lecture1
PDF · 8 pages · 111.2 KB
Open PDF file
Lecture 1 of a course on Lie groups and the method of the moving frame, authored by Jeanne Nielsen Clelland (the text shows her name, not Phil's). It covers 1-forms and p-forms on R^n, the wedge product, the exterior derivative and d^2=0, closed and exact forms, forms on manifolds, pullbacks, the Lie derivative and Cartan's formula. It ends with five exercises, including relating grad, curl and div to d.
AI-written summary; may contain errors.
Extracted text (machine-read; may contain errors)
LECTURE 1: DIFFERENTIAL FORMS
1.1-forms on Rn
In calculus, you may have seen the differential orexterior derivative dfof a
functionf(x,y,z ) defined to be
df=∂f
∂xdx+∂f
∂ydy+∂f
∂zdz.
The expression dfis called a 1-form. But what does this really mean?
Definition: Asmooth 1-form φonRnis a real-valued function on the set
of all tangent vectors to Rn, i.e.,
φ:TRn→R
with the properties that
1.φis linear on the tangent space TxRnfor eachx∈Rn.
2. For any smooth vector field v=v(x), the function φ(v) :Rn→Ris
smooth.
Given a 1-form φ, for eachx∈Rnthe map
φx:TxRn→R
is an element of the dual space ( TxRn)∗. When we extend this notion to all
ofRn, we see that the space of 1-forms on Rnis dual to the space of vector
fields on Rn.
In particular, the 1-forms dx1,... ,dxnare defined by the property that for
any vector v= (v1,... ,vn)∈TxRn,
dxi(v) =vi.
Thedxi’s form a basis for the 1-forms on Rn, so any other 1-form φmay be
expressed in the form
φ=n/summationdisplay
i=1fi(x)dxi.
If a vector field vonRnhas the form
v(x) = (v1(x),... ,vn(x)),
1
2 JEANNE NIELSEN CLELLAND
then at any point x∈Rn,
φx(v) =n/summationdisplay
i=1fi(x)vi(x).
2.p-forms on Rn
The 1-forms on Rnare part of an algebra, called the algebra of differential
forms onRn. The multiplication in this algebra is called wedge product , and
it is skew-symmetric:
dxi∧dxj=−dxj∧dxi.
One consequence of this is that dxi∧dxi= 0.
If each summand of a differential form φcontainspdxi’s, the form is called
ap-form . Functions are considered to be 0-forms, and any form on Rnof
degreep>n must be zero due to the skew-symmetry.
A basis for the p-forms on Rnis given by the set
{dxi1∧···∧dxip: 1≤i1<i2<···<ip≤n}.
Anyp-formφmay be expressed in the form
φ=/summationdisplay
|I|=pfIdxi1∧···∧dxip
whereIranges over all multi-indices I= (i1,... ,i p) of length p.
Just as 1-forms act on vector fields to give real-valued functions, so p-forms
act onp-tuples of vector fields to give real-valued functions. For instance, if
φ,ψare 1-forms and v,ware vector fields, then
(φ∧ψ)(v,w) =φ(v)ψ(w)−φ(w)ψ(v).
In general, if φ1,... ,φ pare 1-forms and v1... ,v pare vector fields, then
(φ1∧···∧φp)(v1,... ,v p) =/summationdisplay
σ∈Spsgn(σ)φ1(vσ(1))φ2(vσ(2))···φn(vσ(n)).
3.The exterior derivative
The exterior derivative is an operation that takes p-forms to (p+ 1)-forms.
We will first define it for functions and then extend this definition to higher
degree forms.
Definition: Iff:Rn→Ris differentiable, then the exterior derivative of
fis the 1-form dfwith the property that for any x∈Rn, v∈TxRn,
dfx(v) =v(f),
i.e.,dfx(v) is the directional derivative of fatxin the direction of v.
LIE GROUPS AND THE METHOD OF THE MOVING FRAME 3
It is not difficult to show that
df=n/summationdisplay
i=1∂f
∂xidxi.
The exterior derivative also obeys the Leibniz rule
d(fg) =gdf+fdg
and the chain rule
d(h(f)) =h/prime(f)df.
We extend this definition to p-forms as follows:
Definition: Given ap-formφ=/summationdisplay
|I|=pfIdxi1∧···∧dxip, the exterior deriv-
ativedφis the (p+ 1)-form
dφ=/summationdisplay
|I|=pdfI∧dxi1∧···∧dxip.
Ifφis ap-form andψis aq-form, then the Leibniz rule takes the form
d(φ∧ψ) =dφ∧ψ+ (−1)pφ∧dψ.
Very Important Theorem: d2= 0. i.e., for any differential form φ,
d(dφ) = 0.
Proof: First suppose that fis a function, i.e., a 0-form. Then
d(df) =d(n/summationdisplay
i=1∂f
∂xidxi)
=/summationdisplay
i,j∂2f
∂xi∂xjdxj∧dxi
=/summationdisplay
i<j(∂2f
∂xj∂xi−∂2f
∂xi∂xj)dxi∧dxj
= 0
because mixed partials commute.
Next, note that dxireally does mean d(xi), wherexiis theith coordinate
function. So by the argument above, d(dxi) = 0. Now suppose that
φ=/summationdisplay
|I|=pfIdxi1∧···∧dxip.
4 JEANNE NIELSEN CLELLAND
Then by the Leibniz rule,
d(dφ) =d(/summationdisplay
|I|=pdfI∧dxi1∧···∧dxip)
=/summationdisplay
|I|=p[d(dfI)∧dxi1∧···∧dxip−dfI∧d(dxi1)∧···∧dxip+...]
= 0.2
Definition: Ap-formφisclosed ifdφ= 0. φisexact if there exists a
(p−1)-formηsuch thatφ=dη.
By the Very Important Theorem, every exact form is closed. The converse
is only partially true: every closed form is locally exact. This means that
given a closed p-formφon an open set U⊂Rn, any point x∈Uhas a
neighborhood on which there exists a ( p−1)-formηwithdη=φ.
4.Differential forms on manifolds
Given a smooth manifold M, asmooth 1-form φonMis a real-valued
function on the set of all tangent vectors to Msuch that
1.φis linear on the tangent space TxMfor eachx∈M.
2. For any smooth vector field vonM, the function φ(v) :M→Ris
smooth.
So for each x∈M, the map
φx:TxM→R
is an element of the dual space ( TxM)∗.
Wedge products and exterior derivatives are defined similarly as for Rn. If
f:M→Ris a differentiable function, then we define the exterior derivative
offto be the 1-form dfwith the property that for any x∈M, v∈TxM,
dfx(v) =v(f).
A local basis for the space of 1-forms on Mcan be described as before in
terms of any local coordinate chart ( x1,... ,xn) onM, and it is possible
to show that the coordinate-based notions of wedge product and exterior
derivative are in fact independent of the choice of local coordinates and so
are well-defined.
More generally, suppose that M1,M2are smooth manifolds and that F:
M1→M2is a differentiable map. For any x∈M1, the differential dF
(also denoted F∗) :TxM1→TF(x)M2may be thought of as a vector-valued
1-form, because it is a linear map from TxM1to the vector space TF(x)M2.
There is an analogous map in the opposite direction for differential forms,
called the pullback and denoted F∗. It is defined as follows.
LIE GROUPS AND THE METHOD OF THE MOVING FRAME 5
Definition: IfF:M1→M2is a differentiable map, then
1. Iff:M2→Ris a differentiable function, then F∗f:M1→Ris the
function
(F∗f)(x) = (f◦F)(x).
2. Ifφis ap-form onM2, thenF∗φis thep-form onM1defined as follows:
ifv1,... ,v p∈TxM1, then
(F∗φ)(v1,... ,v p) =φ(F∗(v1),... ,F ∗(vp)).
In terms of local coordinates ( x1,... ,xn) onM1and (y1,... ,ym) onM2,
suppose that the map Fis described by
yi=yi(x1,... ,xn),1≤i≤m.
Then the differential dFat each point x∈M1may be represented in this
coordinate system by the matrix/bracketleftbigg
∂yi
∂xj/bracketrightbigg
.
Thedxj’s are forms on M1, thedyi’s are forms on M2, and the pullback
mapF∗acts on the dyi’s by
F∗(dyi) =n/summationdisplay
j=1∂yi
∂xjdxj.
The pullback map behaves as nicely as one could hope with respect to the
various operations on differential forms, as described in the following theo-
rem.
Theorem: LetF:M1→M2be a differentiable map, and let φ,ηbe
differential forms on M2. Then
1.F∗(φ+η) =F∗φ+F∗η.
2.F∗(φ∧η) =F∗φ∧F∗η.
3.F∗(dφ) =d(F∗φ).
5.The Lie derivative
The final operation that we will define on differential forms is the Lie de-
rivative. This is a generalization of the notion of directional derivative of a
function.
6 JEANNE NIELSEN CLELLAND
Suppose that v(x) is a vector field on a manifold M, and letϕ:M×(−ε,ε)→
Mbe the flow ofv. This is the unique map that satisfies the conditions
∂ϕ
∂t(x,t) =v(ϕ(x,t))
ϕ(x,0) =x.
In other words, ϕt(x) =ϕ(x,t) is the point reached at time tby flowing
along the vector field v(x) starting from the point xat time 0.
Recall that if f:M→Ris a smooth function, then the directional derivative
offatxin the direction of vis
v(f) = lim
t→0f(ϕt(x))−f(x)
t
= lim
t→0(ϕ∗
t(f)−f)(x)
t.
Similarly, given a differential form φwe define the Lie derivative ofφalong
the vector field v(x) to be
Lvφ= lim
t→0ϕ∗
tφ−φ
t.
Fortunately there is a practical way to compute the Lie derivative. First we
need the notion of the left-hook of a differential form with a vector field.
Given ap-formφand a vector field v, the left-hookvφofφwithv(also
called the interior product ofφwithv) is the (p−1)-form defined by the
property that for any w1,... ,w p−1∈TxRn,
(vφ)(w1,... ,w p−1) =φ(v,w1,... ,w p−1).
For instance,
∂
∂x(dx∧dy+dz∧dx) =dy−dz.
Now according to Cartan’s formula , the Lie derivative of φalong the vector
fieldvis
Lvφ=vdφ+d(vφ).
Exercises
1. Classical vector analysis avoids the use of differential forms on R3by
converting 1-forms and 2-forms into vector fields by means of the following
one-to-one correspondences. ( ε1,ε2,ε3will denote the standard basis ε1=
[1,0,0], ε2= [0,1,0], ε3= [0,0,1].)
LIE GROUPS AND THE METHOD OF THE MOVING FRAME 7
f1dx1+f2dx2+f3dx3←→f1ε1+f2ε2+f3ε3
f1dx2∧dx3+f2dx3∧dx1+f3dx1∧dx2←→f1ε1+f2ε2+f3ε3
Vector analysis uses three basic operations based on partial differentiation:
1.Gradient of a function f:
grad(f) =3/summationdisplay
i=1∂f
∂xiεi
2.Curl of a vector field v=3/summationdisplay
i=1vi(x)εi:
curl(v) =/parenleftbigg∂v3
∂x2−∂v2
∂x3/parenrightbigg
ε1+/parenleftbigg∂v1
∂x3−∂v3
∂x1/parenrightbigg
ε2+/parenleftbigg∂v2
∂x1−∂v1
∂x2/parenrightbigg
ε3
3.Divergence of a vector field v=3/summationdisplay
i=1vi(x)εi:
div(v) =3/summationdisplay
i=1∂vi
∂xi
Prove that all three operations may be expressed in terms of exterior deriva-
tives as follows:
1.df↔grad(f)
2. Ifφis a 1-form and φ↔v, thendφ↔curl(v).
3. Ifηis a 2-form and η↔v, thendη↔div(v)dx1∧dx2∧dx3.
Show that the identities
curl(grad(f)) = 0
div(curl(v)) = 0
follow from the fact that d2= 0.
2. Letfandgbe real-valued functions on R2. Prove that
df∧dg=/vextendsingle/vextendsingle/vextendsingle/vextendsingle/vextendsingle/vextendsingle∂f
∂x∂f
∂y
∂g
∂x∂g
∂y/vextendsingle/vextendsingle/vextendsingle/vextendsingle/vextendsingle/vextendsingledx∧dy.
(You may recognize this from the change-of-variables formula for double
integrals.)
3. Suppose that φ,ψare 1-forms on Rn. Prove the Leibniz rule
d(φ∧ψ) =dφ∧ψ−φ∧dψ.
8 JEANNE NIELSEN CLELLAND
4. Prove the statement above that if F:M1→M2is described in terms of
local coordinates by
yi=yi(x1,... ,xn),1≤i≤m
then
F∗(dyi) =n/summationdisplay
j=1∂yi
∂xjdxj.
5. Let (r,θ) be coordinates on R2and (x,y,z ) coordinates on R3. Let
F:R2→R3be defined by
F(r,θ) = (cosθ,sinθ,r).
Describe the differential dFin terms of these coordinates and compute the
pullbacksF∗(dx),F∗(dy),F∗(dz).