Pi and the curvature of the universe

In summary, the value of Pi is an irrational number used to calculate the circumference of a circle in our universe, assuming a flat curvature of space-time. While our universe is mostly flat, there may be some small amount of curvature, and Earth's gravity also contributes to local curvature. There is no observational evidence suggesting that the calculated value of Pi is different from the actual measured value on Earth, although physical measurements always have errors. Additionally, making measurements on a larger or smaller scale presents challenges due to the concept of a "straight line" in non-zero curvature.
  • #1
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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  • #2
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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  • #3
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".
 
  • #4
Yes, the answer is no (although what we are really doing is looking at the angles of really big triangles).
 
  • #5
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.
 
  • #6
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.
 
  • #7
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.
 

Related to Pi and the curvature of the universe

What is Pi and how is it related to the curvature of the universe?

Pi, also represented by the Greek letter π, is a mathematical constant that represents the ratio of a circle's circumference to its diameter. It is an irrational number, meaning it has an infinite number of decimal places. In the field of cosmology, Pi is used to calculate the curvature of the universe, which is a measure of how the fabric of space curves in the presence of matter and energy.

How is Pi used to determine the curvature of the universe?

In Einstein's theory of general relativity, the curvature of the universe is described by a mathematical equation known as the Einstein field equations. This equation includes a term for the gravitational constant, which is denoted by the letter G, and a term for the energy density of the universe, denoted by the Greek letter ρ. Pi is used to calculate the value of G, which is then used in the equation to determine the curvature of the universe.

What is the significance of the curvature of the universe?

The curvature of the universe is a fundamental property that helps us understand the overall shape and structure of the universe. It can tell us whether the universe is flat, open, or closed, and has implications for the ultimate fate of the universe. A flat universe would continue to expand forever, while a closed universe would eventually collapse in on itself.

Is it possible to measure the curvature of the universe?

Yes, scientists have developed several methods for measuring the curvature of the universe. One method involves studying the cosmic microwave background radiation, which is a remnant of the Big Bang. By analyzing the subtle variations in this radiation, scientists can determine the overall curvature of the universe. Other methods involve studying the distribution of matter and energy in the universe, as well as the large-scale geometry of the universe.

What is the current understanding of the curvature of the universe?

Based on various measurements and observations, the current understanding is that the universe is flat, with a very small amount of positive curvature. This means that the universe will continue to expand forever, but at a gradually decreasing rate. However, there is still ongoing research and debate in the scientific community about the exact value of the curvature and its implications for the fate of the universe.

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