HOMEWORK 4 - SOLUTIONS-2012 - Imperial College …aneves/papers/HW4-solutions-12.pdf · HOMEWORK 4...
Transcript of HOMEWORK 4 - SOLUTIONS-2012 - Imperial College …aneves/papers/HW4-solutions-12.pdf · HOMEWORK 4...
HOMEWORK 4 - SOLUTIONS-2012
ANDRE NEVES
Exercise 8 of Chapter 4.2 of Do Carmo:
The first step is to show that G is a linear map. Fix a point p and considerα1(t) = p+ tX, where X is any vector in R3. Set F (t) = G ◦ α1(t)−G(q).By differentiation in the t variable when t = 0 we have
|F (t)|2 = |tX + p− q|2 =⇒ F ′(0).F (0) = X.(p− q)
=⇒ DGp(X).(G(p)−G(q)) = X.(p−q) =⇒ X.(DGp)>(G(p)−G(q)) = X.(p−q)
for all X and all q. In the last line we use the fact that if A is a 3 × 3matrix with transpose AT , then A(X).Y = X.AT (Y ) for every vectors X,Y .Because the identity we derived is valid for all X it is simple to concludethat
(DGp)>(G(p)−G(q)) = p− q for every q ∈ R3.
In particular the linear map (DGp)T is surjective and thus injective. Denot-
ing by B its inverse we have from the above formula that
G(p) = G(q) +B(p− q)for every p, q ∈ R3.
Using again the hypothesis we obtain that
|B(p− q)| = |G(p)−G(q)| = |p− q|.
Using Exercise 7 of Chapter 4.2 (more precisely, that b) is equivalent to a)– which is simple to show) it follows at once that G is a linear isometry of R3.
Exercise 11 of Chapter 4.2 of Do Carmo:
First a). From the previous exercise we know that F is a linear isometryof R3, which means that DFp = DF0 for all p in R3 (i.e. F is linear) andDF0(X).DF0(Y ) = X.Y for all vectors X,Y in R3. In particular for everyp ∈ S we have that DFp = DF0 and DFp(X).DFp(Y ) = X.Y for all X,Yin TpS, which means that F is an isometry of S. Technically speaking oneshould show that if F is an ambient map of R3, then the restriction of F toS has the property that for every X ∈ TpS, then DFp(X) as it was definedin class is nothing but DFp(X) as it was defined in multivariable calculus.This is just the chain rule and so I will not say anything else to avoid therisk of just ending up making it more confusing.
1
2 ANDRE NEVES
Now b). The orthogonal linear transformations are just those 3 × 3 ma-trices which have ATA = Id, i.e., A−1 = AT . In this case we have
|A(X)|2 = A(X).A(x) = X.ATA(X) = X.X = |X|2
and so A send the unit sphere into the unit sphere. Moreover |A(X) −A(Y )| = |A(X − Y )| = |X − Y |, and so its distance preserving in the senseof Exercise 8. Thus a) can be applied to conclude A is an isometry of thesphere.
Finally c). Take F (x, y, 0) = (cosx, sinx, y) which is an isometry frompart of the plane {z = 0} into part of the cylinder {x2 + y2 = 1}. F isnot distance preserving because |F (0, 0, 0) − F (θ, 0, 0)| = 2(1 − cos θ) and|(0, 0, 0)− (θ, 0, 0)| = |θ|.
Exercise12 of Chapter 4.2 of Do Carmo:
Consider F (x, y, z) = (x,−y,−z). This is an isometry of the cylinderS = {x2 + y2 = 1} because F send the S into S and F is an orthogonallinear transformation. Finally F (x, y, z) = (x, y, z) then z = 0 and y = 0.But x2 + y2 = 1, which means x = ±1, i.e., the only fixed points are (1, 0, 0)and (−1, 0, 0).
Exercise 2 of Chapter 4.3 of Do Carmo:Use the formula which is in Exercise 1 of same chapter and which was provenin class. Set λ = e2u for convenience. Then we have
√EG = e2u,
∂x2E
(EG)1/2= 2∂x2u,
∂x1G
(EG)1/2= 2∂x1u.
Thus, recalling that ∆h = ∂x1x1h+ ∂x2x2h, we obtain
K = −e−2u∆u = − 1
2λ∆ lnλ.
(Recall that ln√λ = 1
2 lnλ).
To be consistent with the rest of the notation I should use λ = (x21 +x2
2 +c)−2 for the last part. Then
∂xi lnλ = −2∂xi ln(x21 + x2
2 + c) = − 4xix2
1 + x22 + c
and
∂2xixi lnλ = − 4
x21 + x2
2 + c+
8x2i
(x21 + x2
2 + c)2.
Thus
∆ lnλ = − 8
x21 + x2
2 + c+
8(x21 + x2
2)
(x21 + x2
2 + c)2=
−8c
(x21 + x2
2 + c)2= −8cλ
and so
K = − 1
2λ∆ lnλ = 4c.
HOMEWORK 4 - SOLUTIONS-2012 3
Exercise 3 of Chapter 4.3 of Do Carmo:
We have
∂x
∂u= (cos v, sin v, u−1),
∂x
∂v= (−u sin v, u cos v, 0)
and so
E =∂x
∂u.∂x
∂u= 1 + u−2, F =
∂x
∂u.∂x
∂v= 0, G =
∂x
∂v.∂x
∂v= u2.
Because ∂vE = 0 we obtain from Exercise 1
K = − 1
2√
1 + u2
∂
∂u
(2u√
1 + u2
)= − 1
(1 + u2)2
We have∂x
∂u= (cos v, sin v, 0),
∂x
∂v= (−u sin v, u cos v, 0)
and so
E =∂x
∂u.∂x
∂u= 1, F =
∂x
∂u.∂x
∂v= 0, G =
∂x
∂v.∂x
∂v= 1 + u2.
Using the formula in Exercise 1 we have
K = − 1
2√
1 + u2
∂
∂u
(2u√
1 + u2
)= − 1
(1 + u2)2.
Therefore the surfaces have the same curvature.If the map x ◦ x−1 were an isometry then by Proposition 1, page 220, we
would have E = E, F = F , and G = G. Because this is false the surfacesare not isometric.
Exercise 6 of Chapter 4.3 of Do Carmo:
If there was a surface with E = G = 1, F = 0 and e = −g = 1, f = 0, thenfrom the definition of Gaussian curvature we would have K = (eg−f)(EG−F )−1 = −1. But from Gauss’s Theorem we know that K is intrinsic, i.e.,depends only on E,F and G. Thus K must be zero because we can surelyput coordinates on a plane which have E = G = 1, F = 0 and a plane hasGaussian curvature zero.
Exercise: Let S be a compact surface in R3 with no boundary which haspositive Gaussian curvature and denote the Gauss map by
N : S −→ {x2 + y2 + z2 = 1}.Show that if γ is a geodesic in S which divides S into a set A and anotherset B (i.e., S = A∪B and ∂A = ∂B = γ), then area(N(A)) = area(N(B)).
4 ANDRE NEVES
Hint: If you have a diffeomorphism
F : S −→ {x2 + y2 + z2 = 1} ⊂ R3,
what is the formula for area(F (A)) in terms of DF and the set A?
Because K > 0, we have from Gauss-Bonnet that S is diffeomorphic to asphere. Thus A andB are both diffeomorphic to a disc and ∂A = ∂B = γ isa geodesic. Hence, if ν denotes the interior unit normal to ∂A we have∫
AKdA+
∫∂Ak.νdσ = 2π =⇒
∫AKdA = 2π.
Likewise ∫BKdA = 2π.
I will show now that
area(N(A)) =
∫AKdA = 2π
and this completes the exercise.The first remark is that the Gaussian map N must be a diffeomorphism.
Why? Well, because K = detA = −detdN , we have from the inverse func-tion theorem that N is locally a diffeomorphism. And it happens that locallydiffeomorphisms from a sphere into a sphere must be global diffeomorphism.
The second remark is to show the hint, namely that
area(F (A)) =
∫A|detdF |dA.
Suppose that φ : D ⊂ R2 −→ A is a chart for A. Then ψ = F ◦ φ is achart for N = {x2 + y2 + z2 = 1} because F is a diffeomorphism. From thelectures we know that
area(ψ(D)) =
∫D
∣∣∣∣∂ψ∂x × ∂ψ
∂y
∣∣∣∣ dxdy.Now let {e1, e2} be a basis for Tφ(p)A which has dFp(e1) = λ1e1 and dFp(e2) =λ2e2, i.e., {e1, e2} is an eigenbasis for dF . Then
∂φ
∂x(p) = a1e1 + b1e2
∂φ
∂y(p) = a2e1 + b2e2
and thus ∣∣∣∣∂φ∂x × ∂φ
∂y
∣∣∣∣ = |a1b2 − a2b1||e1 × e2|.
Furthermore
∂ψ
∂x(p) = dFφ(p)
(∂φ
∂x(p)
)= λ1a1e1 + λ2b1e2
and∂ψ
∂y(p) = dFφ(p)
(∂φ
∂y(p)
)= λ1a2e1 + λ2b2e2.
HOMEWORK 4 - SOLUTIONS-2012 5
Thus∣∣∣∣∂ψ∂x × ∂ψ
∂y
∣∣∣∣ = |λ1λ2||a1b2 − a2b1||e1 × e2| = |detdFφ(p)|∣∣∣∣∂φ∂x × ∂φ
∂y
∣∣∣∣ .(This formula was long to derive but it should be highly expected).
Therefore we have
area(F (φ(D))) = area(ψ(D)) =
∫D
∣∣∣∣∂ψ∂x × ∂ψ
∂y
∣∣∣∣ dxdy.=
∫D|detdFφ(p)|
∣∣∣∣∂φ∂x × ∂φ
∂y
∣∣∣∣ dxdy =
∫φ(D)|detdF |dA.
Covering A with a finite number of charts we arrive at
area(F (A)) =
∫A|detdF |dA.
Using this formula with F = N the Gauss map we obtain
area(N(A)) =
∫A|detdN |dA =
∫A|K|dA =
∫AKdA = 2π.
Exercise: Let S be the cylinder {x2 + y2 = 1} in R3, with the chart
φ : [0, 2π]× R −→ S, φ(θ, z) = (cos θ, sin θ, z).
and let γ be a simple closed curve in S.
(1) Let γ be a simple closed curve in S for which there is a path
α : [0, 1] −→ [0, 2π]× R
so that α(0) = (0, z0), α(1) = (2π, z0), and γ = φ ◦ α. In otherwords, γ loops once around the z-axis. If ~ν denotes a unit normalvector to γ show that ∫
γ
~k.~νdσ = 0.
(2) Let γ be a simple closed curve in S for which there is a path
α : [0, 1] −→ [0, 2π]× R
so that α(0) = (θ0, z0) = α(1). In other words, γ is the boundary ofa disc D in S. Show that γ is not a geodesic.
If the path α(t) = (θ(t), z(t)), choose z1 so that z(t) > z1 for all t ∈ [0, 1]and consider the path β(t) = (2πt, z1). Note that φ ◦ β is a geodesic andthere is a region R in S so that ∂S = γ ∪ φ ◦ β. To recognize this lastfact just let R = φ(A), where A is the region in [0, 2π] × R below α and
6 ANDRE NEVES
above β. Note that R is diffemorphic to a cylinder and thus has zero Eulercharacteristic. Using Gauss-Bonnet we obtain that∫
RKdA+
∫γ
~k.~νdσ +
∫φ◦β
~k.~νdσ = 0,
where ~ν is the interior unit normal. Because K = 0 and φ ◦ β is a geodesicwe obtain that ∫
γ
~k.~νdσ,
which is what we wanted to show.
(1) Let γ be a simple closed curve in S for which there is a path
α : [0, 1] −→ [0, 2π]× Rso that α(0) = (θ0, z0) = α(1). In other words, γ is the boundary ofa disc D in S. Show that γ is not a geodesic.
The Euler characteristic of D is one and so by the Gauss-Bonnet Theoremwe have ∫
DKdA+
∫γ
~k.~νdσ = 2π =⇒∫γ
~k.~νdσ = 2π.
Thus, γ cannot be a geodesic.