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The beta invariant of a flag and the conormal intersection theory In this section, we complete the proof that the degree of π ˚

In document arxiv: v3 [math.co] 29 Oct 2020 (Page 45-50)

S X T ‰ E The length of a biflag is the number of bisubsets in it.

Lemma 4.16. Suppose that the assumption of Lemma 4.15 holds for F|G.

4.4. The beta invariant of a flag and the conormal intersection theory In this section, we complete the proof that the degree of π ˚

pxFqδn´k´1 is equal to the β-invariant βMrFs. To prove by induction, we need a lemma relating the conormal fan of M with that of the contraction M {i, where i is any fixed element of E that has no parallel elements in M.

We may assume that M has no loops and no coloops. Thus, we have iKis the ground set E and i|E is a biflat of M. We consider the simplicial fan

sti|EΣM,MK Ď pNE{ eiq ‘ NE.

We write eSfor the image of eSin NE{ ei, and xF |Gfor the variable in the Chow ring of the star corresponding to a biflat F |G; we set it equal to 0 if F |G does not correspond to a ray in this star. Lemma 4.17. Consider the natural projection ψ : pNE{ eiq ‘ NE ÝÑ NE´i‘ NE´i.

(1) The projection ψ induces a morphism of fans

ψ : sti|EΣM,MK ÝÑ ΣM {i,pM {iqK.

(2) The pullback ψ˚between the Chow rings is given by ψ˚px

P |Qq “ xpP Yiq|Q` xpP Yiq|pQYiq, where at least one of the terms in the right-hand side is nonzero. (3) For any element j of E, the pullback ψ˚maps the class δ to the class

δ “ δj – X iPF, jPF XG

xF |G.

(4) The pullback ψ˚commutes with the degree maps of the star and the conormal fan Σ

M {i,pM {iqK:

degM {ixP|Q“ degMpxi|Eψ˚pxP|Qqq.

Proof. Let F |G be a biflat of M with i P F . The image of a ray corresponding to F |G in the star is ψpeF` fGq “ eF ´i` fG´i,

which is a ray of the conormal fan ΣM {i,pM {iqK because pF ´ iq|pG ´ iq is a biflat of M {i:

clM {ipF ´ iq “ clMpF q ´ i “ F ´ i, and

clMK´ipG ´ iq “ clMKpG ´ iq ´ i Ď clMKpGq ´ i “ G ´ i.

Furthermore, if i|E YF|G is a biflag of M, its gaps occur to the right of i|E, and there will also be gaps in the corresponding positions of the biflag

pF ´ iq|pG ´ iq –npF ´ iq|pG ´ iq o

F |GPF|G of M {i. Therefore, the projection ψ maps cones to cones. This proves the first statement.

The value of the piecewise linear function ψ˚x

P |Qon a ray eF` fGof the star is

ψ˚x

P |QpeF` fGq “ xP |QpeF ´i` fG´iqq “  

1 if F “ P Y i and G P {Q, Q Y i}, 0 if otherwise.

Since Q is a flat of M {i, at least one of Q and Q Y i is a flat of M, and we have the second statement. Given the second statement, the third statement is a straightforward computation

ψ˚ pδjq “ X jPP XQ  xpP Yiq|Q` xpP Yiq|pQYiq  “ X iPF, jPF XG xF |G“ δj,

where the first sum is over the biflats P |Q of M {i and the second sum over the biflats F |G of M. For the last statement, we need to verify that, for any maximal biflagP|Q of M {i,

degM {ixP|Q“ degMpxi|Eψ˚pxP|Qqq.

Applying the second statement to each P |Q inP|Q, we may express xi|Eψ˚px

P|Qqas a sum of square-free monomials. One of the terms in this expression is xi|ExpPYiq| clKpQq, where

pP Y iq| clKpQq – n

pP Y iq| clKpQq o

P |QPP|Q. We need to prove that this is the only nonzero term.

Consider any term xi|ExF|Gthat arises in the expression for xi|Eψ˚px

P|Qq. We automatically have Fj “ PjY ifor all j, so it remains to prove that Gjis the closure of Qjin MKfor all j. Let kbe the largest index satisfying i P clK

pQkq, so that

clKpQjq “ QjY i for j ď k and clKpQjq “ Qj for j ą k. For j ď k, the set Qjis not a flat in MK, and hence Gj

“ QjY i “ clKpQjq. Since Qkand Qk`1are flats of consecutive ranks in pM {iqK“ MK

´i, the flats QkY i “ clKpQkqand Qk`1“ clKpQk`1q of MKalso have consecutive ranks. Since Qk`1

Y iis strictly between the two, it cannot be a flat of MK. Thus, we must have Gk`1 “ Qk`1, and hence Gj “ Qj “ clKpQjqfor j ą k. We conclude thatF|G “ pP Y iq| clK

pQq as desired. 

We can now give an intersection-theoretic interpretation of the beta invariant of a flag. To- gether with the Vanishing Lemma4.15, it gives the identity degpπ˚px

Fq δn´k´1q “ βMrFs. Proposition 4.18. For any strictly increasing flagF of k nonempty proper flats of M, we have

degpxF|FKδn´k´1q “ βMrFs.

Proof. We proceed by induction on k. The base case k “ 0 follows from Proposition4.9: degpδn´1q “ deg

 X

BPβ-nbcpMq

xβ-conepBq“ βM.

When k is positive, write F |FKfor the first biflat inF|FK, and writeF|FKas the disjoint union F |FK \G|GK. We consider the contraction M {F , its flag of flatsG ´ F – {G ´ F }GPG, and the corresponding biflag pG ´ F q|pG ´ F qK – n pG ´ F q|pGK´ F q o GPG.

The displayed description is justified by GK

´ F “ clpM {F qKppE ´ F q ´ pG ´ F qq. Clearly,

βMrFs“ βM |F ¨ βpM {F qrG´F s.

We separately consider two cases, depending on the shortness of the first interval r∅, F s: Case 1. The flat F contains exactly one element i P E.

Recall that the beta invariant of r∅, is is equal to 1. Therefore, βMrFsis equal to βpM {iqrG´is “ degM {i xG´i|pG´iqKδpn´1q´pk´1q´1

M {i



by the inductive hypothesis, “ degM xi|Eψ˚px G´i|pG´iqKq δMn´k´1q  by Lemma4.17.3and4.17.4, “ degM xi|E Y GPG pxG|pGK´iq` xG|GKq δn´k´1M  by Lemma4.17.2. By the Vanishing Lemma4.15, the right-hand side simplifies to

degM xi|ExG|GMn´k´1“ degM xF|FMn´k´1.

Case 2. The flat F contains more than one element.

We may assume the interval r∅, F s is coloopless by Lemma4.15. This means that the flat F is cyclic, that is, FK“ E ´ F. We then have the natural bijections

φ1: n biflats of M |FoÝÑ n biflats F1 |G1of M with F1 Ď F and G1 Ě E ´ F o and φ2:nbiflats of M {FoÝÑ n biflats F1 |G1of M with F1 Ě F and G1 Ď E ´ F o ,

where φ1pA|Bq “ A|pB Y pE ´ F qqand φ2pA|Bq “ pA Y F q|B. The bijection φ1extends to the bi- jection between the biflags of M |F and the biflags of M that are supported on the corresponding set of biflats, and have a gap to the left of F |pE ´ F q. Similarly, the bijection φ2extends to the bi- jection between the biflags of M {F and the biflags of M that are supported on the corresponding set of biflats, and have a gap to the right of F |pE ´ F q.

We now compute the degree of xF|FKδn´k´1 using the following variant of the canonical

expansion of Definition4.1, which proceeds in two stages:

Stage 1. At each step, choose e to be the largest gap element that is in F , if there is one. Stage 2. At each step, choose e to be the largest gap element in E ´ F .

The first |F | ´ 2 steps of this computation will give xF|FK times the image under φ1 of the

canonical expansion of δM |F|F |´2. By Proposition4.9, there will be βM |F square-free monomials. Each such monomial will have a unique nonempty gap before F ; say it is Dj, between biflats Fj|Gjand Fj`1|Gj`1of M. The flats Fjand Fj`1have consecutive ranks, and the coflats Gjand Gj`1have consecutive coranks. In step |F | ´ 1 of the computation, this gap Dj will be filled in a unique way by the biflat Fj`1|Gj. There will no longer be gap elements in F .

In step |F |, the computation will enter Stage 2 for each of the resulting βM |F monomials. The following p|E ´ F | ´ 1q ´ pk ´ 1q ´ 1 steps will compute the image under φ2of the canonical

expansion of xpG´F q|pG´F qKδ|F |´2

M {F . This expansion has βpM {F qrG´F s square-free monomials, by the inductive hypothesis.

This concludes the computation of xF|FKδn´k´1. The result will be the sum of βMrFssquare-

free monomials, as we wished to prove. 

Proposition 4.19. LetF “ {F1Ĺ ¨ ¨ ¨ Ĺ Fk} be a strictly increasing flag of flats of M. We have degpπ˚pxFq δn´k´1q “ βMrFs.

Proof. Since π˚px

Fq “PF|G biflagxF|G, this follows from Lemma4.15and Proposition4.18. 

4.5. A conormal interpretation of the Chern–Schwartz–MacPherson cycles. Recall that the k- dimensional Chern–Schwartz–MacPherson cycle of M is the Minkowski weight csmkpMqon the Bergman fan of M defined by the formula

csmkpMqpσFq “ p´1qr´kβMrFs,

where σF is the k-dimensional cone corresponding to a flag of flatsF of M. Theorem1.1. When M has no loops and no coloops, we have

csmkpMq “ p´1qr´kπ˚pδn´k´1X 1M,MKq for 0 ď k ď r.

Proof. By Proposition4.19, Definition3.4, and the projection formula, we have

βMrFs“ degpπ˚pxFqδn´k´1q “ π˚pxFqδn´k´1X 1M,MK “ π˚pδn´k´1X 1M,MKqpσFq.

The result then follows from the definition of the Chern–Schwartz-MacPherson cycle of M.  Theorem1.2. When M has no loops and no coloops, we have

χMpq ` 1q “ r X

k“0

p´1qr´kdegpγkδn´k´1q qk.

Proof. We use [LdMRS20, Theorem 1.4], which states that χMpq ` 1q “

r X

k“0

αkX csmkpMq qk.

The authors of [AB20] give a non-recursive proof of the identity using tropical intersection the- ory. For representable matroids, the identity was given earlier in [Alu13, Theorem 1.2]. By Theorem1.1and the projection formula, the k-th coefficient of the displayed polynomial is

αkX π˚pδn´k´1X 1M,MKq “ π˚ π˚αkX pδn´k´1X 1M,MKq



“ π˚ γ

kδn´k´1

X 1M,MK.

In document arxiv: v3 [math.co] 29 Oct 2020 (Page 45-50)