Lecture Notes for 120 - UCLA Department of Mathematics
Lecture Notes for 120 - UCLA Department of Mathematics
Lecture Notes for 120 - UCLA Department of Mathematics
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5.1. CURVES ON SURFACES 104<br />
We also restrict the domain to be (µ, ) 2 R =(0, 2⇡) ⇥<br />
⇡<br />
2 , ⇡ 2<br />
and consider a<br />
unit speed curve<br />
q (s) =q (µ (s) ,<br />
(s))<br />
where (µ (s) , (s)) 2 R <strong>for</strong> s 2 [0,L]. The area under consideration will then be<br />
the area bounded by this curve inside this region. We shall further assume that<br />
the curve runs counter clockwise in this region so that S points inwards. Thus the<br />
rotation <strong>of</strong> the curve is 2⇡ if we think <strong>of</strong> it as a planar curve on the rectangle.<br />
We know that<br />
2 3<br />
sin µ<br />
E µ = 4 cos µ 5 = 1 @q<br />
cos @µ = 1 @q<br />
r @µ<br />
0<br />
E<br />
2<br />
= @q<br />
@ = 4<br />
sin cos µ<br />
sin sin µ<br />
cos<br />
3<br />
5<br />
<strong>for</strong>m an orthonormal basis <strong>for</strong> the tangent space at every point so the unit tangent<br />
can be written as<br />
and thus<br />
T = dq<br />
ds = cos (✓ (s)) E µ +sin(✓ (s)) E<br />
S =<br />
sin ✓E µ + cos ✓E<br />
The geodesic curvature can then be computed as<br />
apple g = S · dT<br />
✓<br />
ds<br />
d✓<br />
= S ·<br />
ds S + cos ✓ dE µ<br />
ds +sin✓ dE ◆<br />
ds<br />
= d✓ sin 2 ✓E µ · dE ds<br />
ds + cos2 ✓E · dE µ<br />
ds<br />
= d✓<br />
ds + E · dE µ<br />
ds<br />
2<br />
= d✓<br />
ds + 4<br />
= d✓ dµ<br />
+sin<br />
ds ds<br />
= d✓<br />
ds<br />
dr<br />
d<br />
sin cos µ<br />
sin sin µ<br />
cos<br />
dµ<br />
ds<br />
3<br />
2<br />
5 · 4<br />
We can use Green’s theorem to conclude that<br />
ˆ<br />
ˆ ˆ dr dµ<br />
d ds ds = d2 r<br />
d 2 dµd<br />
cos µ<br />
sin µ<br />
0<br />
3<br />
5 dµ<br />
ds