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Adiabatic limit, Bismut-Freed connection, and
the real analytic torsion form
Xianzhe Daiâ and Weiping Zhangâ
Dedicated to Richard B. Melrose for his sixtieth birthday
Abstract
For a complex flat vector bundle over a fibered manifold, we con-sider the 1-parameter family of certain deformed sub-signature operatorsintroduced by Ma-Zhang in [MZ]. We compute the adiabatic limit ofthe Bismut-Freed connection associated to this family and show that theBismut-Lott analytic torsion form shows up naturally under this proce-dure.
1 Introduction
Adiabatic limit refers to the geometric degeneration when metric in certaindirections are blown up, while the remaining directions are kept fixed.
Typically, the underlying manifold has a so called fibration structure (orfiber bundle structure). That is
Z ââMÏââ B,
where Ï is a submersion and Z ' Zb = Ïâ1(b), for b â B, denotes the typicalfiber. Given a submersion metric on M :
g = ÏâgB + gZ ,
the adiabatic limit refers to the limit as 뵉 0 of
gε = εâ2ÏâgB + gZ .
This is first introduced by Witten [W] in his famous work on global gravitationalanomalies.
Witten considered the adiabatic limit of the eta invariant of Atiyah-Patodi-Singer[APS1]-[APS3]. Full mathematical treatment and generalizations aregiven by Bismut-Freed [BF], Cheeger [C], Bismut-Cheeger [BC1], Dai [D] amongothers. The adiabatic limit of the eta invariant gives rise to the Bismut-Cheegereta form, a canonically defined differential form on the base B. The eta form isâPartially supported by NSF and CNNSF.â Partially supported by MOE and CNNSF.
1
a higher dimensional generalization of the eta invariant as it gives the bound-ary contribution of the family index theorem for manifolds with boundary, seeBismut-Cheeger [BC2, BC3], and Melrose-Piazza [MP1, MP2]. The degree zerocomponent of the eta form here is exactly the eta invariant of the fibers. Thenonzero degree components therefore contain new geometric information aboutthe fibration.
Another important geometric invariant is the analytic torsion. The adia-batic limit of the analytic torsion has been considered by Dai-Melrose [DM](see also the topological treatment of Fried [Fri], Freed [Fr], and Luck-Schick-Thielmann [LST]). In contrast to the case of the eta invariant, the adiabaticlimit here does not give rise to a higher invariant. This is because the associ-ated characteristic class involved here is the Pfaffian, a top form which kills anypossible higher degree components arising from the adiabatic limit.
It should be noted that there is a complex analogue of the analytic torsion forcomplex manifolds called the holomorphic torsion. Its adiabatic limit has beenconsidered by Berthomieu-Bismut [BerB]. And it does produce the holomorphictorsion form of Bismut-Kohler [BK]. The difference can be explained by thefact that the characteristic class here is the Todd classâa stable class.
There is another way to view the higher invariants, namely via transgression.The eta form transgresses between the Chern-Weil representative of the familyindex and its Atiyah-Singer representative. Similarly, the holomorphic torsionform is the double transgression of the family index in the complex setting.Bismut-Lott [BL] uses this view point to define the real analytic torsion form,a higher dimensional generalization of the analytic torsion. It is a canonicaltransgression of certain odd cohomology classes.
There remains the question of whether the real analytic torsion form canbe obtained from the adiabatic limit process. The purpose of this paper isto answer this question in the affirmative. We show that, if one considersthe Bismut-Freed connection of the 1-parameter family of certain deformedsub-signature operators introduced by Ma-Zhang in [MZ], its adiabatic limitessentially gives rise to the Bismut-Lott real analytic torsion form. In fact, itis precisely the positive degree components of the real analytic torsion formthat is captured here. This should be compared with [DM] where the adiabaticlimit of the analytic torsion captures only the degree 0 part of the real analytictorsion form.
More precisely, let Ï : M â B be a smooth fiber bundle with compact fiberZ of dimension n. We assume that the base manifold is even dimensional. LetF be a flat complex vector bundle on M . Fix a connection for the fiber bundle,i.e., a splitting of TM
TM = THM â TZ,
where TZ denotes the vertical tangent bundle of the fiber bundle. If g is asubmersion metric on TM and hF an Hermitian metric on F , we construct,following [MZ, (3.23)], a formally self-adjoint operator of Dirac type DF anda skew-adjoint first order differential operator DF , see (3.19) for the precisedefinition (where we introduce further a complex vector bundle µ on the baseB). These operators arise as the quantizations of the symmetrization and skew-
2
symmetrization of exterior differentiation dM in the sense of [BL], viewed as aninfinite dimensional superconnection on B (cf. Lemma 3.4).
We then define an analytic invariant via zeta function regularization. Thatis, let
ÎŽ(F, r)(s) = â 12Î(s)
â« +â
0tsTrs
[DFDF (r)eât(D
F (r))2]dt,
where r is any real number and
DF (r) = DF +ââ1rDF .
The supertrace here is with respect to the Z2-grading induced by the de Rhamgrading along the fibers and the Hodge grading on the base (see (3.15) whichdefines the grading Ï).
One shows that ÎŽ(F, r)(s), well-defined for < s sufficiently large, has mero-morphic continuation to the whole complex plane with s = 0 a regular point.Therefore we define our invariant by
ÎŽ(F )(r) = ÎŽ(F, r)â²(0).
This invariant can be interpreted as the imaginary part of the Bismut-Freedconnection on certain Quillen determinant line bundle.
Our main result is
Theorem 1.1. Let Ύε(F )(r) denotes the corresponding invariant associated tothe adiabatic metric gε. Under the assumption that the flat vector bundle Fover M is fiberwise acyclic, the following identity holds,
lim뵉0
Ύε(F )(r) =â«BL(TB,âTB
)Tr,
where the torsion form Tr is defined by (3.41)
Unlike the Bismut-Lott torsion form, our torsion form Tr has only positivedegree components. However, up to a degree dependent rescaling, Tr is es-sentially the positive degree components of the Bismut-Lott torsion form (cf.(3.51)).
The paper is organized as follows. We first look at the finite dimensional casein Section 2. Thus in §2.1, we introduce flat cochain complexes, flat supercon-nections and their rescalings. The family of deformed sub-signature operatorsis then introduced in §2.2. After some preparatory results, we define an in-variant which should be interpreted as the imaginary part of the Bismut-Freedconnection form for the family of the deformed sub-signature operators. Finallyin §2.3, we study the adiabatic limit of our invariant. The fibration case is setup as an infinite dimensional analog and studied in Section 3. The flat super-connection in this case is the Bismut-Lott superconnection and is recalled in§3.1. In §3.2, we discuss the analog of the deformed sub-signature operators inthe fibration case. Then we look into the Bismut-Freed connection and definea corresponding invariant in §3.3. Finally, we study the adiabatic limit of ourinvariant in §3.4. Our main result is stated in Theorem 3.8. In §3.5, we compare
3
the Bismut-Lott real analytic torsion form with the torsion form coming out ofthe adiabatic limit.
Acknowledgements. The authors acknowledge interesting discussions withUlrich Bunke, Xiaonan Ma, Thomas Schick and Sebastian Goette. They wouldalso like to thank the referee for the constructive suggestions which have helpedus to improve the paper.
2 The finite dimensional case
In this section, we study the finite dimensional case where instead of aflat vector bundle over a fibered manifold, we consider the situation of a flatcochain complex over an even dimensional manifold. This fits well with thestructures considered in [BL] and [MZ]. The fibered manifold case is the infinitedimensional analog which will be considered in the next section.
2.1 Superconnections and flat cochain complex
Let (E, v) be a Z-graded cochain complex of finite rank complex vectorbundles over a closed manifold B,
(E, v) : 0â E0 vâ E1 vâ · · · vâ En â 0.(2.1)
Let âE = âni=0âEi
be a Z-graded connection on E. We call (E, v,âE) a flatcochain complex if the following two conditions hold,(
âE)2
= 0,[âE , v
]= 0.(2.2)
Let hE = âni=0hEi be a Z-graded hermitian metric on E and denote by
vâ : Eâ â Eââ1 the adjoint of v with respect to hE . Let (âE)â denote theadjoint connection of âE with respect to gE . Then (cf. [BZ, (4.1), (4.2)] and[BL, §1(g)]) (
âE)â
= âE + Ï(E, hE
),(2.3)
where
Ï(E, hE) =(hE)â1 (âEhE) .(2.4)
Consider the superconnections on E in the sense of Quillen [Q] defined by
Aâ² = âE + v, Aâ²â² =(âE)â
+ vâ.(2.5)
Let N â End(E) denote the number operator of E which acts on Ei bymultiplication by i. We extend N to an element of Ω0(B,End(E)).
Following [BL, (2.26), (2.30)], for any u > 0, set
C â²u = uN/2Aâ²uâN/2 = âE +âuv,(2.6)
C â²â²u = uâN/2Aâ²â²uN/2 =(âE)â
+âuvâ,
Cu =12(C â²u + C â²â²u
), Du =
12(C â²â²u â C â²u
).
4
Then we have
C2u = âD2
u, [Cu, Du] = 0.(2.7)
Let
âE,e = âE +12Ï(E, hE
)(2.8)
be the Hermitian connection on (E, hE) (cf. [BL, (1.33)] and [BZ, (4.3)]). Then
Cu = âE,e +âu
2(v + vâ)(2.9)
is a superconnection on E, while
Du =12Ï(E, hE
)+âu
2(vâ â v)(2.10)
is an odd element in Câ(B,Îâ(B)âEnd(E)).
2.2 Deformed signature operators and the Bismut-Freed con-nection
We assume in the rest of this section that p = dimB is even and B isoriented.
Let gTB be a Riemannian metric on TB. For X â TB, let c(X), c(X) bethe Clifford actions on Î(T âB) defined by c(X) = Xââ§âiX , c(X) = Xââ§+iX ,where Xâ â T âB corresponds to X via gTB (cf. [BL, (3.18)] and [BZ, §4(d)]).Then for any X, Y â TB,
c(X)c(Y ) + c(Y )c(X) = â2ãX,Y ã,(2.11)c(X)c(Y ) + c(Y )c(X) = 2ãX,Y ã,c(X)c(Y ) + c(Y )c(X) = 0.
Let e1, · · · , ep be a (local) oriented orthonormal basis of TB. Set
Ï =(ââ1) p(p+1)
2 c(e1) · · · c(ep).(2.12)
Then Ï is a well-defined self-adjoint element such that
Ï2 = Id|Î(T âB).(2.13)
Let µ be a Hermitian vector bundle on B carrying a Hermitian connectionâµ with the curvature denoted by Rµ = (âµ)2. Let âTB be the Levi-Civitaconnection on (TB, gTB) with its curvature RTB. LetâÎ(T âB) be the Hermitianconnection on Î(T âB) canonically induced from âTB. Let âÎ(T âB)âµâE,e bethe tensor product connection on Î(T âB)â µâ E given by
âÎ(T âB)âµâE,e = âÎ(T âB) â IdµâE + IdÎ(T âB) ââµ â IdE + IdÎ(T âB)âµ ââE,e.(2.14)
5
Let the Clifford actions c, c extend to actions on Î(T âB)âµâE by actingas identity on µ â E. Let ε be the induced Z2-grading operator on E, i.e.,ε = (â1)N on E. We extend ε to an action on Î(T âB) â µ â E by acting asidentity on Î(T âB)â µ.
Let Ïâε define the Z2-grading on (Î(T âB)â µ)âE. Then
D嵉Esig =
pâi=1
c(ei)âÎâ(T âB)âµâE,eei(2.15)
defines the twisted signature operator with respect to this Z2-grading. Playingan important role here is its deformation, given by
D嵉Esig,u = D嵉E
sig +âu
2(v + vâ) ,(2.16)
with u > 0, which might be thought of as a quantization of Cu.Let Yu be the skew adjoint element in Endodd(Îâ(T âB)âµâE) defined by
(cf. [MZ, (2.18)])
Yu =12
pâi=1
c(ei)Ï(E, hE
)(ei) +
âu
2(vâ â v) ,(2.17)
which might be thought of as a quantization of Du.Now following [MZ, Definition 2.3], for any r â R, define
D嵉Esig,u (r) = D嵉E
sig,u +ââ1rYu.(2.18)
From (2.15)-(2.18), one has (cf. [MZ, (2.22)])
(2.19) D嵉Esig,u (r) =
pâi=1
c(ei)(âÎâ(T âB)âµâE,eei +
ââ1r2
Ï(E, hE
)(ei))
+âu
2((
1âââ1r
)v +
(1 +ââ1r
)vâ).
Proposition 2.1. We have the following asymptotic expansion
Trs
[D嵉E
sig,u (r)Yueât(DµâEsig,u (r))2
]= c0(u, r) + c1(u, r) t+ · · ·(2.20)
as tâ 0+. The expansion is uniform for (u, r) in a compact set.
Proof. We introduce two auxiliary Grassmann variables z1, z2 and write
Trs
[D嵉E
sig,u (r)Yueât(DµâEsig,u (r))2
]=(2.21)
âtâ2Trs,z1,z2[eât([DµâEsig,u (r)]2âz1DµâEsig,u (r)âz2Yu)
],
where we use the convention that Trs,z1,z2 [a+ bz1 + cz2 + dz1z2] = Trs[d] whena, b, c, d do not contain z1 and z2. Here the minus sign comes from the orderof the appearance of z1, z2 and D嵉E
sig,u (r), Yu.
6
Applying the standard elliptic theory to the right hand side of (2.21), wederive an asymptotic expansion
Trs
[D嵉E
sig,u (r)Yueât(DµâEsig,u (r))2
]= câ p
2â2(u, r)tâ
p2â2 + câ p
2â1(u, r)tâ
p2â1
+ · · ·+ c0(u, r) + c1(u, r) t+ · · · .
On the other hand, by the Lichnerowicz formula (Cf. (2.30)) and the sameargument as in [BF], we have
limtâ0
tTrs
[D嵉E
sig,u (r)Yueât(DµâEsig,u (r))2
]= 0.
It follows then that ci(u, r) = 0 for âp2 â 2 †i †â1. Thus, the asymptotic
expansion starts with the constant term.
Since
Trs
[D嵉E
sig,u (r)Yueât(DµâEsig,u (r))2
]= âTrs
[YuD
µâEsig,u (r)eât(D
嵉Esig,u (r))2
]is easily seen to be exponentially decaying as t â +â, the quantity on theright hand side of the following definition is well-defined.
Definition 2.2. We define
ÎŽu(E, v)(r) =â« â
0Trs
[D嵉E
sig,u (r)Yueât(DµâEsig,u (r))2
]dt.(2.22)
Remark 2.3. If Hâ(E, v) = 0, i.e., (E, v) is acyclic, by [MZ, (2.27)], which werecall as follows,((
1âââ1r
)v +
(1 +ââ1r
)vâ)2
=(1 + r2
)(v + vâ)2 ,(2.23)
(2.19) and proceed as in [BC1], one sees that when u > 0 is large enough,D嵉E
sig,u (r) is invertible for fixed r â R. Since by (2.18) one has
âDµâEsig,u (r)âr
=ââ1Yu,
ââ12 ÎŽu(E, v)(r) is (the imaginary part of) the Bismut-Freed connection form
([BF], see also [DF, (3.8)]) of the Quillen determinant line bundle of the R-family of operators D嵉E
sig,u (r)râR.
2.3 Adiabatic limit as uâ +â
We first rewrite ÎŽu(E, v)(r) as
ÎŽu(E, v)(r) =â« â
0Trs
[Dε(r)Y εeâtD
2ε (r)]dt,(2.24)
7
where ε = uâ12 and
Y ε =ε
2c(Ï) +
12
(vâ â v),(2.25)
Dε(r) = εDµâEsig,u +
ââ1rY ε.
We fix a square root ofââ1 and let Ï : Î(T âB) â Î(T âB) be the homo-
morphism defined by Ï : Ï â Îi(T âB)â (2Ïââ1)âi/2Ï. The formulas in what
follows will not depend on the choice of the square root ofââ1.
Let L(TB,âTB) be the Hirzebruch characteristic form defined by
L(TB,âTB) = Ïdet1/2
(RTB
tanh (RTB/2)
),
and ch(µ,âµ) be the Chern character form defined by
ch(µ,âµ) = ÏTr [exp(âRµ)] .
Proposition 2.4. We have
(2.26) lim뵉0
Trs[Dε(r)Y εeâtD
2ε (r)]
= ââ«BL(TB,âTB
)ch (µ,âµ)
· ÏTrs
[tâ
12Dt
(12
(v + vâ) +ââ1r2
(vâ â v))eâ(Ct+
ââ1rDt)2
].
Proof. As in [BF] and [BC1], we introduce an auxiliary Grassmann variable zand rewrite
Trs[Dε(r)Y εeâtD
2ε (r)]
= Trs,z[Y εtâ
12 eâtD
2ε (r)+z
âtDε(r)
],(2.27)
where for elements of the form A+ zB with A, B containing no z, we have asin [BF] and [BC1] that Trs,z[A+ zB] = Trs[B].
By (2.16) and (2.25), one has
(2.28) Dε(r) = εDµâEsig +
12
(v + vâ) +ââ1r
(ε
2c(Ï) +
12
(vâ â v))
= ε
(D嵉E
sig +ââ1r
12c(Ï)
)+
12
(v + vâ) +ââ1r
12
(vâ â v) .
Denote by
V =12
(v + vâ) +ââ1r
12
(vâ â v) .(2.29)
8
By Lichnerowicz formula, we have (for simplicity we denoteâ = âÎâ(T âB)âµâE,e)
(2.30)
tD2ε (r)âz
âtDε(r) = tε2
(D嵉E
sig
)2+ tε2
[D嵉E
sig ,ââ1r
12c(Ï)
]+ tε
[D嵉E
sig , V]
+ t(ââ1r
ε
2c(Ï) + V
)2â zât(εDµâE
sig +ââ1r
ε
2c(Ï) + V
)= ât
(뵉ei +
12âtzc(ei)
)2
+tε2
4kTB +
tε2
2c(ei)c(ej)âRµâE,e(ei, ej)
+tε2
8RTBijklc(ei)c(ej)c(ek)c(el) + tεc(ei)âeiV +
ââ1r2
tε2c(ei)c(ej)âeiÏj
â tε2ââ1r
pâi=1
Ï(ei)âei + t
(ââ1r2
εc(Ï) + V
)2
â zâtV â z
ââ1r2
âtεc(Ï),
where RTB is the Riemannian curvature and kTB is the scalar curvature of gTB,while RµâE,e is the curvature of the connection on µâE obtained through âµand âE,e.
Now we find ourself exactly in the situation of [BC1]. Near any point x âM ,take a normal coordinate system xi and the associated orthonormal basis ei.
We first conjugate tD2ε (r)â z
âtDε(r) by the exponential e
zPpi=1
xic(ei)
2âtε and then
apply the Getzler transformation Gâtε. One finds that after these procedures,the operator tD2
ε (r)â zâtDε(r) tends to, as εâ 0,
(2.31) â(âi +
14RTBij xj
)2
+14RTBkl c(ek)c(el) +R嵉E,e + t
12âV +
ââ1r2âÏ
+(ââ1r2
Ï + t12V
)2
â zâtV
= â(âi +
14RTBij xj
)2
+14RTBkl c(ek)c(el) +Rµ
+(âE,e +
ââ1r2
Ï + t12V
)2
â zâtV
= â(âi +
14RTBij xj
)2
+14RTBkl c(ek)c(el) +
(Ct +
ââ1rDt
)2â zât
(12
(v + vâ) +ââ1r2
(vâ â v)).
On the other hand, by (2.25) it is clear that under the same procedures, Y ε
tends to, as 뵉 0,
tâ12
(12Ï +ât
2(vâ â v)
)= tâ
12Dt.(2.32)
From (2.27), (2.31) and (2.32), by proceeding with the by now standard localindex techniques, and keeping in mind that the supertrace in the left hand sidesof (2.26) and (2.27) are respect to the Z2-grading defined by Ïâε, one derives(2.26).
9
We now examine the terms appearing in the right hand side of (2.26).By (cf. [MZ, (2.34)])(
Ct +ââ1rDt
)2=(1 + r2
)C2t = â
(1 + r2
)D2t ,(2.33)
and
v + vâ = â2tâ12 [N,Dt] , vâ â v = â2tâ
12 [N,Ct] ,(2.34)
we have
(2.35) â Trs
[tâ
12Dt
(12
(v + vâ) +ââ1r2
(vâ â v))eâ(Ct+
ââ1rDt)2
]= â 1
2âtTrs
[Dt (v + vâ) e(1+r2)D2
t
]âââ1r
2ât
Trs[Dt (vâ â v) e(1+r2)D2
t
]=
1tTrs
[Dt [N,Dt] e(1+r2)D2
t
]+ââ1rt
Trs[Dt [N,Ct] e(1+r2)D2
t
]= â1
tTrs
[ND2
t e(1+r2)D2
t âDtNDte(1+r2)D2
t
]+ââ1rt
dTrs[NDte
(1+r2)D2t
],
where in the last equality we have used (2.7) (compare also with [MZ, (2.75)]).We are now ready to prove the following main result of this section.
Theorem 2.5. Under the assumption that the flat cochain complex (E, v) isacyclic, Hâ(E, v) = 0, the following identity holds:
12
limuâ+â
ÎŽu(E, v)(r) =â«BL(TB,âTB
)ch (µ,âµ) Tr,(2.36)
where
Tr = ââ« â
0ÏTrs
[ND2
t e(1+r2)D2
t
] dtt.(2.37)
Proof. First of all, the assumption that Hâ(E, v) = 0 implies that the eigen-values of Dε(r) are uniformly bounded away from zero. Hence the integral in(2.24) is uniformly convergent at t =â.
We now examine the same issue at t = 0. From Proposition 2.1, one has
Trs[Dε(r)Y εeât(Dε(r))
2]
= c0(ε, r) + c1(ε, r) t+ · · · .(2.38)
We claim that this asymptotic expansion is in fact uniform in ε as ε â 0 andthe coefficients converge to that of asymptotic expansion of the right hand sideof (2.26). This can be seen by an argument similar to that of [BC1], whichis carried out in detail later for the infinite dimensional case; see the proof ofProposition 3.6.
Our theorem now follows from Proposition 2.4, the equation (2.35) and theabove discussion.
10
Remark 2.6. By Remark 2.3, one sees that under the assumption of Theorem2.5, for each r â R, when u > 0 is large enough,
ââ12 ÎŽu(E, v)(r) is the Bismut-
Freed connection form of the R-family of the operators DµâEsig,u (r)râR at r.
On the other hand, by comparing the right hand side of (2.37) with [BL] and[MZ], one sees that Tr here gives, up to rescaling, the nonzero degree termsof the Bismut-Lott torsion form ([BL]). Thus, we can say that one obtainsthe Bismut-Lott torsion form through the adiabatic limit of the Bismut-Freedconnection. This is the main philosophy we would like to indicate in this paper.
3 Sub-signature operators, adiabatic limit and theBismut-Lott torsion form
In this section, we deal with the fibration case. We will show that, foran acyclic flat complex vector bundle over a fibered manifold, if we considerthe Bismut-Freed connection form [BF] on the Quillen determinant line bundleassociated to the 1-parameter family constructed in [MZ, Section 3], then theBismut-Lott analytic torsion form [BL] will show up naturally through theadiabatic limit of this connection form. This tautologically answers a questionasked implicitly in the original article of Bismut-Lott.
3.1 The Bismut-Lott Superconnection
We first set up the fibration case as an infinite dimensional analog of the caseconsidered in the previous section. Let Ï : M â B be a smooth fiber bundlewith compact fiber Z of dimension n. We denote by m = dimM, p = dimB.Let TZ be the vertical tangent bundle of the fiber bundle, and let T âZ be itsdual bundle.
Let TM = THM â TZ be a splitting of TM . Let P TZ , P THM denote the
projection from TM to TZ, THM . If U â TB, let UH be the lift of U in THM ,so that ÏâUH = U .
Let F be a flat complex vector bundle on M and let âF denote its flatconnection.
Let E = âni=0Ei be the smooth infinite-dimensional Z-graded vector bundle
over B whose fiber over b â B is Câ(Zb, (Î(T âZ)â F )|Zb). That is
Câ(B,Ei) = Câ(M,Îi(T âZ)â F ).(3.1)
Definition 3.1. For s â Câ(B,E) and U a vector field on B, let âE be aZ-grading preserving connection on E defined by
âEUs = LUHs,(3.2)
where the Lie derivative LUH acts on Câ(B,E) = Câ(M,Îi(T âZ)â F ).
If U1, U2 are vector fields on B, put
T (U1, U2) = âP TZ [UH1 , UH2 ] â Câ(M,TZ).(3.3)
11
We denote by iT â Ω2(B,Hom(Eâ¢, Eâ¢â1)) the 2-form on B which, to vectorfields U1, U2 on B, assigns the operation of interior multiplication by T (U1, U2)on E.
Let dZ be the exterior differentiation along fibers. We consider dZ to bean element of Câ(B,Hom(Eâ¢, Eâ¢+1)). The exterior differentiation operatordM , acting on Ω(M,F ) = Câ(M,Î(T âM) â F ), has degree 1 and satisfies(dM )2 = 0. By [BL, Proposition 3.4], we have
dM = dZ +âE + iT .(3.4)
So dM is a flat superconnection of total degree 1 on E. We have(dZ)2
= 0,[âE , dZ
]= 0.(3.5)
Let gTZ be a metric on TZ. Let hF be a Hermitian metric on F . Let âFâbe the adjoint of âF with respect to hF . Let Ï(F, hF ) and âF,e be the 1-formon M and the connection on F defined as in (2.3), (2.8).
Let o(TZ) be the orientation bundle of TZ, a flat real line bundle on M . LetdvZ be the Riemannian volume form on fibers Z associated to the metric gTZ
(Here dvZ is viewed as a section of ÎdimZ(T âZ)âo(TZ)). Let ã , ãÎ(T âZ)âF bethe metric on Î(T âZ) â F induced by gTZ , hF . Then E acquires a Hermitianmetric hE such that for α, αⲠâ Câ(B,E) and b â B,
âšÎ±, αâ²
â©hE
(b) =â«Zb
âšÎ±, αâ²
â©Î(T âZ)âF dvZb .(3.6)
Let âEâ, dZâ, (dM )â, (iT )â be the formal adjoints of âE , dZ , dM , iT withrespect to the scalar product ã , ãhE . Set
DZ = dZ + dZâ, âE,e =12(âE +âEâ
),(3.7)
Ï(E, hE) = âEâ ââE .
Let NZ be the number operator of E, i.e. NZ acts by multiplication by kon Câ(M,Îk(T âZ)â F ). For u > 0, set
C â²u = uNZ/2dMuâNZ/2, C â²â²u = uâNZ/2(dM)âuNZ/2,(3.8)
Cu =12(C â²u + C â²â²u
), Du =
12(C â²â²u â C â²u
).
Then C â²â²u is the adjoint of C â²u with respect to hE . Moreover, Cu is a supercon-nection on E and Du is an odd element of Câ(B,End(E)), and
C2u = âD2
u, [Cu, Du] = 0.(3.9)
Let gTB be a Riemannian metric on TB. Then gTM = gTZâÏâgTB is a met-ric on TM . Let âTM , âTB denote the corresponding Levi-Civita connectionson TM, TB. Put âTZ = P TZâTM , a connection on TZ. As shown in [B, The-orem 1.9], âTZ is independent of the choice of gTB. Then 0â = âTZâÏââTB is
12
also a connection on TM . Let S = âTMâ0â. By [B, Theorem 1.9], ãS(·)·, ·ãgTMis a tensor independent of gTB. Moreover, for U1, U2 â TB, X,Y â TZ,âš
S(UH1)X,UH2
â©gTM
= ââšS(UH1)UH2 , X
â©gTM
(3.10)
=âšS(X)UH1 , U
H2
â©gTM
=12âšT(UH1 , U
H2
), Xâ©gTM
,âšS(X)Y,UH1
â©gTM
= ââšS(X)UH1 , Y
â©gTM
=12
(LUH1
gTZ)
(X,Y ),
and all other terms are zero.Let fαpα=1 be an orthonormal basis of TB, let fαpα=1 be the dual basis
of T âB. In the following, itâs convenient to identify fα with fHα . Let eini=1 bean orthonormal basis of (TZ, gTZ). We define a horizontal 1-form k on M by
k(fα) = ââi
ãS(ei)ei, fαã .(3.11)
Set
c(T ) =12
âα,β
fα ⧠fβc (T (fα, fβ)) ,(3.12)
c(T ) =12
âα,β
fα ⧠fβ c (T (fα, fβ)) .
Let âÎ(T âZ) be the connection on Î(T âZ) induced by âTZ . Let âTZâF,ebe the connection on Î(T âZ) â F induced by âÎ(T âZ), âF,e. Then by [BL,(3.36), (3.37), (3.42)],
DZ =âj
c(ej)âTZâF,eej â 12
âj
c(ej)Ï(F, hF )(ej
),(3.13)
dZâ â dZ = ââj
c(ej)âTZâF,eej +12
âj
c(ej)Ï(F, hF
)(ej),
âE,e =âα
fα(âTZâF,efα
+12k (fα)
),
Ï(E, hE
)=âα
fα
âi,j
ãS(ei)ej , fαã c(ei)c(ej) + Ï(F, hF )(fα)
.
By [BL, Proposition 3.9], one has
Cu =âu
2DZ +âE,e â 1
2âuc(T ),(3.14)
Du =âu
2(dZâ â dZ
)+
12Ï(E, hE
)â 1
2âuc(T ).
13
3.2 Deformed sub-signature operators on a fibered manifold
We assume now that TB is oriented.Let (µ, hµ) be a Hermitian complex vector bundle over B carrying a Her-
mitian connection âµ.Let NB, NM be the number operators on Î(T âB),Î(T âM), i.e. they act as
multiplication by k on Îk(T âB),Îk(T âM) respectively. Then NM = NB +NZ .Let âÎ(T âM) be the connection on Î(T âM) canonically induced from âTM .
Let âÎ(T âM)âÏâµâF (resp. âÎ(T âM)âÏâµâF,e) be the tensor product connectionon Î(T âM)â Ïâµâ F induced by âÎ(T âM), Ïââµ and âF (resp. âF,e).
Let eama=1 be an orthonormal basis of TM , and its dual basis eama=1.(Note that eini=1 denotes an orthonormal basis of TZâthe difference lies inthe letter used for the subscript index; namely âiâ vs. âaâ.) Let fαpα=1 be anoriented orthonormal basis of TB. Set
Ï(TB) = (ââ1)
p(p+1)2 c
(fH1)· · · c
(fHp),(3.15)
Ï = (â1)NZÏ(TB).
Then the operators Ï(TB), Ï act naturally on Î(T âM), and
Ï(TB)2 = Ï2 = 1.(3.16)
Let dâµ
: Ωa(M,Ïâµâ F )â Ωa+1(M,Ïâµâ F ) be the unique extension ofâµ,âF which satisfies the Leibniz rule. Let dâ
µâ be the adjoint of dâµ
withrespect to the scalar product ã , ãΩ(M,ÏâµâF ) on Ω(M,Ïâµ â F ) induced bygTM , hµ, hF as in (3.6). As in [BZ, (4.26), (4.27)], we have
dâµ
=âa
ea â§âÎ(T âM)âÏâµâFea ,(3.17)
dâµâ = â
âa
iea â§(âÎ(T âM)âÏâµâFea + Ï
(F, hF
)(ea)
).
Following [Z1], let âÎ(T âM) be the Hermitian connection on Î(T âM) definedby (cf. [Z1, (1.21)])
âÎ(T âM)X = âÎ(T âM)
X â 12
pâα=1
c(P TZS(X)fα
)c (fα) , X â TM.(3.18)
Let âe be the tensor product connection on Î(T âM)âÏâµâF induced byâÎ(T âM), Ïââµ and âF,e. Following [MZ, (3.23)], for any r â R, set
DÏâµâF =mâa=1
c(ea)âeea â12
nâi=1
c(ei)Ï(F, hF
)(ei),(3.19)
DÏâµâF = ânâi=1
c(ei)âeei +12
mâa=1
c(ea)Ï(F, hF
)(ea)
â 14
pâα,β=1
c (T (fα, fβ)) c(fα)c (fβ) ,
DÏâµâF (r) = DÏâµâF +ââ1rDÏâµâF .
14
From (3.19), the operators DÏâµâF , DÏâµâF (r) are formally self-adjoint firstorder elliptic operators, and DÏâµâF is a skew-adjoint first order differentialoperator. Moreover, the operator DÏâµâF is locally of Dirac type.
By [MZ, (3.20) and Proposition 3.4], one has
DÏâµâF =12[(dâ
µ+ dâ
µâ)+ (â1)p+1Ï(dâ
µ+ dâ
µâ) Ï] ,(3.20)
DÏâµâF =12[(dâ
µâ â dâµ)
+ (â1)p+1Ï(dâ
µâ â dâµ)Ï],
which partly explains the motivation of introducing these operators (comparewith (2.25)); see also Lemma 3.4.
By (3.15), (3.16) and (3.20), one verifies (cf. [MZ, (3.28)])
ÏDÏâµâF = (â1)p+1DÏâµâF Ï, ÏDÏâµâF = (â1)p+1DÏâµâF Ï.(3.21)
Remark 3.2. It is important to note that by (3.21), when p = dimB is even,both DÏâµâF and DÏâµâF anti-commute with Ï .
Remark 3.3. When µ = F = C and p = dimB is even, DÏâµâF has beenconstructed in [Z1] and [Z2], where it is called the sub-signature operator.
3.3 Bismut-Freed connection of the deformed family
We assume that p = dimB is even. Moreover, we make the following tech-nical assumption.
Technical assumption. The flat vector bundle F over M is fiberwise acyclic,that is, Hâ(Zb, F |Zb) = 0 on each fiber Zb, b â B.
For any ε > 0, we change gTB to 1εgTB and do everything again for gTMε =
gTZ â 1εÏâgTB. We will use a subscript ε to denote the resulting objects.
For any r â R, one verifies directly that the coefficients of 1âε
in 1âεDÏâµâFε (r)
is given by dZ + dZâ âââ1r
(dZ â dZâ
). Since(
dZ + dZâ âââ1r
(dZ â dZâ
))2=(1 + r2
) (dZ + dZâ
)2,(3.22)
by proceeding as in [BC1], one sees that when ε > 0 is small enough, DÏâµâFε (r)
is invertible. In fact, the eigenvalues of DÏâµâFε (r) are uniformly bounded away
from zero.Consider now DÏâµâF
ε (r)râR as an R-family of operators which anti-commute with the Z2-grading defined by Ï .
Then one can construct the Quillen determinant line bundle over R and theassociated Bismut-Freed connection on it (cf. [BF]). Moreover, by the abovediscussion and by [BF, 3.8], we know that when ε > 0 is small enough, the
15
imaginary part of the Bismut-Freed connection form is given by
12ââ1
F.P.â« +â
0Trs
[DÏâµâFε (r)
âDÏâµâFε (r)âr
eâtâDÏâµâFε (r)
â2]dt
=12
F.P.â« +â
0Trs
[DÏâµâFε (r)DÏâµâF
ε eâtâDÏâµâFε (r)
â2]dt
= â12
F.P.â« +â
0Trs
[DÏâµâFε DÏâµâF
ε (r)eâtâDÏâµâFε (r)
â2]dt,
where the supertrace is with respect to Ï and âF.P.â means taking the finite partof the (divergent) integral. As usual we use the zeta function regularization.Thus, we define
Ύε(F, r)(s) = â 12Î(s)
â« +â
0tsTrs
[DÏâµâFε DÏâµâF
ε (r)eâtâDÏâµâFε (r)
â2]dt.
(3.23)
Remark. Note that we have built the factor 12 into the definition (unlike the
finite dimensional case).
In the next subsection we will study the asymptotic expansions of the inte-grand in (3.23) which implies that the integral, convergent for < s sufficientlylarge, has meromorphic continuation to the whole complex plane with s = 0 aregular point. Therefore we define our invariant by
Ύε(F )(r) = Ύε(F, r)â²(0).(3.24)
Also in the next section we will compute the adiabatic limit of Ύε(F )(r) asεâ 0.
We remark that the definition of Ύε(F )(r) itself need not make use of thetechnical assumption Hâ(Zb, F |Zb) = 0.
3.4 The adiabatic limit and the torsion form
We begin with a lemma.
Lemma 3.4. DÏâµâF is the quantization of D4; namely, it is obtained byreplacing the horizontal differential forms in D4 by the corresponding Cliffordmultiplications. Similarly, DÏâµâF is the quantization of C4.
Proof. By (3.19),
DÏâµâF = ânâi=1
c(ei)âeei+12
mâa=1
c(ea)Ï(F, hF
)(ea)â
14
pâα,β=1
c (T (fα, fβ)) c(fα)c (fβ) ,
where the connection âÎ(T âM) is defined by (3.18). Thus, we now look at theconnection in a bit more detail. Since âTM = 0â+S and 0â = âTZâÏââTB,
16
we find (for simplicity, we denote Sijα = ãS(ei)ej , fαã and so on)
âÎ(T âM)ei = âÎ(T âZ)
ei â14
[Sijα (c(ej)c(fα)â c(ej)c(fα) + c(ej)c(fα)â c(ej)c(fα))
+Siαj(c(fα)c(ej)â c(fα)c(ej) + c(fα)c(ej)â c(fα)c(ej))
+Siαβ(c(fα)c(fβ)â c(fα)c(fβ) + c(fα)c(fβ)â c(fα)c(fβ))]
= âÎ(T âZ)ei â 1
2Siαj [c(fα)c(ej)â c(fα)c(ej)]
â14Siαβ [c(fα)c(fβ)â c(fα)c(fβ) + c(fα)c(fβ)â c(fα)c(fβ)] .
Hence
âÎ(T âM)ei = âÎ(T âZ)
ei â 12Sijαc(fα)c(ej)
â14Siαβ [c(fα)c(fβ)â c(fα)c(fβ) + c(fα)c(fβ)â c(fα)c(fβ)] .
Therefore,
c(ei)âÎ(T âM)ei = c(ei)âÎ(T âZ)
ei
â14Siαβ c(ei) [c(fα)c(fβ)â c(fα)c(fβ) + c(fα)c(fβ)â c(fα)c(fβ)] .
And so
c(ei)âeei = c(ei)âTZâF,eei â 18c(T (fα, fβ))c(fα)c(fβ) +
18c(T (fα, fβ))c(fα)c(fβ)
â18c(T (fα, fβ))[c(fα)c(fβ)â c(fα)c(fβ)].
The last term here, â18 c(T (fα, fβ))[c(fα)c(fβ) â c(fα)c(fβ)], vanishes by the
antisymmetry. Using the formula above together with (3.13), (3.14), (3.19), weprove our lemma. (The other case is dealt with similarly.)
Proposition 3.5. We have
(3.25)
lim뵉0
Trs
[DÏâµâFε DÏâµâF
ε (r)eâtâDÏâµâFε (r)
â2]= â
â«BL(TB,âTB
)ch (µ,âµ)
· ÏTrs
[tâ
12D4t
â
âât
(C4t +
ââ1rD4t
)eâ(1+r2)C2
4t
].
Proof. Again, we introduce an auxiliary Grassmann variable z and rewrite
Trs
[DÏâµâFε DÏâµâF
ε (r)eâtâDÏâµâFε (r)
â2]=
(3.26)
âTrs,z
[tâ
12 DÏâµâF
ε eâtâDÏâµâFε (r)
â2+zâtDÏ
âµâFε (r)
].
17
The following Lichnerowicz formula was proved in [Z1, Theorem 1.1].
(3.27)(DÏâµâF
)2= ââe +
K
4+
12
mâa,b=1
c(ea)c(eb)(Re + ÏâRµ)(ea, eb)
+14
nâi=1
(Ï(F, hF
)(ei))2
+18
nâi,j=1
c(ei)c(ej)(Ï(F, hF
))2(ei, ej)
â 12
mâa=1
c(ea)[ nâi=1
c(ei)âTMâF,eea Ï(F, hF
)(ei)
+pâ
α=1
c(fα)Ï(F, hF
)(P TZS(ea)fα)
].
Similarly, the following formulas are shown in [MZ, Proposition 3.6].
(3.28)(DÏâµâF
)2=
nâi=1
((âeei)
2 â âeâTMei ei
)+
12
nâi,j=1
c(ei)c(ej)(âe)2(ei, ej)
+14
nâi=1
c(ei)[âeei ,
pâα,β=1
c(T (fα, fβ))c(fα)c(fβ)]
+12
pâα,β=1
c(fα)c(fβ)âeT (fα,fβ) â12
nâi=1
mâa=1
c(ei)c(ea)(âTMâF,eei Ï(F, hF
))(ea)
â 14
mâa=1
(Ï(F, hF
)(ea)
)2+
18
mâa,b=1
c(ea)c(eb)(Ï(F, hF
))2(ea, eb)
+116
( pâα,β=1
c(T (fα, fβ))c(fα)c(fβ))2,
(3.29)
[DÏâµâF , DÏâµâF ] = âmâa=1
nâi=1
c(ea)c(ei)(Re + ÏâRµ +
14Ï(F, hF
)2)(ea, ei)
âpâ
α=1
Ï(F, hF
)(fα)âefα +
14
pâα,β=1
Ï(F, hF
)(T (fα, fβ))c(fα)c(fβ)
+14
mâa=1
c(ea)[âeea ,
pâα,β=1
c(T (fα, fβ))c(fα)c(fβ)].
Therefore one can apply the standard Getzler rescaling to (DÏâµâFs,ε )2 and
[DÏâµâFs,ε , DÏâµâF
s,ε ] with no problem and all terms converge as εâ 0.On the other hand, in [Z1, Proposition 2.2], Zhang formulated a Lichnerow-
icz type formula for t(DÏâµâFs,ε )2 â z
âtDÏâµâF
s,ε . The only singular term (for
18
Getzlerâs rescaling) as εâ 0 appears in
âtεâα
(âfα +
âε
2
âi,β
ãS(fα)ei, fβãc(ei)c(fβ) +zc(fα)2âtε
)2.(3.30)
This singular term can be easily eliminated by the exponential transform,namely conjugating by the exponential
(3.31) ez
Ppα=1 yαc(fα)
2âtε .
We then do the Getzler rescaling Gâtε:
yα ââtεyα, âfα â
1âtεâfα , c(fα)â 1â
tεfα ⧠â
âtεifα .
By (3.9), (3.10), (3.19), (3.30), [Z1, Proposition 2.2], and by proceeding similarlyas in [BC1, (4.69)], after the conjugation by (3.31), the Gâtε rescaled operatorof t(DÏâµâF
s,ε (r))2 â zâtDÏâµâF
s,ε (r) converges as εâ 0 to
H+ (1 + r2)(Cµ4t)2 â z
(âtDZ +
c(T )4ât
+ââ1r
(ât(dZâ â dZ) +
c(T )4ât
))= H+ (1 + r2)(C2
4t +Rµ)â z2t âât
(C4t +ââ1rD4t),(3.32)
where
H = ââα
(âfα +
14âšRTBb0 y, fα
â©)2
â 14
âα,β
âšRTBb0 fα, fβ
â©c(fα)c(fβ)
Finally, by the previous lemma, we see that the rescaled operator obtainedfrom the conjugation by (3.31) of DÏâµâF
ε converges to tâ1/2D4t as ε â 0.Proceeding as in [MZ] and noting 2t âât =
ât ââât, we obtain the desired formula.
Proposition 3.6. We have the following uniform asymptotic expansion
(3.33)
Trs
[DÏâµâFε DÏâµâF
ε (r)eâtâDÏâµâFε (r)
â2]= câk(ε) tâk+câk+1(ε) tâk+1+· · · ,
where k = 32 if n (dimension of the fiber) is odd and k = 1 if n is even.
Similarly,
(3.34)
ââ«BL(TB,âTB
)ch (µ,âµ)ÏTrs
[tâ
12D4t
â
âât
(C4t +
ââ1rD4t
)eâ(1+r2)C2
4t
]= câk t
âk + câk+1 tâk+1 + · · · .
Moreover,ci/2(ε) ââ ci/2 as εâ 0.
19
Proof. Using two auxiliary Grassmann variables z1, z2, we write
Trs
[DÏâµâFε DÏâµâF
ε (r)eâtâDÏâµâFε (r)
â2](3.35)
= tâ2Trs,z1,z2
[eâtâ
[DÏâµâFε (r)]2âz1DÏ
âµâFε (r)âz2 bDÏâµâFε
â].
Applying the standard elliptic theory to the right hand side of (3.35), we derivean asymptotic expansion
Trs
[DÏâµâFε DÏâµâF
ε (r)eâtâDÏâµâFε (r)
â2]= câm/2â2(ε) tâm/2â2
+ câm/2â1(ε) tâm/2â1 + · · · .
To prove the vanishing of the coefficients, we revert to one auxiliary Grass-mann variable z and rewrite
t32 Trs
[DÏâµâFε DÏâµâF
ε (r)eâtâDÏâµâFε (r)
â2](3.36)
= âTrs,z
[t DÏâµâF
ε eâtâDÏâµâFε (r)
â2+zâtDÏ
âµâFε (r)
].
As usual, one fixes a point of M and employs the normal coordinates xaround the point. Consider the Getzler rescaling GMâ
t:
xa âât xa, âea â
1âtâea , c(ea)â
1âtea ⧠â
ât iea .
By (3.27), (3.28), (3.29) and the same argument as in [BF], we can formulate
a Lichnerowicz formula for t(DÏâµâFε (r)
)2âzâtDÏâµâF
ε (r). The only singular
term with respect to the Getzler rescaling GMât
as tâ 0 appears in
âtεpâa=1
(âea +
zc(ea)2âtε
)2â t
mâa=p+1
(âea +
zc(ea)2ât
)2.
This singular term can be easily eliminated by the exponential transform,namely conjugating by the exponential
ez
Pma=1 xac(ea)
2ât .
Thus, after the exponential transform and then the Getzler rescaling GMât, we
find that t(DÏâµâFε (r)
)2â zâtDÏâµâF
ε (r) converges as tâ 0 to
H(r, ε)â r2Ï2 + zââ1r
mâa=p+1
c(ea)âa,
20
where
H(r, ε) = âεpâa=1
(âa +
14âšRTMp0 y, ea
â©)2
â(1+r2)mâ
a=p+1
(âa +
14âšRTMp0 y, ea
â©)2
.
On the other hand, after the exponential transform and then the Getzlerrescaling GMâ
t, t DÏâµâF
ε converges to
âz2
mâa=p+1
c(ea) ea ⧠.
It follows that
limtâ0
t32 Trs
[DÏâµâFε DÏâµâF
ε (r)eâtâDÏâµâFε (r)
â2]= â
â« B mâa=p+1
c(ea) ea⧠eâH(ε,r)+r2Ï2,
whereâ« B denotes the Berezin integral (cf. [MZ, Page 604]).
Thus, we deduce that ci(ε) = 0 for ân/2 â 2 †i < âk, with k = 32 if n is
odd. On the other hand, if n is even, the Berezin integral on the right handside vanishes for parity reason, and thus k = 1.
Now we show that the asymptotic expansion is uniform in ε. According tothe discussion above, after the conjugation by (3.4), the Gâε rescaled operatorof (DÏâµâF
s,ε (r))2 â zDÏâµâFs,ε (r) converges as εâ 0 to
H+ (1 + r2)(C24t +Rµ)â z
(DZ +
c(T )4
+ââ1r
((dZâ â dZ) +
c(T )4
)).
Similarly, the Gâε rescaled operator of DÏâµâFε converges to D4. Since the
asymptotic expansion of
Trs
[DÏâµâFε DÏâµâF
ε (r)eâtâDÏâµâFε (r)
â2]depends only on the local symbols of the rescaled operators of (DÏâµâF
s,ε (r))2 âzDÏâµâF
s,ε (r) and DÏâµâFε , the coefficients ci(ε) of its asymptotic expansion con-
verges uniformly to that of
Trs
[D4e
âtâH+(1+r2)(C2
4t+Rµ)âz(DZ+
c(T )4
+ââ1r(dZââdZ+
bc(T )4
))â].
On the other hand, since
Trs
[D4te
ââH+(1+r2)(Cµ4t)
2âzââ
tDZ+c(T )
4ât
+ââ1r
âât(dZââdZ)+
bc(T )
4ât
âââ]= tâ1/2Trs
[D4e
âtâH+(1+r2)(C2
4t+Rµ)âz(DZ+
c(T )4
+ââ1r(dZââdZ+
bc(T )4
))â],
we obtain (3.34) and also the convergence of asymptotic coefficients.
21
Corollary 3.7. The function Ύε(F, r)(s) in (3.23) has a meromorphic contin-uation to the whole complex plane with s = 0 a regular point.
Proof. The integral in (3.23) is convergent at t =â since
Trs
[DÏâµâFε DÏâµâF
ε (r)eâtâDÏâµâFε (r)
â2]is exponentially decaying in t as t â â. On the other hand, it follows im-mediately from Proposition 3.6 that the integral is convergent at t = 0 for< s > kâ1. Moreover the standard method shows that Ύε(F, r)(s) in (3.23) hasa meromorphic continuation to the whole complex plane with simple poles ats = k â 1, k, . . .. However the possible simple pole at s = 0 is canceled by thatof Î(s). Hence s = 0 is a regular point. From this discussion, we also derivethe following formula
Ύε(F )(r) = Ύε(F, r)â²(0)(3.37)
= â12
â« 1
0
(Trs
[DÏâµâFε DÏâµâF
ε (r)eâtâDÏâµâFε (r)
â2]â câk(ε) tâk
)dt
â12
â« +â
1Trs
[DÏâµâFε DÏâµâF
ε (r)eâtâDÏâµâFε (r)
â2]dt+ C,
where C = câ 32(ε) if m is odd (and hence k = 3
2) and C = 12Îâ²(1)câ1(ε) if m is
even (and thus k = â1).
We now define our torsion form. As in the discussion above, we first definethe corresponding zeta function
ζT (s) = â 1Î(s)
â« â0
tsâ1ÏTrs[NZD
2t e
(1+r2)D2t
]dt.(3.38)
From [BL, Theorem 3.21], Trs[NZ(1 + 2D2
t )e(1+r2)D2
t
]has an asymptotic ex-
pansion as tâ 0 with no singular terms (i.e. no singular powers of t). By [BZ]and [DM], Trs
[NZe
(1+r2)D2t
]has an asymptotic expansion as t â 0 starting
with the tâl term, with l = 0 if n is even and l = 12 if n is odd, compare [MZ,
(3.118)]. Hence Trs[NZD
2t e
(1+r2)D2t
]has an asymptotic expansion as t â 0
starting with the tâl term:
Trs[NZD
2t e
(1+r2)D2t
]⌠Aâl tâl +Aâl+1 t
âl+1 + · · · .
It follows that ζT (s) has a meromorphic continuation to the whole complexplane with s = 0 a regular point. Also, for later use, we note that
ζT (0) = 0,(3.39)
when n is odd; and
ζT (0)[i] = 0,(3.40)
22
for i > 0 when n is even. Now we define our torsion form by
Tr = ζ â²T (0).(3.41)
In fact, we have
Tr = ââ« 1
0Ï(
Trs[NZD
2t e
(1+r2)D2t
]âAâl tâl
) dtt
(3.42)
ââ« â
1ÏTrs
[NZD
2t e
(1+r2)D2t
] dtt
+ C â²,
where C â² = Ï (AâlÎâ²(1)) if n is even, and C â² = Ï (2Aâl) if n is odd.We also introduce a variant of the torsion form. From (3.34), we have for
tâ 0 that
Trs
[tâ
12D4t
â
âât
(C4t +
ââ1rD4t
)e(1+r2)D2
4t
]⌠Câktâk + Câk+1t
âk+1 + · · · .
(3.43)
Here k is defined as in (3.34). Define
ζeT (s) = â 1Î(s)
â« â0
tsÏTrs
[tâ
12D4t
â
âât
(C4t +
ââ1rD4t
)e(1+r2)D2
4t
]dt.
(3.44)
As before, this zeta function has analytic continuation to the whole complexplane with s = 0 a regular point. Therefore we can define
Tr = ζ â²eT (0).(3.45)
In fact, one has
Tr = ââ« 1
0Ï
(Trs
[tâ
12D4t
â
âât
(C4t +
ââ1rD4t
)e(1+r2)D2
4t
]â Câk tâk
)dt
(3.46)
ââ« â
1ÏTrs
[tâ
12D4t
â
âât
(C4t +
ââ1rD4t
)e(1+r2)D2
4t
]dt+ C â²â²,
where C â²â² = 2ÏCâ 32
if m is odd (and hence k = 32) and C â²â² = Îâ²(1)ÏCâ1 if m is
even (and thus k = 1).We are now ready for our main result.
Theorem 3.8. Under the assumption that the flat vector bundle F over M isfiberwise acyclic, the following identity holds,
lim뵉0
Ύε(F )(r) =â«BL(TB,âTB
)ch (µ,âµ) Tr.(3.47)
23
Proof. The proof follows the same line as in the proof of Theorem 2.5. UsingProposition 3.5, Proposition 3.6, (3.37) and (3.46), one deduces that
lim뵉0
Ύε(F )(r) =12
â«BL(TB,âTB
)ch (µ,âµ) Tr.
To derive the final result, we use
2uâ
âuCu = â[NZ , Du], 2u
â
âuDu = â[NZ , Cu]
(see [MZ, (3.81)]) to rearrange the right hand side of (3.25) as in (2.35). Namely,one has
âTrs
[tâ
12D4t
â
âât
(C4t +
ââ1rD4t
)e(1+r2)D2
4t
]=(3.48)
â2tTrs
[NZD
2t e
(1+r2)D2t
]+ââ1rt
dTrs[NZDt e
(1+r2)D2t
].
It follows that â2Ai+ââ1r dBi = 0 if i < â1
2 and â2Ai+ââ1r dBi = Ciâ1 if
i ⥠â12 , whereBi is the coefficient of asymptotic expansion of Trs
[NZDt e
(1+r2)D2t
].
Consequently, we obtain by using (3.42) and (3.46),â«BL(TB,âTB
)ch (µ,âµ) Tr = 2
â«BL(TB,âTB
)ch (µ,âµ) Tr.
Remark 3.9. Theorem 3.8 is closely related to [MZ, Theorems 3.17 and 3.18].Indeed, in [MZ] one sees the torsion forms through the transgression of the η-forms, while the η-forms involved come from the adiabatic limits of η-invariants.Our simple observation is that for the r-family considered in [MZ], one may alsoconsider the process of first taking the variation of η-function and then takingthe adiabatic limit thinking r as an element in the base. The transgressedform might then come out explicitly. It is this process that leads us to theBismut-Freed connection form. And thus the appearance of the torsion likeform through this process is not so surprising. Moreover it is quite reasonablethat the torsion forms appeared here are not exactly the same as those appearingin [MZ], as the process of first taking adiabatic limit and then taking variationneed not be the same as that of first taking variation and then taking adiabaticlimit.
3.5 Comparison with the Bismut-Lott torsion form
Recall that the Bismut-Lott torsion form T (THM, gTZ , hF ) is defined by
(3.49) T(THM, gTZ , hF
)= âÏ
â« +â
0
(Trs
[NZ
(1 + 2D2
u
)eD
2u
]â d(H(Z,F |Z)) â
(n2Ï(Z)rk(F )â d(H(Z,F |Z))
)(1â u
2
)eâu/4
) du2u.
24
Now we note that the second and the third terms of the integrand, termsinserted in (3.49) to make the integral convergent, are degree 0 terms. Hence,for i > 0,
T(THM, gTZ , hF
)[i]= â
â« +â
0
ÏTrs
[NZ
(1 + 2D2
u
)eD
2u
][i] du
2u,
where we denote by a superscript [i] the degree i component of the correspond-ing form.
On the other hand, sinceTrs
[NZD
2u exp
(D2u
)][i] = uâi/2
Trs[NZuD
21 exp
(uD2
1
)][i],
Trs[NZ exp
(D2u
)][i] = uâi/2
Trs[NZ exp
(uD2
1
)][i],
one deduces that, for < s > 0 sufficiently large,â« â0
us
Trs[NZD
2u exp
(D2u
)][i] du
u=â« â
0usâ
i2
Trs[NZD
21 exp
(uD2
1
)][i]du
=â« â
0usâ
i2â
âu
Trs
[NZ exp
(uD2
1
)][i]du
=â« â
0(iâ 2s)usâ
i2
Trs[NZ exp
(uD2
1
)][i] du
2u,
=â« â
0(iâ 2s)us
Trs
[NZ exp
(D2u
)][i] du
2u,
Cf. [MZ, (3.140) and (3.141)]. We have used our assumption thatHâ(Zb, F |Zb) =0.
Thus, for i > 0,
(3.50)1
Î(s)
â« +â
0usÏTrs
[NZ
(1 + 2D2
u
)eD
2u
][i] du
2u
=(
1iâ 2s
+ 1)
1Î(s)
â« +â
0usâ1
ÏTrs
[NZD
2u exp
(D2u
)][i]du
Hence,T(THM, gTZ , hF
)[i]= (1 + r2)1â i
2
(2 + ln(1 + r2))ζT (0) +
i+ 1iTr[i]
,
as
ζT (s)[i] = â(1 + r2)âs+i2â1 1
Î(s)
â« â0
usâ1ÏTrs
[NZD
2u exp
(D2u
)][i]du.
In particular, using (3.39) and (3.40), we have
Tr[i] =i
i+ 1(1 + r2)
i2â1T(THM, gTZ , hF
)[i](3.51)
For the degree 0 component, one has
Tr[0] = 0.
This is a direct consequence of [BL, Theorem 3.29]. Thus, up to a scaling factoron each degree component, Tr captures the positive degree components of theBismut-Lott real analytic torsion form.
25
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