magnetism is related to electrostatic fields. In gravity, this is normally an extremely tiny effect, but Gravity Probe B has been attempting to measure it experimentally.
 
  • #3
Here's another insight from Fredrik in another thread:

So why did I say "if the acceleration is linear..."? Because there are situations where it just isn't possible for each microscopic piece to restore itself to its original length in co-moving inertial frames. The simplest example is a rotating disc. When you give a wheel a spin, the material will be forcefully stretched everywhere along the circumference by a factor that exactly compensates for the Lorentz contraction. So in this case we are performing additional work, not to cause the Lorentz contraction but to make sure that lengths remain the same when they do get Lorentz contracted.
 
  • #4
I am unsure of any possible differences between rotational and linear frame dragging, but they might affect light somewhat differently:

(http://en.wikipedia.org/wiki/Frame_dragging)

Rotational frame-dragging (the Lense-Thirring effect) appears in the general principle of relativity and similar theories in the vicinity of rotating massive objects. Under the Lense-Thirring effect, the frame of reference in which a clock ticks the fastest is one which is rotating around the object as viewed by a distant observer. This also means that light traveling in the direction of rotation of the object will move around the object faster than light moving against the rotation as seen by a distant observer. It is now the best-known effect, partly thanks to the Gravity Probe B experiment.

Linear frame dragging is the similarly inevitable result of the general principle of relativity, applied to linear momentum. Although it arguably has equal theoretical legitimacy to the "rotational" effect, the difficulty of obtaining an experimental verification of the effect means that it receives much less discussion and is often omitted from articles on frame-dragging (but see Einstein, 1921).[4]
 
  • #5
Another aspect of rotational versus linear motion in relativity I should have remembered and posted:
Brian Greene's explanation and diagrams showing how we move through spacetime at "c" has interesting visual distinctions between fixed velocity, and linear and rotational acceleration:
Constant velocity is straight line in space time, acceleration is a curve and rotational motion a fixed diameter corkscrew...but I can't see a fundamental insights this provides...maybe more imagination is required! It also provides a rather intuitive insight into why our universe is limited to "c".
 
  • #6

1. What is special and general relativity?

Special and general relativity are theories developed by Albert Einstein to explain the laws of physics in relation to objects moving at high speeds or in the presence of strong gravitational fields. Special relativity deals with the behavior of objects in inertial reference frames, while general relativity extends this to include non-inertial reference frames and gravity.

2. How do special and general relativity impact our understanding of motion?

Special and general relativity have significant implications for our understanding of motion. They show that the laws of physics are the same for all observers in uniform motion, and that the speed of light is constant regardless of the observer's reference frame. Additionally, general relativity explains the effects of gravity on the motion of objects, including the bending of light and the slowing of time in strong gravitational fields.

3. What are some real-life applications of special and general relativity?

Special and general relativity have numerous real-life applications. GPS systems, for example, rely on the precise timing and synchronization of satellites in orbit, which is only possible because of the effects of relativity. Additionally, our understanding of the universe and its origins is heavily influenced by these theories, and they have also been used to make accurate predictions in cosmology and astrophysics.

4. How does time dilation occur in special and general relativity?

Time dilation refers to the slowing of time for an object in motion relative to an observer. In special relativity, time dilation occurs because the speed of light is constant for all observers, so time must adjust to maintain this constant speed. In general relativity, time dilation is caused by the curvature of space-time in the presence of strong gravitational fields.

5. Are there any experimental evidence for special and general relativity?

Yes, there is a large body of experimental evidence that supports special and general relativity. Some famous examples include the Michelson-Morley experiment, which showed the constancy of the speed of light, and the observation of the bending of starlight during a solar eclipse, which confirmed the prediction of general relativity. Furthermore, many technological advancements, such as GPS systems, rely on the principles of relativity and have been proven to be accurate through experimentation.

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