• Source: Arf invariant

In mathematics, the Arf invariant of a nonsingular quadratic form over a field of characteristic 2 was defined by Turkish mathematician Cahit Arf (1941) when he started the systematic study of quadratic forms over arbitrary fields of characteristic 2. The Arf invariant is the substitute, in characteristic 2, for the discriminant for quadratic forms in characteristic not 2. Arf used his invariant, among others, in his endeavor to classify quadratic forms in characteristic 2.
In the special case of the 2-element field F2 the Arf invariant can be described as the element of F2 that occurs most often among the values of the form. Two nonsingular quadratic forms over F2 are isomorphic if and only if they have the same dimension and the same Arf invariant. This fact was essentially known to Leonard Dickson (1901), even for any finite field of characteristic 2, and Arf proved it for an arbitrary perfect field.
The Arf invariant is particularly applied in geometric topology, where it is primarily used to define an invariant of (4k + 2)-dimensional manifolds (singly even-dimensional manifolds: surfaces (2-manifolds), 6-manifolds, 10-manifolds, etc.) with certain additional structure called a framing, and thus the Arf–Kervaire invariant and the Arf invariant of a knot. The Arf invariant is analogous to the signature of a manifold, which is defined for 4k-dimensional manifolds (doubly even-dimensional); this 4-fold periodicity corresponds to the 4-fold periodicity of L-theory. The Arf invariant can also be defined more generally for certain 2k-dimensional manifolds.




Definitions


The Arf invariant is defined for a quadratic form q over a field K of characteristic 2 such that q is nonsingular, in the sense that the associated bilinear form



b
(
u
,
v
)
=
q
(
u
+
v
)
−
q
(
u
)
−
q
(
v
)


{\displaystyle b(u,v)=q(u+v)-q(u)-q(v)}

is nondegenerate. The form



b


{\displaystyle b}

is alternating since K has characteristic 2; it follows that a nonsingular quadratic form in characteristic 2 must have even dimension. Any binary (2-dimensional) nonsingular quadratic form over K is equivalent to a form



q
(
x
,
y
)
=
a

x

2


+
x
y
+
b

y

2




{\displaystyle q(x,y)=ax^{2}+xy+by^{2}}

with



a
,
b


{\displaystyle a,b}

in K. The Arf invariant is defined to be the product



a
b


{\displaystyle ab}

. If the form




q
′

(
x
,
y
)
=

a
′


x

2


+
x
y
+

b
′


y

2




{\displaystyle q'(x,y)=a'x^{2}+xy+b'y^{2}}

is equivalent to



q
(
x
,
y
)


{\displaystyle q(x,y)}

, then the products



a
b


{\displaystyle ab}

and




a
′


b
′



{\displaystyle a'b'}

differ by an element of the form




u

2


+
u


{\displaystyle u^{2}+u}

with



u


{\displaystyle u}

in K. These elements form an additive subgroup U of K. Hence the coset of



a
b


{\displaystyle ab}

modulo U is an invariant of



q


{\displaystyle q}

, which means that it is not changed when



q


{\displaystyle q}

is replaced by an equivalent form.
Every nonsingular quadratic form



q


{\displaystyle q}

over K is equivalent to a direct sum



q
=

q

1


+
⋯
+

q

r




{\displaystyle q=q_{1}+\cdots +q_{r}}

of nonsingular binary forms. This was shown by Arf, but it had been earlier observed by Dickson in the case of finite fields of characteristic 2. The Arf invariant Arf(



q


{\displaystyle q}

) is defined to be the sum of the Arf invariants of the




q

i




{\displaystyle q_{i}}

. By definition, this is a coset of K modulo U. Arf showed that indeed



Arf
⁡
(
q
)


{\displaystyle \operatorname {Arf} (q)}

does not change if



q


{\displaystyle q}

is replaced by an equivalent quadratic form, which is to say that it is an invariant of



q


{\displaystyle q}

.
The Arf invariant is additive; in other words, the Arf invariant of an orthogonal sum of two quadratic forms is the sum of their Arf invariants.
For a field K of characteristic 2, Artin–Schreier theory identifies the quotient group of K by the subgroup U above with the Galois cohomology group H1(K, F2). In other words, the nonzero elements of K/U are in one-to-one correspondence with the separable quadratic extension fields of K. So the Arf invariant of a nonsingular quadratic form over K is either zero or it describes a separable quadratic extension field of K. This is analogous to the discriminant of a nonsingular quadratic form over a field F of characteristic not 2. In that case, the discriminant takes values in F*/(F*)2, which can be identified with H1(F, F2) by Kummer theory.




Arf's main results


If the field K is perfect, then every nonsingular quadratic form over K is uniquely determined (up to equivalence) by its dimension and its Arf invariant. In particular, this holds over the field F2. In this case, the subgroup U above is zero, and hence the Arf invariant is an element of the base field F2; it is either 0 or 1.
If the field K of characteristic 2 is not perfect (that is, K is different from its subfield K2 of squares), then the Clifford algebra is another important invariant of a quadratic form. A corrected version of Arf's original statement is that if the degree [K: K2] is at most 2, then every quadratic form over K is completely characterized by its dimension, its Arf invariant and its Clifford algebra. Examples of such fields are function fields (or power series fields) of one variable over perfect base fields.




Quadratic forms over F2


Over F2, the Arf invariant is 0 if the quadratic form is equivalent to a direct sum of copies of the binary form



x
y


{\displaystyle xy}

, and it is 1 if the form is a direct sum of




x

2


+
x
y
+

y

2




{\displaystyle x^{2}+xy+y^{2}}

with a number of copies of



x
y


{\displaystyle xy}

.
William Browder has called the Arf invariant the democratic invariant because it is the value which is assumed most often by the quadratic form. Another characterization: q has Arf invariant 0 if and only if the underlying 2k-dimensional vector space over the field F2 has a k-dimensional subspace on which q is identically 0 – that is, a totally isotropic subspace of half the dimension. In other words, a nonsingular quadratic form of dimension 2k has Arf invariant 0 if and only if its isotropy index is k (this is the maximum dimension of a totally isotropic subspace of a nonsingular form).




The Arf invariant in topology



Let M be a compact, connected 2k-dimensional manifold with a boundary



∂
M


{\displaystyle \partial M}


such that the induced morphisms in





Z


2




{\displaystyle \mathbb {Z} _{2}}

-coefficient homology





H

k


(
M
,
∂
M
;


Z


2


)
→

H

k
−
1


(
∂
M
;


Z


2


)
,


H

k


(
∂
M
;


Z


2


)
→

H

k


(
M
;


Z


2


)


{\displaystyle H_{k}(M,\partial M;\mathbb {Z} _{2})\to H_{k-1}(\partial M;\mathbb {Z} _{2}),\quad H_{k}(\partial M;\mathbb {Z} _{2})\to H_{k}(M;\mathbb {Z} _{2})}


are both zero (e.g. if



M


{\displaystyle M}

is closed). The intersection form




λ
:

H

k


(
M
;


Z


2


)
×

H

k


(
M
;


Z


2


)
→


Z


2




{\displaystyle \lambda :H_{k}(M;\mathbb {Z} _{2})\times H_{k}(M;\mathbb {Z} _{2})\to \mathbb {Z} _{2}}


is non-singular. (Topologists usually write F2 as





Z


2




{\displaystyle \mathbb {Z} _{2}}

.) A quadratic refinement for



λ


{\displaystyle \lambda }

is a function



μ
:

H

k


(
M
;


Z


2


)
→


Z


2




{\displaystyle \mu :H_{k}(M;\mathbb {Z} _{2})\to \mathbb {Z} _{2}}

which satisfies




μ
(
x
+
y
)
+
μ
(
x
)
+
μ
(
y
)
≡
λ
(
x
,
y
)


(
mod

2
)


∀

x
,
y
∈

H

k


(
M
;


Z


2


)


{\displaystyle \mu (x+y)+\mu (x)+\mu (y)\equiv \lambda (x,y){\pmod {2}}\;\forall \,x,y\in H_{k}(M;\mathbb {Z} _{2})}


Let



{
x
,
y
}


{\displaystyle \{x,y\}}

be any 2-dimensional subspace of




H

k


(
M
;


Z


2


)


{\displaystyle H_{k}(M;\mathbb {Z} _{2})}

, such that



λ
(
x
,
y
)
=
1


{\displaystyle \lambda (x,y)=1}

. Then there are two possibilities. Either all of



μ
(
x
+
y
)
,
μ
(
x
)
,
μ
(
y
)


{\displaystyle \mu (x+y),\mu (x),\mu (y)}

are 1, or else just one of them is 1, and the other two are 0. Call the first case




H

1
,
1




{\displaystyle H^{1,1}}

, and the second case




H

0
,
0




{\displaystyle H^{0,0}}

. Since every form is equivalent to a symplectic form, we can always find subspaces



{
x
,
y
}


{\displaystyle \{x,y\}}

with x and y being



λ


{\displaystyle \lambda }

-dual. We can therefore split




H

k


(
M
;


Z


2


)


{\displaystyle H_{k}(M;\mathbb {Z} _{2})}

into a direct sum of subspaces isomorphic to either




H

0
,
0




{\displaystyle H^{0,0}}

or




H

1
,
1




{\displaystyle H^{1,1}}

. Furthermore, by a clever change of basis,




H

0
,
0


⊕

H

0
,
0


≅

H

1
,
1


⊕

H

1
,
1


.


{\displaystyle H^{0,0}\oplus H^{0,0}\cong H^{1,1}\oplus H^{1,1}.}

We therefore define the Arf invariant




Arf
⁡
(

H

k


(
M
;


Z


2


)
;
μ
)
=
(

number of copies of


H

1
,
1



in a decomposition mod 2

)
∈


Z


2


.


{\displaystyle \operatorname {Arf} (H_{k}(M;\mathbb {Z} _{2});\mu )=({\text{number of copies of }}H^{1,1}{\text{ in a decomposition mod 2}})\in \mathbb {Z} _{2}.}





= Examples

=
Let



M


{\displaystyle M}

be a compact, connected, oriented 2-dimensional manifold, i.e. a surface, of genus



g


{\displaystyle g}

such that the boundary



∂
M


{\displaystyle \partial M}

is either empty or is connected. Embed



M


{\displaystyle M}

in




S

m




{\displaystyle S^{m}}

, where



m
≥
4


{\displaystyle m\geq 4}

. Choose a framing of M, that is a trivialization of the normal (m − 2)-plane vector bundle. (This is possible for



m
=
3


{\displaystyle m=3}

, so is certainly possible for



m
≥
4


{\displaystyle m\geq 4}

). Choose a symplectic basis




x

1


,

x

2


,
…
,

x

2
g
−
1


,

x

2
g




{\displaystyle x_{1},x_{2},\ldots ,x_{2g-1},x_{2g}}

for




H

1


(
M
)
=


Z


2
g




{\displaystyle H_{1}(M)=\mathbb {Z} ^{2g}}

. Each basis element is represented by an embedded circle




x

i


:

S

1


⊂
M


{\displaystyle x_{i}:S^{1}\subset M}

. The normal (m − 1)-plane vector bundle of




S

1


⊂
M
⊂

S

m




{\displaystyle S^{1}\subset M\subset S^{m}}

has two trivializations, one determined by a standard framing of a standard embedding




S

1


⊂

S

m




{\displaystyle S^{1}\subset S^{m}}

and one determined by the framing of M, which differ by a map




S

1


→
S
O
(
m
−
1
)


{\displaystyle S^{1}\to SO(m-1)}

i.e. an element of




π

1


(
S
O
(
m
−
1
)
)
≅


Z


2




{\displaystyle \pi _{1}(SO(m-1))\cong \mathbb {Z} _{2}}

for



m
≥
4


{\displaystyle m\geq 4}

. This can also be viewed as the framed cobordism class of




S

1




{\displaystyle S^{1}}

with this framing in the 1-dimensional framed cobordism group




Ω

1


framed


≅

π

m


(

S

m
−
1


)

(
m
≥
4
)
≅


Z


2




{\displaystyle \Omega _{1}^{\text{framed}}\cong \pi _{m}(S^{m-1})\,(m\geq 4)\cong \mathbb {Z} _{2}}

, which is generated by the circle




S

1




{\displaystyle S^{1}}

with the Lie group framing. The isomorphism here is via the Pontrjagin-Thom construction. Define



μ
(
x
)
∈


Z


2




{\displaystyle \mu (x)\in \mathbb {Z} _{2}}

to be this element. The Arf invariant of the framed surface is now defined




Φ
(
M
)
=
Arf
⁡
(

H

1


(
M
,
∂
M
;


Z


2


)
;
μ
)
∈


Z


2




{\displaystyle \Phi (M)=\operatorname {Arf} (H_{1}(M,\partial M;\mathbb {Z} _{2});\mu )\in \mathbb {Z} _{2}}


Note that




π

1


(
S
O
(
2
)
)
≅

Z

,


{\displaystyle \pi _{1}(SO(2))\cong \mathbb {Z} ,}

so we had to stabilise, taking



m


{\displaystyle m}

to be at least 4, in order to get an element of





Z


2




{\displaystyle \mathbb {Z} _{2}}

. The case



m
=
3


{\displaystyle m=3}

is also admissible as long as we take the residue modulo 2 of the framing.
The Arf invariant



Φ
(
M
)


{\displaystyle \Phi (M)}

of a framed surface detects whether there is a 3-manifold whose boundary is the given surface which extends the given framing. This is because




H

1
,
1




{\displaystyle H^{1,1}}

does not bound.




H

1
,
1




{\displaystyle H^{1,1}}

represents a torus




T

2




{\displaystyle T^{2}}

with a trivialisation on both generators of




H

1


(

T

2


;


Z


2


)


{\displaystyle H_{1}(T^{2};\mathbb {Z} _{2})}

which twists an odd number of times. The key fact is that up to homotopy there are two choices of trivialisation of a trivial 3-plane bundle over a circle, corresponding to the two elements of




π

1


(
S
O
(
3
)
)


{\displaystyle \pi _{1}(SO(3))}

. An odd number of twists, known as the Lie group framing, does not extend across a disc, whilst an even number of twists does. (Note that this corresponds to putting a spin structure on our surface.) Pontrjagin used the Arf invariant of framed surfaces to compute the 2-dimensional framed cobordism group




Ω

2


framed


≅

π

m


(

S

m
−
2


)

(
m
≥
4
)
≅


Z


2




{\displaystyle \Omega _{2}^{\text{framed}}\cong \pi _{m}(S^{m-2})\,(m\geq 4)\cong \mathbb {Z} _{2}}

, which is generated by the torus




T

2




{\displaystyle T^{2}}

with the Lie group framing. The isomorphism here is via the Pontrjagin-Thom construction.
Let



(

M

2


,
∂
M
)
⊂

S

3




{\displaystyle (M^{2},\partial M)\subset S^{3}}

be a Seifert surface for a knot,



∂
M
=
K
:

S

1


↪

S

3




{\displaystyle \partial M=K:S^{1}\hookrightarrow S^{3}}

, which can be represented as a disc




D

2




{\displaystyle D^{2}}

with bands attached. The bands will typically be twisted and knotted. Each band corresponds to a generator



x
∈

H

1


(
M
;


Z


2


)


{\displaystyle x\in H_{1}(M;\mathbb {Z} _{2})}

.



x


{\displaystyle x}

can be represented by a circle which traverses one of the bands. Define



μ
(
x
)


{\displaystyle \mu (x)}

to be the number of full twists in the band modulo 2. Suppose we let




S

3




{\displaystyle S^{3}}

bound




D

4




{\displaystyle D^{4}}

, and push the Seifert surface



M


{\displaystyle M}

into




D

4




{\displaystyle D^{4}}

, so that its boundary still resides in




S

3




{\displaystyle S^{3}}

. Around any generator



x
∈

H

1


(
M
,
∂
M
)


{\displaystyle x\in H_{1}(M,\partial M)}

, we now have a trivial normal 3-plane vector bundle. Trivialise it using the trivial framing of the normal bundle to the embedding



M
↪

D

4




{\displaystyle M\hookrightarrow D^{4}}

for 2 of the sections required. For the third, choose a section which remains normal to



x


{\displaystyle x}

, whilst always remaining tangent to



M


{\displaystyle M}

. This trivialisation again determines an element of




π

1


(
S
O
(
3
)
)


{\displaystyle \pi _{1}(SO(3))}

, which we take to be



μ
(
x
)


{\displaystyle \mu (x)}

. Note that this coincides with the previous definition of



μ


{\displaystyle \mu }

.
The Arf invariant of a knot is defined via its Seifert surface. It is independent of the choice of Seifert surface (The basic surgery change of S-equivalence, adding/removing a tube, adds/deletes a




H

0
,
0




{\displaystyle H^{0,0}}

direct summand), and so is a knot invariant. It is additive under connected sum, and vanishes on slice knots, so is a knot concordance invariant.
The intersection form on the (2k + 1)-dimensional





Z


2




{\displaystyle \mathbb {Z} _{2}}

-coefficient homology




H

2
k
+
1


(
M
;


Z


2


)


{\displaystyle H_{2k+1}(M;\mathbb {Z} _{2})}

of a framed (4k + 2)-dimensional manifold M has a quadratic refinement



μ


{\displaystyle \mu }

, which depends on the framing. For



k
≠
0
,
1
,
3


{\displaystyle k\neq 0,1,3}

and



x
∈

H

2
k
+
1


(
M
;


Z


2


)


{\displaystyle x\in H_{2k+1}(M;\mathbb {Z} _{2})}

represented by an embedding



x
:

S

2
k
+
1


⊂
M


{\displaystyle x\colon S^{2k+1}\subset M}

the value



μ
(
x
)
∈


Z


2




{\displaystyle \mu (x)\in \mathbb {Z} _{2}}

is 0 or 1, according as to the normal bundle of



x


{\displaystyle x}

is trivial or not. The Kervaire invariant of the framed (4k + 2)-dimensional manifold M is the Arf invariant of the quadratic refinement



μ


{\displaystyle \mu }

on




H

2
k
+
1


(
M
;


Z


2


)


{\displaystyle H_{2k+1}(M;\mathbb {Z} _{2})}

. The Kervaire invariant is a homomorphism




π

4
k
+
2


S


→


Z


2




{\displaystyle \pi _{4k+2}^{S}\to \mathbb {Z} _{2}}

on the (4k + 2)-dimensional stable homotopy group of spheres. The Kervaire invariant can also be defined for a (4k + 2)-dimensional manifold M which is framed except at a point.
In surgery theory, for any



4
k
+
2


{\displaystyle 4k+2}

-dimensional normal map



(
f
,
b
)
:
M
→
X


{\displaystyle (f,b):M\to X}

there is defined a nonsingular quadratic form



(

K

2
k
+
1


(
M
;


Z


2


)
,
μ
)


{\displaystyle (K_{2k+1}(M;\mathbb {Z} _{2}),\mu )}

on the





Z


2




{\displaystyle \mathbb {Z} _{2}}

-coefficient homology kernel





K

2
k
+
1


(
M
;


Z


2


)
=
k
e
r
(

f

∗


:

H

2
k
+
1


(
M
;


Z


2


)
→

H

2
k
+
1


(
X
;


Z


2


)
)


{\displaystyle K_{2k+1}(M;\mathbb {Z} _{2})=ker(f_{*}:H_{2k+1}(M;\mathbb {Z} _{2})\to H_{2k+1}(X;\mathbb {Z} _{2}))}


refining the homological intersection form



λ


{\displaystyle \lambda }

. The Arf invariant of this form is the Kervaire invariant of (f,b). In the special case



X
=

S

4
k
+
2




{\displaystyle X=S^{4k+2}}

this is the Kervaire invariant of M. The Kervaire invariant features in the classification of exotic spheres by Michel Kervaire and John Milnor, and more generally in the classification of manifolds by surgery theory. William Browder defined



μ


{\displaystyle \mu }

using functional Steenrod squares, and C. T. C. Wall defined



μ


{\displaystyle \mu }

using framed immersions. The quadratic enhancement



μ
(
x
)


{\displaystyle \mu (x)}

crucially provides more information than



λ
(
x
,
x
)


{\displaystyle \lambda (x,x)}

: it is possible to kill x by surgery if and only if



μ
(
x
)
=
0


{\displaystyle \mu (x)=0}

. The corresponding Kervaire invariant detects the surgery obstruction of



(
f
,
b
)


{\displaystyle (f,b)}

in the L-group




L

4
k
+
2


(

Z

)
=


Z


2




{\displaystyle L_{4k+2}(\mathbb {Z} )=\mathbb {Z} _{2}}

.




See also


de Rham invariant, a mod 2 invariant of



(
4
k
+
1
)


{\displaystyle (4k+1)}

-dimensional manifolds




Notes






References


See Lickorish (1997) for the relation between the Arf invariant and the Jones polynomial.
See Chapter 3 of Carter's book for another equivalent definition of the Arf invariant in terms of self-intersections of discs in 4-dimensional space.
Arf, Cahit (1941), "Untersuchungen über quadratische Formen in Körpern der Charakteristik 2, I", J. Reine Angew. Math., 183: 148–167, doi:10.1515/crll.1941.183.148, S2CID 122490693
Glen Bredon: Topology and Geometry, 1993, ISBN 0-387-97926-3.
Browder, William (1972), Surgery on simply-connected manifolds, Berlin, New York: Springer-Verlag, MR 0358813
J. Scott Carter: How Surfaces Intersect in Space, Series on Knots and Everything, 1993, ISBN 981-02-1050-7.
A.V. Chernavskii (2001) [1994], "Arf invariant", Encyclopedia of Mathematics, EMS Press
Dickson, Leonard Eugene (1901), Linear groups: With an exposition of the Galois field theory, New York: Dover Publications, MR 0104735
Kirby, Robion (1989), The Topology of 4-Manifolds, Lecture Notes in Mathematics, vol. 1374, Springer-Verlag, doi:10.1007/BFb0089031, ISBN 0-387-51148-2, MR 1001966
W. B. Raymond Lickorish, An Introduction to Knot Theory, Graduate Texts in Mathematics, Springer, 1997, ISBN 0-387-98254-X
Martino, J.; Priddy, S. (2003), "Group Extensions And Automorphism Group Rings", Homology, Homotopy and Applications, 5 (1): 53–70, arXiv:0711.1536, doi:10.4310/hha.2003.v5.n1.a3, S2CID 15403121
Lev Pontryagin, Smooth manifolds and their applications in homotopy theory American Mathematical Society Translations, Ser. 2, Vol. 11, pp. 1–114 (1959)




Further reading


Lorenz, Falko; Roquette, Peter (2013), "Cahit Arf and his invariant" (PDF), Contributions to the history of number theory in the 20th century, Heritage of European Mathematics, Zürich: European Mathematical Society, pp. 189–222, ISBN 978-3-03719-113-2, MR 2934052, Zbl 1276.11001
Knus, Max-Albert (1991), Quadratic and Hermitian forms over rings, Grundlehren der Mathematischen Wissenschaften, vol. 294, Berlin: Springer-Verlag, pp. 211–222, doi:10.1007/978-3-642-75401-2, ISBN 3-540-52117-8, MR 1096299, Zbl 0756.11008

Kata Kunci Pencarian:

• Arf invariant
• Cahit Arf
• Arf invariant of a knot
• ARF
• Kervaire invariant
• Trefoil knot
• Seifert surface
• Rokhlin's theorem
• Unknot
• Knot invariant