# R is a function which is of class C 1. We have already thought about its level sets, sets of the form

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1 Manifolds 1 Chapter 5 Manifolds We are now going to begin our study of calculus on curved spaces. Everything we have done up to this point has been concerned with what one might call the flat Euclidean spaces R n. The objects that we shall now be investigating are called manifolds. Each of them will have a certain dimension m. This is a positive integer that tells how many independent coordinates are needed to describe the manifold, at least locally. For instance, the surface of the earth is frequently modeled as a sphere, a 2-dimensional manifold, with points located in terms of the two quantities latitude and longitude. (This description clearly holds only locally for instance, the north pole is described in terms of latitude = 90 and longitude is undefined there. Further, longitude ranges between 180 and 180, so there s a discontinuity if one tries to coordinatize the entire sphere.) We shall thus be concerned with m-dimensional manifolds M which are themselves subsets of the n-dimensional Euclidean space R n. In almost all cases we consider, m = 1, 2,..., or n 1. There is a case m = 0, but these manifolds are zero dimensional and thus are just made up of isolated points. The case m = n is actually of some interest; however, a manifold M R n of dimension n is just an open set in R n and is therefore essentially flat. M and R n are locally the same in this case. When M R n we say that R n is the ambient space in which M lies. We usually call 1-dimensional manifolds curves, and 2-dimensional manifolds surfaces. But we shall generically use the neutral word manifold. A. Hypermanifolds Assume R n is the ambient space, and M R n the manifold. Given that we are not very interested in the case of n-dimensional M, we distinguish manifolds which have the maximal dimension n 1 and we call them hypermanifolds. IMPLICIT DESCRIPTION. Suppose R n g R is a function which is of class C 1. We have already thought about its level sets, sets of the form M = {x x R n, g(x) = c}, where c is a constant; see p The fundamental thinking here is that in R n there are n independent coordinates; the restriction g(x 1,..., x n ) = c removes one degree of freedom, so that points of M can locally be described in terms of only n 1 coordinates. Thus we anticipate that M is a manifold of dimension n 1, a hypermanifold. A very nice example of a hypermanifold is the unit sphere in R n : S(0, 1) = {x x R n, x = 1}.

2 2 Chapter 5 There is a very important restriction we impose on this situation. It is motivated by our recognition from p that g(x) is a vector which should be orthogonal to M at the point x M. If M is truly (n 1)-dimensional, then this vector g(x) should probably be nonzero. For this reason we impose the restriction that for all x M, g(x) 0. Notice how the unit sphere S(0, 1) fits in this scene. If we take g(x) = x 2, then g(x) = 2x. And this vector is not zero for points in the manifold; the fact that g(0) = 0 is irrelevant, as 0 is not a point of the manifold. We could also use g(x) = x, for which g(x) = x x 1 is never 0. The fact that g is not differentiable at the origin is irrelevant, as the restriction x = 1 excludes the origin. We now present four examples in R 2 showing what sort of things can go wrong in the absence of this assumption. In all these cases we write g = g(x, y), c = 0, and the bad point is located at the origin, so g(0, 0) = 0. EXAMPLE 1. x 3 y 2 = 0: g = (3x 2, 2y). EXAMPLE 2. x 2 + x 3 y 2 = 0: g = (2x + 3x 2, 2y). EXAMPLE 3. x 2 + x 3 y 2 = 0: g = ( 2x + 3x 2, 2y).

3 Manifolds 3 EXAMPLE 4. x 4 y 2 = 0: g = (4x 3, 2y). PROBLEM 5 1. This problem generalizes the situation of the sphere S(0, 1) described above. Let A be an n n real symmetric matrix. Suppose that the set M = {x x R n, Ax x = 1} is not empty. Then M is called a quadric in R n. Prove that it is a hypermanifold. That is, prove that for all x M (Ax x) 0. PROBLEM 5 2. Manifolds do not necessarily have to be curved at all. Thus suppose h R n is not zero, and suppose c R is fixed. Prove that {x x R n, h x = c} is a hypermanifold. PROBLEM 5 3. Suppose the set M = {x x R n, Ax x + h x = c} is not empty. (Here A is an n n real symmetric matrix, h R n is not 0, c is a real number.) Assume that A is invertible and that A 1 h h 4c. Prove that M is a hypermanifold. PROBLEM 5 4. matrix. Prove that Continuing with the preceding situation, assume A is the identity is not a hypermanifold. M = {x x R n, x 2 + h x = h 2 /4} B. Intrinsic gradient warm up In this section the scenario is that of a hypermanifold M R n, where M is described

4 4 Chapter 5 implicitly by the level set g(x) = 0. (We can clearly modify g by subtracting a constant from it in order to make M the zero-level set of g.) We assume g(x) 0 for x M. We are definitely thinking that g(x) represents a vector at x M which is orthogonal to M. We haven t actually defined this notion yet, but we shall do so in Section F when we talk about the tangent space to M at x. We ve discussed this orthogonality on p. 2 43, and it is to our benefit to keep this geometry in mind. A recurring theme in this chapter is the understanding of the calculus of a function M f R. For such a function we do not have the luxury of knowing that f is defined in the ambient space R n. As a result, we cannot really talk about partial derivatives f/ x i. These are essentially meaningless. For instance, consider the unit circle x 2 + y 2 = 1 in R 2 and the function f defined only on the unit circle by f(x, y) = x 2 y. We cannot really say that f/ x = 2x. For we could also use the formula f(x, y) = 1 y 2 y for f, which might lead us to believe f/ x = 0. And anyway, the notation f/ x asks us to hold y fixed and differentiate with respect to x, but holding y fixed on the unit circle doesn t allow x to vary at all. Nevertheless, we very much want to have a calculus for functions defined on M, and at the very least we want to be able to define the gradient of M f R in a sensible way. We shall not succeed in accomplishing this right away. In fact, this entire chapter is concerned with giving such a definition, and we shall finish it only when we reach Section F. However, we want to handle a very interesting special case right away. Namely, we assume R n f R, so that f is actually defined in the ambient R n, and we focus attention on a fixed x M. As such, f(x) R n exists, but this is not what we are interested in. We actually want a vector like f(x) but which is also tangent to M. That is, according to our expectations, which is orthogonal to g(x). Here s a schematic view:

5 Manifolds 5 f ( x ) M x f ( x ) g ( x ) What we can do is orthogonally project f(x) onto the tangent space to M at x, by the simple device of subtracting from f(x) the unique scalar multiple of g(x) which makes the resulting vector orthogonal to g(x): Thus ( f(x) c g(x)) g(x) = 0. c = f(x) g(x) g(x) 2. You should recognize this procedure; it s exactly the theme of Problem 1 12 (see also pp and 15). DEFINITION. The intrinsic gradient of f in the above situation is the vector f(x) = f(x) f(x) g(x) g(x) 2 g(x). An immediate example of interest is the defining function g itself. It clearly satisfies g(x) = 0. PROBLEM 5 5. Prove in fact that if R ϕ R is differentiable, then (ϕ g)(x) = 0.

6 6 Chapter 5 PROBLEM 5 6. More generally, prove this form of the chain rule: (ϕ f)(x) = ϕ (f(x)) f(x). Our notation displays the difference between the intrinsic gradient and the ambient gradient. However, it fails to denote which manifold is under consideration. The intrinsic gradient definitely depends on M. Of course, it must depend on M if for no other reason than we are computing f(x) only if x belongs to M. We illustrate this dependence with the simple EXAMPLE. Let M be the sphere S(0, r) in R n. Then we may use g(x) = x 2 (or x 2 r 2 ), so that g = 2x and we obtain the result f(x) = f(x) x f(x) r 2 x. PROBLEM 5 7. Let f(x, y) = x 2 y and calculate for the manifold x 2 + y 2 = 1 f = x(2y + 1)(y, x). Repeat the exercise for the function h(x, y) = 1 y 2 y, and note that f = h. PROBLEM 5 8. The intrinsic gradient in the preceding problem is zero at which four points of the unit circle? Describe the nature of each of these intrinsic critical points (local maximum, local minimum, saddle point?). Repeat the entire discussion for the function obtained by using the polar angle parameter: f(cos θ, sin θ) = h(cos θ, sin θ) = cos 2 θ sin θ. That is, use single variable calculus and the usual first and second deriative with respect to θ. PROBLEM 5 9. Let 1 i n be fixed and let M be the hyperplane {x R n x i = 0}. Calculate f for this manifold.

7 Manifolds 7 PROBLEM Show that in general f(x) = f(x) sin θ, where θ is the angle between the vectors f(x) and g(x). PROBLEM Prove the product rule: (fh) = f h + h f. EXAMPLE. Let f(x) = x 1 and let M be the unit sphere in R n. Then x 1 f(x) = ê 1 (x ê 1 )x = ê 1 x 1 x = (1 x 2 1, x 1 x 2,..., x 1 x n ). x 1 x 1 Notice that f is quite a bit more complicated in form than f. Also, whereas x 1 = ê 1 is never 0, it is clear that x 1 = 0 is a real possibility. In fact, it is zero at the two points ±ê 1. These happen to be the two points of the sphere where the function x 1 attains its extreme values. Another way of phrasing the definition of the intrinsic gradient is to let ˆN denote a unit vector at x which is orthogonal to M. (What this means precisely will be discussed later.) Then we expect that g(x) = c ˆN for some real c 0, so that f(x) = f(x) f(x) ˆN ˆN. PROBLEM Let M be a 1-dimensional manifold (a curve ) in R 2. Let ˆT be a unit vector tangent to M at x, and prove that f(x) is related to the directional derivative of f by the formula f(x) = Df(x; ˆT ) ˆT.

8 8 Chapter 5 PROBLEM Suppose R n f R is homogeneous of degree a. For the manifold which is the sphere S(0, r) of radius r show that f = f afx r 2. Another extremely important property is the fact that f is truly intrinsic: it depends only on the knowledge of f when restricted to the manifold. This is not quite clear at the present stage of our development because we have employed the ambient gradient f in our definition. However, the following argument should serve to make it intuitively clear. In order that f just depend on the function f restricted to M, it must be the case that two functions which are equal on M turn out to have the same intrinsic gradient. Equivalently, their difference has zero intrinsic gradient. Equivalently, if f = 0 on M, then f = 0 on M. This seems reasonable, as we believe that if M is a level set of f, then f must be orthogonal to M; that is, f is a scalar multiple of g. But then the orthogonal projection of f orthogonal to g is zero: f = 0. Rather than continuing with this discussion at the present time, we instead turn to some wonderful numerical calculations. C. Intrinsic critical points We continue with the notation and ideas of Section B, so that M is a hypermanifold in R n described by an equation g(x) = 0. We say that x M is an intrinsic critical point of f if f(x) = 0. That is, f(x) g(x) f(x) = g(x). g(x) 2 This is a rather daunting equation to solve for x, but it helps to notice that it says precisely that f(x) equals a scalar times g(x); for then taking the inner product with g(x) shows that the scalar must be the one displayed. This scalar λ is called a Lagrange multiplier for the problem. We then are required to solve the equations { f(x) = λ g(x), g(x) = 0 (as x M). The unknowns are both x and λ. If we count scalar unknowns and equations, we have n + 1 unknowns x 1,..., x n, λ, as well as n + 1 equations. Hopeful! The equation g(x) = 0 is often referred to as the constraint.

9 Manifolds 9 As is usual in similar situations, setting up the equations is the easy part. Solving them is the hard part, as they are usually nonlinear. Here are some examples. EXAMPLE. Find the intrinsic critical points of f(x, y) = x(y 1) on the unit circle x 2 + y 2 = 1. Solution. To eliminate some 2 s we can use g(x, y) = 1 2 (x2 + y 2 1). Then the Lagrange formulation is: { (y 1, x) = λ(x, y), Thus y 1 = λx and x = λy. Thus x 2 + y 2 = 1. y 1 = λ 2 y, so Thus Finally, the constraint gives Thus y = y(λ 2 1) = 1. 1 λ 2 1, x = λ λ 2 1. λ (λ 2 1) 2 = 1. λ = (λ 2 1) 2 = λ 4 2λ 2 + 1; λ 4 = 3λ 2. Thus λ = 0 or λ 2 = 3. These give three points: λ = 0 : (0, 1); λ = ( ) 3 3 : 2, 1 ; 2 λ = ( ) 3 3 : 2, 1. 2 Here s a sketch, together with the evident natures of the critical points relative to M:

10 10 Chapter 5 f = 0 SADDLE f = MAX MIN f = Notice, by the way, that (0, 1) is actually an ambient critical point of f: f(0, 1) = (0, 0). It is the only one. PROBLEM Just as in Problem 5 8, analyze the function we just studied by examining the function cos θ(sin θ 1). EXAMPLE. Find the intrinsic critical points of f(x, y) = x 3 + 8y on the ellipse x 2 + y2 = Solution. The Lagrange formulation is: 3x 2 = λx/2, 8 = λy, x 2 + y2 = If x = 0, we get y 2 = 2 and thus two points: (0, 2), (0, 2). If x 0, then x = λ 6, y = 8 λ.

11 Manifolds 11 Thus xy = 4/3, so the constraint gives x ( ) 2 4 = 1; 2 3x x = 1; 9x 2 9x = 36x 2 ; 9x 4 36x = 0; (3x 2 4)(3x 2 8) = 0; x 2 = 4/3 or 8/3. ( ) ( 4 Thus we find four more points: ±, 4 8 and ±, intrinsic critical points: 2 3 ). Here is a sketch of the six GLOBAL MAX LOCAL MIN LOCAL MAX LOCAL MIN LOCAL MAX GLOBAL MIN In both of the above examples we drew conclusions about intrinsic extreme values; that is, maximum and minimum values of the relevant function s restriction to the manifold. We shall prove in Section E that such intrinsic extreme values are indeed intrinsic critical points, just as in the case of functions defined on R n (see Section 2G). It is quite interesting to consider the special case of quadratic forms, as we did in proving the principal axis theorem in Chapter 4. So let A be an n n symmetric real matrix. We

12 12 Chapter 5 there were analyzing A by means of the Rayleigh quotient Ax x x 2, and we essentially found its critical points in R n. The homogeneity shows that to be the same as finding the intrinsic critical points of Ax x on the unit sphere. Thus we ask for points x satisfying (Ax x) = 0 and x = 1. The Lagrange formulation gives That is, { Ax { (Ax x) = λ ( x 2 ), x = 1. = λx, x = 1. Thus the intrinsic critical points of Ax x on the unit sphere are precisely the eigenvectors of A! As an example of this procedure, work out the following problem: PROBLEM sphere x 2 + y 2 + z 2 = 1. Find the intrinsic critical points of (x + y)(y + z) on the unit PROBLEM For the Rayleigh quotient function Q(x) = Ax x/ x 2 show that the intrinsic gradient on the unit sphere equals Q = Q = 2Ax 2Ax xx. Here are six more or less routine exercises, followed by six challenging ones. PROBLEM Use the Lagrange technique to find the points on the parabola y 2 + 2x = 8 which are closest to the origin. PROBLEM Find the minimum of x 4 +4axy +y 4 on the hyperbola x 2 y 2 = 1.

13 Manifolds 13 PROBLEM Find the minimum distance from (9, 12, 5) to points on the cone in R 3 given by 4z 2 = x 2 + y 2. PROBLEM Consider the function f(x, y) = x on the level set y 2 x 3 = 0. Show that f attains its minimum value at the origin only. Show that the Lagrange formulation fails to produce this result. Explain why. PROBLEM Repeat the preceding exercise for the function f(x, y) = y on the set M : y 3 = x 6 + x 8. In this case show also that the level set M is a bona fide 1-dimensional manifold in R 2. PROBLEM Let a, b, c be positive constants. Find the intrinsic critical points of a + b + c on the unit sphere x y z x2 + y 2 + z 2 = 1. PROBLEM Find the intrinsic critical points of 2(x 1 + x 2 + x 3 )(x 1 + x 2 + x 4 ) on the unit sphere in R 4. PROBLEM Find all the intrinsic critical points of f(x) = x 3 1+x 3 2+x 3 3+2x 1 x 2 x 3 on the unit sphere in R 3. PROBLEM 5 25*. Find all the intrinsic critical points of f(x) = x 3 1+x 3 2+x 3 3 3x 1 x 2 x 3 on the unit sphere in R 3. PROBLEM 5 26**. Let a be an arbitrary but fixed real number. Find all the intrinsic critical points of f(x) = x x x ax 1 x 2 x 3 on the unit sphere in R 3, and count how many there are depending on the value of a. PROBLEM Find all the intrinsic critical points of f(x) = x x x 3 on the unit sphere in R 3. Determine the maximum and minimum values of f on the sphere. The next problem is a gem I found in the book Ideals, Varieties, and Algorithms, by Cox,

14 14 Chapter 5 Little, and O Shea. (David Cox is a 1970 BA Rice, majoring in mathematics, and is now on the faculty of the Department of Mathematics, Amherst College). PROBLEM 5 28*. Find all the intrinsic critical points of f(x) = x x 1 x 2 x 3 x 2 3 on the unit sphere (there are ten), and the maximum and minimum values as well. PROBLEM 5 29*. Consider the ellipse x2 + y2 = 1 where 0 < b < a. For any a 2 b 2 point (x, y) on the ellipse construct the line through that point which is orthogonal to the ellipse. This line intersects the ellipse in another point (x, y ). Let D(x, y) denote the distance between (x, y) and (x, y ). Find the minimum value of this function by first showing that x2 2( + y2 ) 3/2 a 4 b 4 D(x, y) = x 2 a 6 + y2 b 6 and then using the Lagrange technique to minimize D(x, y). (Answer includes D= 27a 2 b 2 (a 2 +b 2 ) 3/2 in case a 2b.) D. Explicit description of manifolds Frequently hypermanifolds in R n are described in terms of graphs of functions R n 1 ϕ R. This means that on the manifold one of the coordinates in R n is expressed explicitly as a function of the other n 1 coordinates. As there is no particular coordinate to prefer over another, we shall with no loss of generality consider the abstract situation in which M is represented by a formula x n = ϕ(x 1,..., x n 1 ). Of course, M may then be thought of as represented implicitly in terms of the zero level set of R n g R, where we simply define the new function g by The normal vector is then given by Notice that g is definitely not zero! g(x) = x n ϕ(x 1,..., x n 1 ). g = ( D 1 ϕ,..., D n 1 ϕ, 1) = ( ϕ, 1) (for short).

15 Manifolds 15 Now we give an interesting calculation to show what f looks like in this framework. We shall require only the values of the function f on the manifold M. A convenient way to use these values is to define an associated function f 0 on R n 1 by the formula f 0 (x 1,..., x n 1 ) = f ( x 1,..., x n 1, ϕ(x 1,..., x n 1 ) ). Notice that the new function f 0 indeed uses only the evaluation of f at points of M. Note first that the chain rule implies Using vector notation in R n 1, D k f 0 = D k f + D n fd k ϕ, 1 k n 1. f 0 = (D 1 f 0,..., D n 1 f 0 ) = (D 1 f,..., D n 1 f) + D n f(d 1 ϕ,..., D n 1 ϕ). Now we simply regard f 0 as a vector in R n with n th component 0, which we write as Thus 0 = D n f + D n f( 1). f 0 = (D 1 f,..., D n 1 f, D n f) + D n f(d 1 ϕ,..., D n 1 ϕ, 1) = f + D n f( ϕ, 1) = f D n f g. Now we are all set to compute the intrinsic gradient of f. By definition We summarize: f = f f g g 2 g = f ( f 0 + D n f g) g g 2 = f f 0 g g 2 = f 0 f 0 g g 2 g D n f g g. g

16 16 Chapter 5 THEOREM. In the above context, where M is given explicitly we define Then M = {x R n x n = ϕ(x 1,..., x n 1 )}, f 0 (x 1,..., x n 1 ) = f ( x 1,..., x n 1, ϕ(x 1,..., x n 1 ) ). f = f 0 + f 0 ϕ ϕ ( ϕ, 1). In particular, the intrinsic gradient f depends only on the restriction of f to M. This theorem is of great theoretical importance in that it shows dramatically the intrinsic nature of f. However, it does not appear to be of any particular use in solving exercises, as the Lagrange formulation of the preceding section is indeed quite applicable. PROBLEM Prove that f has an intrinsic critical point at x f 0 has a critical point at the corresponding point. E. Implicit function theorem We now turn to a theorem of immense importance in the study of manifolds. It actually provides the complete understanding of intrinsic gradients. More than that, it shows that hypermanifolds which are described implicitly can also be described explicitly. Thus it is well named: THE IMPLICIT FUNCTION THEOREM. We do not prove this theorem (one of the hard ones) in this course. It is commonly proved in beginning courses in mathematical analysis. However, we very much need to understand exactly what it does (and does not) say. Suppose then that the hypermanifold M R n is described implicitly in a neighborhood of x 0 M by the equation g(x) = 0. As usual, R n g R is assumed to be of class C 1, and g(x) 0 for all x in a neighborhood of x 0. We want to describe M explicitly near x 0, so what we need to do is solve the equation g(x) = 0 for one of the variables in terms of the others. Say we succeed in solving for x n as a function of x 1,..., x n 1 : in a neighborhood of x 0 we then have a situation g(x) = 0 x n = ϕ(x 1,..., x n 1 ), for some function ϕ defined on a neighborhood in R n 1.

17 Manifolds 17 It is surely reasonable to expect that we need a condition like g/ x n 0 in order to do this. At the very least, we need g(x 1,..., x n ) to involve x n in a significant way. Furthermore, the manifold x n = ϕ(x 1,..., x n 1 ) has the normal vector ( ϕ, 1) with nonzero n th coordinate, and thus the normal vector g should also have a nonzero n th coordinate. As a simple example take g(x) = x 2 1, so that we are dealing with the all-important unit sphere as M. Then g(x) = 2x. Solving g(x) = 0 goes something like this: x 2 n = 1 x 2 1 x 2 n 1 x n = ± 1 x 2 1 x 2 n 1. The choice of sign gives the upper or lower hemisphere. x n = 1 x x 2 n 1 x n x 1,..., x n 1 x n = 1 x x 2 n 1 We see one thing immediately: we cannot in general expect the explicit presentation of M to be anything but local. We also are going to want ϕ to belong to class C 1 so that we can do calculus. In this example this C 1 quality will not happen if x x 2 n 1 = 1 (the equator x n = 0). Now suppose x 0 S(0, 1) and its n th coordinate x on 0. Then g(x 0 ) = 2x 0 0. Furthermore, we can solve for x n near x 0. If x on > 0, we obtain the + sign above, and the

18 18 Chapter 5 reverse if x on < 0. Thus in the latter case x on < 0, we have = 1 x 2 1 x 2 n 1 for x x 2 n 1 < 1. x n Of course, the entire sphere can be handled in a similar way since g(x 0 ) = 2x 0 0 requires some coordinate x oi of x 0 to be nonzero, and we can then solve for x i locally: x i = ± 1 x 2 1 x 2 i 1 x2 i+1 x2 n. The above simple example of the sphere is completely typical. Here is the result. IMPLICIT FUNCTION THEOREM. Suppose the hypermanifold M R n is described as the level set g(x) = 0, g where R n R is of class C 1 and g 0 on M. Suppose x 0 M. Suppose that g/ x i (x 0 ) 0. Then there exists R n 1 ϕ R of class C 1 such that for all x in a sufficiently small neighborhood of x 0, g(x) = 0 x i = ϕ(x 1,..., x i 1, x i+1,..., x n ). Though this is an existence theorem and as such does not provide a clue about the actual calculation of ϕ, the chain rule gives explicit formulas for the partial derivatives of ϕ. For we may start with the functional identity in the variables x 1,..., x i 1, x i+1,..., x n : g(x 1,..., x i 1, ϕ, x i+1,..., x n ) = 0. Now differentiate this identity with respect to x j for any j i. The chain rule implies Therefore we conclude that D j g + D i gd j ϕ = 0. D j ϕ = D jg D i g. On the right side of the latter equation, the partial derivatives of g are evaluated at x i = ϕ. Notice the appearance of the nonzero quantity D i g in the denominator. There is a nice moral to get from all of this. Solving the equation g(x) = 0 for x i in terms of the other coordinates is likely to be a very difficult task. But once that has been done and the above function ϕ has been produced, the calculation of the partial derivatives D j ϕ is very simple. In fact, it s a linear task. You have seen this sort of implicit differentiation in your

19 Manifolds 19 introductory calculus courses. For instance there are lots of exercises of the following nature: the equation πe xy + sin y y x 2 = 0 is satisfied by a function y = y(x) near x = 0, and y(0) = π. Compute dy/dx. The solution is obtained by performing d/dx: ( πe xy x dy ) dx + y + cos y dy dx dy 2x = 0. dx Then solve: dy dx = 2x πye xy πxe xy + cos y 1. How simple. (Never mind that we don t really know the terms y = y(x) on the right side.) Notice that when x = 0 and y = π, the denominator equals 2 and this is not 0. In particular, dy dx x=0 = π2 2. Another nice result of the implicit function theorem is the proof that the intrinsic gradient f depends only on M and not on the particular function g whose level set is equal to M. This is clear once we check that g is uniquely determined by M, up to a nonzero scalar multiple; for the formula for f shows that the scalar multiple cancels out of the equation. More geometrically, f is just the vector f with the correct multiple of g added so that the resulting vector is orthogonal to g; this makes it clear that only the direction of g is needed. THEOREM. Given a hypermanifold M R n, suppose it is described as the level set {x R n g(x) = 0}, where g 0. Then g is uniquely determined by M, up to a nonzero scalar multiple (which may be a function of x). PROOF. Suppose for instance that D n g(x 0 ) 0. Then the implicit function theorem yields a function R n 1 ϕ R such that near x 0 we have Then as above we obtain on M x M x n = ϕ(x 1,..., x n 1 ). D j g + D n gd j ϕ = 0, 1 j n 1. We conclude g = D n g( ϕ, 1).

20 20 Chapter 5 If another function g also gives the manifold, and g(x 0 ) 0, then g(x 1,..., x n 1, ϕ(x 1,..., x n 1 )) = 0 so that the chain rule again gives g = D n g( ϕ, 1). Thus D n g(x) 0 and g(x) =scalar times g(x). QED We can now clear up an issue that we have been ignoring, thanks to the fact that we understand that the intrinsic gradient f is completely determined by the restriction of the function f to the manifold in question. The issue is this: suppose f attains a local maximum or minimum value at x 0 M relative to the restriction of f to M. Then we want to know that necessarily x 0 is an intrinsic critical point of f. Here s the result: THEOREM. Suppose M is a hypermanifold in R n and suppose R n f R is a C 1 function defined in a neighborhood of a point x 0 M. Suppose that f(x) f(x 0 ) for all x M belonging to some neighborhood of x 0. Then f(x 0 ) = 0. PROOF. Thanks to the implicit function theorem, we know that M can be represented explicitly near x 0 by an equation of the form x n = ϕ(x 1,..., x n 1 ) (we have named x n as the distinguished coordinate for simplicity of writing only). We use the function f 0 of Section D, f 0 (x 1,..., x n 1 ) = f(x 1,..., x n 1, ϕ(x 1,..., x n 1 )). Let x 0 = (x 01,..., x 0,n 1 ). Then our hypothesis means precisely that f 0 (x ) f 0 (x 0) for all x R n 1 sufficiently near x 0. Thus x 0 is a critical point for the function f 0, and we conclude that its gradient f 0 (x 0) = 0. But then the theorem on p yields f(x 0 ) = f 0 + f 0 ϕ ϕ = 0. ( ϕ, 1) QED

21 Manifolds 21 REMARKS. Of course, the conclusion still holds if we are dealing with a local minimum instead: f(x) f(x 0 ) for all x M sufficiently near x 0. In the next section we shall give a somewhat different proof of this result that is even more intrinsic. And in Section G we shall learn that the theorem remains valid for manifolds M R n of any dimension, not just n 1. PROBLEM THE ARITHMETIC-GEOMETRIC MEAN INEQUALITY. Using the following outline, prove that for any x 1 0,..., x n 0, and that equality holds x 1 = = x n. (x 1... x n ) 1/n x x n, n a. Prove first that you may assume that x x n = 1. b. Show that the function f = x 1... x n restricted to the set x x n = 1, x i 0 for all i, attains its maximum value at some x 0. c. Show that all the coordinates of this point x 0 are positive. d. Use the Lagrange technique to determine x 0. PROBLEM Find the minimum of x 1 x 2... x n subject to the constraint 1 x x x n = 1, all x i > 0. F. The tangent space Now we are going to face the problem of actually defining tangent vectors to a manifold. Suppose that M R n is a manifold, not necessarily a hypermanifold. Suppose x 0 M. We want to give a definition of tangent vectors to M at x 0 that is as intrinsic to M as possible (how the inhabitants of M view tangent vectors). We shall accomplish this by focusing attention on curves which lie in the manifold. DEFINITION. In the above situation consider all curves (see p. 2 3) γ from R to R n which

22 22 Chapter 5 satisfy the following: γ(t) M for all t, γ(0) = x 0, γ is of class C 1. Then the velocity vector γ (0) is called a tangent vector to M at x 0. Notice that γ (0) R n. The set of all such vectors is called the tangent space to M at x 0, and is written T x0 M.

23 Manifolds 23 PROBLEM ch T x0 M. (HINT: γ(ct).) Prove that 0 T x0 M and that if h T x0 M and c R, then γ (0) γ ( t ) T x0 M M We anticipate that if M is an m-dimensional manifold, then T x0 M is an m-dimensional subspace of R n. The preceding problem indeed shows that scalar multiples of tangent vectors at x 0 are themselves tangent vectors at x 0, but no such simple technique will handle sums of tangent vectors. We shall prove all these results when we come to Chapter 6. (Though T x0 M is a subspace of R n and contains the origin, we always imagine this subspace attached to M at the point x 0, with the origin in T x0 M being regarded as located at x 0.) For the present time we continue to focus our attention on the hypermanifold case with a theorem that reveals all we really need to know about T x0 M in this case. THEOREM. Let M be a hypermanifold in R n, described implicitly as a level set g(x) = 0, where g is of class C 1 and g 0 on M. Let x 0 M. Then T x0 M = {h R n g(x 0 ) h = 0}. In particular, T x0 M is an (n 1)-dimensional subspace of R n.

24 24 Chapter 5 PROOF. First, suppose h T x0 M. Use a curve γ as in the definition above, with γ (0) = h. Then since γ(t) M, g(γ(t)) = 0. Computing the t derivative and using the chain rule, g(γ(t)) γ (t) = 0. Setting t = 0, g(x 0 ) h = 0. Conversely, suppose h R n satisfies g(x 0 ) h = 0. Now we have to do something quite significant. We are required to produce a curve in M with all the right properties. Since we don t even know how to produce individual points in M, much less a whole curve, we need a theorem of some sort. The implicit function theorem serves the purpose perfectly. For ease in writing let us suppose D n g(x 0 ) 0. Then we know (thanks to the implicit function theorem) that M can be described explicitly as a graph x n = ϕ(x 1,..., x n 1 ) near x 0. Write x 0 = (x 01,..., x 0n ). We then define a curve γ(t) by making it affine in the independent coordinates x 1,..., x n 1 in the following way: γ j (t) = x 0j + h j t, 1 j n 1, γ n (t) = ϕ (γ 1 (t),..., γ n 1 (t)). From the chain rule and the formula on p we obtain γ n(0) = = n 1 D j ϕ (x 01,..., x 0,n 1 ) γ j(0) j=1 n 1 j=1 D jg(x 0 ) D n g(x 0 ) h j. But also we have g(x 0 ) h = 0;

25 Manifolds 25 that is, Thus n 1 D j g(x 0 )h j + D n g(x 0 )h n = 0. j=1 γ n(0) = h n. This proves that γ (0) = h, as desired. QED As a nice bonus, we can now easily give a complete understanding of the intrinsic gradient of a function, relative to the hypermanifold M. Suppose first that R n f R is of class C 1 near a point x 0 M. Suppose that h T x0 M. There are now two ways to view this situation. (1) We use g(x 0 ) h = 0 and the definition from p. 5 5, to conclude that f(x 0 ) = f(x 0 ) f(x 0) g(x 0 ) g(x 0 ) 2 g(x 0 ), f(x 0 ) h = f(x 0 ) h = Df(x 0 ; h). Remember from p that Df(x 0 ; h) is our notation for the directional derivative of f at x 0 in the direction h. Thus f(x 0 ) is the unique vector in T x0 M whose inner product with every h T x0 M equals Df(x 0 ; h). (2) Consider an arbitrary curve γ in M such that γ(0) = x 0 and γ (0) = h. Then the chain rule gives d dt f (γ(t)) = f (γ(t)) γ (t), so that d dt f (γ(t)) t=0 = f(x 0 ) h = f(x 0 ) h. It is this second relationship that is so intriguing, since the function f γ depends on the behavior of f only on the manifold M and not on the ambient R n. We can therefore extend the definition of p. 5 5 as in the theorem we are preparing to consider.

26 26 Chapter 5 But before we state the theorem, we need to explain part of the hypothesis. Namely, we are going to assume that M f R is of class C 1. Since f might be defined only on M, it is not immediately clear how to define this continuous differentiability. In fact, a moment s thought might lead to two competing ideas: (1) Representing M in an explicit manner such as require the resulting function x n = ϕ(x 1,..., x n 1 ), f 0 (x 1,..., x n 1 ) = f(x 1,..., x n 1, ϕ(x 1,..., x n 1 )) to be of class C 1 on (a neighborhood in) R n. (2) Require that there exist a C 1 function R n F R such that F (x) = f(x) for x M (in a neighborhood of some point). PROBLEM Prove that these two definitions are equivalent. THEOREM. Let M be a hypermanifold in R n and x 0 M. Let M f R be a C 1 function defined only on M. Then there exists a unique vector f(x 0 ) in T x0 M such that for all C 1 curves γ in M such that γ(0) = x 0, d dt f (γ(t)) t=0 = f(x 0 ) γ (0). DEFINITION. The tangent vector f(x 0 ) is called the intrinsic gradient of f at x 0. Because of the discussion right before the theorem, it agrees with the definition given on p. 5 5 in case f is defined in a neighborhood of x 0 in R n. PROOF. Use the second of the two definitions of C 1 given above. Thus in a neighborhood of x 0 there exists some C 1 function R n F R which agrees with f on M. Then we simply compute d dt f (γ(t)) t=0 = d dt F (γ(t)) t=0 = F (x 0 ) γ (0),

27 Manifolds 27 thanks to the known properties of the intrinsic gradient F (x 0 ) of the ambient function F. This finishes the existence part of the proof, as we may simply define f(x 0 ) = F (x 0 ). The uniqueness is a separate argument. If there were two vectors v and w T x0 M fulfilling the conclusion of the theorem, then we would have Thus, v γ (0) = w γ (0) for all curves γ. (v w) h = 0 for all h T x0 M. Since v w T x0 M, we conclude that v w = 0. Thus v = w. QED REMARK. Given a C 1 function M f R, there are many ways to extend it to R n F R in a neighborhood of x 0. Each such F has a gradient F (x 0 ), but the intrinsic gradient F (x 0 ) is independent of the choice of the extension F. Our results show that each F (x 0 ) is just equal to f(x 0 ). Thus we have a very practical algorithm for computing f. Namely, first extend f to an ambient C 1 function F ; second, compute F. The resulting vector is precisely f. The above results are in agreement with what we accomplished in the theorem on p. 5 15, where we noticed that the intrinsic gradient of a function depends only on its restriction to the manifold. The extra information we now have comes from the intrinsic understanding of tangent vectors themselves. G. Manifolds that are not hyper In this section we want to move away from the restriction that M R n has dimension n 1. Thus we shall study manifolds of dimension m contained in R n, where 1 m n 1. This range of dimension covers all that we are really concerned with in the present chapter, going from m = 1 ( curves ) to m = 2 ( surfaces ) on up to m = n 1 (hypermanifolds). We do not deal with m = 0, as 0-dimensional manifolds would just consist of isolated points in R n, and no actual calculus could be done. At the other extreme, m = n, we would be talking about n-dimensional manifolds contained in R n and these are simply open subsets of R n. This leads essentially to the flat calculus we have studied in detail in Chapters 2 4 and presents no new ideas at the present time. Again we shall use both an implicit presentation and an explicit presentation of M. In addition we shall also consider a third method, a parametric presentation. Here is a preliminary summary: IMPLICIT M is defined by n m constraints placed on the points of R n.

28 28 Chapter 5 EXPLICIT M is defined by giving n m coordinates of R n as explicit functions of the other m coordinates. PARAMETRIC M is defined by describing its points as a function of m other real variables (called parameters). We devote the rest of this section to the discussion of three examples which happen to be quite interesting manifolds. EXAMPLE 1. M is the ellipse x2 1 + x2 a 2 2 = 1 in the x b 2 1 x 2 plane, but thought of as lying in R 3. (The semiaxes a and b are arbitrary positive numbers.) As M is surely a 1-dimensional manifold, we have m = 1 and n = 3. Implicitly, M = {x R 3 x2 1 a 2 + x2 2 b 2 = 1, x 3 = 0}. Explicitly, we solve the constraint equations near a point of M; for instance, near the point ( a, 0, 0) we can write x 1 = a 1 x2 2 b 2, x 3 = 0. Parametrically, we can express M = {(a cos t, b sin t, 0) 0 t 2π}; thus all three coordinates are given as functions of the single parameter t. PROBLEM Given the ellipse above, suppose 0 < b < a. Through any point on the 0, ellipse draw the straight line which is orthogonal to the ellipse. This straight line contains a point ( a, 0 ) which is closest to the origin; let D be the corresponding distance between this point and the origin. Find a point on D the ellipse which produces the maximum D, and compute this maximum value. ( b ) ( 0, b) ( a, 0)

29 Manifolds 29 PROBLEM Continue with the same ellipse. Through any point on it and in the first quadrant, draw the straight line which is tangent to the ellipse. This line contains a line segment whose end points lie on the coordinate axes. Let L be the length of this segment. Find a point on the ellipse which produces the minimum L, and compute this minimum value. L PROBLEM In the preceding problem calculate the lengths of the two indicated line segments which constitute the optimal L, and show that they are a and b. (Do you see a simple geometric reason for this outcome?) EXAMPLE 2. Torus of revolution. This is obtained by revolving a circle in R 3 about an axis disjoint from it. We arrange things as in the illustration: The circle in the x z plane is z described as (x b) 2 + z 2 = a 2, where 0 < a < b. b a b b + a x Now revolve this around the z-axis. Starting with a point (x, 0, z) on the circle produces points (x, y, z) R 3 for which x 2 + y 2 = x. Thus the equation of the resulting surface is ( ) 2 x2 + y 2 b + z 2 = a 2. Implicit presentation.

30 30 Chapter 5 Of course, m = 2 and n = 3. We can also give a parametric presentation using two angles. The first angle ψ can parametrize the circle in the x z plane in the usual polar coordinate way: x = b + a cos ψ, z = a sin ψ. To get the revolved surface, we leave z alone, but use b + a cos ψ as the distance from the z-axis. If we have revolved through the angle θ, the x, y coordinates are then x = (b + a cos ψ) cos θ, y = (b + a cos ψ) sin θ. Thus we have x = (b + a cos ψ) cos θ, y = (b + a cos ψ) sin θ, Parametric presentation. z = a sin ψ.

31 Manifolds 31 PROBLEM Consider the given implicit presentation of the torus of revolution. The point (b + a, 0, 0) lies on this torus. Show that near this point the torus has the explicit presentation x = ( b + a 2 z 2 ) 2 y2. Show that the maximal region in the y z plane for which this representation is valid has the shape: (0, α ) semicircle (0, 0) ( β, 0 ) ( γ, 0 ) What are α, β, and γ? In a certain sense this torus of revolution can be thought of as the Cartesian product of two circles, as two independent periodic coordinates ψ, θ are used in its presentation. However, it is not really a Cartesian product. There does exist a very interesting surface, a 2-dimensional manifold, which is actually the Cartesian product of two circles. As each circle is contained in R 2, the Cartesian product we are going to exhibit is contained in R 2 R 2 = R 4. This manifold is often called a flat torus: EXAMPLE 3. Just as R 4 is the Cartesian product R 2 R 2 of two planes, this 2-dimensional manifold M is literally the Cartesian product of two circles: M = {(x 1, x 2, x 3, x 4 ) x x 2 2 = 1, x x 2 4 = 1}. Implicit presentation. We can use the polar coordinates for the two unit circles to write the points of M in the form x 1 = cos θ 1, x 2 = sin θ 1, Parametric x 3 = cos θ 2, presentation. x 4 = sin θ 2.

32 32 Chapter 5 In a very definite sense to be explained later, this manifold is flat, unlike the torus of revolution. At any fixed point x M, we can find two linearly independent vectors orthogonal to M, using the implicit presentation; and two linearly independent vectors tangent to M, using the parametric presentation. Namely, orthogonal vectors can be found by using the gradients of the two defining functions: (x 1, x 2, 0, 0) and (0, 0, x 3, x 4 ). And tangent vectors can be found by using the partial derivatives x/ θ i of the parametrizations: ( sin θ 1, cos θ 1, 0, 0) and (0, 0, sin θ 2, cos θ 2 ). Thus we can split R 4 into the 2-dimensional space orthogonal to M at x plus the 2-dimensional space tangent to M at x. We have just found the relevant orthonormal sequence: } (x 1, x 2, 0, 0) (0, 0, x 3, x 4 ) orthogonal to M, } ( x 2, x 1, 0, 0) (0, 0, x 4, x 3 ) tangent to M. Incidentally, we draw no pictures of the flat torus. It cannot be located in R 3, whereas the torus of revolution is a hypermanifold in R 3. Thus it gives us an interesting example of a 2-dimensional manifold in R 4 which is not a hypersurface in R 3. These two manifolds are topologically indistinguishable. Without pausing to define the adjective, we go ahead and display a function flat torus f torus of revolution in a rather obvious fashion. Namely, f(x 1, x 2, x 3, x 4 ) = ( (b + ax 3 )x 1, (b + ax 3 )x 2, ax 4 ). PROBLEM Prove that f is a continuous bijection of the flat torus onto the torus of revolution. Prove that its inverse is given as ( ) f 1 x (x, y, z) = x2 + y, y 2 x2 + y, x2 + y 2 b z, 2 a a and that f 1 is also continuous.

33 Manifolds 33 Thus this function f provides a one-to-one correspondence between the points of these two tori, with the property that f and f 1 are both continuous. More than that, f and f 1 are both infinitely differentiable. Thus the flat torus and the round torus cannot be distinguished in the sense of manifolds. However, these tori are quite different geometrically. The round one is really a curved surface, and the surface appears quite different at different points. However, though we are as yet not equipped to define the adjective flat, it is rather clear that all points of the flat torus look alike from a geometric perspective. Thus the two tori are distinct geometric objects. PROBLEM Prove that at any point of the torus of revolution the vectors ( sin ψ cos θ, sin ψ sin θ, cos ψ), ( sin θ, cos θ, 0), (cos ψ cos θ, cos ψ sin θ, sin ψ), form an orthonormal basis of R 3, the first two being tangent to the torus and the third orthogonal to the torus.

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