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4. Assume the universe to be represented by the two-
dimensional surface of a sphere of radius R. A possible
R
coordinate system on the surface is (r,0), where ' is the
length of the geodesic from the north pole and 0 is the angle
measured relative to some arbitrary "prime meridian". The
metric on the surface is given by
ds2 = dr² + R² sin2(r R) do².
(a) Show that the circumference of a circle of radius l' drawn on the sphere has length
C = 2xRsin(r R). Then prove that for r < R this gives the expected Euclidean
result.
(b) Suppose you are located at the North Pole and look at an object of width w
(transverse to your line of sight) at a distance l' from you. Determine the angular
width A0 that the object subtends from your perspective.
A9-
How does this angle compare to the case of a flat surface?
(Hint: Expand the result in a power series in r.)
(c) Assume that "galaxies" are uniformly distributed on the
surface of the sphere with a number density of n galaxies per
unit area. Show that the number of galaxies inside a circle of
radius l' is N = 2xnR² -cos(r/R)
(Hint: Find the infinitesimal element of area on the surface,
and then integrate.) How does this compare with the Euclidean case? (You may again
expand in a power series and/or plot Nvs. l' for both the Euclidean and spherical
cases.)
5. Now, assume that our 3-dimensional space is a hypersphere of radius R described by
the metric ds² = dr² + R² sin2()R)(d02 + sin² edo?
(a) What is the circumference of a circle of radius r? What is the circumference of the
largest circle that can exist in this space?
(b) Based on your results for part (c) of the previous problem, what would you expect
for the number of galaxies inside a sphere of radius ", as compared to the Euclidean
case?

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