19.02.2013 Views

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

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

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 ,

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!