A geodesic is a locally length-minimizing curve. Equivalently, it is a path that a particle which is not accelerating would follow. In the plane,
the geodesics are straight lines. On the sphere,
the geodesics are great circles
(like the equator). The geodesics in a space depend on the Riemannian metric, which affects the notions of distance and
acceleration.
Geodesics preserve a direction on a surface (Tietze 1965, pp. 26-27) and have many other interesting properties. The normal
vector to any point of a geodesic arc lies along the normal to a surface at that
point (Weinstock 1974, p. 65).
Furthermore, no matter how badly a sphere is distorted, there exist an infinite number of closed geodesics on it. This general
result, demonstrated in the early 1990s, extended earlier work by Birkhoff, who proved
in 1917 that there exists at least one closed geodesic on a distorted sphere, and
Lyusternik and Schnirelmann, who proved in 1923 that there exist at least three closed
geodesics on such a sphere (Cipra 1993, p. 28).
For a surface given parametrically by , , and , the geodesic can be found by minimizing the arc length
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(1)
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But
and similarly for and . Plugging in,
![I=int{[((partialx)/(partialu))^2+((partialy)/(partialu))^2+((partialz)/(partialu))^2]du^2+2[(partialx)/(partialu)(partialx)/(partialv)+(partialy)/(partialu)(partialy)/(partialv)+(partialz)/(partialu)(partialz)/(partialv)]dudv+[((partialx)/(partialv))^2+((partialy)/(partialv))^2+((partialz)/(partialv))^2]dv^2}^(1/2).](/images/equations/Geodesic/NumberedEquation2.gif) |
(4)
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This can be rewritten as
where
and
Starting with equation (◇)
and taking derivatives,
so the Euler-Lagrange
differential equation then gives
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(16)
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In the special case when , , and are explicit functions
of only,
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(17)
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(18)
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(19)
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![v^'=1/(2R(R-c_1^2))[2Q(c_1^2-R)+/-sqrt(4Q^2(R-c_1^2)^2-4R(R-c_1^2)(Q^2-Pc_1^2))].](/images/equations/Geodesic/NumberedEquation7.gif) |
(20)
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Now, if and are explicit functions
of only and ,
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(21)
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so
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(22)
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In the case where and are explicit functions
of only, then
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(23)
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so
![(partialP)/(partialv)+v^('2)(partialR)/(partialv)-2sqrt(P+Rv^('2))R[(v^(''))/(sqrt(P+Rv^('2)))+(-1/2)(v^'(2Rv^'v^('')))/((P+Rv^('2))^(3/2))]=0](/images/equations/Geodesic/NumberedEquation11.gif) |
(24)
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(25)
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(26)
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(27)
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(28)
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(29)
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and
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(30)
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For a surface of revolution in which is rotated about the x-axis so that the equation of the surface is
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(31)
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the surface can be parameterized by
The equation of the geodesics is then
![v=c_1int(sqrt(1+[g^'(u)]^2)du)/(g(u)sqrt([g(u)]^2-c_1^2)).](/images/equations/Geodesic/NumberedEquation19.gif) |
(35)
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Portions of this entry contributed by Todd
Rowland
Cipra, B. What's Happening in the Mathematical Sciences, Vol. 1.
Providence, RI: Amer. Math. Soc., pp. 21-25, 1993.
Tietze, H. Famous Problems of Mathematics: Solved and Unsolved Mathematics
Problems from Antiquity to Modern Times. New York: Graylock Press, 1965.
Weinstock, R. Calculus of Variations, with Applications to Physics and Engineering.
New York: Dover, 1974.
Weyl, H. Mathematische Analyse des Raumproblems: Was Ist Materie?
Berlin: Wissenschaftl. Buchgesellschaft, 1923.
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