• Ingen resultater fundet

Equivariant K -theory of spaes of geodesis

In document Afhandling (Sider 38-51)

Theorem 3.3 (Atiyah). Let

G

be a ompat Lie group. Then

(i) K 0 (BG) ∼ = R(G) [ I

,

(ii) K 1 (BG) = 0

.

I will nowuse this theorem to determine

K (BS 1 )

and

K (BC n )

.

Lemma 3.4. Let

T : S 1 ֒ → C

be the natural 1-dimensional representation of

S 1

, and let

t = [T ] − 1 ∈ K 0 (BS 1 )

. Then

R(S 1 ) = Z[T, T 1 ], I = h T − 1 i , K 0 (BS 1 ) ∼ = R(S \ 1 ) I = Z[[t]].

Proof. Firstnotethatarepresentation

ρ : S 1 −→ GL n (C)

anbeonjugated

to

ρ : S 1 −→ U(n)

, by hoosing an inner produt on

C n

(all of whih are

onjugate) whih is

S 1

-invariant. So it sues to look at representations

ρ : S 1 −→ U (n)

. Now

ρ(t) ∈ U (n)

(for

t ∈ [0, 2π]

) is diagonizable,

ρ(t) ∼

diag

(e 1 , . . . , e n )

. This also diagonalizes

ρ(kt)

,

k ≥ 1

, so if we hoose

t

rationallyindependent of

π

, this diagonalizationworks fora dense subset of

S 1

. Soby ontinuity we an diagonalize

ρ(t)

for all

t

simultaneously, and so

ρ

isgivenbydiag

(ρ 1 (t), . . . , ρ n (t))

,where

ρ k : S 1 −→ S 1

isahomomorphism.

This means

ρ k (z) = z m k , m k ∈ Z

. Using the natural representation

T : z 7→

z

,anditsinverse

T 1 : z 7→ z 1

,weanreformulatethisbysayingthatevery representation of

S 1

has the form

P N

i= − N n i T i

,

n i ≥ 0

. The Groethendiek onstrution yields

R(S 1 ) = ( N

X

i= − N

n i T i | n i ∈ Z )

= Z[T, T 1 ].

Now tothe augmentationideal. By denition

I = ( N

X

i= − N

n i T i | X N i= − N

n i = 0 )

.

Clearly,

T − 1 ∈ I

, and also,

P N

i= − N n i T i ∈ I

is divisible by

T − 1

, beause

the sum of the oeients is zero. So

I = h T − 1 i

. Now

I k =

(T − 1) k

,

and

R(S 1 )/I k

hasgenerators

1, T − 1, (T − 1) 2 , . . . , (T − 1) k 1

. Consequently, putting

t = [T ] − 1

,we get

K 0 (BS 1 ) ∼ = R(S \ 1 ) I = Z[[t]].

Lemma3.5. Let

n ∈ N

be anumber withprime fatorisation

n = Q

p | n p i(p)

.

Then

K 0 (BC n ) ∼ = Z ⊕ M

p | n

(ˆ Z p ) p i(p) 1 ,

where

Z ˆ p

denotes the

p

-adi integers.

Proof. Let

W

be the natural 1-dimensional representation of

C n ⊆ C

. As

in the proof of Lemma 3.4 above, we only need look at representations

ρ : C n −→ U (m)

and diagonalize, so that

ρ =

diag

(ρ 1 , . . . , ρ m )

. Here eah

ρ j : C n −→ S 1

is a group homomorphism, and so is a power of

W

, with

the relation

W n = 1

. Consequently

R(C n ) = Z[W ]/ h W n − 1 i

. The

aug-mentation ideal is

I = h W − 1 i

for the same reason as before, and we must

omputetheinverse limit

lim

←− k

R(C n )/I k

. This wepropose todointwosteps:

First assume

n = p i

. Then

C p i

is a

p

-group, and aording to [Atiyah2℄

the

I

-adi and

p

-adi topologieson

I = I(C p i )

are equivalent,so that

K 0 (BC p i ) ∼ = R(C \ p i ) I = Z ⊕ I \ (C p i ) I ∼ = Z ⊕ I \ (C p i ) p .

To alulate this, let

w = W − 1

, and note that

I(C p i ) = h w i

in the ring

Z[w]/ D

(w + 1) p i = 1 E

,and so

I(C p i ) ∼ = Z p i 1

. Thus

I \ (C p i ) p ∼ = (ˆ Z p ) p i 1

.

Now take any

n ∈ N

. Observe that

C p i(p)

, where

n = p i(p) m

with

gcd(p, m) = 1

, are exatly the Sylow

p

subgroups of

C n

. Then by [Atiyah2℄

Prop. 4.10, there isaninjetivemap

K 0 (BC n ) −→ M

p | n

K 0 (BC p i(p) ),

and inpartiular

I(C \ n ) I(C n ) −→ M

p | n

I(C \ p i(p) ) I(C

pi (p) )

is injetive. By using that

C n ∼ = Q

p | n C p i(p)

by the Chinese Remainder

The-orem, itis easilyseen that this map is an isomorphism,sothat

K 0 (BC n ) ∼ = Z ⊕ M

p | n

I(C \ p i(p) ) ∼ = Z ⊕ M

p | n

(ˆ Z p ) p i(p) 1 ,

by the result for

p i

above.

Withthese results, letusrst take alook atthe

K (BS 1 )

-module

stru-ture on

K (X hS 1 )

, where

X

isan

S 1

-spae,as desribed in Setion1.4. F

ol-lowing the notation in Lemma 3.4, we have the anonial representation

T

of

S 1

, whih by (27) gives a bundle over

BS 1

, whih we also all

T

. On

K

-theory,

T

denes alassin

K (BS 1 )

,and

K (BS 1 ) = Z[[t]]

,where

t = T − 1

.

Usingthe projetion pr

1 : X hS 1 −→ BS 1

,weget lasses pr

1 (T )

and pr

1 (t)

in

K (X hS 1 )

. We willsuppress the map pr

1

from the notation, and simplyall

these lasses

T

and

t

again.

Weannowdeterminethe

K (BS 1 )

modulestrutureon

∆(r) ≃ G(r) hS 1

:

Lemma 3.6. The

K (BS 1 ) = Z[[t]]

module struture on

K(∆(r))

is given

by

t 7→ (x − y)/(y + 1)

. In partiular,

t 2r

ats as

0

.

Proof. We use the results from ohomology, where the

H (BS 1 ) = Z[u]

module struture on

H (G(r)/S 1 ) = Z[x 1 , x 2 ]/ h Q r , Q r+1 i

is given by

u 7→

x 1 − x 2

,f. [Bökstedt-Ottosen℄Cor. 3.7. Reallthat

x = [X] − 1

,

y = [Y ] − 1

,

where

x 1 = c 1 (X)

and

x 2 = c 1 (Y )

aretherstChernlasses. Also

u = c 1 (T )

.

The rst Chern lass gives a group isomorphism fromomplex linebundles

over

∆(r)

to

H 2 (∆(r))

, sosine

c 1 (T ⊗ Y ) = c 1 (T ) + c 1 (Y ) = u + x 2 = x 1 = c 1 (X ).

we get

T ⊗ Y = X

. Then we alulate

(T − 1) ⊗ (Y − 1) = T ⊗ Y − Y − T + 1 = (X − 1) − (Y − 1) − (T − 1)

Isolating

T − 1

gives

(T − 1) = ((X − 1) − (Y − 1)) ⊗ Y 1 .

In

K (∆(r))

this equality gives

t = (x − y)(y + 1) 1

, as desired. Sine in

K(∆(r)) ∼ = Z[x, y]/ h Q r , Q r+1 i

all non-zero elements have a total degree in

x, y

whih is less than

2r

, we see that

t 2r = (x − y) 2r (y + 1) 2r = 0

.

Now we prove the main Theorem of this setion, but rst we introdue

a bit of notation: We write

K hS 1 (X)

for

K (ES 1 × S 1 X)

, when

X

is an

S 1

-spae. Reall the diagram(26)

K hS 1 (G(r) (n) ) oo K (∆(r))

K (BS 1 )

OO

K (BS 1 )

B P n

oo OO

This gives amap

K (BS 1 ) (n) ⊗ K (BS 1 ) K (∆(r)) −→ K hS 1 (G(r) (n) )

where the

K (BS 1 ) (n)

denotes that the map

B P n

should be applied in the

tensor produt, as the diagramindiates.

Theorem 3.7. Let

n ∈ N

. Then the map

K (BS 1 ) (n) ⊗ R(S 1 ) K (∆(r)) −→ K hS 1 (G(r) (n) )

isan isomorphism of rings. In partiular,

K hS 1 1 (G(r) (n) ) = 0

.

Tox the notationand avoidlong, umbersome expressions, put

R = R(S 1 ) = Z[U, U 1 ], R ˆ = K 0 (BS 1 ) = Z[[u]], u = U − 1.

S = R(S 1 ) = Z[T, T 1 ], S ˆ = K 0 (BS 1 ) = Z[[t]], t = T − 1.

M = K (∆(r)) = Z[x, y]/ h Q r , Q r+1 i .

Here

S

isan

R

-module by the map

U 7→ T n

, and likewise

S ˆ

is an

R ˆ

-module

by

u 7→ (t +1) n − 1

. ByLemma3.6,

M

isan

R ˆ

-moduleby

u 7→ (x − y)/(1+y)

,

and thusan

R

-module by

U 7→ (x − y)/(1 + y) + 1

.

The Theorem says that

S ˆ (n)R M ∼ = K hS 1 (G(r) (n) )

. The reason for

restriting to

R

instead of

R ˆ

is given by the following lemma, whih also

shows that for the isomorphism, this restrition does not matter.

Lemma 3.8.

S ˆ

is a at

R

-module, and

S ˆ ⊗ R ˆ N ∼ = ˆ S ⊗ R N.

forany nitely generated

R ˆ

-module

N

where

u m

ats as0 on

N

for some

m

.

In partiular this holds for the ltration modules

M j

from Remark 3.2, for

M = M 2r+1

, and for the quotients

M j /M j+1

.

Proof. Clearly,

S

is a free

R

-module (with basis

{ 1, U, . . . , U n 1 }

), so

S

is

at over

R

. Sine

S

isNoetherian,

S ˆ

isat over

S

,see [Atiyah-MaDonald℄, Prop. 10.14. By the natural isomorphism,for any

R

-module

M

,

S ˆ ⊗ R M ∼ = ˆ S ⊗ S S ⊗ R M,

wesee that

S ˆ

isat over

R

.

Take

N

as inthe lemma. Then the ompletion by the ideal

I = h u i ⊆ R ˆ

gives

N ˆ = lim

k

N/u k N = N.

Also by [Atiyah-MaDonald℄, Prop. 10.13, sine

R

is Noetherian and

N

is nitely generated,

N ˆ ∼ = ˆ R ⊗ R N

. Combining these two fats yields the

isomorphism

S ˆ ⊗ R ˆ N ∼ = ˆ S ⊗ R ˆ N ˆ ∼ = ˆ S ⊗ R ˆ ( ˆ R ⊗ R N ) ∼ = ˆ S ⊗ R N.

Now onsider the

R ˆ

-module

M j

. Sine

u

ats as

(x − y)/(1 + y)

, and

M j

onsistsofpolynomialsdegreeatleast

j

,

u 2r+1

atsaszero. Forthequotient

M j /M j+1

,

u

itself ats as zero. So the requirements of

N

holds for these

modules.

We will use the ltration

M j

of

M

to prove the Theorem, so we need a

Lemma whih proves the Theorem in the ase

M = Z

:

Lemma 3.9. The followingmap is an isomorphism:

K (BS 1 ) ⊗ R(S 1 ) Z −→ K (BC n ).

Proof. Let

A = S ⊗ R Z

and

B = ˆ S ⊗ R Z

, and let

A −→ B

be the map

indued by the ompletion

S −→ S ˆ

. We now deneanother map

A −→ R(C n ) = Z[W ]/ h W n − 1 i , T 7→ W.

This is learly an isomorphism,and preserves the augmentation ideal.

Con-sider the diagram:

B

A

oo = //

R(C n )

ˆ

B oo A ˆ = // K 0 (BC n )

Herethe vertialarrowsdenoteompletionwithrespettotheaugmentation

ideals; respetively

tB

,

(T − 1)A

, and

h W − 1 i )

. To prove the Lemma, we

must show

B ∼ = ˆ A

. Firstnotethat

A ˆ −→ B ˆ

isanisomorphism,sineforany

k

,the map given by

T 7→ t + 1

, is anisomorphism:

A/(T − 1) k = Z[T ]/

T n − 1, (T − 1) k

−→ Z[t]/

(t + 1) n − 1, t k

= B/t k B.

Next we show that

B −→ B ˆ

is anisomorphism. To show this, onsider the exat sequene given by multipliationby

u − 1 ∈ R

,

0 // R u 1 // R // Z // 0 .

Sine

S ˆ

is at over

R

, we obtain anew exat sequene,

0 // S ˆ ⊗ R R 1 (u 1) // S ˆ ⊗ R R // S ˆ ⊗ R Z // 0 ,

whih, afterapplying the natural isomorphism,beomes

0 // S ˆ (t+1)

n − 1

// ˆ S // ˆ S ⊗ R Z // 0 .

(28)

Completing this with respet to the ideal

h t i

, whih is an exat funtor, we

obtainyet another exat sequene

0 // lim

S/ ˆ

t k (t+1) n − 1

// lim

S/ ˆ t k

// lim

← ( ˆ S ⊗ R Z)/

t k

// 0 .

Reall

S ˆ = Z[[t]]

. After applying the isomorphism

lim S/ ˆ

t k ∼ = ˆ S

, we get

the exat sequene,

0 // S ˆ (t+1)

n − 1

// ˆ S // lim ( ˆ S ⊗ R Z)/

t k

// 0 .

(29)

Comparing(28) and (29), we see that

B ∼ = ˆ B

. Asalready noted, this means

that

A ˆ ∼ = B

, and this provesthe result.

Now we an provethe mainTheorem 3.7:

Proof of Theorem3.7. Firstwe laim that the map

K (BS 1 ) ⊗ Z K hS 1 (G(r)) −→ K hS 1 (G(r) (n) )

(30)

issurjetive. Tosee this, werst note that the map

K (BC n ) −→ K (BS 1 )

issurjetive. Thisfollowsfromthefatthatthe mapof representationrings,

R(C n ) −→ R(S 1 )

is surjetive, sine any representation of

C n

an be

ex-tended toarepresentationof

S 1

. Nowtoprove surjetivity of (30), weuse a ltrationargumentin the spetral sequene

H (∆(r); K (BC n )) ⇒ K hS 1 (G(r) (n) ).

This ollapses, sine everything sits in even degrees. As in the proof of

Theorem 3.1, we now use Cor. 2.5 of [Atiyah-Hirzebruh℄, so let

A

denote

the image of

K (BS 1 ) ⊗ Z K hS 1 (G(r))

in

K hS 1 (G(r) (n) )

. In ltration degree

0 we have

K (BC n )

. As already shown

K (BS 1 )

is surjetive onto this,

so the lowest ltration an be hit. Anything else in

H (∆(r); K (BC n ))

is

generatedby monomials

x i 1 x j 2

, andwe have

x i y j ∈ A

withh

(x i y j ) = x i 1 x j 2 +

higherterms. This shows that

A = K hS 1 (G(r) (n) )

,so (30) is surjetive.

Nowweshowthatthemapisinjetive. Wewillusealtrationargument,

where we lter

M = K 0 (S(τ )/S 1 )

as in Remark 3.2. We look at the exat

sequene,

0 −→ M i+1 −→ M i −→ M i /M i+1 −→ 0.

As

S ˆ

isat over

R

by Lemma3.8, weget the exat sequene

0 −→ S ˆ ⊗ R M i+1 −→ S ˆ ⊗ R M i −→ S ˆ ⊗ R M i /M i+1 −→ 0.

(31)

Werstapplythisto

K

-theorywith

F p = Z/pZ

oeients. Forthe eld

F p

,wehavebytheUniversalCoeientTheorem,

K (X; F p ) ∼ = K (X) ⊗ F p

.

Clearly the ltration

M i = M i ⊗ F p

works for

F p

oeients, so we an

use the result above. But sine

F p

is a eld, the exat sequene (31) splits,

so we an do a ounting argument quite easily. Observe that

M i /M i+1 = F p [x, y] i / h Q r , Q r − 1 i = (F p ) n i

, where

n i ∈ N

. By Lemma3.9, we know

S ˆ ⊗ R M i /M i+1 ∼ = (K 0 (BC n ; F p )) n i .

(32)

and in addition,

K 0 (BC n ; F p )

is a nite numberof opies of

F p

, so it makes

sense to ount them. Also

M 2r 1 = F p

, so

S ˆ ⊗ R M 2r 1 ∼ = K 0 (BC n ; F p )

. So

indutively, sine

M ⊗ F p

is a graded ring with a total of

r(r + 1)

opies of

F p

, then

S ˆ ⊗ R M ⊗ F p ∼ = (K 0 (BC n ; F p )) r(r+1) .

Weompare this with

K (G(r) (n) ; F p )

via the spetralsequene for the

ver-tial brationin Prop. 1.6:

E 2 = H (∆(r); K (BC n ; F p )) ⇒ K (G(r) (n) ; F p ).

Weseeeverythingsitsinevendegreesin

E 2

,sotherearenodierentials,and, workingoveraeld

F p

,weansimplyountthedimensionof

K 0 (G(r) (n) ; F p )

as the sum of the dimensions of

E 2 m,n

on the diagonal

m + n = 0

. Sine

H (∆(r); F p ) ∼ = F p [x, y]/ h Q r , Q r+1 i

also has a total of

r(r + 1)

opies of

F p

,

again by Lemma 3.5, we get,

K 0 (G(r) n ; F p ) ∼ = (K 0 (BC n ; F p )) r(r+1) .

Sothe map of

F p

-vetor spaes

S ˆ ⊗ R M ⊗ Z p = K 0 (BS 1 ) ⊗ R(S 1 ) K 0 (S(τ)/S 1 ; Z p ) −→ K 0 (S(τ) (p) hS 1 ; Z p )

isasurjetion between spaesof the samedimension, and isthusan

isomor-phism, and this holds for every prime number

p

.

Nowwe ompare

Z

- and

F p

-oeients (for aprime

p

)by the diagram

K 0 (∆(r)) // K 0 (G(r) (n) ; F p )

S ˆ ⊗ R M //

ϕ

OO

S ˆ ⊗ R M ⊗ F p

∼ =

OO

(33)

Assume

a ∈ S ˆ ⊗ R F

isin the kernel of

ϕ

. Then, by the diagram,

a

redued

mod

p

iszero, so

a = p · a 1

for some

a 1

. But then, sine

K 0 (∆(r))

is torsion

free,

a 1 ∈ ker(ϕ)

, so

a 1 = p · a 2

, et. Consequently, if

a ∈ ker(ϕ)

, then

a

is divisible by

p

innitely often. Reall that this holds for any prime

p

, and

thusalso for

n

, so

a

is innitelyoften divisible by

n

.

Now take a look atthe ltration again

0 −→ S ˆ ⊗ R M i 1 −→ S ˆ ⊗ R M i −→ S ˆ ⊗ R M i /M i 1 −→ 0.

(34)

If

a ∈ S ˆ ⊗ R M i

isdivisible by

n

innitelyoften, then the image in

S ˆ ⊗ R M i /M i − 1 ∼ = Z N ⊕ M

p | n

(ˆ Z p ) N p

is zero (the isomorphism is Lemma 3.5 and Lemma 3.9). So

a

omes from

a

in

S ˆ ⊗ R M i − 1

and

a

is also innitely oftendivisible by

n

. Soindutively

a

omes from

a 0 ∈ S ˆ ⊗ R F 0 ∼ = Z ⊕ L

p | n (ˆ Z p ) p i 1

, and

a 0

is divisible by

n

innitelyoften, and so

a 0 = 0

, whih implies

a = 0

.

This shows that the kernel of

ϕ

is zero,and thusthe map

ϕ : K 0 (BS 1 ) ⊗ R(S 1 ) K 0 (S(τ )/S 1 ) −→ K 0 (S(τ) (p) hS 1 )

(35)

isan isomorphism.

4 The free loop spae and Morse theory

Now we turn to study the free loop spae

L(FP r )

, where as usual

F = C

or

F = H

. First a denition:

Denition 4.1. Let

X

be a topologialspae. The spae

LX = { f : [0, 1] −→ X | f(0) = f (1), f

isontinuous

} ,

with the ompat-open topology,is alled the free loopspae of

X

.

We are going to use Morse theory to study

LM

for a smooth manifold

M

, where we will take

M = FP r

. It is a fat that it does not hange the

homotopy typeof

LM

if we requireall

f ∈ LM

tobe dierentiable,or even smooth, sowe do that.

Now let us onsider how one ould do Morse theory on the free loop

spae

LM

as well the spae of homotopy orbits

LM hS 1

, where

M

denotes

a ompat

n

-dimensional manifold. For details, I refer to [Klilngenberg1℄, and [Bökstedt-Ottosen ℄, espeially hapters 7 and 8.

LM

is not a

nite-dimensionalmanifold,but one an makeamodelof

LM

whihisaso-alled

Hilbert manifold, f. [Klilngenberg1℄ Ÿ1.2, meaning there are harts on

LM

making it loally homeomorphi to a Hilbert spae. The tangent spae of

a loop

f ∈ LM

is the spae

Γ(f )

of vetor elds along

f

. Let

h· , ·i

denote

the Riemannian metri on

M

. Now the tangent spae

T f LM

arries the

struture of a Hilbert spae via

h ξ, η i c = Z

S 1

h ξ(t), η(t) i + c h∇ ξ(t), ∇ η(t) i

dt,

(36)

where

ξ, η ∈ T f LM

are vetor elds along

f

in

LM

, and

denotes the

ovariant derivative along

f

. The onstant

c ∈ R

makes the inner produt

vary. This isneessary toensurethat the

n

-folditerationmap,

P n

, beomes

anisometry

P n = D f ( P n ) : T f LM −→ T P n f LM, P n (ξ(z)) = ξ(z n )

sine

hP n ξ, P n η i 1 = h ξ, η i n 2

,see [Bökstedt-Ottosen ℄ Ÿ7.

Weare going todo Morse theory via the energy funtion

E : LM −→ R, f 7→

Z

S 1 | f (t) | 2 dt.

Foreah

a ∈ R

, weset

F (a) = E 1 (] − ∞ , a]) ⊆ LM

. The ritial points of

E

are the losed geodesis on

M

. We shall assume that the ritial points

are olleted on ompat submanifolds, eah of whih satisfy the Bott

non-degeneray ondition. This strong ondition is needed for the Morse theory

mahinery,anditissatisedfor

M = FP r

,andmoregenerallyforsymmetri

spaes, [Ziller℄. Callthe ritial values

0 = λ 0 < λ 1 < . . .

, and onsider the

ltration

F (λ 0 ) ⊆ F (λ 1 ) ⊆ · · · ⊆ LM.

(37)

This ltration is equivariant with respet to the

S 1

ation. This means it

induesa ltrationof

LM hS 1

,

F (λ 0 ) hS 1 ⊆ F (λ 1 ) hS 1 ⊆ · · · ⊆ LM hS 1 .

(38)

Thenon-degeneray ondition ensurethat eahritialsubmanifold

N (λ) = E 1 (λ)

isnite-dimensional,and the tangent bundle

T (LM ) | N(λ) ⊆ T (LM )

splits

S 1

-equivariantly:

T (LM) | N (λ) ∼ = µ (λ) ⊕ µ 0 (λ) ⊕ µ + (λ),

intothe bundles of negative, zero-,and positivediretions, respetively, and

the negativebundle

µ (λ)

is nite-dimensional. To ease the notation, write

F n = F (λ n )

and

µ n = µ (λ n )

. The main result of Morse theory in this

setting is proved by Klingenberg in [Klilngenberg1℄, Ÿ2.4: There is an

S 1

-equivariant homotopy equivalene

F n )/ F n − 1 ≃ T h(µ n ).

(39)

We want a similar result for

(LM) hS 1

, so we onsider the quotients of the

ltration(38):

ES 1 × S 1 F n /ES 1 × S 1 F n − 1 ∼ = ES + 1 ∧ S 1 F n / F n − 1 ,

where

ES + 1 ∧ S 1 X = (ES + 1 ∧ X)/S 1

is the smash produt modded out by

the diagonal

S 1

ation. The obvious map dened on representatives is a homeomorphism. Thus by the Morse theorem in(39),

ES 1 × S 1 F n /ES 1 × S 1 F n − 1 ≃ ES + 1 ∧ S 1 T h(µ n ).

We an use [Bökstedt-Ottosen ℄ Lemma 5.1tond that

( F n ) hS 1 /( F n − 1 ) hS 1 ≃ ES + 1S 1 T h(µ n ) ∼ = T h((µ n ) hS 1 )

(40)

where for an

S 1

-vetor bundle

ξ

given by a projetion map

p : E −→ B

we

denoteby

ξ hS 1

thebundlewithprojetionid

× p : ES 1 × S 1 E −→ ES 1 × S 1 B

.

This means wealso have a Morse theorem for the

S 1

-equivariantltration.

4.1 The negative bundle

In [Bökstedt-Ottosen ℄ Lemma 5.1, it is shown that the negative bundle

n ) hS 1

is an oriented vetor bundle if

µ n

is. But to use the Thom

iso-morphismin

K

-theoryweneedtoknowthatthenegativebundleisomplex,

ormore preisely

Proposition 4.2. The negative bundle

µ n

for the energyltration of

LCP r

an be written as

ε ⊕ ν

, where

ε

is a trivial real

S 1

-line bundle, and

ν

is a

omplex

S 1

vetor bundle. Consequently, the negative bundle

n ) hS 1

for the

energyltration of

LCP r hS 1

an also be written as

ε ⊕ ν hS 1

.

Proof. ThereisaHermitianinnerprodut

h· , ·i C

on

T CP r

,andthe

Rieman-nian metri is

h· , ·i =

Re

( h· , ·i C )

. The tangent spae

T f LCP r

is a omplex

vetor spae,and itarries the struture of a Hilbert spae via

h ξ, η i = Z

S 1

( h ξ(t), η(t) i + h∇ ξ(t), ∇ η(t) i ) dt,

where

ξ, η ∈ T f LCP r

are vetor elds along

f

in

LCP r

, and

denotes the

ovariant derivativealong

f

. Sine

h· , ·i =

Re

( h· , ·i C )

, weget

h zξ, zη i = h ξ, η i

for

z ∈ S 1 .

(41)

If

f

is a ritial point of the energy funtional

E

(a geodesi), then the

tangent spae of

LCP r

splits as

T f LCP r = Γ(Rf ) ⊕ Γ(Rif ) ⊕ Γ((f ) )

(42)

where e.g.

Γ(Rf ) ⊆ Γ(f)

denotes the vetor elds

ξ

along

f

with

ξ(t) ∈ Rf (t) ⊆ T f(t) CP r

. We an use the inner produt to represent the Hessian

H = D 2 E

of

E

by a linear operator

A = A f

on

T f LCP r

, by requiring

h Aξ 1 , ξ 2 i = H(ξ 1 , ξ 2 )

. Then we get by (41) that

zAz ¯ = A

for

z ∈ S 1

, whih

implies that

A

isomplex linear.

Aording to Klingenberg, [Klilngenberg1℄ Thm. 2.4.2,

A f =

id

− (1 − ∇ 2 ) 1 ◦ ( ˜ K f + 1),

where

K ˜ f (ξ)(t) = R(ξ(t), f (t))f (t)

= π 2 (f (t) h ξ(t), f (t) i − 2f (t) h f (t), ξ(t) i + ξ(t) h f (t), f (t) i )

Notethefator

π 2

;itappearsbeauseourmetrion

CP r

issaledsothatthe

irumferene is 1, not

π

. This gives us the following eigenvalue equation

Aξ = λξ

:

(λ − 1) ∇ 2 ξ = ( ˜ K f + λ)ξ

(43)

Thenegativebundleonsistsofsolutionstothis equationwith

λ < 0

. Notie

thatbytheformulafor

A

,itpreservesthedeomposition(42),sineovariant derivativeommuteswiththeomplexstrutureon

T CP r

. Thusweansolve

(43) inthe three spaes separately.

(i) ξ ∈ Γ(Rf )

: Then

ξ(t) = g(t)f (t)

where

g : [0, 1] −→ R

is a smooth

funtionwith

g(0) = g(1)

. Then

K ˜ f (t) = 0

,andequation(43)beomes

(λ − 1)g ′′ = λg ⇔ g ′′ = λ λ 1 g ⇒ g = 0

sine

λ < 0

and

g

mustbeperiodi. Sowehavenonon-trivialsolutions.

(ii) ξ ∈ Γ((f ) )

: Sine

(f )

is a omplex vetor spae, and

A

is omplex

linear as noted, we see that

Aξ = λξ

implies

A(iξ) = λ(iξ)

. So this

spaeof solutions has a omplex struture.

(iii) ξ ∈ Γ(Rif )

: Then

ξ(t) = g (t)if (t)

, where

g : [0, 1] −→ R

is asmooth

funtionwith

g(0) = g(1)

. Then

K ˜ f (t) = 4π 2 k f (t) k 2 ξ(t) = 4π 2 n 2 ξ(t)

,

sine

f

is ageodesi of length

n

. The equation (43) then beomes

(λ − 1)g ′′ = (4π 2 n 2 + λ)g ⇔ g ′′ = 4π 2 n 2 + λ

λ − 1 g

To get a periodi solution

g

, we must have

2 λ n 2 1 ≤ 0

, i.e.

λ ≥

− 4π 2 n 2

. For

λ = − 4π 2 n 2

we must have

g

onstant, and this gives the

trivialreal linebundle

ε

. If

− 4π 2 n 2 < λ < 0

we have the solution set

spanned over

R

by

g 1 K (t) = cos(K · 2πt),

and

g 2 K (t) = sin(K · 2πt), t ∈ [0, 1]

where

K = s

− 4π 2 n 2 + λ

2π(λ − 1) ,

and

K ∈ N,

sine the funtions must be periodi with period 1. This happens if

and onlyif

λ = 4π 2 (K 2 − n 2 ) 4π 2 K 2 + 1 ,

so for a xed

n

we get solutions with

λ < 0

for

K = 1, . . . , n − 1

.

Thisspae ofsolutionsan be given aomplexstruture

J

by rotating

t 7→ t − 4K 1

,where

t ∈ [0, 1]

,i.e.

J(g 1 K ) = g 2 K , J (g 2 K ) = − g K 1 .

and extendinglinearly. Clearly

J

satises

J 2 = −

id.

This gives the bundle

ν

, whih is learly an

S 1

bundle, with the

S 1

ation

given by rotation.

Nowletussee thattheresultfor

µ n

impliesthatfor

n ) hS 1

. Thebundle

n ) hS 1

isdened sothatthe pullbakof

n ) hS 1

agreeswith pr

n )

inthe

followingdiagram,

µ n

pr

∗ (µ n )

//

oo (µ n ) hS 1

G n (r) ES 1 × G n (r) //

pr

oo ES 1 × S 1 G n (r)

where

G n (r)

denotesthespaeof

n

-timesiteratedgeodesis. Sine

µ n = ε ⊕ ν

isadeompositionin

S 1

-bundles,weautomatiallygetthedeompositionfor

n ) hS 1

.

In document Afhandling (Sider 38-51)