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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

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