Pi and the curvature of the universe

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Discussion Overview

The discussion revolves around the relationship between the mathematical constant Pi and the curvature of the universe, particularly in the context of measuring geometric properties in curved space-time. Participants explore whether observational evidence exists to suggest that the measured value of Pi differs from its mathematical definition, considering both local and cosmic scales.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants note that Pi is defined as the ratio of a circle's circumference to its radius, and question whether this definition holds true in a universe with curvature.
  • Others argue that Pi is a mathematical construct with a fixed value, and current experimental precision supports its applicability in describing circles in our universe, albeit with measurement errors.
  • A participant suggests that while measurements may not show a difference in Pi, they could be inferred from the angles of large triangles in curved space.
  • Another participant raises the challenge of defining a "straight line" in curved space, questioning the feasibility of measuring distances between celestial bodies due to the effects of gravity on light and material objects.
  • One participant points out that in non-zero curvature scenarios, the relationship between the circumference and radius may not hold, as seen in hyperbolic geometry where the circumference grows exponentially with radius.

Areas of Agreement / Disagreement

Participants generally agree that the mathematical definition of Pi is well-established, but there is no consensus on whether measurements in curved space yield a different value or how such measurements could be accurately made. Multiple competing views remain regarding the implications of curvature on geometric relationships.

Contextual Notes

Limitations include the dependence on definitions of straight lines and circles in curved space, as well as the unresolved nature of how to measure distances accurately in the presence of gravitational effects.

Cato
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The ratio of the circumference of a circle to the radius is Pi. Our value of Pi is an irrational number and is calculated assuming a flat curvature of space-time. But our universe as a whole, while very flat, probably has some small amount of curvature -- in addition to the greater local curvature due to Earth's gravity. Is there any observational evidence suggesting that the actual, measured value of Pi on Earth is different from the calculated value?
 
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The number π, being a mathematical construct, is well defined and has a fixed (irrational) value. The question you might ask yourself is whether it describes the relation between the radius and circumference of a circle in our Universe. To the current experimental precision, it does, but physical measurements always have errors and you can only make statements within these errors.
 
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Orodruin said:
The number π, being a mathematical construct, is well defined and has a fixed (irrational) value. The question you might ask yourself is whether it describes the relation between the radius and circumference of a circle in our Universe. To the current experimental precision, it does, but physical measurements always have errors and you can only make statements within these errors.
Yes, thank you. That is what I was asking -- Have we been able to make any measurements, these would probably have to astronomical in scale, which show that a measured Pi is different from the mathematical construction. So the answer if "no".
 
Yes, the answer is no (although what we are really doing is looking at the angles of really big triangles).
 
Yes, thank you, it makes sense that over enormous scales the angles of a triangle would not add to 180, though making such a measurement might not be possible. Also, I could imagine that on a smaller scale -- orbiting a neutron star, maybe -- the discrepancy might actually be measurable.
 
There are more problems here than you may think. Before we can measure a straight line or circle in "real space", we have to decide what a "straight line" is. For example, how do you imagine a line between, say, two planets? Do you think of some huge "measuring stick"? If so, the is no such thing as a "rigid" material, even theoretically, in relativity so such a "measuring stick" would bend in toward the sun- that would give "hyperbolic" geometry. Or do you think a light beam would make a better "straight line"? Then, sicd light is attracted by the sun, you would have to "aim" the light beams away from the sun so that they will curve back to your target. That would give an "elliptic" geometry.
 
The main problem here is that when you have non-zero curvature, the length of a circle is not proportional to the radius: for example in hyperbolic space the length grows exponentially in radius, so there is no "##\pi##" there.
 

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