Chapter 4: Metric quantities Flashcards

1
Q

Lemma 4.4.1: dot product wrt basis

A

Given a smooth regular surface σ : U → R^3, the tangent space
corresponding to (u, v) has a natural basis σ_u(u, v) and σ_v(u, v). The dot product
can be written, with respect to this basis, as follows.
(a_1σ_u(u, v) + b_1σ_v(u, v)) · (a_2σ_u(u, v) + b_2σ_v(u, v))

=
(a_1, b_1)

[σ_u(u, v) · σ_u(u, v) σu(u, v) · σv(u, v)]
[σu(u, v) · σv(u, v) σv(u, v) · σv(u, v)]
[a_2]
[b_2]

1x2 * 2x2 * 2x1
1x2 * FFF I *2x1
σ_u and σ_v form a basis expressed as linear combo

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2
Q

DEF 4.1.2

first fundamental form

A

Suppose σ : U → R3
is a regular parametrized surface. For each (u, v) ∈ U we have an inner product I(u,v) on R^2, known as the first
fundamental form, which has matrix

[E F]
[F G]

=
[E(u, v) F(u, v)]
[F(u, v) G(u, v)]
:=
[σu(u, v) · σu(u, v) σu(u, v) · σv(u, v)]
[σu(u, v) · σv(u, v) σv(u, v) · σv(u, v)]
where this defines the three functions E, F, G : U → R.

  • FFF of σ is the dot product of R^3 restricted to tangent space at (u,v) wrt natural basis σ_u,σ_v
  • FFF changes for different parameterization of the same surface
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3
Q

EXAMPLE: The plane R^2

can be seen as a surface in R^3 and parametrized by σ : R^2 → R^3, (u, v) → (u, v, 0). This has first fundamental form

A
[E(u, v) F(u, v)]
[F(u, v) G(u, v)]
\:=
[1 0]
[0 1]

for all (u, v) ∈ R^2

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4
Q

EXAMPLE: Compute FFF of the plane R^2 seen as a surface in R^3, but parametrized by σ : R^2 → R^3
(u, v) → (2u + v, −u + 3v, 0)

A

σ_u=(2,-1,0) σ_v=(1,3,0)
σ_u . σ_u =4+1=5 etc

[E(u, v) F(u, v)]
[F(u, v) G(u, v)]
\:=
[5 -1]
[-1 10]

for all (u, v) ∈ R^2

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5
Q

EXAMPLE: For parametrised curve
γ: ]α, β[ → R^3
t→ (x(t), 0, z(t))
we obtain the parametrized surface of revolution
σ : ]α, β[ × R → R^3
σ(t, θ) = (x(t) cos θ, x(t) sin θ, z(t)).
The first fundamental form is

A

[x’(t)^2 + z’(t)^2 0 ]

[0 x(t)^2 ]

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6
Q

EXAMPLE: cylinder x(t)=1 z(t)=t for all t

FFF=

A

[1 0]

[0 1]

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7
Q

EXAMPLE:
For the sphere S^2
in Example 3.3.6, x(t) = cos(t) and z(t) = sin(t). So for all (t, θ) the matrix of the first fundamental form is

A

[1 0 ]

[0 cos^2(t)]

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8
Q

EXAMPLE: The catenoid is the surface of rotation of the curve γ(t) := (cosh(t), 0, t) for t ∈ R. Compute the first fundamental form of the catenoid.

A
[cosh^2t      0     ]
[0           cos^2(t)]
= cosh^2t
[1 0]
[0 1]
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9
Q

image on surface

A

For a parametrized surface σ : U→ R^3, a parametrized curve γ: ]α, β[ → U
will have an image γ˜ = σ ◦ γ on the surface. We will see that the first fundamental
form encodes how much the parametrization σ distorts distances.

diagram mapping real line to open subset in R^2, by γto surface in R^3,by σ
]α, β[ on R

line on subset of R^2
by γ
U
to
surface in R^3
by σ
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10
Q

LEMMA 4.2.1: length of γ˜ = σ ◦ γ

A

For a parametrized surface σ:U→ R^3, a parametrized curve γ: ]α, β[ → U and any a, b with α < a ≤ b < β, the length of γ˜ = σ ◦ γ between a and b is
∫ _[a,b] √ [ I_γ(t)(γ˙(t), γ˙(t))]dt.

*we only need tangent vectors to γ and FFF along γ to compute the length of the
image of γ in S.

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11
Q

DEF 4.2.2: local isometry

A

A parametrization σ : U → R^3
is a local isometry if it takes any curve in U to a curve of the same length in the surface

ie alter shape doesn’t change arc lengths

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12
Q

THM 4.2.3

local isometry if

A

A parametrization σ : U → R^3
of surface is a local isometry if
and only if its first fundamental form I is represented by the identity matrix

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13
Q

proof of LEMMA 4.2.1: length of γ˜ = σ ◦ γ

A

proof: we know the arc length of γ˜ from a to b is
∫ _[a,b] ||γ˜•||.dτ
chain rule: γ˜ = σ ◦ γ
γ(t)= (u(t),v(t))
dγ˜/dt = (du/dt)(∂σ/∂t) + (dv/dt)(∂σ/∂t) = u’(t)σu +v’(t)σv
by 4.1.1

(γ˜^•)•(γ˜^•) =
(u’(t) v’(t))
[E F] [u’(t)]
[F G] [v’(t)]

but (γ•)(t)= (u’(t), v’(t))
ie (γ˜^•)•(γ˜^•) = I_γ(t) (γ•,γ•)

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14
Q

proof of

A parametrization σ : U → R^3
of surface is a local isometry if
and only if its first fundamental form I is represented by the identity matrix

A

The arc length functs are
s_γ(t)= ∫ _[t_0,t] ||γ˜•(τ)||.dτ=
∫ _[t_0,t] √ [ γ˙(τ) • γ˙(τ)]dτ by 4.2.1

and
s_γ~(t)= ∫ _t_0,t.dτ

so σ is a local isometry if and only if these two arc lengths equal for all curves γ: ]α, β[ → U and all t in ]α, β[

CONVERSE: if I is represented by the identity matrix then
I_{γ(t)} (γ˙(t),γ˙(t)) = γ˙(t)• γ˙(t) so s_γ (t)=s_γ~ (t) for all γ and t. Then √[γ˙(t)• γ˙(t)]= √[I_{γ(t)} (γ˙(t),γ˙(t))]

but by 3.4.6
every X ∈T_(u,v) σ is of the form γ˙(t) for some curve γ

so X•X=I_(u,v) (X,X) for all (u,v) ∈U X∈T_(u,v) σ. We want to show I_(u,v)(X,Y)= X•Y for all (u,v)∈U and X•Y∈T_(u,v)σ

Here we use a standard fact on inner products in vector spaces:
(FFF is inner prod)
*if g is an inner product on the vector space V then
g( x, y) = 0.5(g(x+y, x+y) - g(x,x) -g(y,y)) for all x,y in V

Now I_(u,v) (X,Y)= 0.5(I_(u,v) (X+Y,X+Y) -I_(u,v) (X,X) - I_(u,v) (Y,Y))

=0.5( (X+Y)•(X+Y)- X•X - Y•Y)
=X•Y
since •is inner product so I is represented by the identity Matrix

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15
Q

EXAMPLE 4.2.4 the cylinder (u, v) 7→ (cos(u), sin(u), v), the matrix of the first fundamental
form of is constant and equal to the identity matrix

is this an isometry

A

By the theorem, this
parametrization is a local isometry. This is a fancy way of saying that a flat
sheet of paper can be rolled into a cylinder without tearing or crumpling
the paper.

rectangle in R^2 rolled up to R^3 cylinder

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16
Q

isometry

A

map that preserves distances between points e.g translations and rotations

17
Q

local isometry

A

local isometry is only guaranteed to
preserve distances between points that are close enough, but not distances
between all points. In Example 4.2.4, the distance between (0,0) and (3π/2, 0)
on R2 is 3π/2, but the distance between their images Φ(0, 0) and Φ(3π/2, 0) on C is π/2

18
Q

angle between two non-zero vectors

u, v ∈ R^3

A

cos θ = (u · v) / [||u|| ||v||] =

u · v)/(√[u · u] √[v · v]

19
Q

Lemma 4.3.1.
two tangent
vectors

The angle θ between them is given by

A

For a parametrized surface σ : U → R^3, consider two tangent
vectors X,Y ∈ T(u0,v0)σ at a point P = σ(u0, v0):

X = aσ_u(u0, v0) + bσ_v(u0, v0),
Y = cσu(u0, v0) + dσv(u0, v0).
The angle θ between them is given by

cos θ = (X · Y) /(√[X · X] √[Y · Y]) =
(I_(u_0,v_0)((a,b)(c,d)) /
(√[I_(u_0,v_0)(a,b)(a,b)] √[I_(u_0,v_0)(c,d)(c,d)])

shows that the first fundamental form determines angles between tangent vectors
on a surface.
*tangent vectors with respect to a basis at point

20
Q

DEF 4.3.2 conformal

A

A parametrized surface σ : U → R^3 is conformal if for any
two curves γ1 and γ2 in U that intersect at a point (u, v) ∈ U, the angle of intersection of γ1 and γ2 at (u, v) is
equal to

the angle of intersection of

γ˜1 = σ ◦ γ1 and γ˜2 = σ ◦ γ2 at σ(u, v)

σ is conformal if it preserves angles

21
Q

THM 4.3.3

conformal if

A

A parametrized surface σ : U → R^3
is conformal if and only if
its first fundamental form is

 [1 0 ] λ   [0 1 ] for some FUNCTION λ: U →R
22
Q

when are locally isometric parametrizations conformal

A

Any locally isometric parameterization is conformal, here

λ =1

23
Q

The inverse stereographic projection

σ : R^2 → S^2\ {(0, 0, 1)},

σ(u, v) = ([2u/(u^2+v^2+1)],[2v/(u^2+v^2+1)],[(u^2+v^2−1)/(u^2+v^2+1)]

is it conformal?

A

yes,

 [1 0 ] λ   [0 1 ]

for FUNCTION λ: U →R

λ is..

Therefore σ^−1
can be used (and is indeed often used) to produce maps of the Earth that correctly represent all angles

*angles on map ≈ angles on earth, bearings and navigation. Distorts relative areas.

24
Q

Lemma 4.4.1. area of vectors

A

Two vectors u and v span a parallelogram of area

area of ||gram= base x height = ||u||·||v||·sinθ =√[||u||^2·||v||^2·sin^2(θ)] =
√[||u||^2·||v||^2·(1- cos^2(θ)] =
√[(u · u)(v · v) − (u · v)^2]

As dot involves cos

25
Q

approximating :

Let σ : U → R3 be a parametrized surface. Given a region R ⊂ U we want
to make sense of the area of σ(R). Decompose R into very small rectangles
of side ∆u and ∆v.

A

Then the image of the rectangle with corner (u0, v0) is
roughly a parallelogram with sides
σu(u0, v0)∆u and σv(u0, v0)∆v.

So its area is approximately
√[(σu(u0, v0) · σu(u0, v0))(σv(u0, v0) · σv(u0, v0)) − (σu(u0, v0) · σv(u0, v0))2∆u∆v]

i.e.
√[E(u0, v0)G(u0, v0) − F(u0, v0)^2] ∆u∆v.

(det of FFF)
*approximating by Taylors thm vector between vertices

diagrams:
small rectangle sides ∆u and ∆v vertices (u_0,v_0) , (u_0+ ∆u, v_0) , (u_0,v_0+∆v), (u_0+∆u,v_0+∆v)

to region R in R^2 squares

to surface in R^3 in parallelograms with vertices σ(u_0,v_0) , σ(u_0+ ∆u, v_0) , σ(u_0,v_0+∆v), σ(u_0+∆u,v_0+∆v)

26
Q

DEF 4.4.2 surface area of a parametrized surface

A

Let σ : U → R3 be a parametrized surface, and let R ⊂ U be a region. Then the surface area of σ(R) is
A_σ(R) = ∫ ∫_R √[EG − F^2] du dv .

27
Q

EXAMPLE:
The catenoid is the surface of revolution of the catenary
(i.e. cosh) curve; it has parametrization
σ : R^2 → R^3,
σ(t, θ) = (cosh t cos θ, cosh t sin θ, t).

The area on between the latitudes t = 0 and t = 1

A

area= π(1 + (1/2)sinh 2)= 8.838 . . . .

FFF is cosh^2(t)*
[1 0]
[0 1]

so √[EG − F^2] = √[cosh^2(t)]

A_σ(R) = ∫ ∫R √[EG − F^2] du dv
=A_σ(R) = ∫
[t=0,1] ∫[θ=0, 2π] [cosh^2(t)] .dt dθ=
(∫
[t=0,1]cosh^2(t) .dt)(∫_[θ=0, 2π] .dθ)= 2π[0.5t + (1/4)sinh2t ]_t=0 to 1
= π(1 + (1/2)sinh 2)

28
Q

Definition 4.4.4

equiareal

A

.A parametrized σ : U → R^3
surface is equiareal if it takes
any region in U to a region of the same area in σ(U)

29
Q

Theorem 4.4.5

equiareal thm

equiareal IF

A

A parametrized surface σ : U → R^3 is equiareal if and only if its
first fundamental form has determinant 1.

*from 4.2.3 and 4.3.3

30
Q

equiareal and isometric?

A

Any local isometry preserves surface areas.

by 4.2.3 local isometry has FFF I_σ =
[1 0]
[0 1]

so det=1 and by 4.4.3 this preserves surface area

31
Q

Example 4.4.7 (Cylindrical coordinates).

The inverse cylindrical projection
of the sphere (minus North and South Poles) is the parametrization corresponding
to the revolution of the parametrized semicircle
γ: ]1, −1[ → R^3,
t → (√[1 − t^2], 0, t).

Writing z for t, the parametrization is
σ : R × ]1, −1[ → R^3,
(θ, z) → (√[1 − z^2] cos θ,√[1 − z^2] sin θ, z).

is this equiareal

A

dots of normal and basis

This is an equiareal parametrization. We can state this another way.
This gives a map of the Earth that correctly represents all areas!

area preserving property of this radial projection from the sphere to the cylinder and formula for surface area of a sphere A= 4 pi r^2

FFF for the surface of Revolution: by 4.1.5

[x’(t)^2 +z’(t)^2 0 ]
[ 0 x(t)^2 ]

where z=t and x=√[1-z^2]
……

[(1/(1-z^2) 0 ]
[ 0 1-z^2]

which has determinant 1 so by 4.4.5 this is a equiarial