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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6.3. ACCELERATION 140<br />
Exercises.<br />
(1) Calculate<br />
6.3. Acceleration<br />
The goal here is to show that the tangential component <strong>of</strong> the acceleration <strong>of</strong><br />
acurveonaparametrizedsurfaceq (u, v) :U ! R 3 can be calculated intrinsically.<br />
The curve is parametrized in U as (u (t) ,v(t)) and becomes a space curve q (t) =<br />
q (u (t) ,v(t)) that lies on our parametrized surface.<br />
The velocity is<br />
˙q = dq<br />
dt = dq<br />
dt = @q<br />
@u<br />
du<br />
dt + @q<br />
@v<br />
dv<br />
dt = ⇥ @q<br />
@u<br />
@q<br />
@v<br />
⇤ apple du<br />
dt<br />
dv<br />
dt<br />
The acceleration can be calculated as if it were a space curve and we explored that<br />
in Chapter 6. Using the velocity representation we just gave and separating the<br />
tangential and normal components <strong>of</strong> the acceleration we obtain:<br />
¨q = ¨q I + ¨q II<br />
= ⇥ @q<br />
@u<br />
@q<br />
@v<br />
⇤<br />
[I]<br />
1 ⇥ @q<br />
@u<br />
@q<br />
@v<br />
⇤ t<br />
¨q +(¨q · N) N<br />
In Chapter 6 we worked with the normal component. Here we shall mostly focus<br />
on the tangential part.<br />
where<br />
Theorem 6.3.1. The acceleration can be calculated as<br />
2<br />
3<br />
¨q = ⇥ @q @q<br />
@u @v<br />
N ⇤ d 2 u<br />
dt<br />
+ u ( ˙q, ˙q)<br />
4<br />
2 d 2 v<br />
dt<br />
+ v ( ˙q, ˙q) 5<br />
2<br />
=<br />
w ( ˙q, ˙q) =<br />
✓ d 2 u<br />
dt 2 +<br />
X<br />
w 1,w 2=u,v<br />
II ( ˙q, ˙q)<br />
◆ ✓ @q d u 2<br />
( ˙q, ˙q)<br />
@u + v<br />
dt 2 +<br />
w dw 1 dw 2<br />
w 1w 2<br />
= ⇥ du<br />
dt dt<br />
dt<br />
◆ @q<br />
v ( ˙q, ˙q) + NII ( ˙q, ˙q) ,<br />
@v<br />
dv<br />
dt<br />
⇤ apple w<br />
uu<br />
w<br />
uv<br />
w<br />
vu<br />
w<br />
vv<br />
apple du<br />
dt<br />
dv<br />
dt<br />
Pro<strong>of</strong>. We start from the <strong>for</strong>mula <strong>for</strong> the velocity and take derivatives. This<br />
clearly requires us to be able to calculate derivatives <strong>of</strong> the tangent fields @q<br />
@u , @q<br />
@v .<br />
Fortunately the Gauss <strong>for</strong>mulas tell us how that is done. This leads us to the<br />
acceleration as follows<br />
¨q = d ✓ ⇥ @q<br />
⇤ apple ◆<br />
du<br />
@q dt<br />
dt<br />
@u @v dv<br />
dt<br />
= ⇥ @q<br />
@u<br />
@q<br />
@v<br />
which after using the chain rule<br />
⇤ " #<br />
d 2 u<br />
dt 2<br />
+<br />
d 2 v<br />
dt 2<br />
✓ d<br />
dt<br />
⇥ @q<br />
@u<br />
d<br />
dt = du @<br />
dt @u + dv @<br />
dt @v<br />
@q<br />
@v<br />
⇤ ◆apple du<br />
dt<br />
dv<br />
dt