ON HOLMES-THOMPSON AREA: HT VALUATION THEORY UNDER  MICROSCOPE

LOUIS YANG LIU

1.

Length and Related

The classic Crofton formula is 1 Length(γ) = 4

ˆ



ˆ



#(γ ∩ l(r, θ))dθdr 0

(1.1)

0

for any rectiable curve in Euclidean plane, where θ is the angle of the normal of the oriented line l to the x-axis and r is its distance to the origin. Let us denote the ane 1-Grassmannians (lines) in R2 by Gr1 (R2 ) . As for Minkowski plane, it is a normed two dimensional space with a norm F (·) = || · || , in which the unit disk is convex and F has some smoothness. Two of the key tools used to obtain the Crofton formula for Minkowski plane are the cosine transform and Gelfand transform. Let us explain them one by one rst and see their connection next. A fact from spherical harmonics about cosine transform is there is some even function on S 1 such that 1 F (·) = 4

ˆ

|hξ, ·i|g(ξ)dξ, S1

(1.2)

if F is an even C 4 function on S 1 . A good reference for this is [G]. As for Gelfand transform, it is the transform of dierential forms nand densities on double brations, o π1 π for instance, R2 ← I →2 Gr1 (R2 ), where I := (x, l) ∈ R2 × Gr1 (R2 ) : x ∈ l is the incidence relations and π1 and π2 are projections. A formula one can take as an example of the fundamental theorem of Gelfand transform is the following ˆ

ˆ π1∗ π2∗ |Ω| =

γ

#(γ ∩ l)|Ω|, l∈Gr1 (R2 )

(1.3)

where Ω := g(θ)dθ ∧ dr. But we give a direct proof here. Proof.

First, consider the case of Ω = dθ ∧ dr. For any v ∈ Tx γ , since there is some

v 0 ∈ Tx0 I , such that π1∗ (v 0 ) = v , then

Date : November 12, 2008. 1

2

LOUIS YANG LIU

(π1∗ π2∗ |Ω|)x (v)

=

´ ( π−1 (x) π2∗ |Ω|)x (v) ´ 1 (π2∗ |Ω|)x0 (v 0 ) −1 0 ´x ∈π1∗ (x) 0 1 (π |dθ ∧ dr|)(v ) ´S 2 0 1 |dr(π2∗ (v ))|dθ ´S |hv, θi|dθ S1

=

4|v|.

= = = =

´

´

(1.4)

So = 4Length(γ) = l∈Gr1 (R2 ) #(γ ∩ l)|Ω| by the classic Crofton formula. When Ω = f (θ)dθ ∧ dr, we just need to replace dθ by g(θ)dθ in the equalities in the rst case.  π π ∗ |Ω| γ 1∗ 2

Moreover, from the above proof and (1.2), for any curve γ(t) : [a, b] → R2 dierentiable almost everywhere in the Minkowski space, ˆ

ˆ

π1∗ π2∗ |Ω| = γ

ˆ

b

(π1∗ π2∗ |Ω|)(γ 0 (t))dt = a

b

4F (γ 0 (t))dt = 4Length(γ),

(1.5)

a

so then by (1.3) we know Length(γ) =

1 4

ˆ #(γ ∩ l)|g(θ)dθ ∧ dr| l∈Gr1 (R2 )

(1.6)

for Minkowski plane. The Holmes-Thompson Area HT 2 (U ) of a measurable set U in a Minkowski ´ plane is dened as HT 2 (U ) := π1 D∗ U |ω0 |2 , where ω0 is the natural symplectic  form on the cotangent bundle of R2 and D∗ U := (x, ξ) ∈ T ∗ R2 : F ∗ (ξ) ≤ 1 . To study it from the perspective of integral geometry, we need to introduce a symplectic form ω on the space of ane lines Gr1 (R2 ), that one can see [A].

2.

HT Area and Related

Now let's see the Crofton formula for Minkowski plane, which is Length(γ) = #(γ ∩ l)|ω|. To prove this, it is sucient to show that it holds for for any Gr1 (R2 ) straight line segment 1 4

´

L : [0, ||p2 − p2 ||] → R2 , L(t) = p1 +

p2 − p1 t, ||p2 − p1 ||

(2.1)

starting at p1 and ending at p2 in R2 . First, using the dieomorphism between the circle bundle and co-circle bundle, which is ϕF : SR2 → S ∗ R2 ϕF (x, ξ) = (x, dFξ ),

(2.2)

ON HOLMES-THOMPSON AREA: HT VALUATION THEORY UNDER  MICROSCOPE

we can obtain a fact that ´



n

p2 −p1 ||p2 −p1 ||

o

ϕ∗F α0

3

´

=

n o α p2 −p1 ϕF (L× ) 0 ´ ||p2 −p1 ||||p2 −p1 || −p1 α0dF p2 −p1 (( ||pp22 −p , 0))dt 0 1 || ||p2 −p1 || ´ ||p2 −p1 || 1 dF p2 −p1 ( ||pp22 −p −p1 || )dt, 0

= =

(2.3)

||p2 −p1 ||

where α0 is the tautological one-form, precisely α0ξ (X) := ξ(π0∗ X) for any X ∈ Tξ T ∗ R2 , and dα0 = ω0 . Applying the the basic equality that dFξ (ξ) = 1, which is derived from the positive homogeneity of F , for all ξ ∈ SR2 , the above quantity ´ becomes 0||p2 −p1 || 1dt, which equals to ||p2 − n p1 ||. o  ∗ 2 Let R := ξx ∈ S R : x ∈ p1 p2 and T = l ∈ Gr1 (R2 ) : l ∩ p1 p2 6= Ø , and p0 is the projection (composition) from S ∗ R2 to Gr1 (R2 ). Apply the above fact and p0∗ ω = ω0 , ´

T

´

|ω| =

p0 (R)

´

|ω| =

R

´

|p0∗ ω| =

= | = |

´R

|ω0 |

+ ´R

ω0 | + |

∂R+

´

α0 | + |

− R ´

ω0 |

∂R−

α0 |

(2.4)

4||p2 − p1 ||.

=

Thus we have shown the Crofton formula for Minkowski plane. Furthermore, combining with (1.6), we have 1 4

ˆ

#(γ ∩ l)|Ω| = l∈Gr1 (R2 )

1 4

ˆ

#(γ ∩ l)|ω|, Gr1 (R2 )

(2.5)

where Ω = g(θ)dθ∧dr. Then, by the injectivity of cosine transform in [G], |Ω| = |ω|. To obtain the HT area, one can dene a map ˜ → R2 π : Gr1 (R2 ) × Gr1 (R2 ) \ 4 π(l, l0 ) = l ∩ l0 ,

(2.6)

˜ := {(l, l0 ) : l k l0 or l = l0 }, extended from Alvarez's construction of taking where 4 intersections, [AF]. The following theorem can be obtained. Theorem 2.1.

HT 2 (U ) =

subset

U

Proof.

On one hand,

1 2π

´ x∈R2

χ(x ∩ U )|π∗ Ω2 |

for any bounded measurable

of a Minkowski plane.

ˆ ˆ 1 1 2 = ω = α0 ∧ ω0 . π ∂D∗ U 0 π S∗ U D∗ U n o On the other hand, let TU := ((l, l0 ) ∈ Gr1 (R2 ) × Gr1 (R2 ) : l ∩ l0 ∈ U , ˆ ˆ ˆ 1 1 1 χ(x ∩ U )π∗ Ω2 = π∗ ω 2 = ω2 . π x∈R2 π U π TU 1 π

ˆ

ω02

(2.7)

(2.8)

4

LOUIS YANG LIU

Let T∗ U := {(ξx , ξx0 ) : ξx , ξx0 ∈ Sx∗ U }, then (p0 × p0 )−1 (TU ) = T∗ U \ {(ξx , ξx ) : ξx ∈ Sx∗ U } .

Therefore

1 π

´ TU

ω2

= = = =

1 π 1 π 2 π 2 π

´ ∗ U \{(ξ

∗ x ,ξx ):ξx ∈Sx U }

∗ U \{(ξ

∗ x ,ξx ):ξx ∈Sx U }

´T ´T ´

∗U } {(ξx ,ξx ):ξx ∈Sx

S∗ U

p0∗ ω 2 ω02

α0 ∧ ω0

(2.10)

α 0 ∧ ω0 .

So the claim follows from (2.7),(2.8) and (2.10). Acknowledgement.

(2.9)



Thanks to Dr. Joseph H. G. Fu for some helpful advices.

References [A] J.C. Álvarez Paiva, Symplectic Geometry and Hilbert's Fourth Problem, J. Dierential Geom. Volume 69, Number 2 (2005), 353-378. [AF] J. C. Álvarez Paiva and E. Fernande, Crofton formulas for projective Finsler spaces, Electronic Research Announcements of the AMS, 4 (1998) 91-100. [G] H. Groemer, Geometric Applications of Fourier Series and Spherical Harmonics, Cambridge University Press, 1996.

On Holmes-Thompson Area: HT Valuation Theory ...

ON HOLMES-THOMPSON AREA: HT VALUATION THEORY. UNDER MICROSCOPE. LOUIS YANG LIU. 1. Length and Related. The classic Crofton formula is. Length(γ) = 1. 4. ˆ ∞. 0. ˆ 2π. 0. #(γ ∩ l(r, θ))dθdr. (1.1) for any rectifiable curve in Euclidean plane, where θ is the angle of the normal of the oriented line l to the ...

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