This paper extends Arason's filtration to the Witt group of quadratic forms over general valued fields, linking it with Witt-like groups of the residue field, including totally singular forms, and recovers the classical case for discretely valued fields.
Contribution
It generalizes Arason's filtration to arbitrary valued fields and relates it to Witt-like groups of the residue field, including totally singular quadratic forms.
Findings
01
Constructed an extended Arason filtration for general valued fields.
02
Connected the filtration subgroups with Witt-like groups of the residue field.
03
Recovered the classical Arason filtration in the discretely valued case.
Abstract
Generalizing a theorem of Springer, we construct an extended Arason filtration by subgroups for the Witt group of quadratic forms of a general valued field, relating these subgroups with Witt-like groups of the residue field, in arbitrary characteristic. These Witt-like groups involve totally singular quadratic forms. In the case of a discretely valued field, we recover the original Arason filtration.
Equations232
Wq(F)tame→ΓF/2ΓF⨁Wq(F),
Wq(F)tame→ΓF/2ΓF⨁Wq(F),
(Wq(F)ε)ε∈E,
(Wq(F)ε)ε∈E,
Wq(F)0=Wq(F)tame
Wq(F)0=Wq(F)tame
Wq(F)<εWq(F)ε∼⎩⎨⎧⨁2∣ΓF/2ΓF∣Wssq(F)⨁ΓF/2ΓFWsq(F)⨁ΓF/2ΓFW(F)if ε∈/ΓFif ε∈ΓF and ε=v(2)if ε=v(2)
Wq(F)<εWq(F)ε∼⎩⎨⎧⨁2∣ΓF/2ΓF∣Wssq(F)⨁ΓF/2ΓFWsq(F)⨁ΓF/2ΓFW(F)if ε∈/ΓFif ε∈ΓF and ε=v(2)if ε=v(2)
Wg(F,ε)∼⎩⎨⎧⨁ΓF/2ΓFWq(F)⨁2∣ΓF/2ΓF∣Wssq(F)⨁ΓF/2ΓFWsq(F)⨁ΓF/2ΓFW(F)if ε=0if ε∈/ΓFif ε∈ΓF and ε=v(2) and ε=0if ε=v(2).
Wg(F,ε)∼⎩⎨⎧⨁ΓF/2ΓFWq(F)⨁2∣ΓF/2ΓF∣Wssq(F)⨁ΓF/2ΓFWsq(F)⨁ΓF/2ΓFW(F)if ε=0if ε∈/ΓFif ε∈ΓF and ε=v(2) and ε=0if ε=v(2).
Wsq(F)∼F∧F2F
Wsq(F)∼F∧F2F
bq(v,w)=q(v+w)−q(v)−q(w):
bq(v,w)=q(v+w)−q(v)−q(w):
(V,b)=(V1,b1)⊥⋯⊥(Vn,bn)⊥(W,b∣W),
(V,b)=(V1,b1)⊥⋯⊥(Vn,bn)⊥(W,b∣W),
(W,b∣W)=(W1′,b1′)⊥⋯⊥(Wr′,br′)
(W,b∣W)=(W1′,b1′)⊥⋯⊥(Wr′,br′)
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Arason’s filtration of the Witt group of dyadic valued fields.
Joachim Verstraete
Joachim Verstraete is a Research Fellow of the Fonds de la Recherche Scientifique - FNRS.
(March 9, 2024)
Abstract
Generalizing a theorem of Springer, we construct an extended Arason filtration by subgroups for the quadratic Witt group of a general valued field, relating these subgroups with Witt-like groups of the residue field, in arbitrary characteristic. These Witt-like groups involve totally singular quadratic forms. In the case of a discretely valued field, we recover the original Arason filtration.
A well-known result of Springer states that the Witt group of quadratic forms Wq(F) of a complete discretely valued field F is isomorphic to a direct sum of two copies of the Witt group of quadratic forms Wq(F) of the residue field F, provided that the residue characteristic is different from 2 (see [MR0070664]). Subsequently, that result has been generalized to Henselian valued fields F of residue characteristic different from 2, see for example the paper of
Tietze [MR0366809]. Tietze also considered the case when charF=2, and he obtained a similar isomorphism from a subgroup U(F)⊂Wq(F) onto a direct sum of copies of Wq(F). In their paper [MR1385276]
in 1996, Aravire and Jacob performed an exhaustive analysis of the Witt group of a dyadic maximally complete field with perfect residue field and showed that the description of the Witt group in that case is extremely delicate. More recently, Arason proposed,
in his note [RH-05-2016], another way to describe completely the Witt group of a discretely valued field by a filtration by subgroups, covering the case of residue characteristic 2. Our purpose in this paper is to obtain results similar to Arason’s, but for
general valued fields, by using techniques of [MR2836073] involving graded structures arising from the valuation. Our approach has the main advantage to employ more intrinsic methods than the computational ones of [RH-05-2016]. In particular, we
develop special Witt-like groups involving totally singular quadratic forms.
More precisely, our main results are the following (expressed in a similar way as [RH-05-2016]):
Let F be a field with a (not necessarily surjective) valuation v:F→Γ∪{∞}, where Γ is a totally ordered abelian group. Without loss of generality, we assume that Γ is divisible, since we may substitute for Γ its divisible hull. Denote by ΓF the value group of (F,v), i.e. ΓF=v(F×)⊂Γ, and let F denote the residue field of (F,v). Let Wq(F) (resp. W(F)) be the Witt group of (nonsingular)
quadratic forms (resp. the Witt group of (nondegenerate) symmetric bilinear forms) over F. Recall that Wq(F) can be identified with W(F) when 2 is invertible in F (to a symmetric bilinear form b, we associate the quadratic form given by x↦b(x,x)).
It is well-known (see for example [MR2836073]*Proposition 8 and Corollary 11) (but a proof of this fact will also be provided in the paper) that there always exists a subgroup Wq(F)tame⊂Wq(F) together with a group epimorphism
[TABLE]
which is an isomorphism when F is Henselian. That epimorphism depends on a choice of uniformizing parameters. When char(F)=2, we always have Wq(F)tame=Wq(F) and, when moreover F is Henselian, the
isomorphism (0.1) is Springer’s theorem. When char(F)=2, it turns out that Wq(F)tame equals the previously mentioned Tietze subgroup U(F), as shown in [MR2836073]*Corollary 17.
Let us now give some informal motivation for the next, but principal, result. If F is a dyadic (i.e., charF=2) Henselian valued field, the preceding isomorphism gives a description of Wq(F)tame. Therefore, it remains to describe the
quotient Wq(F)/Wq(F)tame (this quotient is called Wq(F)wild by Arason in [RH-05-2016] when F is a discretely valued field). It is the description of the structure of the wild part which motivates the following result. (Note that the result
does not require F to be Henselian).
(Main result) If char(F)=2, there exists an ascending filtration
[TABLE]
of Wq(F) by subgroups Wq(F)ε⊂Wq(F).
This filtration is called the Arason filtration of Wq(F) and satisfies
[TABLE]
Moreover, for each ε∈21ΓF such that 0<ε≤v(2),
there is a group isomorphism
[TABLE]
where
[TABLE]
and Wsq(F) along with Wssq(F) are two Witt-like groups of F, with Wssq(F)
nontrivial (see point 3 below). These isomorphisms depend on a choice of uniformizing parameters. Note that if char(F)=2, then v(2)=∞, hence E={ε∈21ΓF∣ε≥0}. Note also that if char(F)=2, then we have v(2)∈ΓF and Wq(F)v(2)=Wq(F) (since the filtration is increasing and covers Wq(F)).
In particular, if ΓF is a well-ordered group (i.e. ΓF≃Z as ordered groups), then for each φ∈Wq(F) there is a minimal ε≥0 such that φ∈Wq(F)ε. Under the same hypothesis, we also
have that Wq(F)<ε=Wq(F)γ for some γ∈E.
Moreover, for a,b∈F, denote by [a,b] the two-dimensional quadratic form q:F×F→F given by q(x1,x2)=ax12+x1x2+bx22.
Corollary 4.12 states that, for each ε∈21ΓF such that 0≤ε<v(2), Wq(F)ε is the subgroup of Wq(F) generated by the Witt classes of two-dimensional quadratic forms [a,b] with a,b∈F satisfying v(a)+v(b)≥−2ε. The condition ε<v(2) ensures that [a,b] is nonsingular. Note also that if F is Henselian and v(a)+v(b)>0, the proof of Lemma 5.3(e) shows that the
Witt class of [a,b] is [math].
Example 0.1**.**
Let k be a field of characteristic 2. Let F=k((t)) be the field of formal Laurent series in an indeterminate t with coefficients in k.
Equip F with the usual t-adic valuation v:F→Z∪{∞}, so that v(t)=1 and v(α)=0 for all α∈k⊂F.
Let also qW be the Witt class of a quadratic form q in Wq(F). It can be shown (by using Lemma 5.3(d)) that the induced map [x,x]W:F×F→Wq(F) is bi-additive since charF=2.
For this field F, we have an infinite ascending filtration of Wq(F) indexed by 21N :
[TABLE]
and the form [a,b]W (with a,b∈F) belongs to Wq(F)ε if (but not only if) v(a)+v(b)≥−2ε, for all ε∈21N.
Consider for example the quadratic form [1+t,t−1+t]. By bi-additivity of [x,x]W, we have
[TABLE]
Since v(1)+v(t)=1>0 and F is Henselian, it follows that [1,t]W=0. Similarly, [t,t]W=0.
We have [t,t−1]W∈Wq(F)tame (since v(t)+v(t−1)≥0), and [1,t−1]W∈Wq(F)1/2 (since v(1)+v(t−1)≥−1=−2⋅21). But it turns out that [1,t−1]W∈Wq(F)tame. (It is an application of
Corollary 5.2.)
Therefore
[TABLE]
Suppose now that α∈k×∖k×2. Then Corollary 5.2 shows as previously that [1,αt−2]W∈Wq(F)1∖Wq(F)1/2 ;
but note that [1,t−2]≃[1,t−1] (by the change of basis given by e1′=e1,e2′=e2+t−1e1, where e1,e2 is the standard basis of [1,t−2]), so that [1,t−2]W=[1,t−1]W∈Wq(F)1/2. ∎
Example 0.2**.**
*This example uses the same notations as Example 0.1. The residue field F of F=k((t)) for the t-adic valuation v is canonically isomorphic to k.
Consider the nonsingular quadratic form [t,t−1] over F. By Lemma 5.3(c), that form is isometric to the form q1:=t[1,1], that is the quadratic form given for all (x1,x2)∈F×F by
[TABLE]
Its nondegenerate associate polar bilinear form bq1 is given for all (x1,x2),(y1,y2)∈F×F by
[TABLE]
Under the group isomorphism Wq(F)tame→Wq(k)⊕Wq(k), the Witt class q1,W is sent to (0,q1,W′), where q1′ is the nonsingular quadratic form over k given for all (x1,x2)∈k×k
[TABLE]
Its nondegenerate associate polar bilinear form bq1′ is given for all (x1,x2),(y1,y2)∈k×k by
[TABLE]
*Similarly, under the same map, the Witt class [1,1]W is sent to (q1,W′,0). (See Theorem 4.9 and Proposition 3.5 (or Corollary 3.6) for the exact description of the map.)
Consider now the nonsingular quadratic form [1,αt−2] for some arbitrary α∈k×∖k×2. It is isometric to the quadratic form q2 given for all (x1,x2)∈F×F
[TABLE]
Its nondegenerate associate polar bilinear form bq2 is given for all (x1,x2),(y1,y2)∈F×F by
[TABLE]
Under the group isomorphism Wq(F)1→Wsq(k)⊕Wsq(k), the Witt class q2,W is sent to (ΦW,0), where ΦW is the Witt class in Wsq(k) of a symplectic quadratic spaceΦ=(q2′,bq2′) (see
Definition 2.1 for a precise definition). That space is made up, partly, of
a quadratic form q2′ over k, induced by q2, which is given for all (x1,x2)∈k×k by
[TABLE]
Therefore, q2′ is a totally singular quadratic form.
But the bilinear form bq2 yields, after scaling by t−1, the nondegenerate alternating bilinear form bq2′ over k given for all (x1,x2),(y1,y2)∈k×k by
[TABLE]
*Similarly, under the same map, the Witt class of the form t[1,αt−2] is sent to (0,ΦW). (See Theorem 4.9 and Proposition 3.5 (or Corollary 3.6) for the exact description of the map.)
Note also that, by Lemma 5.3(c), the quadratic form [1,t−1], which satisfies [1,t−1]W∈Wq(F)1/2∖Wq(F)0, is such that t[1,t−1]≃[1,t−1]. ∎
Example 0.3**.**
Let F=Q2 be the field of dyadic numbers equipped with the usual 2-adic valuation, so that v(2)=1. Its residue field is F=F2, the finite field with two elements. In this case, we have a 3-step filtration
[TABLE]
Consider the one-dimensional nonsingular quadratic form q over F given for all x∈F by
[TABLE]
which can be identified (since charF=2) with the nondegenerate symmetric bilinear form b given for all x,y∈F by
[TABLE]
Under the group isomorphism ∂1:Wq(F)1→W(F)⊕W(F), the Witt class qW is sent to (b′W,0), where b′ is the nondegenerate one-dimensional symmetric bilinear form over F2
given for all x,y∈F2 by
[TABLE]
Its associate totally singular quadratic form qb′ over F2 is given for all x∈F2 by
[TABLE]
*Similarly, under the same map, the Witt class of the form 2q is sent to (0,bW′). (See Theorem 4.9 and Proposition 3.5 (or Corollary 3.6) for the exact description of the map.)
But now consider the two-dimensional nonsingular quadratic form q⊥q over F given for all (x1,x2)∈F×F by
[TABLE]
which can be identified with the nondegenerate symmetric bilinear form b⊥b given for all (x1,x2),(y1,y2)∈F×F by
[TABLE]
Under the group isomorphism ∂1:Wq(F)1→W(F)⊕W(F), the Witt class (q⊥q)W is sent to ((b⊥b)′W,0), where (b⊥b)′ is the nondegenerate two-dimensional symmetric bilinear form
over F2 given for all (x1,x2),(y1,y2)∈F2×F2 by
[TABLE]
The vector (1,1) is clearly an isotropic vector for (b⊥b)′, so that (b⊥b)′ is metabolic.111Note that it is a general fact that, when charF=2, the Witt group W(F) is a 2-torsion group. Hence (q⊥q)W∈ker∂1=Wq(F)1/2. But it turns out that (q⊥q)W∈Wq(F)tame (see Lemma 5.3(e) and Corollary 5.2). ∎
In this paper, each of the preceding homomorphisms (see (0.1) and (0.2)) will be obtained from a composition of two group homomorphisms. The first one is a canonical epimorphism (depending on ε∈E, but not on a
choice of uniformizing parameters)
[TABLE]
whose kernel is Wq(F)<ε when ε>0. The image Wg(F,ε) of the map is a Witt-like group of the graded field grv(F) associated with the filtration of F defined by v. That first canonical epimorphism is followed by
an isomorphism which, in contrast, does depend on a choice of uniformizing parameters: for each ε∈21ΓF such that 0≤ε≤v(2), we have
[TABLE]
Informally, the groups Wg(F,ε) can be thought of as groups containing all the residue forms “in a canonical way”, whereas their descriptions as groups over the residue field depend on a choice of uniformizing parameters.
Suppose charF=2. Then there are group isomorphisms
[TABLE]
(in particular Wssq(F) is nontrivial). Here F2⊂F is the subfield of squares in F.
The structure of the paper is the following. In Section 1, we introduce the basics about the Witt-like groups of graded fields. Section 2 is devoted to the proof of the isomorphisms Wsq(F)∼F∧F2F and Wssq(F)∼F⊗F2F for an arbitrary field F of characteristic 2, which are precisely Theorem 2.3 and Theorem 2.9. In Section 3, we establish isomorphisms between the Witt-like groups (dealt with in
Section 1) of a graded field F and Witt-like groups of F0, the subfield of F consisting of [math] and all the nonzero homogeneous elements of degree [math]. These last isomorphisms depend on a choice of
uniformizing parameters. See Corollary 3.6 of Proposition 3.5, and see also Proposition 3.8. In particular, the proof of the isomorphisms (0.4) follows directly from the results of this section. The
construction of Arason’s filtration and the canonical epimorphism (0.3) is treated in Section 4, see Theorem 4.9. Finally, in the last section, we recover Arason’s results in the case that F is a discretely valued field, with our
methods (Corollary 5.2).
1 Shifted quadratic spaces
Let Γ be a divisible torsion-free abelian group. A Γ-graded commutative ring in which every nonzero homogeneous element is invertible is called a Γ-graded field, and a Γ-graded module over a Γ-graded
field is called a Γ-graded vector space. Since Γ is torsion-free, Γ-graded fields are domains and Γ-graded vector spaces are free modules. The rank of a graded vector space is called its dimension. For
more information, see for example [MR3328410]*§2.1. In this section, F is a Γ-graded field and V denotes an arbitrary finite-dimensional Γ-graded F-vector space. We write ΓF={γ∈Γ∣Fγ={0}} for the grade set of F, where Fγ denotes the additive abelian subgroup of F consisting of [math] and all the nonzero
homogeneous elements of degree γ. A similar notation is used for Γ-graded modules.
For ε∈Γ, an ε-shifted graded bilinear form on V is an F-bilinear map b:V×V→F such that for all γ,δ∈Γ, we have
b(Vγ,Vδ)⊂Fγ+δ+ε. Such a form is called nondegenerate if the only x∈V such that b(x,y)=0 for all y∈V is x=0. When ε=0, we
call b a graded bilinear form.
A graded quadratic form on V is a map q:V→F satisfying the following conditions involving q and its polar formbq:V×V→F defined for all v,w∈V by
[TABLE]
q(αx)=α2q(x) for all x∈V, for all α∈F
2. 2.
bq is a graded bilinear form on V
3. 3.
q(Vγ)⊂F2γ for all γ∈Γ.
The graded quadratic form q is called nonsingular if its polar form bq is nondegenerate. It is called totally singular when q(v+w)=q(v)+q(w) for v,w∈V.
Definition 1.1**.**
Let ε∈Γ. An ε-shifted quadratic space on V is a 3-tuple (V,q,b) where q is a graded quadratic form and b is a nondegenerate ε-shifted graded symmetric bilinear form
such that there exists α∈F satisfying bq=αb. We call α a multiplier of (V,q,b). Note that α=0 is allowed.
The trivialε-shifted quadratic space over F, denoted by [math], is the ε-shifted quadratic space (V,q,b) such that V=0.
Observe that if an ε-shifted quadratic space is not trivial, then the multiplier α is uniquely determined since b is nondegenerate222Every α∈F is a multiplier of the trivial ε-shifted quadratic space [math]..
Observe also that if α=0, then α is homogeneous and ε=−deg(α). In the rest of the text, we will refer to the existence of the multiplier as the “compatibility condition”. Here are the three main classes of ε-shifted
quadratic spaces we are interested in.
Example 1.2**.**
(i) Given F and ε∈Γ, an ε-shifted quadratic space (V,q,b) over F is called an ε-shifted (quadratic) space of type I over F if it satisfies the additional
conditions ε=0 and b=bq (i.e. α=1 is a multiplier), or if it is trivial.
(ii) Given F and ε∈Γ, an ε-shifted quadratic space (V,q,b) over F is called an ε-shifted (quadratic) space of type II over F if q is totally singular and b
is alternating. In this case, α=0 can always be chosen as a multiplier. Those spaces are also called ε-shifted graded symplectic quadratic spaces over F.
(iii) Given F and ε∈ΓF and a nonzero homogeneous τ∈Fε, an ε-shifted quadratic space (V,q,b) over F is called ε-shifted
(quadratic) space of type τ−III over F, if we have q(v)=τ−1b(v,v) for all v∈V. Here α=2τ−1 is always a multiplier since bq(v,w)=q(v+w)−q(v)−q(w)=2τ−1b(v,w) for all v,w∈V.
Note that an ε-shifted quadratic space can belong to more than one of the three classes of Example 1.2, and therefore can be of more than one typeT∈{I,II,τ−III∣τ∈Fε×}.
Two ε-shifted quadratic spaces (V,q,b) and (V′,q′,b′) over F with a common multiplier are isometric if there is a (degree-preserving) graded F-linear isomorphism L:V→V′ which commutes with both q, q′ and b, b′. The orthogonal sum of two ε-shifted quadratic spaces (V,q,b) and (V′,q′,b′) with a common multiplier α is defined in the obvious way. It is an ε-shifted quadratic space of multiplier α again. It is important to note that if (V,q,b) is an ε-shifted quadratic space and if V1 and V2 are graded subspaces of V such that V=V1⊕V2 and b=b∣V1⊥b∣V2, then we automatically get q=q∣V1⊥q∣V2 by the compatibility condition. Note also that the three classes of Example 1.2 are
closed under orthogonal sums.
An ε-shifted quadratic space (V,q,b) is isotropic if there exists a nonzero v∈V such that q(v)=0=b(v,v), and such a nonzero v is called an isotropic vector (if there is no isotropic vector, the space (V,q,b) is anisotropic). Observe that an isotropic space has always a homogeneous isotropic vector. Indeed, since Γ is torsion-free, we can give it a total order (see for example [MR3328410]*Remark 2.2), turning it into a
totally ordered abelian group. Therefore, for an isotropic vector ∑γ∈Γvγ(with vγ∈Vγ), the vγ′ component, where γ′ is the smallest γ∈Γ such that
vγ=0, is clearly isotropic. An ε-shifted quadratic space (V,q,b) is metabolic if it contains a graded subspace L⊂V of dimension dimL=21dimV such that
q(L)={0}=b(L,L). Such a space is called a Lagrangian of (V,q,b). The orthogonal sum of two metabolic spaces is also metabolic (a Lagrangian can be chosen as the direct sum of the Lagrangians).
Besides, for every ε-shifted quadratic space (V,q,b), the orthogonal sum (V,q,b)⊥−(V,q,b) is metabolic (since {(v,v)∣v∈V} is a Lagrangian), where −(V,q,b):=(V,−q,−b).
Example 1.3**.**
(i) An ε-shifted quadratic space (V,q,b) of type I can be identified with a graded quadratic space (V,q). This identification preserves orthogonal sum and isotropy. Moreover, metabolic graded spaces of type I are
metabolic graded quadratic spaces, which are in fact hyperbolic graded quadratic spaces.
(ii) An ε-shifted quadratic space (V,q,b) of type II is isotropic if and only if q is isotropic.
(iii) An ε-shifted quadratic space (V,q,b) of type τ−III can be identified with a nondegenerate graded symmetric bilinear space (V,τ−1b). This identification preserves orthogonal sum, isotropy and metabolicity.
1.1 Normalisation
Lemma 1.4** (Normalisation).**
Let ε∈Γ and b:V×V→F a nondegenerate ε-shifted graded symmetric bilinear form. The space (V,b) can be decomposed as
[TABLE]
where (Vi,bi) is a one-dimensional nondegenerate ε-shifted graded symmetric bilinear graded subspace of (V,b) for all i=1,…,n (with n possibly equal to [math]) and W⊂V is a graded
subspace such that b∣W is a nondegenerate ε-shifted graded alternating symmetric bilinear form. Consequently, n=0 if b is alternating, and W={0} if b is anisotropic. Moreover, W has a
homogeneous basis e1,f1,…,er,fr for some r≥0 such that
b(ei,fj)=δi,j* for all i,j=1…,r (in particular: degei+degfi+ε=0 for i=1…,r)*
2. 2.
b(ei,ej)=b(fi,fj)=0* for all i,j=1,…,r.*
We call such a basis for (W,b∣W) a homogeneous symplectic basis. It induces a decomposition into two-dimensional spaces:
[TABLE]
where Wi′=span⟨ei,fi⟩⊂V and bi′=b∣Wi′ for all i=1,…,n.
Proof.
The existence of the first decomposition is well-known for an (ungraded) symmetric bilinear space (V′,b′) when b′ is nondegenerate. See for example [MR2427530]*Corollary 1.9. The graded case is similar. The existence of a symplectic basis is
well-known for a (ungraded) bilinear space (W′,b′) when b′ is nondegenerate and alternating. See for example [MR2427530]*Proposition 1.8. The graded case is similar.
∎
Note that we can deduce from Lemma 1.4 a corresponding decomposition for an ε-shifted quadratic space (V,q,b) by the compatibility condition.
1.2 Witt decomposition
Proposition 1.5**.**
Let ε∈Γ. Every ε-shifted quadratic space (V,q,b) can be decomposed as follows: (V,q,b)≃φan⊥μ1⊥⋯⊥μn, where φan
is a uniquely determined (up to isometry) anisotropic ε-shifted quadratic space and μi is a metabolic two-dimensional ε-shifted quadratic space for all i∈{1,…,n} (with n possibly equal to [math]). Moreover, if (V,q,b) is metabolic, then φan=0.
Proof.
This result is well-known for (ungraded) nondegenerate symmetric bilinear spaces (V,b), see for example [MR2427530]*Theorem 1.27. The case of graded nondegenerate symmetric bilinear spaces (V,b) is similar since an isotropic
vector for b can always be chosen homogeneous. Adapting the proof to ε-shifted quadratic spaces (V,q,b) is straightforward, because the orthogonality for b implies the orthogonality for bq by the compatibility condition.
∎
Note that the decomposition given in Proposition 1.5 preserves the type, i.e. if φ is an ε-shifted quadratic space of type T (T∈{I,II,τ−III∣τ∈Fε×}), then φan and
all the μi (i=1,…,n) are also of type T.
Mimicking the usual construction, for every ε∈Γ and every type T∈{I,II,τ−III∣τ∈Fε×}, we may define a Witt equivalence of ε-shifted quadratic spaces of type T over a given
graded field F and endow the set WTε(F) of Witt-equivalence classes of ε-shifted quadratic spaces of type T over F with a group structure using the orthogonal sum. Then each equivalence
class is represented by a unique anisotropic space by Proposition 1.5333Clearly, this construction works in general for ε-shifted quadratic spaces of the same multiplier α..
After canonical identifications, we have WI0(F)=Wq(F), which is the quadratic Witt group of F, and Wτ−IIIε(F)=W(F), which is the Witt group of F. Moreover, we
also write Wsqε(F)=WIIε(F) for the Witt group of ε-shifted graded symplectic quadratic spaces.
2 Separated and nonseparated symplectic quadratic spaces
In this section, F is a field of characteristic 2 and V is an arbitrary finite-dimensional F-vector space.
2.1 Symplectic quadratic spaces
Definition 2.1**.**
A symplectic quadratic space over F is a [math]-shifted graded symplectic quadratic space (V,q,b) over F considered as a Γ-graded field with Γ=0.
In other words, (V,q,b) is a symplectic quadratic space if q is a totally singular quadratic form on V and b is a nondegenerate alternating bilinear form on V. As a special case of Lemma 1.4, such a space always admits a symplectic
basis e1,f1,…,er,fr for some r≥0. By Proposition 1.5, we can form a Witt group of symplectic quadratic spaces over F, which will be denoted by Wsq(F).
2.1.1 Structure
For α,α′∈F, we denote by ⟨α,α′⟩ the two-dimensional symplectic quadratic space (F×F,q,b) where q((1,0))=α, q((0,1))=α′ and b((1,0),(0,1))=1. The basis (1,0), (0,1) is called the
standard basis of ⟨α,α′⟩. Note that we use the notation ⟨x,x⟩ instead of the usual square brackets notation [x,x] since this last notation will be used
hereunder (see Corollary 4.12) with another meaning.
Lemma 2.2**.**
For all α,α′,β,β′∈F, and for all ξ∈F×,
⟨α,α⟩* is metabolic*
2. 2.
⟨α,ξ2α′⟩≃⟨ξ2α,α′⟩**
3. 3.
⟨α,α′⟩⊥⟨β,β′⟩≃⟨α+β,α′⟩⊥⟨β,α′+β′⟩.
Proof.
We show (3). If e1,f1 is the standard basis of ⟨α,α′⟩ and e2,f2 the one of ⟨β,β′⟩, then e1+e2 and f1 spans a subspace ⟨α+β,α′⟩ with orthogonal
complement the subspace ⟨β,α′+β′⟩ spanned by e2 and f1+f2. The rest of the proof is left to the reader.
∎
By Lemma 2.2, the map F×F→Wsq(F) which sends (α,α′) to ⟨α,α′⟩ induces a well-defined group homomorphism
[TABLE]
Theorem 2.3**.**
Φ* is an isomorphism.*
Proof.
Since every symplectic quadratic space is a sum of two-dimensional spaces, Φ is surjective. So, we only have to prove that Φ is injective. We begin by proving that if α,α′,β,β′∈F are such that ⟨α,α′⟩≃⟨β,β′⟩, then α∧α′=β∧β′. Let e,f be the standard basis of ⟨α,α′⟩=(V,q,b). Given that ⟨α,α′⟩≃⟨β,β′⟩, we can find vectors x,y∈V such that
[TABLE]
Write x=x1e+x2f and y=y1e+y2f with x1,x2,y1,y2∈F. The previous relations give
[TABLE]
Therefore,
[TABLE]
Now, we show that if α1,α1′,…,αn,αn′∈F are such that ⟨α1,α1′⟩⊥⋯⊥⟨αn,αn′⟩ is isotropic, then we can rewrite α1∧α1′+⋯+αn∧αn′ as a sum of n−1 products. We prove this assertion by induction on n. Suppose that the statement is true for the sums of n−1 terms. Let x∈V be an isotropic vector for ⟨α1,α1′⟩⊥⋯⊥⟨αn,αn′⟩=(V,q,b). We can assume that in the expression x=x1+⋯+xn with xi∈⟨αi,αi′⟩, each xi=0; otherwise we are done by the induction hypothesis. We may then find yi∈⟨αi,αi′⟩ such that xi,yi is a symplectic basis. By putting βi=q(xi) and βi′=q(yi), we have ⟨αi,αi′⟩≃⟨βi,βi′⟩, hence by the first part of the proof αi∧αi′=βi∧βi′. Then,
[TABLE]
Since x is isotropic, β1+⋯+βn=0, which proves the assertion. To complete the proof, we show by induction on n that if Φ(∑i=1nαi∧αi′)=0, then ∑i=1nαi∧αi′=0. This
is clear in the case n=1, for if ⟨α,α′⟩ is metabolic, then ⟨α,α′⟩≃⟨β,0⟩ for some β∈F, thus by the first part of the proof α∧α′=β∧0=0. If
n>1 and Φ(∑i=1nαi∧αi′)=0, then ⟨α1,α1⟩⊥⋯⊥⟨αn,αn′⟩ is metabolic, therefore isotropic and we can rewrite ∑i=1nαi∧αi′ as a sum of n−1 terms. By the induction hypothesis, we have ∑i=1nαi∧αi′=0.
∎
The proof of Theorem 2.3 is inspired by [RH-18-2006]*page 4.
2.2 Separated symplectic quadratic spaces
The dual of an arbitrary finite-dimensional F-vector space E is denoted by E∗. If L:E→G is a linear map between two F-vector spaces E and G, we denote by L∗:G∗→E∗ the dual map of L. If U⊂E is a
subspace, we write Uo={φ∈E∗∣φ(u)=0 for all u∈U} for the subspace in E∗ which is orthogonal to U. If e1,…,en is a basis of E, then the notation e1∗,…,en∗ refers to its dual basis in E∗.
Definition 2.4**.**
A separated symplectic quadratic space (over F) is a 3-tuple (V,q,q′) where q is a totally singular quadratic form on V and q′ is a totally singular quadratic form on V∗.
Two separated symplectic quadratic spaces (V1,q1,q1′) and (V2,q2,q2′) are isometric if there exists an F-linear isomorphism L:V1→V2 such that L is an isometry between q1 and q2, and L∗ is an isometry
between q2′ and q1′. The orthogonal sum of two spaces is defined in the obvious way (note that (V1⊕V2)∗ identifies with V1∗⊕V2∗). A separated symplectic quadratic space (V,q,q′) is isotropic if q or q′
is isotropic, and it is metabolic if it contains a subspace U⊂V such that q(U)={0}=q′(Uo). Such a space U is called a Lagrangian444There is no condition on the dimension of U. of (V,q,q′). The orthogonal sum of
two metabolic spaces is also metabolic (the direct sum of the Lagrangians is a Lagrangian). Besides, for every separated symplectic quadratic space (V,q,q′), the orthogonal sum (V,q,q′)⊥(V,q,q′) is metabolic since {(v,v)∣v∈V} is a
Lagrangian.
2.2.1 Symplectic quadratic spaces and separated symplectic quadratic spaces
In this paragraph, we define a functor U from separated symplectic quadratic spaces to symplectic quadratic spaces.
Given a separated symplectic quadratic space Φ=(V,q,q′), we put U(Φ)=(V⊕V∗,q⊥q′,b) where b:(V⊕V∗)×(V⊕V∗)→F is the nondegenerate alternating bilinear form defined by b((v,φ),(w,ψ))=ψ(v)−φ(w). That is indeed a symplectic quadratic space. Besides, if L:Φ→Ψ is an isometry between two separated symplectic quadratic spaces Φ and Ψ, then U(L):=L⊕L∗ is an isometry U(L):U(Φ)→U(Ψ). It is also easy to see that U(Φ⊥Ψ)≃U(Φ)⊥U(Ψ), and if Φ is metabolic then U(Φ) is also metabolic, since if L is a Lagrangian for Φ then L⊕Lo is a Lagrangian for U(Φ). Finally, if x∈V (or φ∈V∗) is an isotropic vector for Φ, then (x,0) (or (0,φ)) is an isotropic vector for U(Φ).
2.2.2 Normalisation
For α,α′∈F, we denote by ⟨α∣α′⟩ the one-dimensional separated symplectic quadratic space (F,q,q′) where q(1)=α and q′(1∗)=α′. The basis 1 is called the standard basis of ⟨α∣α′⟩.
Remark 2.5*.*
For α,α′,β,β′∈F, consider the two separated symplectic quadratic spaces ⟨α∣α′⟩ and ⟨β∣β′⟩. Let ⟨α∣α′⟩=(V1,q1,q1′). We have ⟨α∣α′⟩≃⟨β∣β′⟩ if and only if there exists a nonzero vector x∈V1 such that q1(x)=β and q1′(x∗)=β′.
Lemma 2.6** (Normalisation).**
Every separated symplectic quadratic space (V,q,q′) splits up into an orthogonal sum of one-dimensional separated symplectic quadratic spaces. More precisely, there exist α1,α1′,…,αn,αn′∈F such that
[TABLE]
Proof.
The proof can be obtained by a variant of the proof of the existence of a symplectic basis in Lemma 1.4. If dimV>0, take a nonzero e∈V and a φ∈V∗ such that φ(e)=1 and write U=span⟨e⟩⊂V. Then decompose (V,q,q′)≃(U,q∣U,q∣U∗′)⊥(kerφ,q∣kerφ,q∣(kerφ)∗′), where (U,q∣U,q∣U∗′)≃⟨α∣α′⟩ for α=q∣U(e) and α′=q∣U∗′(φ∣U).
∎
2.2.3 Witt decomposition
Proposition 2.7**.**
Every separated symplectic quadratic space (V,q,q′) can be decomposed as follows: (V,q,q′)≃φan⊥μ1⊥⋯⊥μn, where φan is a uniquely determined (up to isometry)
anisotropic separated symplectic quadratic space and μi is a metabolic line for all i∈{1,…,n} (with n possibly equal to [math]). Moreover, if (V,q,q′) is metabolic, then φan=0.
Proof.
The proof is a refinement of the proof of Proposition 1.5 (when Γ=0) taking into account the separation of U(V,q,q′) into the two particular spaces V and V∗.
∎
As for symplectic quadratic spaces, we may define a Witt equivalence of separated symplectic quadratic spaces over a given field F and endow the set Wssq(F) of Witt-equivalence classes with a group structure using the orthogonal sum. Then each
equivalence class is represented by a unique anisotropic space by Proposition 2.7.
2.2.4 Structure
Lemma 2.8**.**
For all α,α′,β,β′∈F, and for all ξ∈F×,
⟨α∣ξ2α′⟩≃⟨ξ2α∣α′⟩**
2. 2.
⟨α∣α′⟩⊥⟨β∣β′⟩≃⟨α+β∣α′⟩⊥⟨β∣α′+β′⟩.
Proof.
For (2), note that if e1 is the standard basis of ⟨α∣α′⟩ and e2 the one of ⟨β∣β′⟩, then the basis (e1+e2,e2), whose dual basis is (e1∗,e1∗+e2∗), gives the result. (1) is left
to the reader.
∎
By the previous lemma, the map F×F→Wssq(F) which sends (α,α′) to ⟨α∣α′⟩ induces a well-defined group homomorphism
[TABLE]
Theorem 2.9**.**
Φ* is an isomorphism.*
Proof.
The proof uses the same ideas as the proof of Theorem 2.3. For example, we prove that if α,α′,β,β′∈F are such that ⟨α∣α′⟩≃⟨β∣β′⟩, then α⊗α′=β⊗β′. Let e be the standard basis of ⟨α∣α′⟩=(V,q,q′). Given that ⟨α∣α′⟩≃⟨β∣β′⟩, we can find a vector x∈V such that
[TABLE]
Let’s write x=ξe and e∗=ξx∗ with x1∈F×. The previous relations give
[TABLE]
Therefore,
[TABLE]
Now, we show by induction on n that if α1,α1′,…,αn,αn′∈F are such that ⟨α1∣α1′⟩⊥⋯⊥⟨αn∣αn′⟩ is isotropic, then we can rewrite α1⊗α1′+⋯+αn⊗αn′ as a sum of n−1 products. Suppose that the statement is true for the sums of n−1 terms. Let x be an isotropic vector for ⟨α1∣α1′⟩⊥⋯⊥⟨αn∣αn′⟩=(V,q,q′). Suppose x∈V (the case x∈V∗ is similar). We can assume that in the expression x=x1+⋯+xn with xi∈⟨αi∣αi′⟩, each xi=0. Therefore x1,…,xn is a basis V.
Let x1∗,…,xn∗∈V∗ be its dual basis. By putting βi=q(xi) and βi′=q′(xi∗), we have ⟨α∣α′⟩≃⟨β∣β′⟩, hence by the first part of the proof αi⊗αi′=βi⊗βi′. Then, we conclude the induction as in Theorem 2.3. The rest of the proof is left to the reader.
∎
The functor U of § 2.2.1 induces a group homomorphism Wssq(F)→Wsq(F) which fits in the following commutative diagram, where the left vertical arrow is canonical.
[TABLE]
3 Structure of the Witt group of shifted spaces of type T
This section is built upon the work of Elomary and Tignol ([MR2836073]*Section 2) in which the case of graded quadratic spaces is already handled.
Throughout the section, we use the same notation as in Section 1. In particular, F is a Γ-graded field and V denotes an arbitrary finite-dimensional Γ-graded F-vector space. The grade set
of V is ΓV={γ∈Γ∣Vγ=0}. It is a union of cosets of ΓF. For γ∈Γ, we put [γ]=γ+ΓF∈Γ/ΓF and we define
[TABLE]
Clearly, V[γ] does not depend on the representative γ and is a graded subspace of V such that dimFV[γ]=dimF0Vγ+δ for all δ∈ΓF. Moreover, we have
[TABLE]
which is called the canonical decomposition of V.
For the rest of this section, we fix some ε∈Γ. By an ε-shifted space of type T over F, we mean an ε-shifted quadratic space over F of type I, II or τ−III for some τ∈Fε×. Note that if (V,q,b) is an ε-shifted space of type T and v∈V, then v is isotropic if and only if q(v)=0, hence (V,q,b) anisotropic implies ΓV⊂21ΓF.
Note also that if (V,q,b) is an ε-shifted space of type I or τ−III, then we always have ε∈ΓF≤21ΓF by definition.
Lemma 3.1**.**
Suppose (V,q,b) is a nonzero anisotropic ε-shifted symplectic quadratic space. Let e,f∈V be homogeneous elements such that b(e,f)=1. Then
ε∈21ΓF**
2. 2.
dege* and degf are in the same equivalence class in 21ΓF/ΓF if and only if ε∈ΓF.*
Proof.
The lemma follows from the equation dege+degf+ε=0, since dege,degf∈21ΓF by anisotropy of (V,q,b).
∎
For γ∈Γ, we put γ=−(γ+ε).
Lemma 3.2**.**
There exists a well-defined involution Γ/ΓF→Γ/ΓF:[γ]↦[γ]:=[γ]. Assume moreover ε∈21ΓF. Then the above involution restricts to a well-defined involution 21ΓF/ΓF→21ΓF/ΓF. If ε∈ΓF, then [γ]=[γ] for all γ∈21ΓF. If ε∈21ΓF∖ΓF, then there is no γ∈21ΓF such that [γ]=[γ]. For ε∈21ΓF, the above involution also restricts to a well-defined involution (Γ/ΓF)∖(21ΓF/ΓF)→(Γ/ΓF)∖(21ΓF/ΓF), and this involution has no fixed points when ε∈ΓF.
Proof.
The proof is left to the reader. ∎
Now suppose ε∈21ΓF. The involution of Lemma 3.2 induces a group action Z/2Z→Aut(Γ/ΓF) that preserves 21ΓF/ΓF and its
complement in Γ/ΓF. Let P be the set of orbits under the action, which is a partition of Γ/ΓF. Similarly, let Pp the induced partition on 21ΓF/ΓF, and Pm the induced partition on (Γ/ΓF)∖(21ΓF/ΓF). So we have P=Pp⊔Pm. We call Pp the principal-parts set of P and Pm the metabolic-parts set of P. Now, for P∈P and (V,q,b) an ε-shifted space of type T, let VP=⨁Λ∈PVΛ,
qP=q∣VP, bP=b∣VP and ΦP=(VP,qP,bP). The next lemma shows that ΦP=(VP,qP,bP) is also an ε-shifted space of (the same) type T.
Lemma 3.3**.**
Let b:V×V→F be a nondegenerate ε-shifted graded symmetric bilinear form. For all γ∈Γ, V[γ]⊥=⨁[δ]=[γ]V[δ], dimV[γ]=dimV[γ], and bP is nondegenerate, where P∈P is the orbit of [γ].
Proof.
The proof uses the same ideas as in [MR2330736]*Proposition 1.1, and is based on the fact that b(V[γ],V[δ])=0 whenever γ+δ+ε∈/ΓF.
∎
Our next goal is to describe the Witt group WTε(F) in terms of a Witt group of F0. As suggested by Lemma 3.1, we will distinguish two cases: when ε∈ΓF and when ε∈21ΓF∖ΓF.
3.1 Case 1 : if ε∈ΓF
Proposition 3.4**.**
Suppose ε∈ΓF and T∈{I,II,τ−III∣τ∈Fε×}. Let Φ=(V,q,b) be an ε-shifted space of type T over F.
The canonical decomposition of V yields a decomposition of Φ :
[TABLE]
where Ψ and all the ΦP (for P∈Pp) are ε-shifted spaces of type T over F. Moreover Ψ is metabolic.
Proof.
The proof is similar to the one of [MR2836073]*Proposition 1, which deals with the case of nonsingular graded quadratic spaces; it uses the fact that q(V[γ])=0 when γ∈/21ΓF.
∎
Recall that ε∈ΓF is fixed, and fix also a type T∈{I,II,τ−III∣τ∈Fε×} over F. By a choice of uniformizing parameters (for ε and T), we mean a pair
C=(ρ,π), where ρ∈Fε× is a nonzero homogeneous element and π:Pp→F is a map such that, for all P∈Pp, we have πP:=π(P)∈F2γ× for
some γ∈21ΓF (depending on P) such that P={[γ]}. Moreover, we always assume (i.e., it is part of the definition) ρ=1 if T=I, and ρ=τ if T=τ−III. Now, given a choice of uniformizing
parameters C=(ρ,π), for every ε-shifted space Φ=(V,q,b) of type T, let for each P∈Pp,
[TABLE]
where δ:=degπP∈ΓF.
Consider the field F0 as a graded field with trivial graduation.555Trivial graduation means here Δ-grading with Δ=0, i.e. Δ is the trivial group. Let T′∈{I,II,1−III} be the following type over F0 : if T=I then T′=I, if T=II then T′=II, and if T=τ−III for some τ∈Fε× then T′=1−III (where 1∈F0× is the multiplicative unit).
Since the restriction of b to VC,P:=V21δ is nondegenerate (if e∈V21δ and f∈V−21δ−ε are such that b(e,f)=1, then bC,P(e,πδρf)=1), we have that ΦC,P=(VC,P,qC,P,bC,P) is a [math]-shifted quadratic space of type T′ on the trivially graded F0-vector space VC,P. Indeed, if T=I then, since in this case bC,P=bqC,P, we clearly have that ΦC,P is of type T′=I, i.e. ΦC,P can be identified with the nonsingular F0-quadratic space (VC,P,qC,P). If T=II then we clearly have that ΦC,P is of type T′=II, i.e. ΦC,P is a symplectic F0-quadratic space. And if T=τ−III then, since in this case qC,P(v)=bC,P(v,v) for all v∈VC,P, we clearly have that ΦC,P is of type T′=1−III, i.e. ΦC,P can be identified with the nondegenerate symmetric F0-
bilinear space (VC,P,bC,P).
Recall that WTε(F) is the Witt group of ε-shifted spaces of type T over F and let WT′(F0) be the Witt group of [math]-shifted spaces of type T′ over F0. In other words, after
canonical identifications, if T=I then WT′(F0)=WI(F0)≃Wq(F0) is the Witt group of nonsingular quadratic spaces over F0, if T=II then WT′(F0)=WII(F0)≃Wsq(F0) is the Witt group of symplectic quadratic spaces over F0, and if T=τ−III then WT′(F0)=W1−III(F0)≃W(F0) is the Witt group of nondegenerate symmetric
bilinear spaces over F0.
Note that, since ε∈ΓF, it follows that ∣Pp∣=∣21ΓF/ΓF∣=∣ΓF/2ΓF∣.
Proposition 3.5**.**
Assume that ε∈ΓF and T∈{I,II,τ−III∣τ∈Fε×}. Then for each choice of uniformizing parameters C, the map that carries each ε-shifted space Φ of type T over F to the collection (ΦC,P)P∈Pp induces a group homomorphism
[TABLE]
That isomorphism depends on the choice of the uniformizing parameters.
Proof.
The proof is routine. See [MR2836073]*Proposition 2 for the case of nonsingular graded quadratic forms. The general case is similar.
∎
Corollary 3.6**.**
Assume that ε∈ΓF. Then for each choice of uniformizing parameters C,
the map that carries each ε-shifted graded symplectic quadratic space Φ to the collection (ΦC,P)P∈Pp induces a group homomorphism
[TABLE]
2. 2.
the map that carries each nonsingular graded quadratic space Φ to the collection (ΦC,P)P∈Pp induces a group homomorphism
[TABLE]
3. 3.
the map that carries each nondegenerate graded symmetric bilinear space Φ to the collection (ΦC,P)P∈Pp induces a group homomorphism
[TABLE]
Those isomorphisms depend on the choice of the uniformizing parameters.
3.2 Case 2 : if ε∈21ΓF∖ΓF
In this case, Lemma 3.2 shows that each orbit in Pp has exactly two different elements of 21ΓF/ΓF. This case occurs only for ε-shifted space of type II.
Proposition 3.7**.**
Suppose ε∈21ΓF∖ΓF. Let Φ=(V,q,b) be an ε-shifted graded symplectic quadratic space over F.
The canonical decomposition yields a decomposition of Φ :
[TABLE]
For each P={Λ,Λ}∈Pp, ΦP=(VP,qP,bP) is an ε-shifted graded symplectic quadratic space over F, and both VΛ and VΛ
are totally isotropic subspaces for bP. Moreover, Ψ is a metabolic ε-shifted graded symplectic quadratic space over F.
Proof.
The existence of the decomposition is clear by Lemma 3.3. Now, let γ∈Γ. If γ∈21ΓF, then γ+γ+ε∈/ΓF since ε∈/ΓF, hence V[γ] is a totally isotropic subspace for b. To complete the proof, it remains only to prove the metabolicity of ΦP when P∈Pm. But this is clear, since q(VP)=0 when P∈Pm, and since bP is alternating.
∎
Recall that ε∈21ΓF∖ΓF is fixed. For each ε-shifted graded symplectic quadratic space Φ=(V,q,b) and each γ∈21ΓF,
consider the F0-bilinear map b∣Vγ×Vγ:Vγ×Vγ→F0:(x,y)↦b(x,y). This map is
nondegenerate because for every nonzero x∈Vγ, there exists a homogeneous y∈V such that b(x,y)=1, that is degy=−γ−ε=γ. Since moreover dimF0Vγ=dimFV[γ]=dimFV[γ]=dimF0Vγ, where the middle equation comes from Lemma 3.3, we
obtain a linear isomorphism bγ:Vγ→Vγ∗:z↦b∣Vγ×Vγ(z,⋅).
By a choice of uniformizing parameters (for ε), we mean a pair C=(ρ,π), where ρ∈F2ε is a nonzero homogeneous element and π:Pp→F is a map such that
for all P∈Pp, we have πP:=π(P)∈F2γ× for some γ∈21ΓF (depending on P) such that P={[γ],[γ]}. Now, given a choice of uniformizing
parameters C=(ρ,π), for every ε-shifted graded symplectic quadratic space Φ=(V,q,b), let for each P∈Pp,
[TABLE]
where δ:=degπP∈ΓF.
It is clear that ΦC,P=(V21δ,qC,P,qC,P′) is a separated symplectic quadratic space over V21δ viewed as an F0-vector space.
Proposition 3.8**.**
Assume that ε∈21ΓF∖ΓF. Then for each choice of uniformizing parameters C, the map that carries each ε-shifted graded symplectic
quadratic space Φ to the collection (ΦC,P)P∈Pp induces a group homomorphism
[TABLE]
That isomorphism depends on the choice of the uniformizing parameters.
Proof.
The proof is routine and is based on the same ideas as the ones of the proof of Proposition 3.4, except that we use the nondegenerate alternating bilinear form b of Φ to identify V21δP with V21δP∗ for each P∈Pp, where δP=deg(πP) if we let C=(ρ,π).
∎
4 Arason’s filtration
Let F be a field of arbitrary characteristic and let v:F→Γ∪{∞} be a valuation, where Γ is an arbitrary totally ordered (hence torsion-free, see [MR2215492]*Lemma 2.1.1) abelian group. Without loss of generality, we
may also assume Γ divisible, since we may substitute for Γ its divisible hull (cf. [MR2215492]Proposition 1.2.4 & Proposition 2.1.2). Denote by F the residue field. Let also V be a finite-dimensional F-vector space.
We recall from [MR3328410]§3.1.1 that a v-value function is a map α:V→Γ∪{∞} such that for all x,y∈V and λ∈F
(i)
α(x)=0 if and only if x=0
(ii)
α(λx)=v(λ)+α(x)
(iii)
α(x+y)≥min{α(x),α(y)}.
The v-value function is called a v-norm if there is a basis (ei)i=1,…,n of V such that
[TABLE]
Such a basis is called a splitting basis for α. For example, it turns out that if F is maximally complete for v (e.g., F is complete and v is discrete), then every v-value function on V is a v-norm (see [MR3328410]*Proposition
3.8). Nevertheless, maximal completeness is not required for the results of this section.
The value function α yields a filtration of V. We also recall from [MR3328410]*§3.1.1 the construction of grα(V), the associated graded vector space over grv(F). For each γ∈Γ we let
[TABLE]
and we define
[TABLE]
Similarly, let grv(F) be the Γ-graded ring associated with the filtration of F defined by the valuation v. The field structure on F induces canonically a structure of graded ring on grv(F), for which every nonzero homogeneous element is
invertible. Similarly, the F-vector space structure on V induces a structure of grv(F)-module on grα(V). In particular, every Vγ is a F0-vector space. For each nonzero x∈V×, we let
[TABLE]
We also set 0=0 and use a similar notation for elements in grv(F). Note that F0=F , so that x=x if v(x)=0. It is shown in [MR3328410]*Corollary 3.6 that a family of vectors (ei)i=1,…,n
of V is a splitting basis for α if and only if (ei)i=1,…,n is a homogeneous grv(F)-basis of grα(V), and that α is a v-norm if and only if dimgrv(F)grα(V)=dimFV. We also write ΓF:=Γgrv(F) for the value group of v.
4.1 Depth of norms and induced spaces
If q:V→F is a quadratic form, the polar form of q is the symmetric bilinear form bq:V×V→F defined for all v,w∈V by
[TABLE]
Definition 4.1**.**
Let q:V→F be a quadratic form, with polar form b:V×V→F and let ε∈Γ, ε≥0. We say that a v-norm α:V→Γ∪{∞} is compatible
of depth ε (or ε-compatible) with q if
(a)
v(b(x,y))≥α(x)+α(y)+ε for all x,y∈V
2. (b)
v(q(x))≥2α(x) for all x∈V
3. (c)
for all nonzero x∈V, there exists a nonzero y∈V such that v(b(x,y))=α(x)+α(y)+ε.
Such a compatible v-norm is said to be tame if ε=0.
Note that it suffices to check conditions (a) and (b) for a splitting basis of α.
Observe also that if the quadratic form q admits a ε-compatible v-norm (for some ε), then q is nonsingular.
Finally note that Elomary and Tignol consider tame compatible v-norms in [MR2836073]*Section 3.
If φ=(V,q) is a quadratic space over F with polar form b and if α is a v-norm on V which is ε-compatible with q for some depth ε≥0, we set for all nonzero x,y∈V,
[TABLE]
and we extend bα to a map
[TABLE]
by bilinearity. This map is an ε-shifted graded symmetric bilinear form.
Condition c in Definition 4.1 means exactly that bα is nondegenerate. We may also define a graded quadratic form
[TABLE]
which satisfies for all nonzero x∈V,
[TABLE]
Indeed, if ε>0, the above formula can be extended to define a totally singular quadratic form on grα(V); whereas if ε=0, for xγ∈Vγ, we extend the above formula by setting
[TABLE]
which defines a nonsingular quadratic form of polar form bα. The straightforward verifications are omitted. We put
[TABLE]
and we call φα the ε-shifted (quadratic) space induced by φ (and α). Note that if ε<v(2) then bα is alternating since for all nonzero x∈V,
[TABLE]
We also have that if ε=v(2)<∞, then 2 is a nonzero homogeneous element (but we have 2=1+1 only if v(2)=0) and qα(v)=2−1bα(v,v) for
all v∈grα(V). Therefore, for ε∈Γ and ε≥0, if ε=0 then φα, which is an ε-shifted space of type I over grv(F), can be identified with the usual induced
graded quadratic space over (grα(V),qα) over grv(F) (the ones considered in [MR2836073]*Section 3). If 0<ε<v(2), then φα is an ε-shifted graded symplectic
quadratic space grv(F). Finally, if ε=v(2) then φα, which is an ε-shifted space of type 2−III over grv(F), can be identified with the nondegenerate graded symmetric bilinear space (grα(V),2−1bα).
4.2 The filtration
In this section, we construct and describe Arason’s filtration.
Lemma 4.2**.**
Let φ1=(V1,q1) and φ2=(V2,q2) be two quadratic spaces over F, and let α1,α2 be v-norms on V1, V2 that are ε-compatible with q1 and q2 respectively, for
some depth ε≥0. Define α1⊕α2:V1⊕V2→Γ∪{∞} by
[TABLE]
Then α1⊕α2 is a v-norm on V1⊕V2 which is ε-compatible with q1⊕q2, and there is a canonical identification of ε-shifted quadratic spaces
[TABLE]
Proof.
The case of tame v-norms is treated in [MR2836073]*Lemma 6, the general case is similar.
∎
Lemma 4.3**.**
If a quadratic space φ=(V,q,b) admits a compatible v-norm β′ of depth δ≥0, then it also admits a compatible v-norm β of depth γ for all γ>δ.
Proof.
Suppose that β′ is a compatible v-norm of depth δ≥0. Then we construct β by letting β=β′−21(γ−δ), so that for all x,y∈V
[TABLE]
Then β is a v-norm which is γ-compatible with φ.
∎
Lemma 4.4**.**
Let q:F×F→F:(x,y)↦xy be a two-dimensional hyperbolic quadratic form. Then q admits a tame compatible v-norm.
2. 2.
Suppose v(2)>0 and let
[TABLE]
*(with a,b∈F) be a two-dimensional quadratic form such that v(4ab)>0. Then q is nonsingular. *
If v(a)+v(b)≤0, then q admits a compatible v-norm of depth
[TABLE]
*satisfying 0≤ε<v(2). *
If v(a)+v(b)>0, then q admits a compatible v-norm of depth ε=0.
3. 3.
Suppose char(F)=0 and let
[TABLE]
(with a∈F×) be a one-dimensional nonsingular quadratic space. Then q admits a compatible v-norm of depth ε=v(2).
Proof.
(1) It is easy to check that the map α:F×F→Γ∪{∞} defined for all x,y∈F by
[TABLE]
is a tame compatible v-norm with q.
(2) Note that the condition v(4ab)>0 implies that q is nonsingular.
If v(a)+v(b)≤0, then
[TABLE]
and the map α:F×F→Γ∪{∞} defined for all x,y∈F by
[TABLE]
is a v-norm which is
compatible of depth
[TABLE]
with q.
If v(a)+v(b)>0 and for example v(b)<0, then v(a)>−v(b) and the map α:F×F→Γ∪{∞} defined for all x,y∈F by
[TABLE]
is a v-norm which is
compatible of depth ε=0 with q.
Finally, if v(a)+v(b)>0 and v(a),v(b)≥0, then the map α:F×F→Γ∪{∞} defined for all x,y∈F by
[TABLE]
is also a v-norm which is compatible of depth ε=0 with q. (3) Now suppose charF=0. Then, the map α:F→Γ∪{∞} defined by
[TABLE]
for all x∈F is clearly a v-norm which is compatible of depth ε=v(2) with q.
∎
Proposition 4.5**.**
Every nonsingular quadratic space admits a compatible v-norm of depth ε, for some ε∈21ΓF such that 0≤ε≤v(2). Moreover, every hyperbolic quadratic space
admits a tame compatible v-norm.
Proof.
Let q:V→F be a nonsingular quadratic form with polar form bq. Assume first that charF=2 (so that v(2)=∞) and dimV=2. Since bq is nondegenerate, there exist e,f∈V such that bq(e,f)=1, so that q is
isometric to the form (x,y)∈F×F↦q(e)x2+xy+q(f)y2 which admits a compatible v-norm of depth ε≥0 by Lemma 4.4. Now suppose charF=0. In this case, we have 0≤v(2)<∞. Suppose also dimV=1 and pick e∈V so that q(e)=0. Then, q is isometric to the form x∈F↦q(e)x2 which admits a compatible v-norm of depth ε=v(2) by Lemma 4.4. In
general, no matter the characteristic of F, if dimV=n>0, we write V=(V1,q1)⊥⋯⊥(Vn,qn) for some F-quadratic spaces (Vi,qi) for i=1,…,n, each of them admitting a compatible v-norm αi of depth εi≤v(2). Note that such a decomposition exists by the first two steps and by normalisation of nonsingular quadratic forms, cf. Lemma 1.4 applied to bq for F with trivial graduation. Then, by Lemma 4.3,
we can assume that all the αi’s are compatible of the same depth ε=maxi=1,…,nεi∈21ΓF with 0≤ε≤v(2). Finally, by Lemma 4.2, the map α=α1⊕⋯⊕αn is a compatible v-norm of depth ε. For the second part of the proof, if (V,q) is moreover hyperbolic, then it can be decomposed as an orthogonal sum of hyperbolic planes, each of them admitting a compatible v-norm αi of depth [math] by Lemma 4.4. This concludes the proof.
∎
Lemma 4.6**.**
Let φ=(V,q) be a quadratic space with a compatible v-norm α of depth ε. If φ is hyperbolic, then φα is metabolic.
Proof.
If U⊂V is a totally isotropic subspace for q of dimension 21dimV, then grα(U) is a Lagrangian for φα.
∎
Lemma 4.7**.**
Let φ=(V,q) be a quadratic space and α,β two v-norms which are compatible with q of the same depth ε. Then the spaces φα and φβ are Witt
equivalent.
Proof.
By Lemma 4.2, the space (−φ)⊥φ admits α⊕β as compatible v-norm of depth ε. Therefore, by Lemma 4.6, the graded space (−φα)⊥φβ is metabolic.
∎
Theorem 4.8**.**
Let α be a v-norm which is compatible of depth γ∈Γ with a quadratic space φ=(V,q). If 0<γ≤v(2), the space φ admits a compatible v-norm of depth δ<γ if and
only if the space φα is metabolic.
Proof.
First suppose that φ admits a compatible norm β′ of depth δ<γ≤v(2). Then by Lemma 4.3, there exists a norm β=β′−21(γ−δ) of depth γ such that
[TABLE]
We will see that φβ is metabolic, hence φα is metabolic by Lemma 4.7. Since δ<v(2), (bq)β′ is an alternating bilinear form. Consequently, there exists a symplectic
basis e1,f1,…,en,fn of φβ such that v(bq(ei,ej))>β′(ei)+β′(ej)+δ for i,j=1,…,n. Therefore v(bq(ei,ej))>β(ei)+β(ej)+γ for all
i,j=1,…,n. Since e1,f1…,en,fn is a splitting basis for β′, it is also a splitting basis of β (by construction of β), hence e1,f1,…,en,fn∈grβ(V) is a basis such that
the graded subspace spanned by e1,…,en is a totally isotropic subspace for bβ. Moreover, the condition β(x)<β′(x) implies that qβ is identically zero. That shows φβ is metabolic. Conversely, assume that φα is metabolic and decompose it as a sum of metabolic planes, by Proposition 1.5. We can therefore find a basis e1,f1,…,en,fn of
V which splits α and such that for all i,j=1,…,n with i=j,
[TABLE]
We put
[TABLE]
(0<ε≤γ), and we define a new v-norm α′ on V by
[TABLE]
It is easily seen that α′ is compatible of depth γ−ε with q.
∎
For each ε∈Γ such that 0≤ε≤v(2), let Wg(F,ε):=WTε(grv(F)) be the Witt group of ε-shifted spaces of type T over grv(F), where T=I if ε=0, T=II if
0<ε<v(2), and T=2−III if ε=v(2). Therefore,
[TABLE]
Note that if v(2)=0, Wg(F,ε) is well-defined since in this case [math]-shifted spaces of type I are exactly v(2)-shifted spaces type 2−III. Note also that Wg(F,ε)=0 when ε∈21ΓF by
Lemma 3.1. Let ε∈Γ be such that 0≤ε≤v(2) and let Wq(F)ε⊂Wq(F) be the set of Witt classes represented by a quadratic space which admits a compatible v-norm of
depth γ≤ε (hence also a compatible v-norm of depth ε, by Lemma 4.3). Since a hyperbolic space always admits a tame compatible norm (by Proposition 4.5) and by
Lemma 4.2, Wq(F)ε is a subgroup of Wq(F). Moreover, by definition, if γ≤ε then Wq(F)γ⊂Wq(F)ε. Therefore, by Proposition 4.5, we get
an ascending filtration by subgroups of Wq(F) such that
[TABLE]
Note that if v(2)∈Γ, then we have Wq(F)v(2)=Wq(F) since in that case
[TABLE]
Note also that for our valued field F, Proposition 1.4 induces a decomposition into two-dimensional spaces of every representative φ of a class [φ]∈Wg(F,ε) when ε<v(2). But when ε=v(2), the same proposition induces an orthogonal decomposition of every anisotropic representative φ of a class [φ]∈Wg(F,ε).
Theorem 4.9**.**
Let ε∈Γ such that 0≤ε≤v(2). There exists a group epimorphism
[TABLE]
that carries the Witt class of a nonsingular quadratic space φ with a compatible v-norm α of depth ε to the Witt class of φα. If ε>0, the kernel of this map is given by ker∂ε=Wq(F)<ε, which is the subgroup of Wq(F) consisting of Witt classes with a representative admitting a compatible v-norm of depth γ<ε. If ε=0 and F is Henselian, then ∂ε is an
isomorphism.
Note that this result was already proved by Elomary and Tignol for the subgroup Wq(F)0 in [MR2836073]*Proposition 8 and Theorem 10.
Proof.
Using Lemma 4.2, Lemma 4.6 and Lemma 4.7, it is routine to check that the map ∂ε:Wq(F)ε→Wg(F,ε) is a well-defined group homomorphism. Suppose first ε<v(2). In this case, in order to prove the surjectivity of ∂ε, we only need to check that every anisotropic 2-dimensional ε-shifted space (V′,q′,b′) is in the image. Here the proof uses the same ideas as
[MR2836073]*Proposition 8. Since b′ is nondegenerate and q′ anisotropic, there exist homogeneous ξ1,ξ2∈V′ and a1,a2∈F× such that b′(ξ1,ξ2)=1, q′(ξ1)=a1 and q′(ξ2)=a2 (so
that 21v(a1)+21v(a2)+ε=0). Consider the quadratic form given for all x1,x2∈F by q(x1,x2)=a1x12+x1x2+a2x22, which is nondegenerate since ε<v(2). Then (grα(F×F),qα,bα)≃(V′,q′,b′) under the map (x1,x2)↦x1ξ1+x2ξ2, where the compatible v-norm α of depth ε is given for all nonzero vector (x1,x2)∈F×F by α(x1,x2)=min{21v(a1)+v(x1),21v(a2)+v(x2)}. If ε=v(2), in order to prove the surjectivity of ∂ε, we only need to check that every anisotropic one-dimensional ε-
shifted space (V′,q′,b′), is in the image. Since b′ is nondegenerate, we may find a homogeneous vector ξ∈V such that b′(ξ,ξ)=0. Consequently, there exists a∈F× such that q′(ξ)=a. Now consider the quadratic
form on F given for all x∈F by q(x)=ax2, which is nondegenerate when v(2)∈Γ, and define the v-norm α:F→Γ∪{∞} given for every nonzero vector x∈F by α(x)=21v(a)+v(x), which
is compatible with (F,q) of depth ε=v(2). From this, straightforward computations show that (grα(F),qα,bα)≃(V′,q′,b′) under the map x↦xξ. When ε>0,
the identity ker∂ε=Wq(F)<ε follows from Theorem 4.8. When ε=0 and F is Henselian, the injectivity follows from [MR2836073]*Theorem 10.
∎
Note that the Henselian hypothesis is required only for ∂0:Wq(F)0→Wg(F,0) being injective. That ∂ε induced an isomorphism Wq(F)ε/Wq(F)<ε∼Wg(F,ε) if ε>0 holds for every valued field (F,v).
4.3 Wq(F)ε with generators
In this section, we give another description of the subgroups Wq(F)ε when 0≤ε<v(2), and we complete the proof of the result (2) of the introduction by showing that
[TABLE]
if 0<ε≤v(2). For that, we first prove the next proposition.
Proposition 4.10**.**
If (V,q) is a quadratic space and α is a v-norm on V that is compatible of depth ε<v(2) with q, then we can find subspaces (V1,q1),…,(Vn,qn) of dimension 2 such that
(V,q)=(V1,q1)⊥⋯⊥(Vn,qn), and
2. 2.
each αi=α∣Vi is a v-norm on Vi which is ε-compatible with qi, and α=α1⊕⋯⊕αn.
For the proof, we will use the following result, which is a particular case of [coyette]*Proposition 2.5.
Proposition 4.11**.**
Let (F,v) be a valued field (of arbitrary characteristic). Consider (V,α) a F-vector space with v-value function α, and a subspace U⊂V. Suppose that p:V→U is a linear map such that p(u)=u for
all u∈U. If α(p(x))≥α(x) for all x∈V, then V=U⊕kerp and α(u+v)=min{α(u),α(v)} for all u∈U and v∈kerp.
Let (V,q) be a quadratic space admitting a compatible v-norm α of depth ε, with 0≤ε<v(2). Suppose dimV>0 and take two nonzero vectors e,f∈V such that v(bq(e,f))=α(e)+α(f)+ε. Consider the subspace U=span⟨e,f⟩⊂V spanned by e and f. Since ε<v(2), the vectors e and f are linearly independent, and bq∣U is
nondegenerate. So we can write
[TABLE]
for the two nonsingular quadratic spaces (U,q∣U) and (U⊥,q∣U⊥). Since α is a v-norm, it follows that α∣U and α∣U⊥ are v-norms too (see [MR3328410]*Proposition 3.14). Since ε<v(2), it is straightforward to see that α∣U is ε-compatible with (U,q∣U). To conclude the proof, it remains to show that
α∣U⊥ is ε-compatible with (U⊥,q∣U⊥), because the proposition then follows by induction on the dimension. Consider the orthogonal projection p:V→U given for all x∈V by
[TABLE]
where
[TABLE]
[TABLE]
Using that
[TABLE]
standard calculations yield
[TABLE]
[TABLE]
Those inequalities imply α(p(x))≥α(x). Therefore, by Proposition 4.11,
[TABLE]
for all u∈U and v∈U⊥. Now, suppose x∈U⊥ is a nonzero vector. There exists a nonzero (y1,y2)∈U⊕U⊥ such that
[TABLE]
This implies:
[TABLE]
Consequently v(bq(x,y2))=α(x)+α(y2)+ε for some nonzero y2∈U⊥, and α∣U⊥ is compatible with (U⊥,q∣U⊥) of depth ε.
∎
For a,b∈F, we denote by [a,b] the quadratic space (F×F,q) where q is given by q(x1,x2)=ax12+x1x2+bx22 for all x1,x2∈F. The following description of Wq(F)ε is inspired by the definitions of
[RH-05-2016]*section 2.
Corollary 4.12**.**
Let ε∈Γ such that 0≤ε<v(2). Then Wq(F)ε is the subgroup generated by the classes represented by some form [a,b] with a,b∈F and v(a)+v(b)≥−2ε.
Proof.
First note that, for ε<v(2), the condition v(a)+v(b)≥−2ε implies that [a,b] is nonsingular. Suppose now [a,b] is a quadratic space with a,b∈F and v(a)+v(b)≥−2ε. Then, by
Lemma 4.4, [a,b] admits a compatible v-norm of depth ≤ε. Conversely, assume q:V→F is a 2-dimensional nonsingular quadratic form that admits a compatible v-norm of depth γ≤ε. Pick e,f∈V such that v(bq(e,f))=α(e)+α(f)+γ and moreover bq(e,f)=1. Then e,f are linearly independent since γ<v(2), and (V,q)≃[q(e),q(f)] with
[TABLE]
We have thus shown that the spaces [a,b] with a,b∈F and v(a)+v(b)≥−2ε are the 2-dimensional nonsingular spaces that carry a compatible v-norm of depth ≤ε, and the corollary follows by
Proposition 4.10.
∎
In order to prove completely the result announced in (2) of the introduction, it remains to prove the following.
Lemma 4.13**.**
Let φ=(V,q) be a quadratic space. If φ admits a compatible v-norm of depth ε such that 0≤ε≤v(2), then φ also admits a compatible v-norm of depth γ≤ε such that 0≤γ≤v(2) and moreover γ∈21ΓF. Consequently,
[TABLE]
Proof.
We only show the existence of the v-norm of depth γ≤ε such that γ∈21ΓF. If ε=v(2), the assertion is clear. Suppose now 0≤ε<v(2). First assume φ is a 2-
dimensional space. Then, by the proof of Corollary 4.12, write φ≃[a,b] for some a,b∈F such that v(a)+v(b)≥−2ε. Therefore, by Lemma 4.4, [a,b] admits a compatible
v-norm of depth γ≤ε with γ∈21ΓF. Now, if φ is a general nonsingular quadratic space which admits a compatible v-norm of depth ε<v(2), decompose it, by
Proposition 4.10, into 2-dimensional subspaces φi, each of them admitting a compatible v-norm of depth ε. By the first part of the proof, each space φi admits a compatible v-norm of depth γi≤ε for some γi∈21ΓF. Therefore, by Lemmas 4.3 and 4.2, φ admits a compatible v-norm of depth γ=maxiγi∈21ΓF.
∎
5 Relation with Arason’s results
In this section, we relate our work in the particular case of ΓF=Z with Arason’s results, and we give an example of application of those results. From now on, we suppose ΓF=Z. Note that in this case, for ε∈21Z
such that 0<ε≤v(2), we have Wq(F)<ε=Wq(F)ε−(1/2).
Let φ be a nonsingular quadratic space. Since ΓF=Z, there exists a minimal depth ε≥0 such that φ admits a compatible v-norm of depth ε. We put w(φ)=ε and we call it the
wildness index of φ. Let π∈F be such that v(π)=1. Note that the ascending filtration (Wq(F)ε)ε∈E, where E={ε∈21N∣0≤ε≤v(2)}, is infinite if charF=2,
whereas it is finite (and satisfies Wq(F)v(2)=Wq(F)) if charF=2.
Observe that, in Arason’s note [RH-05-2016], the index ε of the subgroups Wq(F)ε ranges from [math] to 2v(2). In this paper, we use half the values, so that ε ranges from [math] to v(2).
5.1 Arason’s isomorphisms
In his note [RH-05-2016], Arason defines the subgroups Wq(F)ε, for a discretely valued field F, in terms of 2-dimensional generators. He also describes those subgroups using isomorphisms which are given in terms of those
generators. Corollary 5.2 is the corresponding description explained from our point of view.
For ε∈21N such that ε<v(2) and n=2ε, we have that Wq(F)ε is the subgroup generated by the classes represented by some form [α,π−nβ] or π[α,π−nβ]≃[πα,π−1−nβ], with α,β∈F such that v(α)≥0 and v(β)≥0.
Proof.
By Corollary 4.12, Wq(F)ε is the subgroup generated by the classes represented by some forms [a,b] with a,b∈F such that v(a)+v(b)≥−2ε. Note that, given an arbitrary π∈F×, we
have π[a,b]≃[πa,π−1b] and π2[a,b]≃[a,b] for all a,b∈F. To complete the proof, it remains to apply these general relations with π∈F× such that v(π)=1.
∎
For the rest of the paper, we write φW for the Witt class in Wq(F) of a nonsingular quadratic space φ. Given elements αi∈F (i=1,…,n), we denote by ⟨α1,…,αn⟩ the symmetric bilinear space
(V,b) with orthogonal basis e1,…,en∈V such that b(ei,ei)=αi and b(ei,ej)=0 if i=j, for all i,j=1,…,n. When charF=2, we identify nondegenerate symmetric bilinear forms with nonsingular quadratic forms
(with a symmetric bilinear form b, we associate the quadratic form given by x↦b(x,x), and with a quadratic form q we associate 21bq).
Corollary 5.2** ([RH-05-2016]*Proposition 1.1, Proposition 3.1 and Proposition 2.1).**
*Assume666Observe that if v(2)=0, the well-known epimorphism (or isomorphism when F is Henselian) Wq(F)(=Wq(F)v(2)=Wq(F)0)→Wq(F)⊕Wq(F) can also be deduced from our results (and is also in [RH-05-2016]Proposition 1.1). charF=2. In the following, α,β represent elements in F such that v(α)≥0 and
v(β)≥0.
There is always a group epimorphism
[TABLE]
*which maps a Witt class [α,β]W to ([α,β]W,0) and a Witt class [πα,π−1β]W to (0,[α,β]W). That epimorphism is an isomorphism when F is Henselian.
Let ε∈21N such that 0<ε<v(2).
If ε∈/N, there exists a group isomorphism*
[TABLE]
*which maps the class of a Witt class [α,π−2εβ]W to α⊗β and the class of a Witt class [πα,π−1−2εβ]W to β⊗α.
If ε∈N, there exists a group isomorphism*
[TABLE]
*which maps the class of a Witt class [α,π−2εβ]W to (α∧β,0) and the class of a Witt class [πα,π−1−2εβ]W to (0,α∧β).
If charF=2, there is a group isomorphism*
[TABLE]
which maps the class of a Witt class ⟨α⟩W with v(α)=0 to (⟨α⟩W,0) and the class of a Witt class ⟨πβ⟩W with v(β)=0 to (0,⟨β⟩W).
Proof.
Fix π′:21Z/Z→grv(F) such that π′([0])=1 and π′([21])=π. For the first map, compose the group homomorphisms of Theorem 4.9 and Proposition 3.5, with a choice of
uniformizing parameters given by C=(ρ,π′) where ρ=1. If ε∈/N, compose the group homomorphisms of Theorem 4.9, Proposition 3.5 and Theorem 2.9, with a choice of
uniformizing parameters given by C=(ρ,π′) where ρ=π2ε. If ε∈N, compose the group homomorphisms of Theorem 4.9, Proposition 3.8 and Theorem 2.3, with
a choice of uniformizing parameters given by C=(ρ,π′) where ρ=πε. In those three cases (put ε=0 in the first), the map defined by α(x,y)=min{v(x),v(y)−ε} for all x,y∈F is a ε-compatible v-norm with [α,π−2εβ], and the map defined by α(x,y)=min{v(x)+21,v(y)−ε−21} for all x,y∈F is a ε-compatible v-norm with [πα,π−1−2εβ]. In the last case when charF=2, compose the group homomorphism of Theorem 4.9 and Proposition 3.5, with a choice of uniformizing parameters given by C=(ρ,π′)
where ρ=2. Here the v-norms constructed in Lemma 4.5 are compatible of depth v(2) with ⟨α⟩ and ⟨πβ⟩.
∎
Corollary 5.2 can also be found in [RH-19-2006]*Theorem 2 in the particular case of F=K((S)) being the field of formal Laurent series in an indeterminate S over a field K of characteristic 2.
5.2 An application
Our goal for this section is to prove Proposition 5.4 as an illustration of the results of Corollary 5.2. In order to achieve this purpose, we need the following lemma.
Lemma 5.3**.**
Let ε∈21N and k∈N. For a,b,c,d∈F and α,β,γ∈F such that v(α)≥0, v(β)≥0 and v(γ)≥0, the following relations hold:
(a)
[a,b]≃[b,a]**
(b)
[c2a,b]≃[a,c2b],
(c)
If c=0 then c[a,b]≃[c−1a,cb], hence
π[α,βπ−2k−1]≃[β,απ−2k−1].
(d)
([RH-05-2016]Proposition 2.3)
If [a,b] and [c,d] are nonsingular then*
[TABLE]
Hence if 0<ε<v(2) then
[TABLE]
Moreover, if either charF=2 or F is a complete field satisfying charF=2, then
[TABLE]
(e)
[a,b]W=0* if v(ab)>0 and F is complete.*
(f)
If charF=2 and a=0, ⟨a,b⟩≃[a,4a21(a+b)]
(g)
If charF=2, ⟨a⟩W+⟨b⟩W=⟨a+b⟩W+⟨ab(a+b)⟩W for all a,b∈F× such that a+b=0.
Proof.
The easy proofs of (a) and (b) are left to the reader. The first part of (c) is left to the reader, and the second part of (c) follows directly from (a) and (b) since π[α,π−2k−1β]≃[π−1α,π−2kβ] by the first part of
(c). For (e), observe that since F is complete and v(ab)>0, by Hensel’s lemma, there exists u∈F such that u2+u+ab=0. Now, if a=0, then [a,b]W=0. If a=0, (a−1u,1) is an isotropic vector for [a,b] and the conclusion
follows. The first part of (d) comes from [RH-05-2016]*Proposition 2.3. It is a direct calculation: if e1,f1,e2,f2 is the standard basis of [a,b]⊥[c,d], then consider the change of basis given by e1′=e1+e2, f1′=f1, e2′=(e2−2cf2)/(1−4cd) and f2′=(2be1−f1+(1−4ab)f2)/(1−4ab). The first part of (d) yields
[TABLE]
The last summand is clearly isotropic if charF=2, hence [α,γ]W+[β,γ]W=[α+β,γ]W in this case. This last equality also holds if F is a complete field such that
charF=2 by (e), since v(2)>0 in that case. Suppose now 0<ε<v(2), then
[TABLE]
by Corollary 4.12 since in this case we have v(4βπ−2εγ)>0 and v(απ−2εγ)>0, v(1−4βπ−2εγ)=0 and v(1−4απ−2εγ)=0, v(2)≥1 and finally v(β2π−2εγ)≥−2(ε−21). The rest of the proof of (d) is left to the reader. For (f), note that ⟨a,b⟩≃[a,4a21(a+b)] by the
change of basis given by e′=e and f′=2ae−f, where e,f is the standard basis of ⟨a,b⟩. Finally, (g) is well-known. See for example [MR2427530]*Lemma 4.1.
∎
The following proposition and its proof are inspired by [MR3437769]*Lemma 8.1 and Proposition 8.2.
Proposition 5.4**.**
Suppose F is a complete discretely valued field with perfect dyadic residue field F and let π∈F be such that v(π)=1. If charF=2, then every Witt class of a quadratic form over F can be
written as
[TABLE]
for some n∈N and αk,βk∈F such that v(αk)≥0 and v(βk)≥0 for all k. If charF=2, then every Witt class of a quadratic form over F can be written as
[TABLE]
for some α,β∈{0,1} uniquely determined and some αk,βk∈F such that v(αk)≥0 and v(βk)≥0 for all k. Moreover, in both cases, if we fix a (set) section s:F→O of the
canonical quotient map O→F (where O:={x∈F∣v(x)≥0}), we can always choose αk,βk∈s(F) for all k. Provided that αk,βk∈s(F) for all k, the decomposition
of a Witt class is unique.777When charF=2, if K is a coefficient field (i.e., a subfield K of F contained in O that maps isomorphically onto F under the canonical quotient map O→F), one can
choose for s the isomorphism from F to K.
Note that the decompositions given in Proposition 5.4 are in general neither decompositions with anisotropic forms nor the decompositions with the least number of summands. For example, in the case when charF=2, the
stated decomposition can be rewritten as
[TABLE]
Proof.
First, let α,β∈F such that v(α)≥0 and v(β)≥0. Since F2=F, there exist α′,τ∈F such that α=α′2+τ and v(α′)≥0, v(τ)>0. Similarly, write β=β′2+μ for some β′,μ∈F such that v(β′)≥0 and v(μ)>0. Then, for k∈N such that k<2v(2), by Lemma 5.3(b) and (d), we have [α,βπ−k]W=[1,(α′β′)2π−k]W+[α′2,μπ−k]+[τ,β′2π−k]+[τ,μπ−k]+w for some w∈Wq(F) such that w∈Wq(F)(k−1)/2 if k>0 and w=0 if k=0. Observe that [α′2,μπ−k],[τ,β′2π−k],[τ,μπ−k]∈Wq(F)(k−1)/2 if k>0. Moreover, since F is complete and v(α′2μ),v(τβ′2),v(τμ)>0, we have that [α′2,μπ−k], [τ,β′2π−k] and [τ,μπ−k] are hyperbolic when k=0, by
Lemma 5.3(e). Similarly, [πα,π−1−kβ]W=[π,π−1−k(α′β′)2]+w for some w∈Wq(F) such that w∈Wq(F)(k−1)/2 if k>0 and w=0 if k=0. Second, note that since F2=F, we have Wq(F)ε⊂Wq(F)ε−(1/2) when ε∈N∖{0}. Indeed, that follows from Corollary 5.2 since here F∧F2F={0}. Third, we
show the existence of the decomposition of a Witt class φW by induction on the depth ε of a v-norm which is ε-compatible with the form φ. Suppose that φ admits a compatible v-norm of depth ε=0. Then Corollary 5.1 and the first part of the proof show that φW can be written as a sum of classes of two-dimensional spaces of the form [1,a2] and [π,π−1b2] with a,b∈F such that v(a),v(b)≥0. So we
conclude by Corollary 5.3(d) and the first part of the proof again. Suppose now that φ admits a compatible v-norm of depth ε∈21N satisfying 0<ε<v(2). By the second part of the proof, we
way assume ε∈/N. By Corollary 5.1, Lemma 5.3(c) and the first part of the proof, φW can be written as a sum of some w∈Wq(F)ε−(1/2) (hence w∈Wq(F)ε−1, by the second part of the proof) and a sum of classes of two-dimensional spaces of the form [1,a2π−2ε] for some a∈F such that v(a)≥0. So we conclude here by using by Corollary 5.3(d), the first part
of the proof, and the induction hypothesis. This shows the existence of the decomposition when charF=2. Suppose now that charF=2 and that φ admits a compatible v-norm of depth ε=v(2). Let a∈F× be
such that v(a)=0 and write a=α2+μ for some α∈F× such that v(α)=0 and μ∈F such that v(μ)>0. If μ=0, then ⟨a⟩≃⟨α2⟩≃⟨1⟩. Otherwise, if μ=0, then ⟨a⟩W=⟨α2⟩W+⟨μ⟩W−⟨α2μa⟩W=⟨1⟩W+⟨μ,−μα−2a⟩W, by Corollary 5.3(g). But ⟨μ,−μα−2a⟩W∈Wq(F)v(2)−(1/2), since by Lemma 5.3(f)⟨μ,−μα−2a⟩≃[μ,2−2μ−1(1−α−2a)] with v(μ2−2μ−1(1−α−2a))=−2v(2)+v(1−α−2a)≥−2(v(2)−21). Indeed, v(1−α−2a))=v(α−2μ)=v(μ)≥1. Note also that the space ⟨1,1⟩≃[2−1,1] admits a compatible norm of depth 21v(2)<v(2). Since every nondegenerate bilinear form can
be written as ⟨α1,…,αn⟩⊥⟨π⟩⟨α1′,…,αm′⟩ for some αi,αj′ such that v(αi)=0=v(αj) for all i,j, the existence of the decomposition in the second case
can easily be concluded by the induction hypothesis. Now, the proof given a section s:F→O of the canonical quotient O→F is the same, except that each time we use the first part of the proof, we add the
following step. We choose α′′∈s(F) such that (α′β′)2=α′′2+μ′ for some μ∈F such that v(μ)>0. Then we write [1,π−k(α′β′)2]W=[1,π−kα′′2]W+w for some w∈Wq(F) such
that w∈Wq(F)(k−1)/2 if k>0 and w=0 if k=0. Similarly for [π,π−1−k(α′β′)2]W. For the uniqueness, proceed as [MR3437769]*Proposition 8.2. Note that in our case W(F)=Z/2Z.
∎
Acknowledgements
This paper has been written during my doctoral training. I would like to thank my supervisor, Professor Jean-Pierre Tignol, for suggesting me this topic and for guiding me all along the road. Joachim Verstraete is a Research Fellow of the Fonds de la
Recherche Scientifique - FNRS.
References
ICTEAM Institute/INMA, Université catholique de Louvain, Euler Building, Avenue Georges Lemaître 4 box L4.05.01, 1348 Ottignies-Louvain-la-Neuve, Belgium