Re: Mathman or any other math experts...
Now you have the opposite problem -- an overabundance of resources. Two very complete summaries are "The History of Pi" by David Blatner and "The Joy of Pi" by Peter Beckman. Also, as I'm sure you've discovered, just type "History of Pi" into your search engine and you get thousands of hits, lots of them of quality.
Here's an interesting summary of attempts to calculate pi from antiquity to now.
www.cecm.sfu.ca/projects/...story.html
Did you know that you can use Pi to measure the curvature of the universe? (And I mean for real -- this is what astronomers actually do -- not just in theory). If we define Pi to be the ratio of the circumference to the diameter of the circle, then the usual constant Pi that we calculate, Pi = 3.14159..., means that ratio for circles drawn in the flat Euclidean plane.
In a space of positive curvature, the ratio C/D is less than this value, and increasingly less and less as the size of the circle gets bigger. In a negatively curved space, the ratio C/D is larger than this Euclidean vaule of 3.14159....
The formulas relating the Circumference, the Radius, the Cuvature (k), and the Euclidean value of Pi (P) are:
C = 2pr (flat surface)
C =(2p/k)*sin(kr) (surface of positive curvature)
C = (2p/k)*sinh(kr) (surface of negative curvature)
"sin" is the ordinary trigonometric sine function and "sinh" is the "hyperboic sine" function.
So all we have to do to find out if we live in a falt universe or in a universe of negative or positive curvature is to draw a big circle in the sky, measure its circumference and diameter, and see which formula gives the best fit.
Astronomers can estimate the radius by red shift and the circumference by observing density of galaxy clusters.
Say that in your report -- it'll blow your Prof away.:lol:
Mathman
PS. Your signature is funny to me because I often have to do exactly that. I have a slight visual handicap that makes me nervous about turning left. So sometimes I do make three rights.