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DIFFERENTIAL GEOMETRY: A First Course in Curves and Surfaces

DIFFERENTIAL GEOMETRY: A First Course in Curves and Surfaces

DIFFERENTIAL GEOMETRY: A First Course in Curves and Surfaces

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38 Chapter 2. <strong>Surfaces</strong>: Local Theoryhypothesis, the vectors x u <strong>and</strong> x v are l<strong>in</strong>early <strong>in</strong>dependent <strong>and</strong> must therefore span a plane. Wenow make this an officialDef<strong>in</strong>ition. Let M be a regular parametrized surface, <strong>and</strong> let P ∈ M. Then choose a regularparametrization x: U → M ⊂ R 3 with P = x(u 0 ,v 0 ). We def<strong>in</strong>e the tangent plane of M at P tobe the subspace T P M spanned by x u <strong>and</strong> x v (evaluated at (u 0 ,v 0 )).Remark. The alert reader may wonder what happens if two people pick two different such localparametrizations of M near P .Dothey both provide the same plane T P M? This sort of questionis very common <strong>in</strong> differential geometry, <strong>and</strong> is not one we <strong>in</strong>tend to belabor <strong>in</strong> this <strong>in</strong>troductorycourse. However, to get a feel for how such arguments go, the reader may work Exercise 11.There are two unit vectors orthogonal to the tangent plane T P M. Given a regular parametrizationx, weknow that x u × x v is a nonzero vector orthogonal to the plane spanned by x u <strong>and</strong> x v ;we obta<strong>in</strong> the correspond<strong>in</strong>g unit vector by tak<strong>in</strong>gn =x u × x v‖x u × x v ‖ .This is called the unit normal of the parametrized surface.Example 4. We know from basic geometry <strong>and</strong> vector calculus that the unit normal of theunit sphere centered at the orig<strong>in</strong> should be the position vector itself. This is <strong>in</strong> fact what wediscovered <strong>in</strong> Example 1(d). ▽Example 5. Consider the helicoid given <strong>in</strong> Example 1(b). Then, as we saw, x u × x v =1(b s<strong>in</strong> v, −b cos v, u), <strong>and</strong> n = √u 2 + b (b s<strong>in</strong> v, −b cos v, u). As we move along a rul<strong>in</strong>g v = v 0,2the normal starts horizontal at u =0(where the surface becomes vertical) <strong>and</strong> rotates <strong>in</strong> the planeorthogonal to the rul<strong>in</strong>g, becom<strong>in</strong>g more <strong>and</strong> more vertical as we move out the rul<strong>in</strong>g. ▽We saw <strong>in</strong> Chapter 1 that the geometry of a space curve is best understood by calculat<strong>in</strong>g (atleast <strong>in</strong> pr<strong>in</strong>ciple) with an arclength parametrization. It would be nice, analogously, if we couldf<strong>in</strong>d a parametrization x(u, v) ofasurface so that x u <strong>and</strong> x v form an orthonormal basis at eachpo<strong>in</strong>t. We’ll see later that this can happen only very rarely. But it makes it natural to <strong>in</strong>troducewhat is classically called the first fundamental form, I P (U, V) =U · V, for U, V ∈ T P M.Work<strong>in</strong>g<strong>in</strong> a parametrization, we have the natural basis {x u , x v }, <strong>and</strong> so we def<strong>in</strong>eE =I P (x u , x u )=x u · x uF =I P (x u , x v )=x u · x v = x v · x u =I P (x v , x u )G =I P (x v , x v )=x v · x v ,<strong>and</strong> it is often convenient to put these <strong>in</strong> as entries of a (symmetric) matrix:[ ]E FI P = .F GThen, given tangent vectors U = ax u + bx v <strong>and</strong> V = cx u + dx v ∈ T P M,wehaveU · V =I P (U, V) =(ax u + bx v ) · (cx u + dx v )=E(ac)+F (ad + bc)+G(bd).

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