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Path Integrals, asymptotic expansions and Zeta determinants - - PowerPoint PPT Presentation

Path Integrals, asymptotic expansions and Zeta determinants Matthias Ludewig Universitt Potsdam February 11, 2016 Matthias Ludewig (Uni Potsdam) 11.02.16 1 / 24 The heat equation Let L = be a Laplace type operator, acting on


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SLIDE 1

Path Integrals, asymptotic expansions and Zeta determinants

Matthias Ludewig

Universität Potsdam

February 11, 2016

Matthias Ludewig (Uni Potsdam) 11.02.16 1 / 24

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SLIDE 2

The heat equation

Let L = ∇∗∇ be a Laplace type operator, acting on sections of a vector bundle V on a compact n-dimensional Riemannian manifold M. The heat or diffusion equation ∂ ∂tu(t, x) + Lu(t, x) = 0, u(0, x) = u0(x) has a unique solution for given initial data u0 ∈ L2(M, V), and it is given by u(t, x) = ˆ

M

pL

t (x, y)u(y)dy,

t > 0 where pL

t ∈ C∞(M × M, V ⊠ V∗) is the heat kernel of L.

Matthias Ludewig (Uni Potsdam) 11.02.16 2 / 24

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SLIDE 3

The heat kernel as a path integral

By physicist’s reasoning, the heat kernel can be written as the "sum over all histories", weighted with their probability. pL

t (x, y) formally

= (4πt)−n/2

paths x→y

exp

  • − 1

4t ˆ 1

  • ˙

γ(s)

  • 2ds
  • [γ1

0]−1 Dγ

Matthias Ludewig (Uni Potsdam) 11.02.16 3 / 24

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SLIDE 4

The heat kernel as a path integral

By physicist’s reasoning, the heat kernel can be written as the "sum over all histories", weighted with their probability. pL

t (x, y) formally

= (4πt)−n/2

paths x→y

exp

  • − 1

4t ˆ 1

  • ˙

γ(s)

  • 2ds
  • Classical action
  • [γ1

0]−1 Dγ

Matthias Ludewig (Uni Potsdam) 11.02.16 3 / 24

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SLIDE 5

The heat kernel as a path integral

By physicist’s reasoning, the heat kernel can be written as the "sum over all histories", weighted with their probability. pL

t (x, y) formally

= (4πt)−n/2

paths x→y

exp

  • − 1

4t ˆ 1

  • ˙

γ(s)

  • 2ds
  • Classical action
  • [γ1

0]−1 Dγ

The slash in the integral sign denotes division by the normalization Z = (4πt)N/2, N = dimension of path space Dγ denotes the Riemannian volume measure of the space of paths.

Matthias Ludewig (Uni Potsdam) 11.02.16 3 / 24

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SLIDE 6

The heat kernel as a path integral

pL

t (x, y) formally

= (4πt)−n/2

paths x→y

e−E(γ)/2t [γ1

0]−1 Dγ

Matthias Ludewig (Uni Potsdam) 11.02.16 4 / 24

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SLIDE 7

The heat kernel as a path integral

pL

t (x, y) formally

= (4πt)−n/2

paths x→y

e−E(γ)/2t [γ1

0]−1 Dγ

Theorem

We have pL

t (x, y) =

ˆ

Cxy(M)

[γ1

0]−1 dWxy;t(γ).

In the theorem, [γ1

0]−1 is the stochastic parallel transport in V, Wxy;t is a

conditional Wiener measure and Cxy;t(M) = {γ ∈ C([0, t], M) | γ(0) = x, γ(1) = y}

Matthias Ludewig (Uni Potsdam) 11.02.16 4 / 24

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SLIDE 8

The heat kernel as a path integral

pL

t (x, y) formally

= (4πt)−n/2

paths x→y

e−E(γ)/2t [γ1

0]−1 Dγ

Theorem (L. ’15)

We have pL

t (x, y) = lim |τ|→0 Hxy;τ(M)

e−E(γ)/2t [γ1

0]−1 dΣ-H1γ

where the limit goes over any sequence of partitions τ = {0 = τ0 < τ1 < · · · < τN = 1} of the interval [0, 1], the mesh of which tends to zero. In the theorem, Hxy;τ(M) =

  • γ ∈ Hxy(M) | γ|[τj−1,τj] is a geodesic ∀j
  • Matthias Ludewig (Uni Potsdam)

11.02.16 5 / 24

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SLIDE 9

The space of finite energy paths

An important path space is the space of finite energy paths Hxy(M) :=

  • γ ∈ H1([0, t], M) | γ(0) = x, γ(1) = y
  • .

This is an infinite-dimensional Hilbert manifold with the Riemannian metric (X, Y )H1 := ˆ 1

  • ∇sX, ∇sY
  • ds,

X, Y ∈ TγHxy(M). It is the "Cameron-Martin-manifold" corresponding to the Wiener measure.

Matthias Ludewig (Uni Potsdam) 11.02.16 6 / 24

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SLIDE 10

pL

t (x, y) formally

= (4πt)−n/2

Hxy(M)

e−E(γ)/2t[γ1

0]−1Dγ

Matthias Ludewig (Uni Potsdam) 11.02.16 7 / 24

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SLIDE 11

pL

t (x, y) formally

= (4πt)−n/2

Hxy(M)

e−E(γ)/2t[γ1

0]−1Dγ

  • The heat kernel has an asymptotic expansion

pL

t (x, y) ∼ et(x, y) ∞

  • j=0

tjΦj(x, y), et(x, y) = e−d(x,y)2/4t (4πt)n/2

Matthias Ludewig (Uni Potsdam) 11.02.16 7 / 24

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SLIDE 12

pL

t (x, y) formally

= (4πt)−n/2

Hxy(M)

e−E(γ)/2t[γ1

0]−1Dγ

  • The heat kernel has an asymptotic expansion

pL

t (x, y) ∼ et(x, y) ∞

  • j=0

tjΦj(x, y), et(x, y) = e−d(x,y)2/4t (4πt)n/2

  • The path integral has a formal Laplace expansion.

Matthias Ludewig (Uni Potsdam) 11.02.16 7 / 24

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SLIDE 13

pL

t (x, y) formally

= (4πt)−n/2

Hxy(M)

e−E(γ)/2t[γ1

0]−1Dγ

  • The heat kernel has an asymptotic expansion

pL

t (x, y) ∼ et(x, y) ∞

  • j=0

tjΦj(x, y), et(x, y) = e−d(x,y)2/4t (4πt)n/2

  • The path integral has a formal Laplace expansion.

Goal

Compare the two asymptotic expansions. In this talk: The lowest order term.

Matthias Ludewig (Uni Potsdam) 11.02.16 7 / 24

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SLIDE 14

pL

t (x, y) formally

= (4πt)−n/2

Hxy(M)

e−E(γ)/2t[γ1

0]−1Dγ

  • The heat kernel has an asymptotic expansion

pL

t (x, y) ∼ et(x, y) ∞

  • j=0

tjΦj(x, y), et(x, y) = e−d(x,y)2/4t (4πt)n/2

  • The path integral has a formal Laplace expansion.

Goal

Compare the two asymptotic expansions. In this talk: The lowest order term.

Matthias Ludewig (Uni Potsdam) 11.02.16 7 / 24

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SLIDE 15

Laplace’s Expansion

Let Ω be a finite-dimensional Riemannian manifold. If φ : Ω − → R has the unique non-degenerate minimum x0, then

e−φ(x)/2ta(x) dx ∼ e−φ(x0)/2t a(x0) det

  • ∇2φ|x0

1/2

Matthias Ludewig (Uni Potsdam) 11.02.16 8 / 24

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SLIDE 16

Laplace’s Expansion

Let Ω be a finite-dimensional Riemannian manifold. If φ : Ω − → R has the unique non-degenerate minimum x0, then

e−φ(x)/2ta(x) dx ∼ e−φ(x0)/2t a(x0) det

  • ∇2φ|x0

1/2

Formal conclusion

If there is a unique shortest geodesic γxy connecting x to y, then formally

Hxy(M)

e−E(γ)/2t[γt

0]−1Dγ ∼ e−d(x,y)2/4t

[γxy1

0]−1

det

  • ∇2E|γxy

1/2 since E(γxy) = d(x, y)2/2.

Matthias Ludewig (Uni Potsdam) 11.02.16 8 / 24

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SLIDE 17

A formal proof

Taylor expand E(γ) = E(γxy) + 1

2∇2E|γxy[X, X] + O(|X|3), where X is

the vector field with expγxy(X) = γ.

Matthias Ludewig (Uni Potsdam) 11.02.16 9 / 24

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SLIDE 18

A formal proof

Taylor expand E(γ) = E(γxy) + 1

2∇2E|γxy[X, X] + O(|X|3), where X is

the vector field with expγxy(X) = γ. Then exp

  • −E(γ)

2t

= exp

  • − 1

2t

  • E(γxy) + 1

2∇2E|γxy[X, X] + O(|X|3)

  • DX

Matthias Ludewig (Uni Potsdam) 11.02.16 9 / 24

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SLIDE 19

A formal proof

Taylor expand E(γ) = E(γxy) + 1

2∇2E|γxy[X, X] + O(|X|3), where X is

the vector field with expγxy(X) = γ. Then exp

  • −E(γ)

2t

= exp

  • − 1

2t

  • E(γxy) + 1

2∇2E|γxy[X, X] + O(|X|3)

  • DX

substitute X → t1/2X gives = e−E(γxy)/2t exp

  • −1

4∇2E|γxy[X, X] + O(t1/2|X|3)

  • DX

Matthias Ludewig (Uni Potsdam) 11.02.16 9 / 24

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A formal proof

Taylor expand E(γ) = E(γxy) + 1

2∇2E|γxy[X, X] + O(|X|3), where X is

the vector field with expγxy(X) = γ. Then exp

  • −E(γ)

2t

= exp

  • − 1

2t

  • E(γxy) + 1

2∇2E|γxy[X, X] + O(|X|3)

  • DX

substitute X → t1/2X gives = e−E(γxy)/2t exp

  • −1

4∇2E|γxy[X, X] + O(t1/2|X|3)

  • DX

and in the limit t → 0 ∼ e−E(γxy)/2t exp

  • −1

4∇2E|γxy[X, X]

  • DX

Matthias Ludewig (Uni Potsdam) 11.02.16 9 / 24

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SLIDE 21

A formal proof

Taylor expand E(γ) = E(γxy) + 1

2∇2E|γxy[X, X] + O(|X|3), where X is

the vector field with expγxy(X) = γ. Then exp

  • −E(γ)

2t

= exp

  • − 1

2t

  • E(γxy) + 1

2∇2E|γxy[X, X] + O(|X|3)

  • DX

substitute X → t1/2X gives = e−E(γxy)/2t exp

  • −1

4∇2E|γxy[X, X] + O(t1/2|X|3)

  • DX

and in the limit t → 0 ∼ e−E(γxy)/2t exp

  • −1

4∇2E|γxy[X, X]

  • DX

∼ e−E(γxy)/2t det

  • ∇2E|γxy

−1/2

Matthias Ludewig (Uni Potsdam) 11.02.16 9 / 24

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SLIDE 22

Remark

At a geodesic γ, the Hessian of the energy is given by ∇2E|γ[X, Y ] = ˆ 1

  • ∇sX, ∇sY
  • ds +

ˆ 1

  • R
  • ˙

γ(s), X(s)

  • ˙

γ(s) , Y (s)

  • ds

Matthias Ludewig (Uni Potsdam) 11.02.16 10 / 24

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SLIDE 23

Remark

At a geodesic γ, the Hessian of the energy is given by ∇2E|γ[X, Y ] = ˆ 1

  • ∇sX, ∇sY
  • ds +

ˆ 1

  • R
  • ˙

γ(s), X(s)

  • ˙

γ(s)

  • :=Rγ(s)X(s)

, Y (s)

  • ds

Matthias Ludewig (Uni Potsdam) 11.02.16 10 / 24

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SLIDE 24

Remark

At a geodesic γ, the Hessian of the energy is given by ∇2E|γ[X, Y ] = ˆ 1

  • ∇sX, ∇sY
  • ds +

ˆ 1

  • R
  • ˙

γ(s), X(s)

  • ˙

γ(s)

  • :=Rγ(s)X(s)

, Y (s)

  • ds

=

  • X, (−∇2

s + RγY )

  • L2

Matthias Ludewig (Uni Potsdam) 11.02.16 10 / 24

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SLIDE 25

Remark

At a geodesic γ, the Hessian of the energy is given by ∇2E|γ[X, Y ] = ˆ 1

  • ∇sX, ∇sY
  • ds +

ˆ 1

  • R
  • ˙

γ(s), X(s)

  • ˙

γ(s)

  • :=Rγ(s)X(s)

, Y (s)

  • ds

=

  • X, (−∇2

s + RγY )

  • L2

Therefore, setting P := −∇2

s, we have

∇2E|γ[X, Y ] =

  • X, (P + Rγ)Y )L2

Matthias Ludewig (Uni Potsdam) 11.02.16 10 / 24

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SLIDE 26

Remark

At a geodesic γ, the Hessian of the energy is given by ∇2E|γ[X, Y ] = ˆ 1

  • ∇sX, ∇sY
  • ds +

ˆ 1

  • R
  • ˙

γ(s), X(s)

  • ˙

γ(s)

  • :=Rγ(s)X(s)

, Y (s)

  • ds

=

  • X, (−∇2

s + RγY )

  • L2

Therefore, setting P := −∇2

s, we have

∇2E|γ[X, Y ] =

  • X, (P + Rγ)Y )L2

=

  • ∇−1

s X, ∇−1 s (P + Rγ)Y

  • H1

Matthias Ludewig (Uni Potsdam) 11.02.16 10 / 24

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SLIDE 27

Remark

At a geodesic γ, the Hessian of the energy is given by ∇2E|γ[X, Y ] = ˆ 1

  • ∇sX, ∇sY
  • ds +

ˆ 1

  • R
  • ˙

γ(s), X(s)

  • ˙

γ(s)

  • :=Rγ(s)X(s)

, Y (s)

  • ds

=

  • X, (−∇2

s + RγY )

  • L2

Therefore, setting P := −∇2

s, we have

∇2E|γ[X, Y ] =

  • X, (P + Rγ)Y )L2

=

  • ∇−1

s X, ∇−1 s (P + Rγ)Y

  • H1

=

  • X, P −1(P + Rγ)Y
  • H1

Matthias Ludewig (Uni Potsdam) 11.02.16 10 / 24

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SLIDE 28

Remark

At a geodesic γ, the Hessian of the energy is given by ∇2E|γ[X, Y ] = ˆ 1

  • ∇sX, ∇sY
  • ds +

ˆ 1

  • R
  • ˙

γ(s), X(s)

  • ˙

γ(s)

  • :=Rγ(s)X(s)

, Y (s)

  • ds

=

  • X, (−∇2

s + RγY )

  • L2

Therefore, setting P := −∇2

s, we have

∇2E|γ[X, Y ] =

  • X, (P + Rγ)Y )L2

=

  • ∇−1

s X, ∇−1 s (P + Rγ)Y

  • H1

=

  • X, P −1(P + Rγ)Y
  • H1

Hence det

  • ∇2E|γ
  • = det
  • P −1(P + Rγ)
  • = det
  • id + P −1Rγ

trace-class

)

  • .

Matthias Ludewig (Uni Potsdam) 11.02.16 10 / 24

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SLIDE 29

Theorem (L. ’15)

For points x, y ∈ M such that there is a unique minimal geodesic connecting x to y, we have pL

t (x, y)

et(x, y) ∼ [γxy1

0]−1

det

  • ∇2E|γxy

1/2 where et(x, y) is the "Euclidean heat kernel".

Matthias Ludewig (Uni Potsdam) 11.02.16 11 / 24

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SLIDE 30

Theorem (L. ’15)

For points x, y ∈ M such that there is a unique minimal geodesic connecting x to y, we have pL

t (x, y)

et(x, y) ∼ [γxy1

0]−1

det

  • ∇2E|γxy

1/2 where et(x, y) is the "Euclidean heat kernel".

Corollary

The Jacobian of the exponential map is a Fredholm determinant, det

  • d expx | ˙

γxy(0)

  • = det
  • ∇2E|γxy
  • Matthias Ludewig (Uni Potsdam)

11.02.16 11 / 24

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SLIDE 31

Theorem (L. ’15)

For points x, y ∈ M such that there is a unique minimal geodesic connecting x to y, we have pL

t (x, y)

et(x, y) ∼ [γxy1

0]−1

det

  • ∇2E|γxy

1/2 where et(x, y) is the "Euclidean heat kernel".

Corollary

The Jacobian of the exponential map is a Fredholm determinant, det

  • d expx | ˙

γxy(0)

  • = det
  • ∇2E|γxy
  • Proof of Corollary. It is well-known that

pL

t (x, y)

et(x, y) ∼ [γxy1

0]−1

det

  • d expx | ˙

γxy(0)

1/2 .

  • Matthias Ludewig (Uni Potsdam)

11.02.16 11 / 24

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SLIDE 32

This can be proved by finite-dimensional approximation, but one has to make precise error estimates for the approximation.

Theorem (L. ’15)

We have pL

t (x, y) = lim |τ|→0 Hxy;τ(M)

e−E(γ)/2t [γ1

0]−1 dΣ-H1γ

where the limit goes over any sequence of partitions τ = {0 = τ0 < τ1 < · · · < τN = 1} of the interval [0, 1], the mesh of which tends to zero.

Matthias Ludewig (Uni Potsdam) 11.02.16 12 / 24

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SLIDE 33

In the physics literature, one reads e−E(γ)/2tDγ ∼ e−E(γxy)/2t exp

  • −1

4∇2E|γxy[X, X]

  • DX

Matthias Ludewig (Uni Potsdam) 11.02.16 13 / 24

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SLIDE 34

In the physics literature, one reads e−E(γ)/2tDγ ∼ e−E(γxy)/2t exp

  • −1

4∇2E|γxy[X, X]

  • DX

∼ e−E(γxy)/2t exp

  • −1

4

  • X, (P + Rγxy)X
  • L2
  • DX

Matthias Ludewig (Uni Potsdam) 11.02.16 13 / 24

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SLIDE 35

In the physics literature, one reads e−E(γ)/2tDγ ∼ e−E(γxy)/2t exp

  • −1

4∇2E|γxy[X, X]

  • DX

∼ e−E(γxy)/2t exp

  • −1

4

  • X, (P + Rγxy)X
  • L2
  • DX

∝ e−E(γxy)/2t detζ

  • P + Rγxy

−1/2 where detζ is the zeta-regularized determinant.

Matthias Ludewig (Uni Potsdam) 11.02.16 13 / 24

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SLIDE 36

In the physics literature, one reads e−E(γ)/2tDγ ∼ e−E(γxy)/2t exp

  • −1

4∇2E|γxy[X, X]

  • DX

∼ e−E(γxy)/2t exp

  • −1

4

  • X, (P + Rγxy)X
  • L2
  • DX

∝ e−E(γxy)/2t detζ

  • P + Rγxy

−1/2 where detζ is the zeta-regularized determinant. From the english Wikipedia article on "Functional Determinants". "This path integral is only well defined up to some divergent multiplicative constant. To give it a rigorous meaning, it must be divided by another functional determinant, thus effectively cancelling the problematic constants."

Matthias Ludewig (Uni Potsdam) 11.02.16 13 / 24

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SLIDE 37

Zeta determinant

The zeta function of a zeta-admissible operator P is defined by ζP (z) =

  • λ=0

λ−z, Re(z) ≫ 0. where the sum goes over its eigenvalues.

Matthias Ludewig (Uni Potsdam) 11.02.16 14 / 24

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SLIDE 38

Zeta determinant

The zeta function of a zeta-admissible operator P is defined by ζP (z) =

  • λ=0

λ−z, Re(z) ≫ 0. where the sum goes over its eigenvalues. We have in this domain ζ′

P (z) = −

  • λ=0

log(λ)λ−z = ⇒ e−ζ′

P (z) =

  • λ=0

λλ−z.

Matthias Ludewig (Uni Potsdam) 11.02.16 14 / 24

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SLIDE 39

Zeta determinant

The zeta function of a zeta-admissible operator P is defined by ζP (z) =

  • λ=0

λ−z, Re(z) ≫ 0. where the sum goes over its eigenvalues. We have in this domain ζ′

P (z) = −

  • λ=0

log(λ)λ−z = ⇒ e−ζ′

P (z) =

  • λ=0

λλ−z. This motivates to set detζ(P) := e−ζ′

P (0)

formally

=

  • λ=0

λ, defined by analytic continuation.

Matthias Ludewig (Uni Potsdam) 11.02.16 14 / 24

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SLIDE 40

Zeta determinant and Fredholm determinants

Theorem (Scott ’04)

Let P be a closed operator on a Hilbert space H and let T = id + W with W trace-class. If P is a zeta-admissible, then so is PT and detζ(PT) = detζ(P) det(T).

Matthias Ludewig (Uni Potsdam) 11.02.16 15 / 24

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SLIDE 41

Zeta determinant and Fredholm determinants

Theorem (Scott ’04)

Let P be a closed operator on a Hilbert space H and let T = id + W with W trace-class. If P is a zeta-admissible, then so is PT and detζ(PT) = detζ(P) det(T).

Corollary

With P = −∇2

s, we have

det

  • ∇2E|γ
  • = det
  • P −1(P + Rγ)
  • = detζ(P + Rγ)

detζ(P) .

Matthias Ludewig (Uni Potsdam) 11.02.16 15 / 24

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SLIDE 42

Application

Theorem

For x, y ∈ M such that there is a unique minimizing geodesic γxy connecting x and y, we have pL

t (x, y)

et(x, y) ∼ det

  • ∇2E|γxy

−1/2 = detζ(−∇2

s + Rγxy)−1/2

detζ(−∇2

s)−1/2

Matthias Ludewig (Uni Potsdam) 11.02.16 16 / 24

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SLIDE 43

The degenerate case

Let Ω be a finite-dimensional Riemannian manifold. If φ : Ω − → R is a function such that φ ≥ λ and C = φ−1(λ) is a non-degenerate submanifold

  • f dimension k, then

e−φ(x)/2ta(x) dx ∼ (4πt)−k/2 ˆ

C

e−λ/2ta(x) det

  • ∇2φ|NxC

1/2 dx

Matthias Ludewig (Uni Potsdam) 11.02.16 17 / 24

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SLIDE 44

The degenerate case

Let Ω be a finite-dimensional Riemannian manifold. If φ : Ω − → R is a function such that φ ≥ λ and C = φ−1(λ) is a non-degenerate submanifold

  • f dimension k, then

e−φ(x)/2ta(x) dx ∼ (4πt)−k/2 ˆ

C

e−λ/2ta(x) det

  • ∇2φ|NxC

1/2 dx

Formal conclusion

If the set of minimal geodesics Γmin

xy ⊆ Hxy(M) is a non-degenerate

submanifold of dimension k (with respect to the energy functional E), then formally

Hxy(M)

e−E(γ)/2t[γt

0]−1Dγ ∼ (4πt)−k/2

ˆ

Γmin

xy

e−d(x,y)2/4t[γ1

0]−1

det

  • ∇2E|NγΓmin

xy

1/2 dγ.

Matthias Ludewig (Uni Potsdam) 11.02.16 17 / 24

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SLIDE 45

Theorem (L. ’15, H1 picture)

Suppose that Γmin

xy ⊆ Hxy(M) is a non-degenerate submanifold of

dimension k, then pL

t (x, y)

et(x, y) ∼ (4πt)−k/2 ˆ

Γmin

xy

[γ1

0]−1

1 det

  • ∇2E|NγΓmin

xy

1/2 dH1γ.

Matthias Ludewig (Uni Potsdam) 11.02.16 18 / 24

slide-46
SLIDE 46

Theorem (L. ’15, H1 picture)

Suppose that Γmin

xy ⊆ Hxy(M) is a non-degenerate submanifold of

dimension k, then pL

t (x, y)

et(x, y) ∼ (4πt)−k/2 ˆ

Γmin

xy

[γ1

0]−1

1 det

  • ∇2E|NγΓmin

xy

1/2 dH1γ.

Theorem (L. ’15, L2 picture)

Suppose that Γmin

xy ⊆ Hxy(M) is a non-degenerate submanifold of

dimension k, then pL

t (x, y)

et(x, y) ∼ (4πt)−k/2 ˆ

Γmin

xy

[γ1

0]−1

det(∇2

s)1/2

det′

ζ

  • −∇2

s + Rγ

1/2 dL2γ.

Matthias Ludewig (Uni Potsdam) 11.02.16 18 / 24

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SLIDE 47

Theorem (L. ’15, L2 picture)

Suppose that Γmin

xy ⊆ Hxy(M) is a non-degenerate submanifold of

dimension k, then pL

t (x, y)

et(x, y) ∼ (4πt)−k/2 ˆ

Γmin

xy

[γ1

0]−1

detζ

  • −∇2

s

1/2 det′

ζ

  • −∇2

s + Rγ

1/2 dL2γ.

Matthias Ludewig (Uni Potsdam) 11.02.16 19 / 24

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SLIDE 48

Theorem (L. ’15, L2 picture)

Suppose that Γmin

xy ⊆ Hxy(M) is a non-degenerate submanifold of

dimension k, then pL

t (x, y)

et(x, y) ∼ (4πt)−k/2 ˆ

Γmin

xy

[γ1

0]−1

detζ

  • −∇2

s

1/2 det′

ζ

  • −∇2

s + Rγ

1/2 dL2γ.

  • Proof. We have

pL

t (x, y)

et(x, y) ∼ (4πt)−k/2 ˆ

Γmin

xy

[γ1

0]−1

1 det

  • ∇2E|NγΓmin

xy

1/2 dH1γ

Matthias Ludewig (Uni Potsdam) 11.02.16 19 / 24

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SLIDE 49

Theorem (L. ’15, L2 picture)

Suppose that Γmin

xy ⊆ Hxy(M) is a non-degenerate submanifold of

dimension k, then pL

t (x, y)

et(x, y) ∼ (4πt)−k/2 ˆ

Γmin

xy

[γ1

0]−1

detζ

  • −∇2

s

1/2 det′

ζ

  • −∇2

s + Rγ

1/2 dL2γ.

  • Proof. We have

pL

t (x, y)

et(x, y) ∼ (4πt)−k/2 ˆ

Γmin

xy

[γ1

0]−1

1 det

  • ∇2E|NγΓmin

xy

1/2 dH1γ ∼ (4πt)−k/2 ˆ

Γmin

xy

[γ1

0]−1 det

  • d
  • id : (Γmin

xy , L2) → (Γmin xy , H1)

  • det
  • ∇2E|NγΓmin

xy

1/2 dL2γ

Matthias Ludewig (Uni Potsdam) 11.02.16 19 / 24

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SLIDE 50

Let e1, . . . , ek be an L2-orthonormal basis of Γmin

xy . Then we have, setting

again P := −∇2

s

det

  • d
  • id : (Γmin

xy , L2) → (Γmin xy , H1)

  • Matthias Ludewig (Uni Potsdam)

11.02.16 20 / 24

slide-51
SLIDE 51

Let e1, . . . , ek be an L2-orthonormal basis of Γmin

xy . Then we have, setting

again P := −∇2

s

det

  • d
  • id : (Γmin

xy , L2) → (Γmin xy , H1)

  • = det
  • ei, ej
  • H1

1/2

1≤i,j≤k

Matthias Ludewig (Uni Potsdam) 11.02.16 20 / 24

slide-52
SLIDE 52

Let e1, . . . , ek be an L2-orthonormal basis of Γmin

xy . Then we have, setting

again P := −∇2

s

det

  • d
  • id : (Γmin

xy , L2) → (Γmin xy , H1)

  • = det
  • ei, ej
  • H1

1/2

1≤i,j≤k

= det

  • ∇sei, ∇sej
  • L2

1/2

1≤i,j≤k

Matthias Ludewig (Uni Potsdam) 11.02.16 20 / 24

slide-53
SLIDE 53

Let e1, . . . , ek be an L2-orthonormal basis of Γmin

xy . Then we have, setting

again P := −∇2

s

det

  • d
  • id : (Γmin

xy , L2) → (Γmin xy , H1)

  • = det
  • ei, ej
  • H1

1/2

1≤i,j≤k

= det

  • ∇sei, ∇sej
  • L2

1/2

1≤i,j≤k

= det

  • ei, Pej
  • L2

1/2

1≤i,j≤k

Matthias Ludewig (Uni Potsdam) 11.02.16 20 / 24

slide-54
SLIDE 54

Let e1, . . . , ek be an L2-orthonormal basis of Γmin

xy . Then we have, setting

again P := −∇2

s

det

  • d
  • id : (Γmin

xy , L2) → (Γmin xy , H1)

  • = det
  • ei, ej
  • H1

1/2

1≤i,j≤k

= det

  • ∇sei, ∇sej
  • L2

1/2

1≤i,j≤k

= det

  • ei, Pej
  • L2

1/2

1≤i,j≤k

Matthias Ludewig (Uni Potsdam) 11.02.16 20 / 24

slide-55
SLIDE 55

Let e1, . . . , ek be an L2-orthonormal basis of Γmin

xy . Then we have, setting

again P := −∇2

s

det

  • d
  • id : (Γmin

xy , L2) → (Γmin xy , H1)

  • = det
  • ei, ej
  • H1

1/2

1≤i,j≤k

= det

  • ∇sei, ∇sej
  • L2

1/2

1≤i,j≤k

= det

  • ei, Pej
  • L2

1/2

1≤i,j≤k

= det

  • P|TγΓmin

xy

1/2

Matthias Ludewig (Uni Potsdam) 11.02.16 20 / 24

slide-56
SLIDE 56

Hence in the splitting TγHxy(M) = TγΓmin

xy ⊕ NγΓmin xy

det

  • d
  • id : (Γmin

xy , L2) → (Γmin xy , H1)

  • det
  • ∇2E|NγΓmin

xy

1/2 = det

  • P|TγΓmin

xy

1/2 det

  • P −1(P + Rγ)|NγΓmin

xy

1/2

Matthias Ludewig (Uni Potsdam) 11.02.16 21 / 24

slide-57
SLIDE 57

Hence in the splitting TγHxy(M) = TγΓmin

xy ⊕ NγΓmin xy

det

  • d
  • id : (Γmin

xy , L2) → (Γmin xy , H1)

  • det
  • ∇2E|NγΓmin

xy

1/2 = det

  • P|TγΓmin

xy

1/2 det

  • P −1(P + Rγ)|NγΓmin

xy

1/2 = det

  • P −1|TγΓmin

xy

P −1(P + Rγ)|NγΓmin

xy

−1/2

Matthias Ludewig (Uni Potsdam) 11.02.16 21 / 24

slide-58
SLIDE 58

Hence in the splitting TγHxy(M) = TγΓmin

xy ⊕ NγΓmin xy

det

  • d
  • id : (Γmin

xy , L2) → (Γmin xy , H1)

  • det
  • ∇2E|NγΓmin

xy

1/2 = det

  • P|TγΓmin

xy

1/2 det

  • P −1(P + Rγ)|NγΓmin

xy

1/2 = det

  • P −1|TγΓmin

xy

P −1(P + Rγ)|NγΓmin

xy

−1/2 = det

  • P −1

id P + Rγ −1/2

Matthias Ludewig (Uni Potsdam) 11.02.16 21 / 24

slide-59
SLIDE 59

Hence in the splitting TγHxy(M) = TγΓmin

xy ⊕ NγΓmin xy

det

  • d
  • id : (Γmin

xy , L2) → (Γmin xy , H1)

  • det
  • ∇2E|NγΓmin

xy

1/2 = det

  • P|TγΓmin

xy

1/2 det

  • P −1(P + Rγ)|NγΓmin

xy

1/2 = det

  • P −1|TγΓmin

xy

P −1(P + Rγ)|NγΓmin

xy

−1/2 = det

  • P −1

id P + Rγ −1/2 =

  • det′

ζ(P + Rγ)

detζ(P) −1/2

Matthias Ludewig (Uni Potsdam) 11.02.16 21 / 24

slide-60
SLIDE 60

Therefore finally pL

t (x, y)

et(x, y) ∼ (4πt)−k/2 ˆ

Γmin

xy

[γ1

0]−1 det

  • d
  • id : (Γmin

xy , L2) → (Γmin xy , H1)

  • det
  • ∇2E|NγΓmin

xy

1/2 dL2γ = (4πt)−k/2 ˆ

Γmin

xy

[γ1

0]−1

detζ(P)1/2 det′

ζ(P + Rγ)1/2 dL2γ

  • Matthias Ludewig (Uni Potsdam)

11.02.16 22 / 24

slide-61
SLIDE 61

Wrapup

Matthias Ludewig (Uni Potsdam) 11.02.16 23 / 24

slide-62
SLIDE 62

Wrapup

For the quotient of one-dimensional path integrals, there is an "H1-picture", and an "L2-picture".

Matthias Ludewig (Uni Potsdam) 11.02.16 23 / 24

slide-63
SLIDE 63

Wrapup

For the quotient of one-dimensional path integrals, there is an "H1-picture", and an "L2-picture". For x close to y, we have pL

t (x, y)

et(x, y)

formally

= ffl

Hxy(M) e−E(γ)/2t Dγ

ffl

Hxy(Rn) e−E(γ)/2t Dγ ∼ det(∇2E|γxy)−1/2

det(∇2E|γRn

xy )−1/2

  • r

∼ det(−∇2

s + Rγxy)−1/2

detζ(−∇2

s)

Similar results hold in the degenerate case.

Matthias Ludewig (Uni Potsdam) 11.02.16 23 / 24

slide-64
SLIDE 64

Thank you for your attention!

Matthias Ludewig (Uni Potsdam) 11.02.16 24 / 24