Blaga P. Lectures on the differential geometry of - tiera.ru
Blaga P. Lectures on the differential geometry of - tiera.ru
Blaga P. Lectures on the differential geometry of - tiera.ru
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Examples <strong>of</strong> geodesics<br />
4.19. Geodesics 181<br />
The geodesics <strong>of</strong> <strong>the</strong> plane. By <strong>the</strong> geometrical interpretati<strong>on</strong> <strong>of</strong> <strong>the</strong> geodesics, as<br />
<strong>the</strong> curves that project <strong>on</strong> <strong>the</strong> tangent plane <strong>on</strong> straight lines, we deduce immediately<br />
that <strong>the</strong> geodesics <strong>of</strong> <strong>the</strong> plane are <strong>the</strong> straight lines and <strong>on</strong>ly <strong>the</strong>m. On <strong>the</strong> o<strong>the</strong>r hand,<br />
by using cartesian coordinates, we fined immediately that <strong>the</strong> Christ<strong>of</strong>fel’s coefficients<br />
vanish identically, <strong>the</strong>refore <strong>the</strong> equati<strong>on</strong>s <strong>of</strong> geodesics become<br />
⎧<br />
⎪⎨ u<br />
⎪⎩<br />
′′ = 0<br />
v ′′ ,<br />
= 0<br />
which lead to u(s) = a1s + b1, v(s) = a2s + b2, i.e., again, <strong>the</strong> geodesics are straight lines.<br />
The geodesics <strong>of</strong> <strong>the</strong> sphere. The geodesics <strong>of</strong> <strong>the</strong> sphere can be found very easily<br />
from <strong>the</strong>ir interpretati<strong>on</strong> as being those curves for which <strong>the</strong> osculating plane c<strong>on</strong>tains<br />
<strong>the</strong> normal to <strong>the</strong> surface. As we know, in <strong>the</strong> case <strong>of</strong> <strong>the</strong> sphere all <strong>the</strong> normals are<br />
passing through <strong>the</strong> center <strong>of</strong> <strong>the</strong> sphere, <strong>the</strong>refore <strong>the</strong> osculating planes should pass, all<br />
<strong>of</strong> <strong>the</strong>m through <strong>the</strong> center, which leads immediately to <strong>the</strong> idea that <strong>the</strong> geodesics are<br />
arcs <strong>of</strong> great circles <strong>of</strong> <strong>the</strong> sphere.<br />
Also, using a standard parameterizati<strong>on</strong> <strong>of</strong> <strong>the</strong> sphere (with spherical coordinates),<br />
we can find (do that!) <strong>the</strong> equati<strong>on</strong>s <strong>of</strong> <strong>the</strong> geodesics as:<br />
⎧<br />
⎪⎨ ¨θ − sin θ cos θ ˙ϕ<br />
⎪⎩<br />
2 = 0<br />
.<br />
¨ϕ + 2 cot θ˙θ ˙ϕ = 0<br />
We assume that <strong>the</strong> explicit equati<strong>on</strong> <strong>of</strong> <strong>the</strong> geodesic is θ = θ(ϕ). Then<br />
˙θ = dθ<br />
ds<br />
¨θ = d<br />
ds<br />
dθ<br />
= · ˙ϕ,<br />
dϕ<br />
� �<br />
dθ<br />
· ˙ϕ +<br />
dϕ<br />
dθ dθ<br />
¨ϕ =<br />
dϕ dϕ · ¨ϕ + d2θ dϕ2 · ˙ϕ2 .<br />
Therefore, <strong>the</strong> first equati<strong>on</strong> <strong>of</strong> <strong>the</strong> system becomes:<br />
On <strong>the</strong> o<strong>the</strong>r hand, from <strong>the</strong> first equati<strong>on</strong>,<br />
¨ϕ · dθ<br />
dϕ + d2 θ<br />
dϕ 2 · ˙ϕ2 − sin θ cos θ · ˙ϕ 2 = 0.<br />
¨ϕ = −2 cot θ˙θ · ˙ϕ = −2 cot θ dθ<br />
dϕ · ˙ϕ2 ,