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The Wave Kernel on Asymptotically Complex Hyperbolic Manifolds

Hadrian Quan
Abstract.

We study the behavior of the wave kernel of the Laplacian on asymptotically complex hyperbolic manifolds for finite times. We show that the wave kernel on such manifolds belongs to an appropriate class of Fourier integral operators and analyze its trace. This construction proves that the singularities of its trace are contained in the set of lengths of closed geodesics and we obtain an asymptotic expansion for the trace at time zero.

1. Introduction

There is a long-standing research program investigating the spectral and scattering theory of real asymptotically hyperbolic manifolds, see e.g. [An10, AlMa10, AlBaNa20, ChDeLeSk05, FeGr85, GrWi99, GrZw01, JoSá00, Va17] and references contained therein, for a small sample of the surrounding work. However there is comparatively much less work concerning the analogous setting of asymptotically complex hyperbolic manifolds. These spaces were first introduced by Epstein, Mendoza, and Melrose [EpMeMe91], and more recently have been investigated extensively by [GuSa06, FeHi03, GuSa06, HMM17, PeHiTa08, Ma16, Ma18]. This class of manifolds includes certain quotients of complex hyperbolic space by discrete groups, as well as strictly pseudoconvex domains in Stein manifolds equipped with Kähler metrics of Bergman type.

In this work we extend major results which study the wave kernel of asymptotically real hyperbolic manifolds to this complex setting. Joshi-Sá Barreto [JoSá01] study the wave kernel by exhibiting this operator as an element of a certain algebra of Fourier integral operators which have been adapted to the geometry at infinity of this class of real asymptotically hyperbolic manifolds. In the case of both works, moving from the real to the complex case presents new difficulties to the analysis. On the other hand, the original methods of both Vasy and Joshi-Sá Barreto are robust enough to permit an analysis of this class of manifolds of hyperbolic-type.

Before introducing the structure of complex hyperbolic manifolds we briefly recall the geometry of real asymptotically hyperbolic manifolds. A non-compact Riemannian manifold (M,g)(M,g) of real dimension (n+1)(n+1) is called asymptotically hyperbolic if it compactifies to a 𝒞{\mathcal{C}}^{\infty} manifold M¯\overline{M} with compact boundary M¯\partial\overline{M}, equipped with a boundary defining function ρ\rho, and such that ρ2g\rho^{2}g is a 𝒞{\mathcal{C}}^{\infty} metric which is non-degenerate up to the boundary, and moreover that |dρ|ρ2g21|d\rho|_{\rho^{2}g}^{2}\equiv 1 at M¯\partial\overline{M}. This name is due to the fact that the final hypothesis ensures that along any smooth curve in M¯M¯\overline{M}\setminus\partial\overline{M} approaching a point in M¯\partial\overline{M}, all sectional curvatures of gg approach 1-1, see e.g. [MaMe87].

As proven in [JoSá00], these geometric hypotheses are equivalent to the existence of a product-type decomposition at infinity M[0,ε)ρ×MM\sim[0,\varepsilon)_{\rho}\times\partial M, such that

g=dρ2+g0(ρ)ρ2,g=\frac{d\rho^{2}+g_{0}(\rho)}{\rho^{2}},

where g0(ρ)g_{0}(\rho) is a 𝒞{\mathcal{C}}^{\infty} 1-parameter family of 𝒞{\mathcal{C}}^{\infty} metrics on M¯\partial\overline{M}. In this model, the boundary M¯\partial\overline{M} represents the geometric infinity of M¯\overline{M}, analogous to the role played by the 𝕊n\mathbb{S}^{n} at infinity in n+1\mathbb{H}_{\mathbb{R}}^{n+1}. In particular the metric ρ2g|M\rho^{2}g|_{\partial M} fixes a conformal representative of a metric on M¯\partial\overline{M}.

The spectrum of the Laplacian of such manifolds was first studied by [MaMe87]; they determined that it is comprised of finitely many L2L^{2}-eigenvalues σpp(Δg)(0,(n+1)24)\sigma_{\text{pp}}(\Delta_{g})\subset(0,\tfrac{(n+1)^{2}}{4}) and the absolutely continuous spectrum σac(Δg)=[(n+1)24,)\sigma_{\text{ac}}(\Delta_{g})=[\tfrac{(n+1)^{2}}{4},\infty). In particular, they prove that the resolvent

R(ζ)=(Δgζ(n+1ζ))1,R(\zeta)=(\Delta_{g}-\zeta(n+1-\zeta))^{-1},

is well-defined as a bounded operator on Lg2(X)L_{g}^{2}(X) whenever Re(ζ)>n+12\operatorname{Re}(\zeta)>\tfrac{n+1}{2}. Further they prove that R(ζ)R(\zeta) has a meromorphic extension to 12((n+1)0)\mathbb{C}\setminus\tfrac{1}{2}((n+1)-\mathbb{N}_{0}), as an operator R(ζ):𝒞0(X)𝒞(X)R(\zeta):{\mathcal{C}}^{\infty}_{0}(X)\to{\mathcal{C}}^{\infty}(X), and with only finite order poles (this extension is meromorphic on the whole complex plane assuming the metric is even in the sense of [Gu05]).

We now move to introducing the complex analogue of these spaces, and introduce our results. We say a non-compact Riemannian manifold (X,g)(X,g), of complex dimension (n+1)(n+1), is an asymptotically complex hyperbolic manifold (hereafter ACH manifold) if the following holds. We assume XX compactifies to a 𝒞{\mathcal{C}}^{\infty} manifold X¯\overline{X}, compact with boundary, equipped with a choice of boundary defining function rr (hereafter, a bdf). This is a smooth nonnegative function on X¯\overline{X} which such that

X¯={r=0},dr|X¯0.\overline{X}=\{r=0\},\quad dr|_{\partial\overline{X}}\neq 0.

We further assume the boundary admits: (1) a contact form θΩ1(X¯)\theta\in\Omega^{1}(\partial\overline{X}) defined as satisfying θ(dθ)n0\theta\wedge(d\theta)^{n}\neq 0; (2) an almost complex structure J:KerθKerθJ:\operatorname{Ker}\theta\to\operatorname{Ker}\theta; such that dθ(,J)d\theta(\cdot,J\cdot) is a symmetric, positive-definite bilinear form on Kerθ\operatorname{Ker}\theta. Then we say (X,g)(X,g) is an ACH manifold if there is a tubular neighborhood Φ:UX¯×[0,ε)r\Phi:U\to\partial\overline{X}\times[0,\varepsilon)_{r} of the boundary X¯\partial\overline{X} such that

gΦgθ as r0,gθ=(4dr2r2+dθ(,J)r2+θ2r4)=4dr2+g0(r)r2.g\sim\Phi^{*}g_{\theta}\;\text{ as $r\to 0$},\hskip 17.07164ptg_{\theta}=\left(\frac{4dr^{2}}{r^{2}}+\frac{d\theta(\cdot,J\cdot)}{r^{2}}+\frac{\theta^{2}}{r^{4}}\right)=\frac{4dr^{2}+g_{0}(r)}{r^{2}}. (1.1)

In particular, for another choice of boundary defining function, r~\widetilde{r}, we observe that r4g|X¯=e4fθr^{4}g|_{\partial\overline{X}}=e^{4f}\theta, for some f𝒞(X¯)f\in{\mathcal{C}}^{\infty}(\overline{X}). Denoting the conformal class of our contact structure by [θ][\theta] we can consider the boundary as being endowed with the structure of a conformal pseudohermitian manifold (X¯,[θ],J)(\partial\overline{X},[\theta],J). This is analogous to the natural conformal structure on (M¯,[ρ2g])(\partial\overline{M},[\rho^{2}g]) in the real hyperbolic case.

Before continuing, we require an additional hypothesis, which is that gg is an even metric; i.e., the dual metric g1g^{-1} defined on TX¯T^{*}\overline{X} has only even powers of rr in a Taylor expansion at r=0r=0. This is automatic in the case of n+1\mathbb{H}_{\mathbb{C}}^{n+1}, and necessary for the existence of a meromorphic continuation of the resolvent of Δg\Delta_{g} to all of \mathbb{C}, (in fact, the failure of this hypothesis implies the existence of at least one essential singularity in the continuation of the resolvent, see [Gu05], [GuSa06]).

In the case that the metric of (X,g)(X,g) is even in the above sense, we can replace the smooth structure on this manifold with its even smooth structure, denoted XevenX_{\operatorname{even}}. In this case the smooth structure on XX has been modified by declaring that only functions which are even in rr are smooth with respect to XevenX_{\operatorname{even}}. This change of the smooth structure permits us to define a square root of our original defining function, and guarantee that it is an element of 𝒞(Xeven){\mathcal{C}}^{\infty}(X_{\operatorname{even}}). Equivalently, the even smooth structure can be defined by declaring XevenX_{\operatorname{even}} is a smooth manifold with boundary, with bdf r2r^{2}. Throughout we shall denote the square root of our bdf ρ=r2\rho=r^{2}.

Now we state our main results on the behavior of solutions to the wave equation for small times. This question can be approached by a study of the fundamental solution to the wave equation, as in the work of Joshi-Sá Barreto [JoSá01] who studied the wave operator
cos(tΔg(n+1)2/4)\cos\big{(}t\sqrt{\Delta_{g}-(n+1)^{2}/4}\big{)} in the setting of real asymptotically hyperbolic manifolds. This operator has Schwartz kernel U(t,p,p)U(t,p,p^{\prime}) satisfying

{(t2+Δg(n+1)24)U(t,p,p)=0U(0,p,p)=δ(p,p),tU(0,p,p)=0,\begin{cases}\left(\partial_{t}^{2}+\Delta_{g}-\tfrac{(n+1)^{2}}{4}\right)U(t,p,p^{\prime})=0\\ U(0,p,p^{\prime})=\delta(p,p^{\prime}),\quad\partial_{t}U(0,p,p^{\prime})=0\end{cases},

and they prove that cos(tΔg(n+1)2/4)\cos\big{(}t\sqrt{\Delta_{g}-(n+1)^{2}/4}\big{)} resides in an algebra of Fourier integral operators. Having shown this, they use the results of [DuGu75, Hö68, Hör71] to study its (regularized) trace.

This construction of the wave group U(t,p,p)U(t,p,p^{\prime}) as a Fourier integral operator was motivated by the analysis of the resolvent of a real asymptotically hyperbolic manifold initiated in [MaMe87]. Mazzeo-Melrose obtained their results by exhibiting the resolvent as an element of the “large” calculus of zero pseudodifferential operators Ψ0(M)\Psi_{0}^{*}(M); i.e., those pseudodifferential operators with Schwartz kernels constructed as distributions on the blown-up space M¯×0M¯\overline{M}\times_{0}\overline{M}, obtained by blowing up the intersection of the the corner M¯×M¯\partial\overline{M}\times\partial\overline{M} with the diagonal M¯diagM¯×M¯\overline{M}_{\operatorname{diag}}\hookrightarrow\overline{M}\times\overline{M} in M¯×M¯\overline{M}\times\overline{M}. The new boundary hypersurface resulting from this blow-up is called the front face. (For an extended treatment on such blow-ups see [MaMe87, §3], [Mel96], and [Gr01])

Along such lines [JoSá01] construct a class of zero Fourier integral operators as those operators whose Schwartz kernels, when lifted to M¯×0M¯\overline{M}\times_{0}\overline{M}, have support away from the left and right boundary faces (i.e. the lifts of M¯×M¯\partial\overline{M}\times\overline{M} and M¯×M¯\overline{M}\times\partial\overline{M} respectively). This greatly simplifies the construction of this class of operators, as typically the corners formed by the intersections of the left face (resp. right) with the front face would need to be incorporated into the definition of the operators; requiring the support of the Schwartz kernels avoid such corners allows their contributions to be neglected. In particular, due to the finite speed of propagation for the wave equation, a distribution which is initially supported only on the front face (such as U(t,p,p)U(t,p,p^{\prime})) will remain supported in the interior of the front face for all finite time. Thus [JoSá01] can construct a small time parametrix for the wave group while remaining entirely in this restricted calculus of zero Fourier integral operators.

Following this strategy we begin with the notion of the Θ\Theta-stretched product, X¯×ΘX¯\overline{X}\times_{\Theta}\overline{X}, which is the analogous blow-up of the double space X¯×X¯\overline{X}\times\overline{X} defining the class of Θ\Theta-pseudodifferential operators ΨΘ(X)\Psi_{\Theta}^{*}(X) used in the study of the resolvent initiated by [EpMeMe91]. With the appropriate definition of Θ\Theta-Fourier integral operators, we can quickly conclude:

Theorem 1.1.


Let GG be the length functional on TXT^{*}X, (i.e. the dual metric). For each tt\in\mathbb{R}, the graph of the time-tt flow-out of the diagonal in TX×TXT^{*}X\times T^{*}X by the Hamilton vector field HGH_{G} is a canonical relation, denoted CC. Furthermore, the wave group U(t)U(t) is a Θ\Theta-FIO with respect to this canonical relation.

Once we know the wave group is a Θ\Theta-Fourier integral operator, it is straightforward to use the results of [DuGu75, Hör71] to analyze the trace of U(t,p,p)U(t,p,p^{\prime}). One subtlety is that the trace needs to replaced with a regularized trace, defined using a Hadamard regularization procedure using our choice of bdf ρ\rho. Defining the cut-off wave trace,

Tε(t)={ρ>ε}U(t,p,p)T_{\varepsilon}(t)=\int_{\{\rho>\varepsilon\}}U(t,p,p)

we obtain

Proposition 1.2.

There exists ε0>0\varepsilon_{0}>0 such that for all ε<ε0\varepsilon<\varepsilon_{0}, the singular support of TεT_{\varepsilon} is contained in the set of periods of closed geodesics of XX.

With this result in hand, after choosing a smooth cutoff χ(t)𝒞0()\chi(t)\in{\mathcal{C}}^{\infty}_{0}(\mathbb{R}) supported away from the lengths of all non-zero periods of closed geodesics, and using the results of [Hö68] we obtain a Duistermaat-Guillemin type result for the cutoff wave trace.

Theorem 1.3.

There exists {ωk}k0\{\omega_{k}\}_{k\in\mathbb{N}_{0}}\subset\mathbb{R} such that the renormalized trace TrRU(t){}^{R}\operatorname{Tr}U(t) satisfies,

TrRU(t)χ(t)etμ𝑑t1(2π)2n+2k=0ωkμ2n+22k,\int_{\mathbb{R}}{}^{R}\operatorname{Tr}U(t)\chi(t)e^{t\mu}dt\sim\frac{1}{(2\pi)^{2n+2}}\sum_{k=0}^{\infty}\omega_{k}\mu^{2n+2-2k},

as μ0\mu\to 0 and is rapidly decaying as μ\mu\to-\infty. The leading term, ω0=VolgR(X)\omega_{0}={}^{R}\operatorname{Vol}_{g}(X), is called the renormalized volume, and can be computed as

VolgR(X)=limε0[{ρ>ε}dVolgj=2n21djεjd0log(1/ε)],{}^{R}\operatorname{Vol}_{g}(X)=\lim_{\varepsilon\to 0}\left[\int_{\{\rho>\varepsilon\}}d\operatorname{Vol}_{g}-\sum_{j=-2n-2}^{-1}d_{j}\varepsilon^{j}-d_{0}\log(1/\varepsilon)\right], (1.2)

where djd_{j} are the unique real numbers such that this limit exists.

Finally, we remark on the appearance of the renormalized volume in Theorem (1.3). In the real hyperbolic setting it is known that the renormalized volume is, in certain dimensions, independent on the choice of representative of the conformal infinity. Namely, for (Mn+1,g)(M^{n+1},g) a real asymptotically hyperbolic manifold, one can similarly define the renormalized volume as the finite part of the in the expansion of Volg({xε})\operatorname{Vol}_{g}(\{x\geq\varepsilon\}) as ε0\varepsilon\to 0, given a choice of bdf xx. For nn odd, the real hyperbolic renormalized volume is independent of h0h_{0}, the choice of conformal representative. On the other hand, for nn even, we suddenly have the dependence of the renormalized volume on this choice of representative of [h][h]. This is result is the so-called holographic anomaly (see [HeSk98]) and motivates much of the interest of asymptotically hyperbolic manifolds in mathematical physics, for their connection with the anti deSitter/conformal field theory (AdS/CFT) correspondence.

More concretely, the volume expansion of (Mn+1,g)(M^{n+1},g) of an Einstein asymptotically hyperbolic metric, for nn even, is given by

Volg({xε})=Vnεn+Vn+2εn+2++V2ε2+V0log(1/ε)+VolgR(M)+o(1),\operatorname{Vol}_{g}(\{x\geq\varepsilon\})=V_{-n}\varepsilon^{-n}+V_{-n+2}\varepsilon^{-n+2}+\ldots+V_{-2}\varepsilon^{-2}+V_{0}\log(1/\varepsilon)+{}^{R}\operatorname{Vol}_{g}(M)+o(1),

and [GrZw01] first made the connection of V0V_{0} to Branson’s QQ-curvature [Br95],

V0=2cn/2MQ,V_{0}=2c_{n/2}\int_{\partial M}Q,

for cn/2c_{n/2} a dimensional constant. In the ACH setting, the renormalized volume was first studied at this level of generality by Matsumoto in [Ma16]. Our construction of the renormalized wave trace thus provides an alternate proof of Matsumoto’s result, via formula (1.2). For a general ACH metric, [Ma16] generalizes this result for an analogue of Bransons QQ-curvature. From his result we obtain as a corollary that the constant d0d_{0} in our Theorem 1.3, is given by,

d0=2(1)n+1n!2(n+1)!XQθgθ(dθ)n.d_{0}=\frac{2(-1)^{n+1}}{n!^{2}(n+1)!}\int_{\partial X}Q_{\theta}^{g}\theta\wedge(d\theta)^{n}.

This quantity is a global CR invariant of the boundary, thus leading to a pseudoconformal analogue of the holographic anomaly. Given these results there is strong connection between the renormalized volume of an ACH manifold and its spectrum. On the mathematical physics side there seems to be relatively scarce work on this complex analogue of the AdS/CFT correspondence.


Funding This work was supported by the National Science Foundation grant numbers DGE-1746047, DMS-1440140, and DMS-1711325, growing out of conversations while the author was in residence at the Mathematical Sciences Research Institute in Berkeley, California during the Fall 2019 semester.


Acknowledgements. The author is very grateful to acknowledge the kind discussions and suggestions of Andras Vasy, Antônio Sá Barreto, and Pierre Albin.

2. The geometry of asymptotically complex hyperbolic manifolds

Because the construction of our adapted FIO-calculus entails a finer understanding of the geometry of an asymptotically complex hyperbolic manifold, we briefly recall the geometry of the Bergman-type metric our manifold is endowed with.

Let (X,X)(X,\partial X) be a non-compact manifold with closed boundary. We assume the boundary admits a contact form θ\theta and an almost complex structure J:Ker(θ)Ker(θ)J:\operatorname{Ker}(\theta)\to\operatorname{Ker}(\theta) (i.e., an endomorphism satisfying JJ=IdKer(θ)J\circ J=-\text{Id}_{\operatorname{Ker}(\theta)}) such that dθ(,J)d\theta(\cdot,J\cdot) is symmetric positive definite on Ker(θ)\operatorname{Ker}(\theta). We consider a metric gACHg_{ACH} of the following form: there is a boundary defining function ρ\rho,

X={ρ=0},dρ|X0\partial X=\{\rho=0\},\quad d\rho\rvert_{\partial X}\neq 0

such that in a collar neighborhood φ:[0,1)ρ×Xω,zU\varphi:[0,1)_{\rho}\times\partial X_{\omega,z}\to U it takes the form

φgACH=dρ2ρ2+dθ(,J)ρ2+θθρ4+ρQρ=dρ2+h(ρ,ω,z,dω,dz)ρ2,\varphi^{*}g_{ACH}=\frac{d\rho^{2}}{\rho^{2}}+\frac{d\theta(\cdot,J\cdot)}{\rho^{2}}+\frac{\theta\otimes\theta}{\rho^{4}}+\rho Q_{\rho}=\frac{d\rho^{2}+h(\rho,\omega,z,d\omega,dz)}{\rho^{2}}, (2.1)

where (𝒟ρ)Qρ(\mathcal{D}_{\rho}^{\mathbb{H}})^{*}Q_{\rho} is a smooth section of S2(TX)Ker(ιρ)S^{2}(T^{*}X)\cap\operatorname{Ker}(\iota_{\partial_{\rho}}). Here, 𝒟ρ\mathcal{D}_{\rho}^{\mathbb{H}} denotes the anisotropic dilation map

TqX=q𝒱q(vH,vV)𝒟ρ(ρvH,ρ2vV)q𝒱q=TqX,T_{q}\partial X=\mathscr{H}_{q}\oplus\mathscr{V}_{q}\ni(v_{H},v_{V})\xmapsto{\phantom{x}\mathcal{D}_{\rho}^{\mathbb{H}}\phantom{x}}(\rho v_{H},\rho^{2}v_{V})\in\mathscr{H}_{q}\oplus\mathscr{V}_{q}=T_{q}\partial X,

with splitting induced by the choice of contact structure (X,θ)(\partial X,\theta), (i.e., =Kerθ\mathscr{H}=\operatorname{Ker}\theta).

We observe that for any other choice of defining function ρ~\widetilde{\rho} we have

ρ~4g|X=e4ω0θθ, for some ω0𝒞(X),\widetilde{\rho}^{4}g\rvert_{\partial X}=e^{4\omega_{0}}\theta\otimes\theta,\text{ for some }\omega_{0}\in{\mathcal{C}}^{\infty}(X),

thus it is more natural to associate to gACHg_{ACH} a conformal class of 1-forms [Θ][\Theta]. The boundary manifold equipped with the data of (X,θ,J)(\partial X,\theta,J) is a closed pseudohermitian manifold. The corresponding conformal pseudohermitian structure ([Θ],J)([\Theta],J) was called a Θ\Theta-structure in [EpMeMe91].

This Riemannian metric structure describes a non-compact incomplete manifold whose metric is asymptotic to complex hyperbolic space n+1\mathbb{H}_{\mathbb{C}}^{n+1}. A useful model of complex hyperbolic space n+1\mathbb{H}_{\mathbb{C}}^{n+1} is given by

n+1={ζn+1:Q(ζ,ζ)>0},whereQ(ζ,ζ)=i2(ζ1ζ1)12j>1ζjζj¯\mathbb{H}_{\mathbb{C}}^{n+1}=\{\zeta\in\mathbb{C}^{n+1}:Q(\zeta,\zeta)>0\},\quad\text{where}\quad Q(\zeta,\zeta^{\prime})=-\tfrac{i}{2}(\zeta_{1}-\zeta_{1}^{\prime})-\tfrac{1}{2}\sum_{j>1}\zeta_{j}\overline{\zeta_{j}}^{\prime}

with boundary sphere equal to a compactification of the (2n+1)(2n+1)-dimensional Heisenberg group,

Hn:={ζn+1:Q(ζ,ζ)=0}={(ζ1,w)n+1:12|w|2=Im(ζ1)}n×.H_{n}:=\{\zeta\in\mathbb{C}^{n+1}:Q(\zeta,\zeta)=0\}=\{(\zeta_{1},w)\in\mathbb{C}^{n+1}:\tfrac{1}{2}|w|^{2}=\operatorname{Im}(\zeta_{1})\}\simeq\mathbb{C}^{n}\times\mathbb{R}.

This model of complex hyperbolic space realizes n+1+×Hn\mathbb{H}_{\mathbb{C}}^{n+1}\simeq\mathbb{R}^{+}\times H_{n} with the coordinates

ρ(ζ)=Q(ζ,ζ)1/2,wn,z=Re(ζ1),\rho(\zeta)=Q(\zeta,\zeta)^{1/2},\;\;w\in\mathbb{C}^{n},\;\;z=\operatorname{Re}(\zeta_{1}),

foliating n+1\mathbb{H}_{\mathbb{C}}^{n+1} by a family of HnH_{n}-hypersurfaces. Writing w=x+iyw=x+iy, in these coordinates we can also write the contact form at the boundary as

θ0=dz+j=1nyjdxjxjdyj,\theta_{0}=dz+\sum_{j=1}^{n}y_{j}dx^{j}-x_{j}dy^{j},

and the metric on complex hyperbolic is the Bergman metric,

gBerg=4dρ2+2|dw|2ρ2+θ02ρ4.g_{\text{Berg}}=\frac{4d\rho^{2}+2|dw|^{2}}{\rho^{2}}+\frac{\theta_{0}^{2}}{\rho^{4}}.

The Heisenberg group is a Lie group of dimension 2n+12n+1. In these coordinates the group law is given by

(x,y,z)H(x,y,z)=(x+x,y+y,z+z+Im[(x,y)(x,y¯)]),(x,y,z)\cdot_{H}(x^{\prime},y^{\prime},z^{\prime})=(x+x^{\prime},y+y^{\prime},z+z^{\prime}+\operatorname{Im}[(x,y)\cdot(\overline{x^{\prime},y^{\prime}})]),

which is abelian in the first 2n2n components. Its Lie algebra 𝔥\mathfrak{h} has a basis {Xj,Yj,Z}\{X_{j},Y_{j},Z\}, which satisfies the non-trivial bracket relations: [Xj,Yj]=Z[X_{j},Y_{j}]=Z for all j=1,,nj=1,\ldots,n and all brackets vanishing. This structure of a nilpotent Lie algebra gives an identification Hn𝔥H_{n}\to\mathfrak{h} of the form

n×((x,y),z)j=1nxjXj+yjYj+zZT{e}Hn,\mathbb{C}^{n}\times\mathbb{R}\;\ni\;((x,y),z)\mapsto\sum_{j=1}^{n}x_{j}X_{j}+y_{j}Y_{j}+zZ\;\in\;T_{\{e\}}H_{n},

after which the group law can be written via Lie algebra elements W,W𝔥W,W^{\prime}\in\mathfrak{h} as,

WHW=πKerθ0(W+W)+(θ0(W+W)dθ0(W,W))Z.W\cdot_{H}W^{\prime}=\pi_{\operatorname{Ker}\theta_{0}}(W+W^{\prime})+(\theta_{0}(W+W^{\prime})-d\theta_{0}(W,W^{\prime}))Z.

It is a consequence the nilpotence of HnH_{n} that the group law is a finite order polynomial in the Lie algebra elements, rather than the asymptotic series given by the Baker-Campbell-Hausdorff formula, (see e.g. [Ei68]).

Finally, we explain how the complexified hyperbolic space arises as a semi-direct product: there is parabolic dilation on HnH_{n} (consistent with the bracket relations of the Lie algebra 𝔥\mathfrak{h}) given by 𝒟δ(x,y,z)=(δx,δy,δ2z)\mathcal{D}_{\delta}(x,y,z)=(\delta x,\delta y,\delta^{2}z). The group law on the semidirect product n+1+𝒟δHn\mathbb{H}_{\mathbb{C}}^{n+1}\simeq\mathbb{R}^{+}\rtimes_{\mathcal{D}_{\delta}}H_{n} is given as

(ρ,W)(ρ,W)=(ρρ,WH𝒟ρ(W)).(\rho,W)\cdot_{\mathbb{H}_{\mathbb{C}}}(\rho^{\prime},W^{\prime})=(\rho\rho^{\prime},W\cdot_{H}\mathcal{D}_{\rho}(W^{\prime})). (2.2)

The geometric picture described above of complex hyperbolic space being foliated by a family of Heisenberg groups as level-set hypersurfaces of ρ\rho is compatible with this group law: an open set in {ρ=c}Hn\{\rho=c\}\simeq H_{n} is related to the corresponding set in {ρ=c+ε}\{\rho=c+\varepsilon\} by pullback along MεM_{\varepsilon}.

Our reason for expressing the Lie group law of m+1\mathbb{H}_{\mathbb{C}}^{m+1} at the level of its Lie algebra is that the Lie algebra arises more naturally at the level of tangent spaces in our later analysis.

3. The wave kernel on asymptotically complex hyperbolic manifolds

In this section we begin the construction of a Fourier Integral Operator Calculus, which is adapted to the asymptotic geometry of the metric (2.1). Such a calculus will be comprised of operators whose Schwartz kernels have prescribed asymptotics on a manifold with corners, the Θ\Theta-stretched product X×ΘXX\times_{\Theta}X of [EpMeMe91].

Analogously to the 0-blow up, Epstein-Mendoza-Melrose defined the Θ\Theta-blow up of an ACH manifold; this will be very similar to the zero-blow up of an AH manifold. The biggest distinction being the blow-up at the front face is non-isotropic, reflecting the different asymptotics in ρ\rho of boundary vector fields (namely those vector fields whose gACHg_{ACH}-duals span dθ(,J)d\theta(\cdot,J\cdot) vs θθ\theta\otimes\theta).

Following [EpMeMe91], we next explain how we will modify the product X×XX\times X to construct our algebra of Fourier integral operators. We begin with the notion of the Θ\Theta-vector fields 𝒱Θ\mathcal{V}_{\Theta}:

V𝒱ΘVρ𝒞(X;TX),θ~(V)ρ2𝒞(X;TX),V\in\mathcal{V}_{\Theta}\iff V\in\rho\cdot{\mathcal{C}}^{\infty}(X;TX),\quad\widetilde{\theta}(V)\in\rho^{2}\cdot{\mathcal{C}}^{\infty}(X;TX),

where θ~𝒞(X;TX)\widetilde{\theta}\in{\mathcal{C}}^{\infty}(X;TX) is any smooth extension of θ\theta to all of XX. It is shown in [EpMeMe91, §1] that this definition is dependent only on the choice of conformal class of [θ][\theta]. This is partly because a representative of [θ][\theta] determines a local frame by requiring

{X1,,Xn,Y1,,Yn} is an orthonormal frame of dθ(,J),θ(Z)=1,θ(ρ)=0,\{X_{1},\ldots,X_{n},Y_{1},\ldots,Y_{n}\}\text{ is an orthonormal frame of }d\theta(\cdot,J\cdot),\hskip 11.38109pt\theta(Z)=1,\;\;\theta(\partial_{\rho})=0, (3.1)

in which we can express

𝒱Θ=span𝒞{ρρ,ρX1,,ρXn,ρY1,,ρYn,ρ2Z},\mathcal{V}_{\Theta}=\text{span}_{{\mathcal{C}}^{\infty}}\{\rho\partial_{\rho},\rho X_{1},\ldots,\rho X_{n},\rho Y_{1},\ldots,\rho Y_{n},\rho^{2}Z\},

and a different choice of bdf ρ\rho^{\prime} produces a frame as in (3.1) associated to a contact form θ\theta^{\prime} conformal to θ\theta.

Given this 𝒞(X){\mathcal{C}}^{\infty}(X)-module, we can define the Θ\Theta-tangent bundle TΘX{}^{\Theta}TX. This is a vector bundle over XX, with a bundle map ιΘ:TΘXTX\iota_{\Theta}:{}^{\Theta}TX\to TX, which is an isomorphism over XXX\setminus\partial X such that

𝒞(X;TΘX)=ιΘ(𝒱Θ).{\mathcal{C}}^{\infty}(X;{}^{\Theta}TX)=\iota_{\Theta}^{*}(\mathcal{V}_{\Theta}).

Next, we construct the Θ\Theta-stretched product of [EpMeMe91, §8]. Notice first that in the product X×XX\times X, the boundary of the diagonal XdiagX\partial X_{\operatorname{diag}}\simeq\partial X is an embedded submanifold,

XdiagX×XX×X\partial X_{\operatorname{diag}}\hookrightarrow\partial X\times\partial X\hookrightarrow X\times X

and is a clean submanifold in the sense of [DuGu75], since it is an embedded submanifold of the corner, and thus all differentials of bdfs vanish at Xdiag\partial X_{\operatorname{diag}}. The 1-form θ\theta on XX defines a line subbundle

NX×X(Xdiag)\mathscr{H}^{*}\subset N_{X\times X}^{*}(\partial X_{\operatorname{diag}})

spanned by

πLθπRθ,\pi_{L}^{*}\theta-\pi_{R}^{*}\theta,

with π():X×XX\pi_{(\cdot)}:X\times X\to X denoting the projection onto the left and right factors respectively.

Refer to caption
Figure 1. The blow-down map β\beta of the Θ\Theta-stretched product space X×ΘXX\times_{\Theta}X

With this trivialization of the conormal bundle, we define the Θ\Theta-blow up of the corner as the \mathscr{H}^{*}-parabolic blow-up (defined using the dilation structure on fibers given in (2.2)) of the boundary diagonal:

X×ΘX=[X×X;Xdiag,]:=(X×XXdiag)𝕊N,+(Xdiag)𝕊N,+(Xdiag)=(NX×XXdiag)/𝒟+\begin{gathered}X\times_{\Theta}X=[X\times X;\partial X_{\operatorname{diag}},\mathscr{H}^{*}]:=(X\times X\setminus\partial X_{\operatorname{diag}})\sqcup\mathbb{S}N_{\mathscr{H},+}(\partial X_{\operatorname{diag}})\\ \mathbb{S}N_{\mathscr{H},+}(\partial X_{\operatorname{diag}})=(N_{X\times X}\partial X_{\operatorname{diag}})/\mathbb{R}^{+}_{\sim_{\mathcal{D}^{\mathscr{H}}}}\end{gathered}

where the equivalence on fibers 𝒟\mathcal{D}^{\mathscr{H}} is defined using the decomposition N(Xdiag)+=,N(\partial X_{\operatorname{diag}})_{+}=\mathscr{H}\oplus\mathscr{H}^{\perp}, with =Ann()\mathscr{H}=\text{Ann}(\mathscr{H}^{*}),

(W,Z)𝒟δ(W,Z)δ>0,(W,Z)=(δW,δ2Z).(W,Z)\sim_{\mathcal{D}_{\delta}^{\mathscr{H}}}(W^{\prime},Z^{\prime})\iff\exists\delta>0,\;(W,Z)=(\delta W^{\prime},\delta^{2}Z^{\prime}).

This real unoriented blow-up replaces the submanifold Xdiag\partial X_{\operatorname{diag}} with its inward-pointing parabolic-sphere bundle. This blow-up procedure furnishes a blow-down map

β:X×ΘXX×X,\beta:X\times_{\Theta}X\to X\times X,

which is the identity on X×XXdiagX\times X\setminus\partial X_{\operatorname{diag}}, and given by the bundle projection map of the parabolic-sphere bundle on 𝕊N,+(Xdiag)\mathbb{S}N_{\mathscr{H},+}(\partial X_{\operatorname{diag}}). This is a manifold with corners, and has three new boundary faces:

𝔅F=β1(Xdiag)=𝕊N,+(Xdiag)𝔅L=β1{(X×X)Xdiag}¯,𝔅R=β1{(X×X)Xdiag}¯.\begin{gathered}\mathfrak{B}_{F}=\beta^{-1}(\partial X_{\operatorname{diag}})=\mathbb{S}N_{\mathscr{H},+}(\partial X_{\operatorname{diag}})\\ \mathfrak{B}_{L}=\overline{\beta^{-1}\{(X\times\partial X)\setminus\partial X_{\operatorname{diag}}\}},\quad\quad\mathfrak{B}_{R}=\overline{\beta^{-1}\{(\partial X\times X)\setminus\partial X_{\operatorname{diag}}\}}.\end{gathered}

By construction, the front face 𝔅F\mathfrak{B}_{F} is a fiber bundle over Xdiag\partial X_{\operatorname{diag}} with fiber a projective quotient of the inward pointing normal bundle NX×X(Xdiag)+N_{X\times X}(\partial X_{\operatorname{diag}})_{+}; the front face has fiber over pXp\in\partial X given by

𝔅F|p=[NX×X(Xdiag)+\displaystyle\mathfrak{B}_{F}|_{p}=[N_{X\times X}(\partial X_{\operatorname{diag}})_{+} Xdiag]/𝒟δ.\displaystyle\setminus\partial X_{\operatorname{diag}}]/\sim_{\mathcal{D}_{\delta}^{\mathscr{H}}}.

For more details and the proof of diffeomorphism invariance of this construction see [EpMeMe91, §5-7].

3.1. The Θ\Theta-symplectic structure on TΘX{}^{\Theta}T^{*}X

Similarly as in the [JoSá01], associated to the Lie algebra 𝒱Θ\mathcal{V}_{\Theta} we can define the notion of a Θ\Theta-Fourier integral operator, which will be operators whose Schwartz kernels have prescribed asymptotics on a resolution of the product X×XX\times X, the Θ\Theta-stretched product X×ΘXX\times_{\Theta}X. A standard Fourier integral operator is characterized by its Schwartz kernel having singular support conormal to a Lagrangian inside (TXo)×(TXo)(T^{*}X\setminus o)\times(T^{*}X\setminus o); to generalize this notion we must first understand how Lagrangians arise in the symplectic structure of TΘX{}^{\Theta}T^{*}X.

In a neighborhood of the boundary UU, if we use coordinates (x,ζ)=((ρ,w,z);(ξ,ηH,ηV))TΘX(x,\zeta)=((\rho,w,z);(\xi,\eta_{H},\eta_{V}))\in{}^{\Theta}T^{*}X, where X={ρ=0}\partial X=\{\rho=0\}, then

θ|U{ρ=0}=dz12j=1nwxjdwyjwyjdwxj\theta|_{U\cap\{\rho=0\}}=dz-\tfrac{1}{2}\sum_{j=1}^{n}w_{x_{j}}dw_{y_{j}}-w_{y_{j}}dw_{x_{j}}

the induced map on the dual bundles is given by

ι¯Θ:TXTΘX,((ρ,w,z);(ξ,ηH,ηV))((ρ,w,z);(ρξ,ρηH,ρ2ηV))=:((ρ,w,z);(μ,u,t)).\overline{\iota}_{\Theta}:T^{*}X\to{}^{\Theta}T^{*}X,\;\;((\rho,w,z);(\xi,\eta_{H},\eta_{V}))\mapsto((\rho,w,z);(\rho\xi,\rho\eta_{H},\rho^{2}\eta_{V}))=:((\rho,w,z);(\mu,u,t)). (3.2)

In these coordinates the canonical 1-form

α=ξdρ+ηHdw+ηVdz\alpha=\xi d\rho+\eta_{H}\cdot dw+\eta_{V}dz

pulls back to the 1-form

ι¯Θα=αΘ=μρdρ+uρdw+tρ2dz,\overline{\iota}_{\Theta}\alpha={}^{\Theta}\alpha=\frac{\mu}{\rho}d\rho+\frac{u}{\rho}dw+\frac{t}{\rho^{2}}dz,

and hence we have a symplectic form,

ωΘ=d(αΘ)=1ρdμdρ+1ρdudω+1ρ2(dtdzdρ(udω))2ρ3dρ(tdz).{}^{\Theta}\omega=d({}^{\Theta}\alpha)=\tfrac{1}{\rho}d\mu\wedge d\rho+\tfrac{1}{\rho}du\wedge d\omega+\tfrac{1}{\rho^{2}}\left(dt\wedge dz-d\rho\wedge(ud\omega)\right)-\tfrac{2}{\rho^{3}}d\rho\wedge(tdz). (3.3)

With this symplectic structure on TΘX{}^{\Theta}T^{*}X we can explore the many ways to create Lagrangian submanifolds on this rescaled bundle.

Following [JoSá01], we can define extendible Lagrangian submanifolds. Set

(X×ΘX)d=X×ΘX𝔅FX×ΘX,(X\times_{\Theta}X)_{d}=X\times_{\Theta}X\bigsqcup_{\mathfrak{B}_{F}}X\times_{\Theta}X,

the double of the Θ\Theta-stretched product across the front face. We say that a smooth conic closed Lagrangian submanifold ΛT(X×ΘX)\Lambda\subset T^{*}(X\times_{\Theta}X) is extendible, if it intersects T(X×ΘX)|𝔅FT^{*}(X\times_{\Theta}X)\rvert_{\mathfrak{B}_{F}} transversely. This implies there exists a smooth conic Lagrangian ΛextT(X×ΘX)d\Lambda_{\emph{ext}}\subset T^{*}(X\times_{\Theta}X)_{d} such that

Λ=ΛextT(X×ΘX),ΛΘ:=ΛT(X×ΘX)|𝔅F\Lambda=\Lambda_{\emph{ext}}\cap T^{*}(X\times_{\Theta}X),\quad\Lambda_{\Theta}:=\Lambda\pitchfork T^{*}(X\times_{\Theta}X)\rvert_{\mathfrak{B}_{F}}

One reason for the interest in extendible Lagrangians is that their intersection with the cotangent bundle over the front face is again a Lagrangian submanifold.

Lemma 3.1.

If ΛT(X×ΘX)\Lambda\subset T^{*}(X\times_{\Theta}X) is extendible then ΛΘ=ΛT(X×ΘX)|𝔅F\Lambda_{\Theta}=\Lambda\cap T^{*}(X\times_{\Theta}X)\rvert_{\mathfrak{B}_{F}} is a Lagrangian submanifold of T𝔅FT^{*}\mathfrak{B}_{F}

Proof.

Fix coordinates (ρ,w1,,w2n,z)(\rho,w_{1},\ldots,w_{2n},z) of X×ΘXX\times_{\Theta}X valid near 𝔅F={ρ=0}\mathfrak{B}_{F}=\{\rho=0\}, and with dual variables (ξ,ηH1,,ηH2n,ηV)(\xi,\eta_{H}^{1},\ldots,\eta_{H}^{2n},\eta_{V}). Then (ρ,w,z;ξ,ηH,ηV)(\rho,w,z;\xi,\eta_{H},\eta_{V}) give local coordinates for T(X×ΘX)T^{*}(X\times_{\Theta}X) near 𝔅F\mathfrak{B}_{F}. By transversality, dρ|Λ0d\rho\rvert_{\Lambda}\neq 0, thus ρ\rho and some subset of (w,z;ξ,ηH,ηV)(w,z;\xi,\eta_{H},\eta_{V}) must give local coordinates for Λ\Lambda. Since Λ\Lambda is Lagrangian, the canonical 2-form

ωT(X×ΘX)=dρdξ+j=12ndwjdηHj+dzdηV\omega_{T^{*}(X\times_{\Theta}X)}=d\rho\wedge d\xi+\sum_{j=1}^{2n}dw^{j}\wedge d\eta_{H}^{j}+dz\wedge d\eta_{V}

must vanish on Λ\Lambda; hence it vanishes on ΛΘ\Lambda_{\Theta} as well. From the overall vanishing of this symplectic form, and the non-vanishing of dρd\rho on Λ\Lambda, we must have that dξd\xi restricted to TΛ|ΛΘT\Lambda\rvert_{\Lambda_{\Theta}} is a multiple of dρd\rho. This implies existence of a function ϕ(ρ,w,z;ηHj,ηV)\phi(\rho,w,z;\eta_{H}^{j},\eta_{V}) satisfying

Λ{ξ=ρϕ(ρ,w,z;ηHj,ηV)}.\Lambda\subset\{\xi=\rho\phi(\rho,w,z;\eta_{H}^{j},\eta_{V})\}.

In particular, ξ|ΛΘ=0\xi|_{\Lambda_{\Theta}}=0 and dwjdηHj+dzdηV=0\sum dw_{j}\wedge d\eta_{H}^{j}+dz\wedge d\eta_{V}=0 on TΛΘT\Lambda_{\Theta}. ∎

Having introduced extendible Lagrangians we immediately explain their relation to our the class of distributions we will ultimately be concerned with. We define a Lagrangian distribution associated to an extendible Lagrangian, (either ΛT(X×ΘX)\Lambda\subset T^{*}(X\times_{\Theta}X) or ΛT×T(X×ΘX)\Lambda\subset T^{*}\mathbb{R}\times T^{*}(X\times_{\Theta}X)), to be the restriction to X×ΘXX\times_{\Theta}X of a distribution which is Lagrangian with respect to an extension Λext\Lambda_{ext} of Λ\Lambda across 𝔅F\mathfrak{B}_{F}. As usual we denote the set of order mm distributions which are Lagrangian with respect to Λ\Lambda by Im(X×ΘX;Λ,Ω1/2Θ)I^{m}(X\times_{\Theta}X;\Lambda,{}^{\Theta}\Omega^{1/2}) (resp. Im(×X×ΘX;Λ,Ω1/2Θ)I^{m}(\mathbb{R}\times X\times_{\Theta}X;\Lambda,{}^{\Theta}\Omega^{1/2})).

Now that we have introduced Lagrangians in this setting we can see some ways they arise naturally. If X,YX,Y are two ACH manifolds, a Θ\Theta-canonical relation between them is a 𝒞{\mathcal{C}}^{\infty}-map

χ:ΓTΘXTΘY\chi:\Gamma\subset{}^{\Theta}T^{*}X\to{}^{\Theta}T^{*}Y

defined on an open conic subset ΓTΘX\Gamma\subset{}^{\Theta}T^{*}X such that χ(αYΘ)=αXΘ\chi^{*}({}^{\Theta}\alpha_{Y})={}^{\Theta}\alpha_{X}. Certain Θ\Theta-canonical relations will define Lagrangian submanifolds in T(X×ΘX)T^{*}(X\times_{\Theta}X), by associating to χ\chi its graph relation

χ:TΘXTΘXGr(χ)TΘX×TΘX\chi:{}^{\Theta}T^{*}X\to{}^{\Theta}T^{*}X\leftrightsquigarrow\text{Gr}(\chi)\subset{}^{\Theta}T^{*}X\times{}^{\Theta}T^{*}X

and we denote such Lagrangians by Λχ\Lambda_{\chi}. Particularly relevant Lagrangians will arise from liftable canonical transformations; these are homogeneous canonical transformations χ:TΘXTΘX\chi:{}^{\Theta}T^{*}X\to{}^{\Theta}T^{*}X, whose projections to the base is the identity over X\partial X.

Using the left and right projections we can define a symplectic form on TΘX×TΘX{}^{\Theta}T^{*}X\times{}^{\Theta}T^{*}X by

ω=π1ωΘπ2ωΘ.\omega=\pi_{1}^{*}\omega_{\Theta}-\pi_{2}^{*}\omega_{\Theta}. (3.4)

Further, the dual to the differential of the blow-down map β:X×ΘXX×X\beta:X\times_{\Theta}X\to X\times X induces a smooth map

TX×TXT(X×X)T(X×ΘX)T^{*}X\times T^{*}X\simeq T^{*}(X\times X)\to T^{*}(X\times_{\Theta}X) (3.5)

which is an isomorphism over Int(X×X)\text{Int}(X\times X) between ω\omega and the standard symplectic form on TX×TXT^{*}X\times T^{*}X.

Lemma 3.2.

(Liftable Canonical Transformations induce Extendible Lagrangians)
Let χ:TΘXTΘX\chi:{}^{\Theta}T^{*}X\to{}^{\Theta}T^{*}X be a liftable canonical transformation. The map (3.5), combined with the identification (over Int(X×X)\text{Int}(X\times X)) TX×TXTΘX×TΘXT^{*}X\times T^{*}X\sim{}^{\Theta}T^{*}X\times{}^{\Theta}T^{*}X gives a smooth map

φΘ:TΘX×TΘXT(X×ΘX)overInt(X×X)\varphi_{\Theta}:{}^{\Theta}T^{*}X\times{}^{\Theta}T^{*}X\xrightarrow{\simeq}T^{*}(X\times_{\Theta}X)\quad\text{over}\quad\emph{Int}(X\times X) (3.6)

which, restricted to the graph of χ\chi, extends by continuity to the boundary and embeds into it as a smooth Lagrangian of T(X×ΘX)T^{*}(X\times_{\Theta}X), denoted Λχ\Lambda_{\chi}. Further Λχ\Lambda_{\chi} intersects the boundary of T(X×ΘX)T^{*}(X\times_{\Theta}X) only over T𝔅F(X×ΘX)T^{*}_{\mathfrak{B}_{F}}(X\times_{\Theta}X), it is extendible across the front face, and this intersection

ΛχΘ:=ΛχT𝔅F(X×ΘX)\Lambda_{\chi_{\Theta}}:=\Lambda_{\chi}\cap T^{*}_{\mathfrak{B}_{F}}(X\times_{\Theta}X)

defines a Lagrangian submanifold of T𝔅FT^{*}\mathfrak{B}_{F}.

Proof.

On the two copies of XX in the product X×XX\times X we consider respectively coordinates (ρ,w,z)(\rho,w,z), and (ρ,w,z)(\rho^{\prime},w^{\prime},z^{\prime}) valid near the boundary. These induce corresponding local coordinates on the cotangent bundles, which we denote by

(ρ,w,z;ξ,ηH,ηV) and (ρ,w,z;ξ,ηH,ηV) corresponding to TX,(\rho,w,z;\xi,\eta_{H},\eta_{V})\text{ and }(\rho^{\prime},w^{\prime},z^{\prime};\xi^{\prime},\eta_{H}^{\prime},\eta_{V}^{\prime})\text{ corresponding to }T^{*}X, (3.7)

and

(ρ,w,z;μ,u,t) and (ρ,w,z;μ,u,t) corresponding to TΘX,(\rho,w,z;\mu,u,t)\text{ and }(\rho^{\prime},w^{\prime},z^{\prime};\mu^{\prime},u^{\prime},t^{\prime})\text{ corresponding to }{}^{\Theta}T^{*}X, (3.8)

on the left and right copies of the respective cotangent bundles. We fix

V=ρρW=wwρ,Z=zz(ρ)2V=\frac{\rho}{\rho^{\prime}}\quad W=\frac{w-w^{\prime}}{\rho^{\prime}},\quad Z=\frac{z-z^{\prime}}{(\rho^{\prime})^{2}}

as coordinates valid near the front face 𝔅F\mathfrak{B}_{F}, away from β#({ρ=0})\beta^{\#}(\{\rho^{\prime}=0\}). The map (3.6) gives an identification between the 1-forms

μρdρμρdρ+uρdwuρdw+tρ2dzt(ρ)2dz,\frac{\mu}{\rho}d\rho-\frac{\mu^{\prime}}{\rho^{\prime}}d\rho^{\prime}+\frac{u}{\rho}dw-\frac{u^{\prime}}{\rho^{\prime}}dw^{\prime}+\frac{t}{\rho^{2}}dz-\frac{t^{\prime}}{(\rho^{\prime})^{2}}dz^{\prime},

and

αdV+ξ~dρ+βdW+κ~dw+γdZ+η~dz,\alpha\;dV+\widetilde{\xi}d\rho^{\prime}+\beta dW+\widetilde{\kappa}dw^{\prime}+\gamma dZ+\widetilde{\eta}dz^{\prime},

defined on TΘX×TΘX{}^{\Theta}T^{*}X\times{}^{\Theta}T^{*}X and T(X×ΘX)T^{*}(X\times_{\Theta}X) respectively. We will first determine how the coefficients of these 1-forms are related under the map (3.6), in this neighborhood of 𝔅F\mathfrak{B}_{F}. Since ρ=Vρ,w=w+ρW,z=z+(ρ)2Z\rho=V\rho^{\prime},\;w=w^{\prime}+\rho^{\prime}W,\;z=z^{\prime}+(\rho^{\prime})^{2}Z we have

dρ=Vdρ+ρdV,dw=dw+ρdW+Wdρ,dz=dz+2ρZdρ+(ρ)2dZd\rho=Vd\rho^{\prime}+\rho^{\prime}dV,\quad dw=dw^{\prime}+\rho^{\prime}dW+Wd\rho^{\prime},\quad dz=dz^{\prime}+2\rho^{\prime}Zd\rho^{\prime}+(\rho^{\prime})^{2}dZ

and so the canonical 1-form in T(X×ΘX)T^{*}(X\times_{\Theta}X) is given by,

(μρVμρ+uρW+2tρρ2Z)\displaystyle\left(\frac{\mu}{\rho}V-\frac{\mu^{\prime}}{\rho^{\prime}}+\frac{u}{\rho}W+\frac{2t\rho^{\prime}}{\rho^{2}}Z\right) dρ+μρρdV+(uρuρ)dw+uρρdW+(tρ2t(ρ)2)dz+t(ρ)2ρ2dZ\displaystyle d\rho^{\prime}+\frac{\mu\rho^{\prime}}{\rho}dV+\left(\frac{u}{\rho}-\frac{u^{\prime}}{\rho^{\prime}}\right)dw^{\prime}+\frac{u\rho^{\prime}}{\rho}dW+\left(\frac{t}{\rho^{2}}-\frac{t^{\prime}}{(\rho^{\prime})^{2}}\right)dz^{\prime}+\frac{t(\rho^{\prime})^{2}}{\rho^{2}}dZ
=αdV+ξ~dρ+βdW+κ~dw+γdZ+η~dz\displaystyle=\alpha\;dV+\widetilde{\xi}d\rho^{\prime}+\beta dW+\widetilde{\kappa}dw^{\prime}+\gamma dZ+\widetilde{\eta}dz^{\prime}

where

α=μρρ,β=uρρ,γ=t(ρρ)2,\displaystyle\alpha=\mu\frac{\rho^{\prime}}{\rho},\quad\beta=u\frac{\rho^{\prime}}{\rho},\quad\gamma=t\left(\frac{\rho^{\prime}}{\rho}\right)^{2},
ξ~=μρμρ+uρwwρ+2tρzzρ2,κ~=uρuρ,η~=tρ2t(ρ)2.\displaystyle\quad\;\widetilde{\xi}=\frac{\mu}{\rho^{\prime}}-\frac{\mu^{\prime}}{\rho^{\prime}}+\frac{u}{\rho^{\prime}}\frac{w-w^{\prime}}{\rho}+\frac{2t}{\rho^{\prime}}\frac{z-z^{\prime}}{\rho^{2}},\quad\widetilde{\kappa}=\frac{u}{\rho}-\frac{u^{\prime}}{\rho^{\prime}},\quad\widetilde{\eta}=\frac{t}{\rho^{2}}-\frac{t^{\prime}}{(\rho^{\prime})^{2}}.

Now, using the fact that χ\chi is a Θ\Theta-canonical relation (and thus αXΘχ(αXΘ)=0{}^{{\Theta}}\alpha_{X}-\chi^{*}({}^{\Theta}\alpha_{X})=0), and the fact that χ\chi restricts to the identity over X\partial X. To determine Gr(χ)\text{Gr}(\chi) in the coordinates (3.8) we observe first that ρ\rho and ρ\rho^{\prime} are both bdfs on XX and thus conformal: ρ=fρ\rho^{\prime}=f\rho. Further, we have that πX:TΘXX\pi_{X}:{}^{\Theta}T^{*}X\to X, and (0,w,z):=(πXχ)|X(x,ζ)=(0,w,z)(0,w^{\prime},z^{\prime}):=(\pi_{X}\circ\chi)|_{\partial X}(x,\zeta)=(0,w,z), hence w=w+ρA,z=z+ρ2Bw^{\prime}=w+\rho A,\;z^{\prime}=z+\rho^{2}B for some smooth functions A,BA,B on TΘX{}^{\Theta}T^{*}X. Finally, we use the relation between the fundamental 1-forms to observe that

μdρρ\displaystyle\mu\frac{d\rho}{\rho} +udwρ+tdzρ2=χ(μdρρ+udwρ+tdz(ρ)2)\displaystyle+u\frac{dw}{\rho}+t\frac{dz}{\rho^{2}}=\chi^{*}\left(\mu^{\prime}\frac{d\rho^{\prime}}{\rho^{\prime}}+u^{\prime}\frac{dw^{\prime}}{\rho^{\prime}}+t^{\prime}\frac{dz^{\prime}}{(\rho^{\prime})^{2}}\right)
=μ(dρρ+dff)+ua(dwρ+dA+Adρρ)+ta2(dzρ2+2Bdρρ+dB)\displaystyle=\mu^{\prime}\left(\frac{d\rho}{\rho}+\frac{df}{f}\right)+\frac{u^{\prime}}{a}\left(\frac{dw}{\rho}+dA+A\frac{d\rho}{\rho}\right)+\frac{t^{\prime}}{a^{2}}\left(\frac{dz}{\rho^{2}}+2B\frac{d\rho}{\rho}+dB\right)
=(μ+ufA+2tf2)dρρ+ufdwρ+2tf2dzρ2+(μfdf+ufdA+tf2dB).\displaystyle=\left(\mu^{\prime}+\frac{u^{\prime}}{f}A+\frac{2t^{\prime}}{f^{2}}\right)\frac{d\rho}{\rho}+\frac{u^{\prime}}{f}\frac{dw}{\rho}+\frac{2t^{\prime}}{f^{2}}\frac{dz}{\rho^{2}}+\left(\frac{\mu^{\prime}}{f}df+\frac{u^{\prime}}{f}dA+\frac{t^{\prime}}{f^{2}}dB\right).

The final bracketed term will only contribute terms which are 𝒪(ρ)\mathcal{O}(\rho) or 𝒪(ρ2)\mathcal{O}(\rho^{2}) after computing their Θ\Theta-differential (e.g. df=ρρfdρρ+ρwfdwρ+ρ2zfdzρ2df=\rho\partial_{\rho}f\tfrac{d\rho}{\rho}+\rho\partial_{w}f\frac{dw}{\rho}+\rho^{2}\partial_{z}f\frac{dz}{\rho^{2}}), thus after grouping such terms we obtain

μdρρ+udwρ+tdzρ2=(μ+ufA+2tf2+ρC)dρρ+(uf+ρD)dwρ+(2tf2+ρ2E)dzρ2,\mu\frac{d\rho}{\rho}+u\frac{dw}{\rho}+t\frac{dz}{\rho^{2}}=\left(\mu^{\prime}+\frac{u^{\prime}}{f}A+\frac{2t^{\prime}}{f^{2}}+\rho C\right)\frac{d\rho}{\rho}+\left(\frac{u^{\prime}}{f}+\rho D\right)\frac{dw}{\rho}+\left(\frac{2t^{\prime}}{f^{2}}+\rho^{2}E\right)\frac{dz}{\rho^{2}},

where f>0,A,B,C,Df>0,A,B,C,D are smooth functions of (ρ,w,z,μ,u,t)(\rho,w,z,\mu,u,t). Taken together, these computations imply that its graph is of the form

Gr(χ)\displaystyle\text{Gr}(\chi) ={((ρ,w,z,μ,u,t),(ρ,w,z,μ,u,t))|ρ=fρ,w=w+ρA,z=z+ρ2B\displaystyle=\{((\rho,w,z,\mu,u,t),(\rho^{\prime},w^{\prime},z^{\prime},\mu^{\prime},u^{\prime},t^{\prime}))\;|\;\rho^{\prime}=f\rho,\;w^{\prime}=w+\rho A,\;z^{\prime}=z+\rho^{2}B\;
μ=μuA2tB+ρC,u=fu+ρD,t=f2t+ρ2E}\displaystyle\mu^{\prime}=\mu-uA-2tB+\rho C,\;u^{\prime}=fu+\rho D,\;t^{\prime}=f^{2}t+\rho^{2}E\}

From this we can see that

α=efμ,β=efu,γ=e2ft,ξ~=efC,κ~=efD,η~=e2fE.\alpha=e^{f}\mu,\quad\beta=e^{f}u,\quad\gamma=e^{2f}t,\quad\widetilde{\xi}=-e^{-f}C,\quad\widetilde{\kappa}=-e^{-f}D,\quad\widetilde{\eta}=-e^{-2f}E.

Since ef=ρρe^{f}=\tfrac{\rho^{\prime}}{\rho} is smooth and positive on Λχ\Lambda_{\chi}, the map (3.6) (defined over the interior Int(X×X)\text{Int}(X\times X)), extends by continuity to the boundary when restricted to Gr(χ)\text{Gr}(\chi), thus defining Λχ\Lambda_{\chi}

Gr(χ)ΛχT(X×ΘX)\text{Gr}(\chi)\simeq\Lambda_{\chi}\hookrightarrow T^{*}(X\times_{\Theta}X)

as the image of Gr(χ)\text{Gr}(\chi) under the map (3.6). Further, this shows that Λχ\Lambda_{\chi} intersects the boundary of T(X×ΘX)T^{*}(X\times_{\Theta}X) only over 𝔅F={ρ=0}\mathfrak{B}_{F}=\{\rho^{\prime}=0\} and does so transversely. Thus it is an extendible Lagrangian, and we have by the previous lemma that this intersection ΛχΘ\Lambda_{\chi_{\Theta}} is a Lagrangian submanifold of T𝔅FT^{*}\mathfrak{B}_{F}. ∎

This lemma elucidates the name liftable canonical transformation as they provide examples of canonical transformation with “good” lifts to T(X×ΘX)T^{*}(X\times_{\Theta}X) as the associated Lagrangian meets the diagonal only in the front face 𝔅F\mathfrak{B}_{F}.

Given p𝒞(TΘX)p\in{\mathcal{C}}^{\infty}({}^{\Theta}T^{*}X) we define its Θ\Theta-Hamiltonian vector field by the relation ωΘ(,HpΘ)=dp{}^{\Theta}\omega(-,{}^{\Theta}H_{p})=dp. In local coordinates in which ωΘ{}^{\Theta}\omega is given by (3.3), HpΘ{}^{\Theta}H_{p} is given by

HpΘ=\displaystyle{}^{\Theta}H_{p}= ρpμρ(ρpρ+wjpwj+2tpt)μ\displaystyle\rho\frac{\partial p}{\partial\mu}\partial_{\rho}-\left(\rho\frac{\partial p}{\partial\rho}+w_{j}\frac{\partial p}{\partial w_{j}}+2t\frac{\partial p}{\partial t}\right)\partial_{\mu}
+j=12n(ρpuj)wj(ρpwjujpμ)uj+ρ2ptz(ρ2pz2tpμ)t\displaystyle+\sum_{j=1}^{2n}\left(\rho\frac{\partial p}{\partial u_{j}}\right)\partial_{w_{j}}-\left(\rho\frac{\partial p}{\partial w_{j}}-u_{j}\frac{\partial p}{\partial\mu}\right)\partial_{u_{j}}+\rho^{2}\frac{\partial p}{\partial t}\partial z-\left(\rho^{2}\frac{\partial p}{\partial z}-2t\frac{\partial p}{\partial\mu}\right)\partial_{t}

And observe that this vector field has the special property that the projection of the vector field to the base vanishes when restricted to X\partial X.

Because our focus is the wave equation we are most interested in the Hamiltonian associated to our ACH metric. Since our metric satisfies

gACH=dρ2+hΘ(w,z,dw,dz)+ρQ(ρ,w,z,dw,dz)ρ2g_{ACH}=\frac{d\rho^{2}+h_{\Theta}(w,z,dw,dz)+\rho Q(\rho,w,z,dw,dz)}{\rho^{2}}

we can conclude its dual metric on TXT^{*}X has the form

G=(ρξ)2+ρ2hΘ(w,z,ηH,ηV)+ρ3Q(ρ,w,z,ηH,ηV)G=(\rho\xi)^{2}+\rho^{2}h_{\Theta}(w,z,\eta_{H},\eta_{V})+\rho^{3}Q(\rho,w,z,\eta_{H},\eta_{V})

or in the coordinates (ρ,w,z,μ,u,t)(\rho,w,z,\mu,u,t) on TΘX{}^{\Theta}T^{*}X our dual metric is given by

G=μ2+hΘ(w,z,u,t)+ρQ(ρ,w,z,u,t).G=\mu^{2}+h_{\Theta}(w,z,u,t)+\rho Q(\rho,w,z,u,t). (3.9)

This function on TΘX{}^{\Theta}T^{*}X will be the Hamiltonian of interest in our study of the wave equation.

Lemma 3.3.

Θ\Theta-canonical flowouts

Let G𝒞(TΘX)G\in{\mathcal{C}}^{\infty}({}^{\Theta}T^{*}X) be the dual metric associated to the metric gACHg_{ACH}, and let HGΘ{}^{\Theta}H_{G} be its Θ\Theta-Hamilton vector field. For all s>0s>0, the canonical transformation χs:TΘXTΘX\chi_{s}:{}^{\Theta}T^{*}X\to{}^{\Theta}T^{*}X, given as the flow-out of the Hamiltonian,

χs(q):=exp(sHGΘ)(q),\chi_{s}(q):=\emph{exp}(s\;{}^{\Theta}H_{G})(q),

is a liftable canonical transformation. Thus the graph of χs\chi_{s} defines a smooth extendible Lagrangian submanifold of T(X×ΘX)T^{*}(X\times_{\Theta}X). Further, the intersection

Λ𝔅F(s):=ΛsT(X×ΘX)|𝔅F\Lambda_{\mathfrak{B}_{F}}(s):=\Lambda_{s}\cap T^{*}(X\times_{\Theta}X)|_{\mathfrak{B}_{F}}

is a smooth Lagrangian submanifold of T𝔅FT^{*}\mathfrak{B}_{F} given by

exp(sHGΘ)(T𝔅F|DΘ𝔅F)=Λ𝔅F(s)\emph{exp}(s\;H_{G_{\Theta}})(T^{*}\mathfrak{B}_{F}|_{D_{\Theta}\cap\mathfrak{B}_{F}})=\Lambda_{\mathfrak{B}_{F}}(s)

where GΘ=G~|𝔅FG_{\Theta}=\widetilde{G}\rvert_{\mathfrak{B}_{F}}, the restriction to the front face of the lift of GG to T(X×ΘX)T^{*}(X\times_{\Theta}X).

Proof.

Since the flow-out of a Hamilton vector field is always a canonical transformation, the first claim follows from the fact that only the projection onto the base vanishes. Thus we only to check the claim regarding Λ𝔅F(s)\Lambda_{\mathfrak{B}_{F}}(s). We can study the graph of χs\chi_{s} after viewing G𝒞(TΘX×TΘX)G\in{\mathcal{C}}^{\infty}({}^{\Theta}T^{*}X\times{}^{\Theta}T^{*}X) as a function depending only on the second copy of TΘX{}^{\Theta}T^{*}X.

On this space, we can write our canonical 1-form in the coordinates

π1(αΘ)π2(αΘ)\displaystyle\pi_{1}^{*}({}^{\Theta}\alpha)-\pi_{2}^{*}({}^{\Theta}\alpha) :=μρdρμρdρ+uρdwuρdw+tρ2dzt(ρ)2dz,\displaystyle:=\tfrac{\mu}{\rho}d\rho-\tfrac{\mu^{\prime}}{\rho^{\prime}}d\rho^{\prime}+\tfrac{u}{\rho}dw-\tfrac{u^{\prime}}{\rho^{\prime}}dw^{\prime}+\tfrac{t}{\rho^{2}}dz-\tfrac{t^{\prime}}{(\rho^{\prime})^{2}}dz^{\prime}, (3.10)

thus we can write the Hamilton vector field of a function on this space with respect to this 1-form, with the same formula as we calculated above. In this case χs\chi_{s} is the flow-out of the diagonal in TΘX×TΘX{}^{\Theta}T^{*}X\times{}^{\Theta}T^{*}X along the vector field HGΘ{}^{\Theta}H_{G}. In these coordinates our length function is given by

G=(μ)2+hΘ(w,z,u,t)+ρQ(ρ,w,z,u,t)G=(\mu^{\prime})^{2}+h_{\Theta}(w^{\prime},z^{\prime},u^{\prime},t^{\prime})+\rho^{\prime}Q(\rho^{\prime},w^{\prime},z^{\prime},u^{\prime},t^{\prime})

and we can consider local coordinates near the front face, projective with respect to the left face:

V=ρρ,W=wwρ,Z=zzρ2V=\frac{\rho^{\prime}}{\rho},\quad W=\frac{w^{\prime}-w}{\rho},\quad Z=\frac{z^{\prime}-z}{\rho^{2}}

with blow-down map

β:X×ΘXX×X(ρ,w,z,V,W,Z)\displaystyle\beta:\;X\times_{\Theta}X\to X\times X\quad\quad(\rho,w,z,V,W,Z) (ρ,w,z,ρ,w,z)\displaystyle\mapsto(\rho,w,z,\rho^{\prime},w^{\prime},z^{\prime})
=(ρ,w,z,ρV,w+ρW,z+ρ2Z).\displaystyle=(\rho,w,z,\rho V,w+\rho W,z+\rho^{2}Z).

The pullback of (3.10) by β\beta is,

adρ+afdV+bdw+bfdW+cdz+cfdZ,ad\rho+a_{f}dV+bdw+b_{f}dW+cdz+c_{f}dZ,

and in these coordinates we have that 𝔅F={ρ=0}\mathfrak{B}_{F}=\{\rho=0\} and the interior lift of the diagonal DΘD_{\Theta} is given by DΘ={V=1,W=Z=0}D_{\Theta}=\{V=1,W=Z=0\}. The lift of pp to T(X×ΘX)T^{*}(X\times_{\Theta}X) is given by

p~\displaystyle\widetilde{p} =(afV)2+h0(w+ρW,z+ρ2Z,Vbf,V2cf)+ρVQ(ρV,w+ρW,z+ρ2Z,Vbf,V2cf))\displaystyle=(a_{f}V)^{2}+h_{0}(w+\rho W,z+\rho^{2}Z,-Vb_{f},-V^{2}c_{f})+\rho VQ(\rho V,w+\rho W,z+\rho^{2}Z,-Vb_{f},-V^{2}c_{f}))
=(afV)2+V2h0(w+ρW,z+ρ2W,bf,cf)+ρV3Q(ρV,w+ρW,z+ρ2Z,bf,cf)\displaystyle=(a_{f}V)^{2}+V^{2}h_{0}(w+\rho W,z+\rho^{2}W,b_{f},c_{f})+\rho V^{3}Q(\rho V,w+\rho W,z+\rho^{2}Z,b_{f},c_{f})

where the functions h0,Qh_{0},Q are 𝒟ρ\mathcal{D}_{\rho}^{\mathbb{H}}-homogeneous of order 2 in the fiber variables.

Now we lift our symplectic form (3.4) to T(X×ΘX)T^{*}(X\times_{\Theta}X), and denote it by ω~\widetilde{\omega}, HGΘ{}^{\Theta}H_{G} lifts to HG~H_{\widetilde{G}}. In the coordinates

[(ρ,w,z,V,W,Z);(a,b,c,af,bf,cf)]T(X×ΘX)[(\rho,w,z,V,W,Z)\;;(a,b,c,a_{f},b_{f},c_{f})]\in T^{*}(X\times_{\Theta}X)

our lifted Hamilton vector field has the form

HG~\displaystyle H_{\widetilde{G}} =(G~aρG~ρa)+(G~afVG~Vaf)\displaystyle=\left(\frac{\partial\widetilde{G}}{\partial a}\partial_{\rho}-\frac{\partial\widetilde{G}}{\partial\rho}\partial_{a}\right)+\left(\frac{\partial\widetilde{G}}{\partial a_{f}}\partial_{V}-\frac{\partial\widetilde{G}}{\partial V}\partial_{a_{f}}\right)
+j=12n(G~bjwjG~wjbj)+j=12n(G~bfjWjG~Wj(bf)j)\displaystyle+\sum_{j=1}^{2n}\left(\frac{\partial\widetilde{G}}{\partial b^{j}}\partial_{w_{j}}-\frac{\partial\widetilde{G}}{\partial w^{j}}\partial_{b_{j}}\right)+\sum_{j=1}^{2n}\left(\frac{\partial\widetilde{G}}{\partial b_{f}^{j}}\partial_{W_{j}}-\frac{\partial\widetilde{G}}{\partial W^{j}}\partial_{(b_{f})_{j}}\right)
+(G~czG~zc)+(G~cfZG~Zcf)\displaystyle+\left(\frac{\partial\widetilde{G}}{\partial c}\partial_{z}-\frac{\partial\widetilde{G}}{\partial z}\partial_{c}\right)+\left(\frac{\partial\widetilde{G}}{\partial c_{f}}\partial_{Z}-\frac{\partial\widetilde{G}}{\partial Z}\partial_{c_{f}}\right)
=2afV2V2V[af2+hΘ]afV2jWjG~wjaV2jhΘwjbj\displaystyle=2a_{f}V^{2}\partial_{V}-2V[a_{f}^{2}+h_{\Theta}]\partial_{a_{f}}-V^{2}\sum_{j}W_{j}\frac{\partial\widetilde{G}}{\partial w^{j}}\partial_{a}-V^{2}\sum_{j}\frac{\partial h_{\Theta}}{\partial w_{j}}\partial_{b_{j}}
+V2jhΘbfjWj+V2hΘcfZ+𝒪(ρ),\displaystyle+V^{2}\sum_{j}\frac{\partial h_{\Theta}}{\partial b_{f}^{j}}\partial_{W_{j}}+V^{2}\frac{\partial h_{\Theta}}{\partial c_{f}}\partial_{Z}+\mathcal{O}(\rho),

thus Hp~H_{\widetilde{p}} is smooth all the way down to 𝔅F={ρ=0}\mathfrak{B}_{F}=\{\rho=0\}. Further, with respect to our coordinate transformation on T(X×ΘX)T^{*}(X\times_{\Theta}X) induced by the blow-down map β\beta, we have that the diagonal

{ρ=ρ,w=w,z=z,μ=μ,u=u,t=t}=(TΘX)diagTΘX×TΘX\{\rho=\rho^{\prime},w=w^{\prime},z=z^{\prime},\mu=\mu^{\prime},u=u^{\prime},t=t^{\prime}\}=({}^{\Theta}T^{*}X)_{\operatorname{diag}}\subset{}^{\Theta}T^{*}X\times{}^{\Theta}T^{*}X

lifts to

𝒟~Θ={V=1,W=Z=a=b=c=0}T(X×ΘX).\widetilde{\mathcal{D}}_{\Theta}=\{V=1,W=Z=a=b=c=0\}\subset T^{*}(X\times_{\Theta}X).

Thus 𝒟~Θ\widetilde{\mathcal{D}}_{\Theta} transversely intersects T(X×ΘX)|𝔅FT^{*}(X\times_{\Theta}X)|_{\mathfrak{B}_{F}} at {ρ=0,V=1,W=Z=a=b=c=0}\{\rho=0,V=1,W=Z=a=b=c=0\}. Finally we see that Hp~H_{\widetilde{p}} projects down to T𝔅FT^{*}\mathfrak{B}_{F} as

2afV2V\displaystyle 2a_{f}V^{2}\partial_{V} 2V(af2+hΘ(w,z,bf,cf))af\displaystyle-2V(a_{f}^{2}+h_{\Theta}(w,z,b_{f},c_{f}))\partial_{a_{f}}
+2V2i,jhΘij(w,z)bf(j)bf(j)+2V2hΘ0,0(w,z)cfcf\displaystyle+2V^{2}\sum_{i,j}h_{\Theta}^{ij}(w,z)\cdot b_{f}^{(j)}\frac{\partial}{\partial b_{f}^{(j)}}+2V^{2}h_{\Theta}^{0,0}(w,z)\cdot c_{f}\frac{\partial}{\partial c_{f}}

which is precisely the Hamilton vector field of af2V2+V2hΘ(w,z,bf,cf)a_{f}^{2}V^{2}+V^{2}h_{\Theta}(w,z,b_{f},c_{f}). ∎

Remark 1.

Notice that because

G~|𝔅F=V2(af2+hΘ(w,z,bf,cf))=:GΘ\widetilde{G}|_{\mathfrak{B}_{F}}=V^{2}(a_{f}^{2}+h_{\Theta}(w,z,b_{f},c_{f}))=:G_{\Theta}

the projection of the Hamilton vector field of GG to T𝔅FT^{*}\mathfrak{B}_{F} is precisely the Hamilton vector field of the restriction of GG to 𝔅F\mathfrak{B}_{F}, with respect to the induced symplectic form on T𝔅FT^{*}\mathfrak{B}_{F}.

In other words, for the Hamiltonian given by our length functional (3.9), we have that: s>0\forall s>0, the twisted graph of exp(sHGΘ):TΘXTΘX\text{exp}(s\;{}^{\Theta}H_{G}):{}^{\Theta}T^{*}X\to{}^{\Theta}T^{*}X defines a Lagrangian submanifold Λ(s)T(X×ΘX)\Lambda(s)\subset T^{*}(X\times_{\Theta}X). Further this Lagrangian intersects the boundary only over 𝔅F\mathfrak{B}_{F}, and it does so transversely. The transversal intersection is itself a Lagrangian flow-out

ΛF(s):=exp(sHGΘ)(T𝔅F|DΘ𝔅F)T𝔅F\Lambda_{F}(s):=\text{exp}(s\;H_{G_{\Theta}})(T^{*}\mathfrak{B}_{F}|_{D_{\Theta}\cap\mathfrak{B}_{F}})\subset T^{*}\mathfrak{B}_{F}

which is the flow-out by the Hamilton vector field of GΘ=σ2(N𝔅F(Δ))G_{\Theta}=\sigma_{2}(N_{\mathfrak{B}_{F}}(\Delta)), the principal symbol of the normal operator at the front face.

3.2. Θ\Theta-FIOs and the Wave Kernel


Here we construct the calculus of operators that our wave group cos(tΔn2/4)\cos(t\sqrt{\Delta-n^{2}/4}) will lie in. These shall be restricted to the subclass of Lagrangian distributions whose support does not meet the left or right faces, β(X×X)\beta^{*}(\partial X\times X), and β(X×X)\beta^{*}(X\times\partial X) respectively. Due to the finite speed of propagation, initial data U(t,p,p)U(t,p,p^{\prime}) supported in the interior of 𝔅F\mathfrak{B}_{F} which evolves according to the wave equation,

{(Dt2+Δgn24)U(t,p,p)=0U(0,p,p)=δ(p,p),tU(0,p,p)=0\begin{cases}\left(D_{t}^{2}+\Delta_{g}-\tfrac{n^{2}}{4}\right)U(t,p,p^{\prime})=0\\ U(0,p,p^{\prime})=\delta(p,p^{\prime}),\quad\partial_{t}U(0,p,p^{\prime})=0\end{cases}

remains supported away from the left and right faces, 𝔅L,𝔅R\mathfrak{B}_{L},\mathfrak{B}_{R}. In particular, when considering our calculus of FIOs, we can ignore the complement of the front face in the corner, and restrict ourselves to Lagrangians which meet the boundary only at 𝔅F\mathfrak{B}_{F}.

Since the canonical relation CC of the wave group will be a Lagrangian in T×T(X×ΘX)T^{*}\mathbb{R}\times T^{*}(X\times_{\Theta}X), we mildly extend our class of Lagrangians from the last section. The canonical 1-form on T×TΘX×TΘXT^{*}\mathbb{R}\times{}^{\Theta}T^{*}X\times{}^{\Theta}T^{*}X is given by

α=tdτ+μρdρμρdρ+uρdwuρdw+sρ2dzs(ρ)2dz.\alpha=td\tau+\tfrac{\mu}{\rho}d\rho-\tfrac{\mu^{\prime}}{\rho^{\prime}}d\rho^{\prime}+\tfrac{u}{\rho}dw-\tfrac{u^{\prime}}{\rho^{\prime}}dw^{\prime}+\tfrac{s}{\rho^{2}}dz-\tfrac{s^{\prime}}{(\rho^{\prime})^{2}}dz.^{\prime}

With this 1-form, we can define a canonical relation

C={(t,τ,ζ1,ζ2)|τ+G(ζ1,ζ1)=0,ζ2=exp(tHGΘ)(ζ1)}T×TΘX×TΘX,C=\left\{(t,\tau,\zeta_{1},\zeta_{2})\bigg{|}\,\tau+\sqrt{G(\zeta_{1},\zeta_{1})}=0,\;\zeta_{2}=\text{exp}(t\;{}^{\Theta}H_{G})(\zeta_{1})\right\}\subset T^{*}\mathbb{R}\times{}^{\Theta}T^{*}X\times{}^{\Theta}T^{*}X,

and this canonical relation in turn defines a Lagrangian of T×T(X×ΘX)T^{*}\mathbb{R}\times T^{*}(X\times_{\Theta}X) given by

ΛC={(t,τ,ζ1,ζ2)|τ+G~(ζ1,ζ2)=0,(ζ1,ζ2)Λt}T×T(X×ΘX)\Lambda_{C}=\left\{(t,\tau,\zeta_{1},\zeta_{2})\bigg{|}\,\tau+\sqrt{\widetilde{G}(\zeta_{1},\zeta_{2})}=0,\;(\zeta_{1},\zeta_{2})\in\Lambda_{t}\right\}\subset T^{*}\mathbb{R}\times T^{*}(X\times_{\Theta}X)

where Λt\Lambda_{t} is an extendible Lagrangian associated to the graph of the liftable canonical transformation

χt:=exp(tHGΘ)(q):TΘXTΘX,\chi_{t}:=\text{exp}(t\;{}^{\Theta}H_{G})(q):{}^{\Theta}T^{*}X\to{}^{\Theta}T^{*}X,

and G~\widetilde{G} is the lift of GG from the second copy of TΘX{}^{\Theta}T^{*}X. In particular, this Lagrangian intersects the boundary only over the front face 𝔅F\mathfrak{B}_{F}, and

ΛCΘ={(t,τ,ζ¯1,ζ¯2)|τ+GΘ(ζ¯1,ζ¯2)=0,(ζ¯1,ζ¯2)Λ𝔅F(t)}T×T𝔅F\Lambda_{C}^{\Theta}=\left\{(t,\tau,\overline{\zeta}_{1},\overline{\zeta}_{2})\bigg{|}\,\tau+\sqrt{G_{\Theta}(\overline{\zeta}_{1},\overline{\zeta}_{2})}=0,\;(\overline{\zeta}_{1},\overline{\zeta}_{2})\in\Lambda_{\mathfrak{B}_{F}}(t)\right\}\subset T^{*}\mathbb{R}\times T^{*}\mathfrak{B}_{F}

where GΘG_{\Theta} is the restriction of G~\widetilde{G} to 𝔅F\mathfrak{B}_{F}.

Now, given a liftable canonical transformation χ:TΘXTΘX\chi:{}^{\Theta}T^{*}X\to{}^{\Theta}T^{*}X we define our Θ\Theta-Fourier Integral Operators associated to χ\chi to be the linear operators L:(X)𝒟(X)L:\mathcal{E}^{\prime}(X)\to\mathcal{D}^{\prime}(X) whose Schwartz kernels lie in the space of distributions

IΘm,s(X;χ,Ω1/2Θ):={\displaystyle I_{\Theta}^{m,s}(X;\chi,{}^{\Theta}\Omega^{1/2}):=\{ ρFs𝒦L|𝒦LIm(X×ΘX;Λχ,Ω1/2Θ),ρFs𝒦L vanishes\displaystyle\rho_{F}^{s}\mathcal{K}_{L}\big{|}\,\mathcal{K}_{L}\in I^{m}(X\times_{\Theta}X;\Lambda_{\chi},{}^{\Theta}\Omega^{1/2}),\;\rho_{F}^{s}\mathcal{K}_{L}\text{ vanishes}
in a neighborhood of (X×ΘX)𝔅F}\displaystyle\text{ in a neighborhood of }\partial(X\times_{\Theta}X)\setminus\mathfrak{B}_{F}\}

where Λχ\Lambda_{\chi} is the extendible Lagrangian submanifold of T(X×ΘX)T^{*}(X\times_{\Theta}X) associated to χ\chi by lemma 3.2. Similarly, for the canonical relation CC defined above, we say that Θ\Theta-Fourier Integral Operators associated to CC are the linear operators B:(×X)𝒟(X)B:\mathcal{E}^{\prime}(\mathbb{R}\times X)\to\mathcal{D}^{\prime}(X) whose Schwartz kernels lie in the space of distributions

IΘm,s(×X,X;C,Ω1/2Θ):={\displaystyle I_{\Theta}^{m,s}(\mathbb{R}\times X,X;C,{}^{\Theta}\Omega^{1/2}):=\{ ρFs𝒦B|𝒦BIm(×X×ΘX;ΛC,Ω1/2Θ),ρFs𝒦B vanishes\displaystyle\rho_{F}^{s}\mathcal{K}_{B}\big{|}\,\mathcal{K}_{B}\in I^{m}(\mathbb{R}\times X\times_{\Theta}X;\Lambda_{C},{}^{\Theta}\Omega^{1/2}),\;\rho_{F}^{s}\mathcal{K}_{B}\text{ vanishes}
in a neighborhood of (×X×ΘX)(×𝔅F)}\displaystyle\text{ in a neighborhood of }\partial(\mathbb{R}\times X\times_{\Theta}X)\setminus(\mathbb{R}\times\mathfrak{B}_{F})\}

In both cases, such operators are those whose Schwartz kernels are Lagrangian distributions with respect to Λχ\Lambda_{\chi}, (ΛC\Lambda_{C} resp.), and vanish to order ss at the front face 𝔅F\mathfrak{B}_{F}. Such operators carry two different principal symbol mappings: one is the usual symbol of a Lagrangian distribution, in the interior; the second operator is obtained by the principal symbol of the normal operator 𝒦L|𝔅F\mathcal{K}_{L}\rvert_{\mathfrak{B}_{F}} (resp. 𝒦B|×𝔅F\mathcal{K}_{B}\rvert_{\mathbb{R}\times\mathfrak{B}_{F}}) associated to the Lagrangian in T𝔅FT^{*}\mathfrak{B}_{F} (resp. T×T𝔅FT^{*}\mathbb{R}\times T^{*}\mathfrak{B}_{F}).

This second symbol is again the symbol of a Lagrangian distribution from the fact that our Lagrangian Λχ\Lambda_{\chi} (resp. ΛC\Lambda_{C}) has transversal intersection with T(X×ΘX)|𝔅FT^{*}(X\times_{\Theta}X)\rvert_{\mathfrak{B}_{F}} (resp. T×T(X×ΘX)|𝔅FT^{*}\mathbb{R}\times T^{*}(X\times_{\Theta}X)\rvert_{\mathfrak{B}_{F}}), thus the restriction of Lagrangian distribution to 𝔅F\mathfrak{B}_{F} is again a Lagrangian distribution with respect to Λχ\Lambda_{\chi} (resp. ΛC\Lambda_{C}).

We now take a moment again to highlight the normal operator. If 𝒦AIΘm,s\mathcal{K}_{A}\in I_{\Theta}^{m,s}, then Np(A)=(ρFs𝒦A)|𝔅FN_{p}(A)=(\rho_{F}^{-s}\mathcal{K}_{A})|_{\mathfrak{B}_{F}}, and Np(A)N_{p}(A) is a Lagrangian distribution with respect to Λχ\Lambda_{\chi} (resp. ΛC\Lambda_{C}). Further the normal operator satifies an analogue of the short exact sequence for principal symbols of operators:

Proposition 3.4.

The normal operator participates in a short exact sequence

0IΘm,1(×X,X;C,Ω1/2Θ)IΘm,0(×X,X;C,Ω1/2Θ)Np()Im(×𝔅F;ΛCΘ,Ω1/2)00\to I_{\Theta}^{m,1}(\mathbb{R}\times X,X;C,{}^{\Theta}\Omega^{1/2})\hookrightarrow I_{\Theta}^{m,0}(\mathbb{R}\times X,X;C,{}^{\Theta}\Omega^{1/2})\xrightarrow{N_{p}(-)}I^{m}(\mathbb{R}\times\mathfrak{B}_{F};\Lambda_{C}^{\Theta},\Omega^{1/2})\to 0

such that for any Θ\Theta-differential operator PDiffΘm(X)P\in\emph{Diff}_{\Theta}^{m}(X) and any Θ\Theta-Fourier integral operator BIΘm,s(×X,X;C,Ω1/2Θ)B\in I_{\Theta}^{m,s}(\mathbb{R}\times X,X;C,{}^{\Theta}\Omega^{1/2}) we have

Np((Dt2P)B)=(Dt2Np(P))Np(B)N_{p}((D_{t}^{2}-P)\circ B)=(D_{t}^{2}-N_{p}(P))\ast N_{p}(B)
Proof.

This is an analogue of [MaMe87, prop 5.19], and [JoSá01, prop 3.1].

The injectivity portion of the statement of exactness is immediate from the definition. Since we have Np^()N_{\widehat{p}}(-) is 𝒞{\mathcal{C}}^{\infty} in p^X\widehat{p}\in\partial X and defines an operator on 𝒞(𝔅Fp^){\mathcal{C}}^{\infty}(\mathfrak{B}_{F_{\widehat{p}}}) for each p^\widehat{p} fixed. In particular, since the kernels of these operators are smooth up to the front face, it makes sense to consider their Taylor series on 𝔅Fp^\mathfrak{B}_{F_{\widehat{p}}}. The surjectivity of Np^()N_{\widehat{p}}(-) thus arises from a version of Borel’s lemma for the Taylor series of Np^()N_{\widehat{p}}(-) in local coordinates for 𝔅Fp^\mathfrak{B}_{F_{\widehat{p}}}.

To prove the composition formula, we can use the structure of the Normal operator at 𝔅F\mathfrak{B}_{F}, and the fact that we are not blowing up in the tt variable, so it commutes with the normal operator.

We observe first that such a PDiffΘm(X)P\in\text{Diff}_{\Theta}^{m}(X) can be written with respect to our frame {ρρ,ρVwi,ρ2z}\{\rho\partial_{\rho},\rho V_{w_{i}},\rho^{2}\partial_{z}\} for TΘM{}^{\Theta}TM:

P=j+|α|+kmajαk(ρ,w,z)(ρρ)j(ρVw)α(ρ2z)k\displaystyle P=\sum_{j+|\alpha|+k\leq m}a_{j\alpha k}(\rho,w,z)(\rho\partial_{\rho})^{j}(\rho V_{w})^{\alpha}(\rho^{2}\partial_{z})^{k}
\displaystyle\implies Np^(P)=j+|α|+kmajαk(0,w,z)(ρρ)j(ρVw)α(ρ2z)k.\displaystyle N_{\widehat{p}}(P)=\sum_{j+|\alpha|+k\leq m}a_{j\alpha k}(0,w,z)(\rho\partial_{\rho})^{j}(\rho V_{w})^{\alpha}(\rho^{2}\partial_{z})^{k}.

As usual we choose to identify this as acting on 1/21/2-densities: if we choose coordinates (ρ,w,z)(\rho,w,z), these induce a trivialization of the square root of the Θ\Theta-density bundle ΩΘ1/2=Ω1/2\Omega_{\Theta}^{1/2}=\Omega^{1/2}

γ=(ρ)(2n+3)|dρdwdz|1/2\gamma=(\rho)^{-(2n+3)}\left|d\rho dwdz\right|^{1/2}

and PP acts on f𝒞(X;ΩΘ1/2)f\in{\mathcal{C}}^{\infty}(X;\Omega_{\Theta}^{1/2}) by Pf=P(fγ1)γPf=P(f\gamma^{-1})\gamma. Of course this is simply for Θ\Theta-differential operators. More generally Θ\Theta-FIOs will act on 1/21/2-densities via their normal operator: Np^(A)=(ρFs𝒦A)|𝔅Fp^N_{\widehat{p}}(A)=(\rho_{F}^{-s}\mathcal{K}_{A})|_{\mathfrak{B}_{F_{\widehat{p}}}}

(Btf)(ρ,w,z)γ=𝔅Fp𝒦Bt(0,w,z;V,W,Z)f(ρV,wρVW,z(ρV)2Z)dVdWdZVγ(B_{t}f)(\rho,w,z)\cdot\gamma=\int_{\mathfrak{B}_{F_{p}}}\mathcal{K}_{B_{t}}(0,w,z;V,W,Z)f\left(\frac{\rho}{V},w-\frac{\rho}{V}W,z-\left(\frac{\rho}{V}\right)^{2}Z\right)\frac{dVdWdZ}{V}\cdot\gamma

In particular, this implies that the normal operator of PBP\circ B

Np^(PB)=(j+|α|+kmajαk(0,w,z)(ρρ)j(ρVw)α(ρ2z)k(𝒦Bt(0,w,z;V,W,Z)))γN_{\widehat{p}}(P\circ B)=\left(\sum_{j+|\alpha|+k\leq m}a_{j\alpha k}(0,w,z)(\rho\partial_{\rho})^{j}(\rho V_{w})^{\alpha}(\rho^{2}\partial_{z})^{k}\circ\left(\mathcal{K}_{B_{t}}(0,w,z;V,W,Z)\right)\right)\cdot\gamma

Having proven this lemma, we arrive at a short time parametrix for the wave group.

Proposition 3.5.


For each tt\in\mathbb{R}, for the canonical relation

C={[(t,τ),\displaystyle C=\{[(t,\tau), (ρ,w,z;μ,u,s),(ρ,w,z;μ,u,s)]:\displaystyle(\rho,w,z;\mu,u,s),(\rho^{\prime},w^{\prime},z^{\prime};\mu^{\prime},u^{\prime},s^{\prime})]:
τ+G(ρ,w,z;μ,u,s)=0;(ρ,w,z;μ,u,s)=exp(tHGΘ)(ρ,w,z;μ,u,s)}\displaystyle\tau+\sqrt{G(\rho,w,z;\mu,u,s)}=0\;;\;\;(\rho^{\prime},w^{\prime},z^{\prime};\mu^{\prime},u^{\prime},s^{\prime})=\emph{exp}(t{}^{\Theta}H_{G})(\rho,w,z;\mu,u,s)\}

the wave group U(t)U(t) is Θ\Theta-Fourier integral operator of the class

U(t)=cos(tΔgn2/4)IΘ1/4,0(×X,X;C,Ω1/2Θ)U(t)=\cos\left(t\sqrt{\Delta_{g}-n^{2}/4}\right)\in I_{\Theta}^{-1/4,0}(\mathbb{R}\times X,X;C,{}^{\Theta}\Omega^{1/2})
Proof.

Given the normal sequence, the argument reduces to a purely local one: using proposition 3.4, and the fact that

Np^(Id)=δ(V1)δ(W)δ(Z)γ=δ(0p)γN_{\widehat{p}}(\operatorname{Id})=\delta(V-1)\delta(W)\delta(Z)\gamma=\delta(0_{p})\gamma

we can take as ansatz U0(t,p^)=Np^(U(t))U_{0}(t,\widehat{p})=N_{\widehat{p}}(U(t)) the wave group in this fiber 𝔅Fp^\mathfrak{B}_{F_{\widehat{p}}}:

{(Dt2+Np^(Δg)n24)U0(t,p^)=0U(0,p^)=δ(0p^),tU(0,p^)=0\begin{cases}\left(D_{t}^{2}+N_{\widehat{p}}(\Delta_{g})-\tfrac{n^{2}}{4}\right)U_{0}(t,\widehat{p})=0\\ U(0,\widehat{p})=\delta(0_{\widehat{p}}),\quad\partial_{t}U(0,\widehat{p})=0\end{cases}

here 0p^𝔅Fp^𝕏p^0_{\widehat{p}}\in\mathfrak{B}_{F_{\widehat{p}}}\simeq\mathbb{X}_{\widehat{p}} corresponds to the identity element in the group. Note also that the specific form of the model Laplacian

Np^(Δg)=14(ρρ)2+n+12ρρ+ρ2ΔH(p^)ρ4Z2(p^)N_{\widehat{p}}(\Delta_{g})=-\tfrac{1}{4}(\rho\partial_{\rho})^{2}+\tfrac{n+1}{2}\rho\partial_{\rho}+\rho^{2}\Delta_{H}(\widehat{p})-\rho^{4}Z^{2}(\widehat{p})

means we can also construct the model wave group, and study its asymptotics via analyzing those of the wave group in n+1\mathbb{H}_{\mathbb{C}}^{n+1}.

Since 0p^Int(𝔅Fp^)0_{\widehat{p}}\in\text{Int}(\mathfrak{B}_{F_{\widehat{p}}}), it does not meet the corners of 𝔅Fp^\mathfrak{B}_{F_{\widehat{p}}}. Similarly ΛC\Lambda_{C} does not meet the corners in finite time, so we can follow the argument of Duistermaat-Guillemin prop 1.1 to conclude U0(t)I1/4(×𝔅F;ΛCΘ,Ω)U_{0}(t)\in I^{-1/4}(\mathbb{R}\times\mathfrak{B}_{F};\Lambda_{C}^{\Theta},\Omega)

Now we iterate. Choose a u0IΘ1/4,0(X×,X;C,Ω1/2Θ)u_{0}\in I_{\Theta}^{-1/4,0}(X\times\mathbb{R},X;C,{}^{\Theta}\Omega^{1/2}) such that Np^(u0)=U0(t)N_{\widehat{p}}(u_{0})=U_{0}(t). Then

βL(Dt2+Δgn2/4)(U(t)u0)=r0IΘ1/4,1(X×,X;C,Ω1/2Θ)\beta_{L}^{*}(D_{t}^{2}+\Delta_{g}-n^{2}/4)(U(t)-u_{0})=r_{0}\in I_{\Theta}^{-1/4,1}(X\times\mathbb{R},X;C,{}^{\Theta}\Omega^{1/2})

and ρ1r0I1/4,0\rho^{-1}r_{0}\in I^{-1/4,0} where ρ\rho is a defining function for the left face. (This is well-defined since r0r_{0} is supported away from the left face, as u0u_{0} was, and the wave operator preserves this support due to the condition on wave front of U0U_{0}, via [Hör71, Thm 2.5.15]). Now we solve the inhomogeneous wave equation to find a u1IΘ1/4,0u_{1}\in I_{\Theta}^{-1/4,0} solving

{(Dt2+Np^(Δg)n24)Np^(u1)=Np^(ρ1r0)Np^(u1)|t=0=Np^(ρ1r0),tNp^(u1)|t=0=tNp^(ρ1r0)|t=0\begin{cases}\left(D_{t}^{2}+N_{\widehat{p}}(\Delta_{g})-\tfrac{n^{2}}{4}\right)N_{\widehat{p}}(u_{1})=N_{\widehat{p}}(\rho^{-1}r_{0})\\ N_{\widehat{p}}(u_{1})|_{t=0}=N_{\widehat{p}}(\rho^{-1}r_{0}),\quad\partial_{t}N_{\widehat{p}}(u_{1})|_{t=0}=\partial_{t}N_{\widehat{p}}(\rho^{-1}r_{0})|_{t=0}\end{cases}

solving as before we obtain such a u1u_{1}. We now have βL(Dt2+Δgn2/4)(U(t)u0ρu1)=r1IΘ1/4,2\beta_{L}^{*}(D_{t}^{2}+\Delta_{g}-n^{2}/4)(U(t)-u_{0}-\rho u_{1})=r_{1}\in I_{\Theta}^{-1/4,-2}.

Proceeding iteratively we obtain Uj0ρjujU_{\infty}\sim\sum_{j\geq 0}\rho^{j}u_{j} such that βL(Dt2+Δgn2/4)U\beta_{L}^{*}(D_{t}^{2}+\Delta_{g}-n^{2}/4)U_{\infty} vanishes to infinite order at 𝔅F\mathfrak{B}_{F}. The error term also has infinite order vanishing at 𝔅F\mathfrak{B}_{F} in the Cauchy data from the construction. Finally, after extending this error term to be identically zero across the front face, we can use Hörmander’s transverse intersection calculus to remove this error term (see e.g. [Hör71, Thm 2.5.15]). ∎

Unfortunately, this is a short time parametrix, as this construction is only valid for finite tt. If we allow tt\to\infty, our Lagrangian flow-out Λ(t)\Lambda(t) will meet the corners of 𝔅F\mathfrak{B}_{F}, which would require a more sophisticated composition formula.

4. Wave Trace Asymptotics

Now that we know the wave group is a Θ\Theta-Fourier integral operator we can ask whether its trace can be studied, as in the case of the wave trace on a compact manifold without boundary. This presents some technical difficulties, since the operator cos(tΔg(n+1)24)\cos\left(t\sqrt{\Delta_{g}-\tfrac{(n+1)^{2}}{4}}\right) is not trace class, so we need to introduce a regularization of its trace.

Heuristically, our goal is to study the trace,

TrU(t)=X¯diagU(t,x,x)dVolg=ΠιdiagU\operatorname{Tr}U(t)=\int_{\overline{X}_{\operatorname{diag}}}U(t,x,x)\;d\operatorname{Vol}_{g}=\Pi_{\ast}\iota_{\operatorname{diag}}^{*}U (4.1)

using appropriate maps ιdiag,Π\iota_{\operatorname{diag}},\Pi, to define this integral via pullback and pushforward. An analysis of the wavefront sets of these maps will permit an analysis of their associated operators, and prove that the resulting object is well-defined distribution on \mathbb{R}, with wavefront set to be determined.

First, notice that for all p,pX¯p,p^{\prime}\not\in\partial\overline{X}, the restriction of U(t,p,p)U(t,p,p^{\prime}) to the diagonal X¯diag\overline{X}_{\operatorname{diag}} is well-defined. To see this we proceed as in [DuGu75, §1] by introducing the map,

ιdiag:×X¯diag×X¯×X¯,(t,p)(t,p,p)\iota_{\operatorname{diag}}:\mathbb{R}\times\overline{X}_{\operatorname{diag}}\to\mathbb{R}\times\overline{X}\times\overline{X},\quad(t,p)\mapsto(t,p,p)

of the inclusion of the diagonal. Pullback along this map is a Fourier integral operator of order n+12\tfrac{n+1}{2}, defined by the canonical relation

WF(ιdiag)={(((t,τ),(p,ζ+ζ)),((t,τ),(p,ζ),(p,ζ)))}=N{ιdiag(t,p)=(t,p,p)}.\text{WF}^{\prime}(\iota_{\operatorname{diag}}^{*})=\left\{\big{(}((t,\tau),(p,\zeta+\zeta^{\prime})\big{)},\;\big{(}(t,\tau),(p,\zeta),(p,\zeta^{\prime}))\big{)}\right\}=N^{*}\{\iota_{\operatorname{diag}}(t,p)=(t,p,p^{\prime})\}.

Now, using the fact that WF(U)=C\text{WF}(U)=C (as defined in proposition 3.5), assuming p,pX¯p,p^{\prime}\not\in\partial\overline{X}, then whenever ((t,τ),(p,ζ),(p,ζ))WF(U)((t,\tau),(p,\zeta),(p,\zeta^{\prime}))\in\text{WF}^{\prime}(U) we have τ0\tau\neq 0, thus WF(U)Nιdiag=\text{WF}(U)\cap N_{\iota_{\operatorname{diag}}}=\emptyset at such points (where Nιdiag={(ι(t,p),τ,ζ,ζ)T(×X¯×X¯):Dιdiag(τ,ζ,ζ)=0}N_{\iota_{\operatorname{diag}}}=\{(\iota(t,p),\tau,\zeta,\zeta^{\prime})\in T^{*}(\mathbb{R}\times\overline{X}\times\overline{X}):D\iota_{\operatorname{diag}}^{\intercal}(\tau,\zeta,\zeta^{\prime})=0\} is the set of normals of the map). Thus we can apply [Hör71, Thm 2.5.112.5.11^{\prime}] to conclude that ιdiagU\iota_{\operatorname{diag}}^{*}U is a well-defined distribution on ×(X¯X¯)\mathbb{R}\times(\overline{X}\setminus\partial\overline{X}) with wavefront set

WF(ιdiagU)={((t,τ),(p,ζζ)):τ+G(p,ζ)=0,(p,ζ)=exp(tHGΘ)(p,ζ)}.\text{WF}^{\prime}(\iota_{\operatorname{diag}}^{*}U)=\{((t,\tau),(p,\zeta-\zeta^{\prime})):\tau+\sqrt{G(p,\zeta)}=0,\;(p,\zeta)=\text{exp}(t{}^{\Theta}H_{G})(p,\zeta^{\prime})\}.

Duistermaat-Guillemin next study the wavefront set of the projection Π:×X¯\Pi:\mathbb{R}\times\overline{X}\to\mathbb{R}. In our case we now introduce the regularization procedure. For ε>0\varepsilon>0, define X¯ε={ρ>ε}\overline{X}_{\varepsilon}=\{\rho>\varepsilon\} for our bdf ρ\rho. Consider the cutoff projection

Πε:×X¯ε,(t,p)t,\Pi_{\varepsilon}:\mathbb{R}\times\overline{X}_{\varepsilon}\to\mathbb{R},\quad(t,p)\mapsto t,

for which integration over the range pp is equal to the pushforward along Πε\Pi_{\varepsilon} (the transpose of the operator Π\Pi^{*}). This map thus defines a Fourier integral operator of order 12n+12\tfrac{1}{2}-\tfrac{n+1}{2} defined by the canonical relation

WF(Π)={((t,τ),((t,τ),(x,0)))}.\text{WF}^{\prime}(\Pi_{*})=\left\{\big{(}(t,\tau),\;((t,\tau),(x,0))\big{)}\right\}.

Again applying Hörmander’s Theorem [Hör71, Thm 2.5.112.5.11^{\prime}] we can conclude that the cutoff wave trace

Tε(t)=ρ>εU(t,p,p)=(Πε)(ιdiagU(t))T_{\varepsilon}(t)=\int_{\rho>\varepsilon}U(t,p,p)=(\Pi_{\varepsilon})_{*}(\iota_{\operatorname{diag}}^{*}U(t))

is a well-defined distribution on \mathbb{R} satisfying

WF(Tε(t))={(t,τ):τ<0and (p,ζ)=exp(tHGΘ)(p,ζ) for some (p,ζ),ρ(p)>ε}.\text{WF}(T_{\varepsilon}(t))=\{(t,\tau):\tau<0\;\text{and }(p,\zeta)=\text{exp}(t\;{}^{\Theta}H_{G})(p,\zeta^{\prime})\text{ for some }(p,\zeta),\;\rho(p)>\varepsilon\}.

We obtain as a corollary

Corollary 4.1.

For ε>0\varepsilon>0, the singular support of Tε𝒟()T_{\varepsilon}\in\mathcal{D}^{\prime}(\mathbb{R}) is contained in the set of periods of closed geodesics in X¯ε\overline{X}_{\varepsilon}. Moreover, there exists ε0>0\varepsilon_{0}>0 such that all closed geodesics of (X,g)(X,g) with period greater than zero are contained in X¯ε0\overline{X}_{\varepsilon_{0}}.

In particular for all ε<ε0\varepsilon<\varepsilon_{0}, the singular support of TεT_{\varepsilon} is contained in the set of period of closed geodesics of XX.

Proof.

Only the claim regarding closed geodesics remaining in X¯ε0\overline{X}_{\varepsilon_{0}} remains to be proven. This is a statement about strict convexity of the geodesic flow in a neighborhood of infinity (see e.g. [JoSá01, Proposition 4.1], [DaVa12, Lemma 4.1]). We show that if ε\varepsilon sufficiently small, any geodesic γ\gamma which intersects {ρ<ε}\{\rho<\varepsilon\} cannot be closed. Introducing coordinates (ρ,w,z)(\rho,w,z) with corresponding dual coordinates (ξ,ηH,ηV)(\xi,\eta_{H},\eta_{V}), such that ρ\rho is a boundary defining function for X¯\partial\overline{X}.

In these coordinates, we write the metric in a collar neighborhood of the boundary as

g=4dρ2+g~ρρ2,g~ρ=h+ρ2θ2g=\frac{4d\rho^{2}+\widetilde{g}_{\rho}}{\rho^{2}},\quad\widetilde{g}_{\rho}=h_{\mathscr{H}}+\rho^{-2}\theta^{2}

and we write

Gρ(η,η)=h(ηH,ηH)+ρ2θ2(ηV,ηV)G_{\rho}(\eta,\eta)=h_{\mathscr{H}}(\eta_{H},\eta_{H})+\rho^{2}\theta^{2}(\eta_{V},\eta_{V})

for the bilinear form on TXT^{*}X induced by the dual metric of g~ρ\widetilde{g}_{\rho}. In these coordinates the geodesic Hamiltonian is given by

|ζ|g2=σ2+G¯(μ,μ)=σ2+h(μH,μH)+θ2(μV,μV)|\zeta|_{g}^{2}=\sigma^{2}+\overline{G}(\mu,\mu)=\sigma^{2}+h_{\mathscr{H}}(\mu_{H},\mu_{H})+\theta^{2}(\mu_{V},\mu_{V})

where σ=ρξ,μH=ρηH,μV=ρ2ηV\sigma=\rho\xi,\mu_{H}=\rho\eta_{H},\mu_{V}=\rho^{2}\eta_{V}, and G¯=ρ2Gρ\overline{G}=\rho^{2}G_{\rho}. The Hamilton vector field of this function is given by

H|ζ|g2=ξ|ζ|2ρρ|ζ|2ξ+(ηH|ζ|2)Y(Y|ζ|2)ηH+(ηV|ζ|2)z(z|ζ|2)ηVH_{|\zeta|_{g}^{2}}=\partial_{\xi}|\zeta|^{2}\partial_{\rho}-\partial_{\rho}|\zeta|^{2}\partial_{\xi}+(\partial_{\eta_{H}}|\zeta|^{2})\cdot Y-(Y|\zeta|^{2})\cdot\partial_{\eta_{H}}+(\partial_{\eta_{V}}|\zeta|^{2})\partial_{z}-(\partial_{z}|\zeta|^{2})\partial_{\eta_{V}}

where {Yj}j=12n\{Y_{j}\}_{j=1}^{2n} is a local hh_{\mathscr{H}}-orthonormal frame dual to {dηHj}j=12n\{d\eta_{H}^{j}\}_{j=1}^{2n}. Computing the change in these vector fields with respect to the change of coordinates (ρ,w,z,ξ,ηH,ηV)(ρ,w,z,σ,μH,μV)(\rho,w,z,\xi,\eta_{H},\eta_{V})\mapsto(\rho,w,z,\sigma,\mu_{H},\mu_{V}) gives

ξ=ρσ,ηH=ρμH,ηV=ρ2μV,\partial_{\xi}=\rho\partial_{\sigma},\;\partial_{\eta_{H}}=\rho\partial_{\mu_{H}},\;\partial_{\eta_{V}}=\rho^{2}\partial_{\mu_{V}},
ρ=ρ+ρ1σσ+ρ1(μHμH+2μVμV),Y=Y,z=z.\partial_{\rho}=\partial_{\rho}+\rho^{-1}\sigma\partial_{\sigma}+\rho^{-1}(\mu_{H}\cdot\partial_{\mu_{H}}+2\mu_{V}\partial_{\mu_{V}}),\;Y=Y,\;\partial_{z}=\partial_{z}.

Thus the Hamilton vector field can be re-expressed as

H|ζ|2\displaystyle H_{|\zeta|^{2}} =(ρσ|ζ|2)(ρ+ρ1CC)(ρρ+CC)(|ζ|2)σ+ρ[(μH|ζ|2)Y(Y|ζ|2)μH]\displaystyle=(\rho\partial_{\sigma}|\zeta|^{2})(\partial_{\rho}+\rho^{-1}\mathcal{R}_{CC})-(\rho\partial_{\rho}+\mathcal{R}_{CC})(|\zeta|^{2})\partial_{\sigma}+\rho[(\partial_{\mu_{H}}|\zeta|^{2})\cdot Y-(Y|\zeta|^{2})\cdot\partial_{\mu_{H}}]
+ρ2[(μV|ζ|2)z(z|ζ|2)μV]\displaystyle\quad\quad+\rho^{2}[(\partial_{\mu_{V}}|\zeta|^{2})\partial_{z}-(\partial_{z}|\zeta|^{2})\partial_{\mu_{V}}]

where we have defined CC=μHμH+2μVμV\mathcal{R}_{CC}=\mu_{H}\cdot\partial_{\mu_{H}}+2\mu_{V}\partial_{\mu_{V}}, the infinitesimal generator of the Heisenberg dilation action on TX¯T^{*}\partial\overline{X}. Using the facts that

σ|ζ|2=2σ,CC|ζ|2=2G¯(μ,μ),\partial_{\sigma}|\zeta|^{2}=2\sigma,\quad\mathcal{R}_{CC}|\zeta|^{2}=2\overline{G}(\mu,\mu),

and writing the vector field Hg~ρ=[(μH|ζ|2)Y(Y|ζ|2)μH]+ρ[(μV|ζ|2)z(z|ζ|2)μV]H_{\widetilde{g}_{\rho}}=[(\partial_{\mu_{H}}|\zeta|^{2})\cdot Y-(Y|\zeta|^{2})\cdot\partial_{\mu_{H}}]+\rho[(\partial_{\mu_{V}}|\zeta|^{2})\partial_{z}-(\partial_{z}|\zeta|^{2})\partial_{\mu_{V}}], we can re-express this formula as

H|ζ|2=2σρρ+2σCC(2G¯(μ,μ)+ρρG¯)σ+ρHg~ρ.H_{|\zeta|^{2}}=2\sigma\rho\partial_{\rho}+2\sigma\mathcal{R}_{CC}-(2\overline{G}(\mu,\mu)+\rho\partial_{\rho}\overline{G})\partial_{\sigma}+\rho\cdot H_{\widetilde{g}_{\rho}}.

Thus, along integral curves of the vector field H|ζ|2H_{|\zeta|^{2}} we have ρ˙=2σρ,τ˙=(2G¯+ρρG¯)\dot{\rho}=2\sigma\rho,\dot{\tau}=-(2\overline{G}+\rho\partial_{\rho}\overline{G}). Thus, at a critical point of ρ\rho along the flow which is an interior point of XX we have

ρ˙=0σ=0,\dot{\rho}=0\implies\sigma=0,

hence at such points we have

ρ¨=0+2σ˙ρ=2ρ(2G¯+ρρG¯)=4ρG¯2ρ2ρG¯.\ddot{\rho}=0+2\dot{\sigma}\rho=-2\rho(2\overline{G}+\rho\partial_{\rho}\overline{G})=-4\rho\overline{G}-2\rho^{2}\partial_{\rho}\overline{G}.

Now, using the fact that G¯|ρ=0\overline{G}|_{\rho=0} is positive definite, thus for sufficiently small ρ\rho this quantity is negative. Thus we have shown that for all geodesic curves γ\gamma which intersect {ρε}\{\rho\leq\varepsilon\} satisfy,

ρ˙γ=0ρ¨γ<0.\dot{\rho}\circ\gamma=0\implies\ddot{\rho}\circ\gamma<0.

Now, assuming for the sake of contradiction that γ\gamma is closed. Then there exists δ(0,ε)\delta\in(0,\varepsilon) such that γ\gamma intersects {ρ=δ}\{\rho=\delta\} in at least two points. Therefore there exists a s0s_{0} with ργ(s0)>0\rho\circ\gamma(s_{0})>0 where ργ\rho\circ\gamma has a minimum. However at such a minimum we have ρ˙γ(s0)=0\dot{\rho}\circ\gamma(s_{0})=0 and ρ¨γ(s0)>0\ddot{\rho}\circ\gamma(s_{0})>0, contradicting our convexity statement. ∎

Using this corollary, we can now begin an analysis of the renormalized wave trace. If we denote by ujIΘ1/4,j(×X,X;C,Ω1/2Θ)u_{j}\in I_{\Theta}^{-1/4,j}(\mathbb{R}\times X,X;C,{}^{\Theta}\Omega^{1/2}) be the operators defined in the proof of proposition 3.5. The same arguments used above can be used to show that the distribution

Ij(t,ε)=ρ>ερjuj(t,p,p)I_{j}(t,\varepsilon)=\int_{\rho>\varepsilon}\rho^{j}u_{j}(t,p,p)

is well-defined, with singular support satisfying the conclusions of corollary 4.1. Since 𝔅F\mathfrak{B}_{F} and ΛC\Lambda_{C} intersect transversally, only the density factor implicit in this operator can obstruct the convergence of Ij(t,ε)I_{j}(t,\varepsilon) as ε0\varepsilon\to 0. Since this density, a trivialization of the Ω1/2Θ{}^{\Theta}\Omega^{1/2}-bundle, diverges at the rate ρ(2n+3)\rho^{-(2n+3)} at X¯\partial\overline{X}, the integrals Ij(t,ε)I_{j}(t,\varepsilon) converges for any j2n+3j\geq 2n+3. Applying Taylor’s Theorem to uj(t,p,p)u_{j}(t,p,p) as ρ0\rho\to 0, we see that there exists constants CjC_{j} such that the limit

TrRU(t)=limε0[ρ>εU(t,p,p)j=2n21Cjεj+C0log(1ε)]{}^{R}\operatorname{Tr}U(t)=\lim_{\varepsilon\to 0}\left[\int_{\rho>\varepsilon}U(t,p,p)-\sum_{j=-2n-2}^{-1}C_{j}\varepsilon^{j}+C_{0}\log(\tfrac{1}{\varepsilon})\right]

exists, which we call the renormalized wave trace. From corollary 4.1, we immediately obtain

Proposition 4.2.

The singular support of TrRU(t){}^{R}\operatorname{Tr}U(t) is contained in the set of periods of closed geodesics of (X,g)(X,g).

Finally, we can begin our analysis of the renormalized wave trace as t0t\to 0 (in fact its inverse Fourier transform). First we choose a cutoff function χ𝒞c()\chi\in{\mathcal{C}}^{\infty}_{c}(\mathbb{R}), with the appropriate support to study the transform of the cutoff wave trace. If we denote the first non-zero period of a closed geodesic on (X,g)(X,g) as t0t_{0}, then choose χ\chi such that χ(t)=1\chi(t)=1 for |t|>t02|t|>\tfrac{t_{0}}{2} and χ(t)0\chi(t)\equiv 0 for |t|>2t03|t|>\tfrac{2t_{0}}{3}.

Now, using the arguments of [Hö68], (which are purely local, applying to any paracompact manifold), or alternatively the proof of [DuGu75, Prop 2.1], we immediately obtain

Proposition 4.3.

There exists coefficients {wk}k0\{w_{k}\}_{k\in\mathbb{N}_{0}}\subset\mathbb{R} such that the cutoff wave trace Tε(t)T_{\varepsilon}(t) satisfies,

Tε(t)χ(t)etμ𝑑t1(2π)2n+2k=0wkμ2n+22k,\int_{\mathbb{R}}T_{\varepsilon}(t)\chi(t)e^{t\mu}dt\sim\frac{1}{(2\pi)^{2n+2}}\sum_{k=0}^{\infty}w_{k}\mu^{2n+2-2k}, (4.2)

as μ0\mu\to 0 and rapidly decaying as μ\mu\to-\infty. The leading term, ω0=Volg(X¯ε)\omega_{0}=\operatorname{Vol}_{g}(\overline{X}_{\varepsilon})

Given this result for the asymtotics of the cutoff wave trace Tε(t)T_{\varepsilon}(t) we can then conclude similarly for the full wave trace 4.1 that

Theorem 4.4.

There exists coefficients {ωk}k0\{\omega_{k}\}_{k\in\mathbb{N}_{0}}\subset\mathbb{R} such that the renormalized trace TrRU(t){}^{R}\operatorname{Tr}U(t) satisfies,

TrRU(t)χ(t)etμ𝑑t1(2π)2n+2k=0ωkμ2n+22k,\int_{\mathbb{R}}{}^{R}\operatorname{Tr}U(t)\chi(t)e^{t\mu}dt\sim\frac{1}{(2\pi)^{2n+2}}\sum_{k=0}^{\infty}\omega_{k}\mu^{2n+2-2k},

as μ0\mu\to 0 and rapidly decaying as μ\mu\to-\infty. The leading term, ω0=VolgR(X)\omega_{0}={}^{R}\operatorname{Vol}_{g}(X), is called the renormalized volume, and can be computed as

VolgR(X)=limε0[{ρ>ε}dVolgj=2n21djεjd0log(1ε)],{}^{R}\operatorname{Vol}_{g}(X)=\lim_{\varepsilon\to 0}\left[\int_{\{\rho>\varepsilon\}}d\operatorname{Vol}_{g}-\sum_{j=-2n-2}^{-1}d_{j}\varepsilon^{j}-d_{0}\log(\tfrac{1}{\varepsilon})\right], (4.3)

where the djd_{j} are the unique real numbers such that this limit exists.

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