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Obstructions to a chirality index for frame-free Weyl operators

Status
Lemma 1, Theorems 1 and 2, Corollary 1 and Propositions 3 and 4 proved in any dimension. Propositions 1, 2, 5 and 6 (mean symbol, boost covariance, row noise, smearing) proved for one two-dimensional kernel. Computed in two dimensions: the Euclidean overlap index (twelve cases), eigenvalues near the imaginary axis on a 72-point diamond, and a propagation table.
Excludes
A nonzero overlap index for a retarded operator with chirally even on-site part, or for an operator self-adjoint for a chirality-exchanging involution (for example a Hermitian or anti-Hermitian Weyl block with a Hermitian chirally even Wilson term); a bulk-sensitive integer from the finite boundary-projected index of Proposition 3. Chirally asymmetric Wilson terms are not excluded.
Revised

A Weyl fermion on a lattice or on a random point set is certified chiral by an integer: the index of a Ginsparg–Wilson (overlap) Dirac operator, the number of zero modes of one handedness minus those of the other, which in a gauge field equals the flux through a torus up to sign. We ask whether such an integer exists for an operator on a Poisson sprinkling in Minkowski space that is built from the causal order and the invariant interval alone, so that no preferred frame enters. For two classes of operator, with any weights on any finite causal set, it is zero or undefined: the retarded operators, supported on pairs of points in causal order (Theorem 1), and the operators self-adjoint for a matrix that exchanges the two chiralities, which include those whose off-diagonal (Weyl) block is Hermitian or anti-Hermitian (Theorem 2 and Corollary 1). Both statements are made for a Wilson term, which gives the doublers a mass, that acts identically on the two chiralities.

For retarded operators only the on-site part of the Wilson term enters, and Theorem 2 asks only that the whole operator be self-adjoint for the exchanging matrix, which holds for the Wilson-term part if that term is Hermitian and acts identically on both chiralities. A third construction, an index defined by projecting initial and final data onto spectral subspaces of boundary operators on finite antichains (sets of mutually unrelated points), gives an integer that is generally nonzero but depends on the boundary operators alone (Proposition 3). A product with an internal point set whose overlap operator has zero modes, for example a flux torus, gives copies of a retarded block whose grading is set by those zero modes, so that the chirality of the product is carried by the internal factor (Proposition 4). The proofs are finite-dimensional linear algebra and use neither the sprinkling nor a frame. The two classes are defined algebraically; the signed Benincasa–Dowker kernel of Definition 1, which is frame-free, falls in the first, and its symmetrisation (Section 4) in the second. A Euclidean overlap operator on a Poisson torus shows the expected index in the twelve cases we computed (Example 1), at the price of a choice of Euclidean time axis.

The overlap construction is due to Neuberger [N1], [N2] and gives an exact solution of the Ginsparg–Wilson relation [GW]. Lüscher showed that the relation yields an exact index theorem on the lattice [L]. Lorentz-invariant retarded kernels on causal sets were constructed by Aslanbeigi, Saravani and Sorkin [ASS], and Bombelli, Henson and Sorkin proved that a sprinkling carries no preferred direction and no finite-valency graph [BHS]. In the continuum, Bär and Strohmaier proved an index theorem for the Lorentzian Dirac operator on a compact globally hyperbolic region, with Atiyah–Patodi–Singer conditions on the two spacelike boundaries [BS], and a lattice version of the Atiyah–Patodi–Singer index has been given through the eta invariant of a domain-wall operator [F]. Kimura and Watanabe built the overlap operator for each symmetry class of the tenfold way and established the Ginsparg–Wilson relation for the charge-conjugation and time-reversal symmetries and a mod-two index theorem [KW].

The theorems and Propositions 3 and 4 of Sections 2 to 6 hold in every dimension. Sections 1 and 7 concern the two-dimensional kernel of Definition 1, and Propositions 1, 2, 5 and 6, Example 1, the numerical statements and the symbol paragraph of Section 4 refer to two dimensions.

1. The frame-free retarded Weyl operator

Let P\mathcal P be a Poisson process of density ρ\rho in two-dimensional Minkowski space, ordered by y≺xy\prec x when x−yx-y is future timelike. In null coordinates u=t−xu=t-x, v=t+xv=t+x one has dt dx=12 du dvdt\,dx=\tfrac12\,du\,dv, and y≺xy\prec x exactly when U=ux−uy>0U=u_x-u_y>0 and V=vx−vy>0V=v_x-v_y>0. A boost of rapidity ξ\xi multiplies (U,V)(U,V) by (e−ξ,eξ)(e^{-\xi},e^{\xi}). For y≺xy\prec x let nxyn_{xy} be the number of points of P\mathcal P strictly between yy and xx. The pair (nxy,(U,V))(n_{xy},(U,V)) is what we call frame-free: the count is a property of the order, and the null displacements are only rescaled by a boost. No timelike unit vector is used.

Definition 1 (signed-BD retarded Weyl operator). Let w0=1w_0=1, w1=−2w_1=-2, w2=1w_2=1 and wn=0w_n=0 for n≥3n\ge 3. These are the layer coefficients of the two-dimensional Benincasa–Dowker d’Alembertian, in the convention of mixed-Poisson and signed substrates. Only the coefficients are used, so the signature and the overall sign of the d’Alembertian do not enter. For a point set P\mathcal P with NN elements put, for y≺xy\prec x,

D+[x,y]=ρ wnxy (ux−uy),D−[x,y]=ρ wnxy (vx−vy),D_+[x,y]=\rho\,w_{n_{xy}}\,(u_x-u_y),\qquad D_-[x,y]=\rho\,w_{n_{xy}}\,(v_x-v_y),

and zero when y⊀xy\not\prec x. On CN⊗C2\mathbb C^N\otimes\mathbb C^2, with the two components called RR and LL and γ5=diag(1,−1)\gamma_5=\mathrm{diag}(1,-1), the retarded Dirac operator is D=(0D+D−0)D=\begin{pmatrix}0&D_+\\ D_-&0\end{pmatrix}. A smeared version replaces wnw_{n} by ε2f(n,ε)\varepsilon^2 f(n,\varepsilon) with f(n,ε)=∑kwk(nk)εk(1−ε)n−kf(n,\varepsilon)=\sum_k w_k\binom nk\varepsilon^k(1-\varepsilon)^{n-k}, the Poisson-thinning form of the generalised causal-set d’Alembertians of [ASS]. The value ε=1\varepsilon=1 is the unsmeared operator.

The operator D+D_+ is meant to approximate ∂v\partial_v and D−D_- to approximate ∂u\partial_u. The weights are chosen so that the Poisson average of wnw_n over the number of points in an interval of mean size z=ρUV/2z=\rho UV/2, namely f0(z)=e−z(1−2z+z2/2)f_0(z)=e^{-z}(1-2z+z^2/2), has vanishing zeroth and first moments, ∫0∞f0 dz=∫0∞zf0 dz=0\int_0^\infty f_0\,dz=\int_0^\infty zf_0\,dz=0. Without this cancellation the sum over the past of a point does not converge. The zeroth moment gives ∫f0(ρUV/2) dV=0\int f_0(\rho UV/2)\,dV=0 at fixed UU, so in mean D+D_+ annihilates every function of uu alone, as ∂v\partial_v does. The first moment makes the VV-integral against e−ikvVe^{-ik_vV} vanish quadratically in kv/(ρU)k_v/(\rho U) at large UU. The term linear in kvk_v comes from the region U∼kv/ρU\sim k_v/\rho, and Proposition 1 gives its coefficient exactly, in the limit in which the region is large compared with the discreteness scale ρ−1/2\rho^{-1/2}. The computation uses the Mecke formula, E∑y∈Pg(y,P)=ρ∫E g(y,P∪{y}) dy\mathbb E\sum_{y\in\mathcal P}g(y,\mathcal P)=\rho\int\mathbb E\,g(y,\mathcal P\cup\{y\})\,dy [LP]. Applied to the points xx and yy, it says that, given points at xx and y≺xy\prec x, the number of other points in the order interval between them is Poisson with mean ρUV/2\rho UV/2.

Proposition 1 (mean symbol; two dimensions). Let ψ(y)=ei(kuuy+kvvy)\psi(y)=e^{i(k_uu_y+k_vv_y)} and let Sε(k)S_\varepsilon(k) be the expectation of (D+εψ)(x)/ψ(x)(D^{\varepsilon}_+\psi)(x)/\psi(x) given a point at xx, the sum over the past of xx being taken first over VV and then over UU. Then

Sε(k)=i kv h ⁣(−2kukvερ),h(ω)=1+ω−ω(2+ω) eωE1(ω)=2∫0∞t e−ωt(1+t)3 dt,(1)S_\varepsilon(k)=i\,k_v\,h\!\Big(\frac{-2k_uk_v}{\varepsilon\rho}\Big),\qquad h(\omega)=1+\omega-\omega(2+\omega)\,e^{\omega}E_1(\omega)=2\int_0^\infty\frac{t\,e^{-\omega t}}{(1+t)^3}\,dt, \tag{1}

where E1E_1 is the exponential integral. For kukv<0k_uk_v<0 the argument ω\omega is positive and (1) holds as written. For kukv>0k_uk_v>0 one takes the boundary value ω→ω+i0 sgn(ku+kv)\omega\to \omega+i0\,\mathrm{sgn}(k_u+k_v) on the cut ω<0\omega<0. Moreover h(0)=1h(0)=1, hh has no zero on the real line (on either side of the cut), and ∣h(ω)∣≤C/(1+ω2)\lvert h(\omega)\rvert \le C/(1+\omega^2) for a constant CC. In particular Sε(k)=0S_\varepsilon(k)=0 exactly on the null line kv=0k_v=0, and Sε(k)→ikvS_\varepsilon(k)\to i k_v as k→0k\to0.

Proof. Rescaling VV by ερ\varepsilon\rho reduces the claim to ε=ρ=1\varepsilon=\rho=1, with kvk_v replaced by kv/(ερ)k_v/(\varepsilon\rho) and an overall factor ερ\varepsilon\rho that cancels against it, so we take ε=ρ=1\varepsilon=\rho=1. The sum over the past becomes a one-dimensional integral by the Mecke formula, and the integral is evaluated on a rotated contour.

By the Mecke formula the expectation is 12∬U f0(UV/2) e−i(kuU+kvV) dU dV\tfrac12\iint U\,f_0(UV/2)\,e^{-i(k_uU+k_vV)}\,dU\,dV (for general ε\varepsilon one averages f(n,ε)f(n,\varepsilon) over n∼Poisson(λ)n\sim\mathrm{Poisson}(\lambda) and obtains f0(ελ)f_0(\varepsilon\lambda)). Write this as i∂kuGi\partial_{k_u}G with G=12∬f0(UV/2) e−i(kuU+kvV)dU dVG=\tfrac12\iint f_0(UV/2)\,e^{-i(k_uU+k_vV)}dU\,dV. With s=U/2s=U/2 and β=ikv\beta=ik_v the VV-integral of the term an(sV)ne−sVa_n(sV)^ne^{-sV} of f0f_0, where (a0,a1,a2)=(1,−2,12)(a_0,a_1,a_2)=(1,-2,\tfrac12), equals an n! sn/(s+β)n+1a_n\,n!\,s^n/(s+\beta)^{n+1}, and

∑nan n! sn(s+β)n+1=(s+β)2−2s(s+β)+s2(s+β)3=β2(s+β)3.\sum_n \frac{a_n\,n!\,s^n}{(s+\beta)^{n+1}}=\frac{(s+\beta)^2-2s(s+\beta)+s^2}{(s+\beta)^3}=\frac{\beta^2}{(s+\beta)^3}.

Hence

G=∫0∞e−2ikus β2(s+β)3 ds,G=\int_0^\infty e^{-2ik_us}\,\frac{\beta^2}{(s+\beta)^3}\,ds ,

which converges absolutely. For kv=0k_v=0 the integrand vanishes and S=0S=0. If kukv<0k_uk_v<0 one rotates the contour to s=βts=\beta t, which sweeps a quadrant that contains neither the pole s=−βs=-\beta nor a contribution from the arc at infinity, and finds G=∫0∞e−ωt(1+t)−3dtG=\int_0^\infty e^{-\omega t}(1+t)^{-3}dt with ω=−2kukv>0\omega=-2k_uk_v>0. Since S=i∂kuG=ikv (−2G′(ω))S=i\partial_{k_u}G=ik_v\,(-2G'(\omega)) one gets the integral form of hh, and integrating by parts twice gives the closed form in (1). For kv>0k_v>0, GG is analytic in kuk_u in the lower half plane, which corresponds to Im ω>0\mathrm{Im}\,\omega>0; the formula, analytic in ω\omega off the cut, agrees with GG on the real half line and therefore everywhere in that half plane. The real timelike values are the boundary values ω+i0\omega+i0. For kv<0k_v<0 the same argument gives ω−i0\omega-i0. This is the stated rule, since for kukv>0k_uk_v>0 the sign of ku+kvk_u+k_v equals the sign of kvk_v.

For ω>0\omega>0 the integral form gives h>0h>0 and h(ω)≤2∫0∞te−ωtdt=2/ω2h(\omega)\le 2\int_0^\infty t e^{-\omega t}dt=2/\omega^2. For ω=−a±i0\omega=-a\pm i0 with a>0a>0 the identity E1(−a±i0)=−Ei(a)∓iπE_1(-a\pm i0)=-\mathrm{Ei}(a)\mp i\pi gives Im h=∓πa(2−a)e−a\mathrm{Im}\,h=\mp\pi a(2-a)e^{-a}, which vanishes only at a=2a=2, where ω(2+ω)=0\omega(2+\omega)=0 and h=1+ω=−1≠0h=1+\omega=-1\neq0. So hh has no real zero. For the decay on the cut, rotate the integral form to the ray t=τe∓2πi/3t=\tau e^{\mp 2\pi i/3} for ω=−a±i0\omega=-a\pm i0, which is allowed because the pole of (1+t)−3(1+t)^{-3} at t=−1t=-1 is not crossed; there ∣e−ωt∣=e−aτ/2\lvert e^{-\omega t}\rvert =e^{-a\tau/2} and ∣1+t∣≥3/2\lvert 1+t\rvert \ge\sqrt3/2, so ∣h(−a±i0)∣≤2(2/3)3 (4/a2)=64/(33 a2)\lvert h(-a\pm i0)\rvert \le 2(2/\sqrt3)^3\,(4/a^2)=64/(3\sqrt3\,a^2). Continuity of hh near ω=0\omega=0 gives the uniform bound. □\square

The mean symbol therefore vanishes on the null line kv=0k_v=0 in the entry D+D_+ (and on ku=0k_u=0 in D−D_-) and has no other zero. Boost covariance alone restricts the further zeros of a frame-free symbol, which would be doublers.

Proposition 2 (boost covariance fixes the symbol on the null half-lines; two dimensions). Let D(p)D(p) be a 2×22\times2 matrix function of p=(pu,pv)p=(p_u,p_v), continuous at 00 with D(0)=0D(0)=0, covariant under boosts: ΩξD(Λξp)Ωξ−1=D(p)\Omega_\xi D(\Lambda_\xi p)\Omega_\xi^{-1}=D(p) with Λξ(pu,pv)=(eξpu,e−ξpv)\Lambda_\xi(p_u,p_v)=(e^{\xi}p_u,e^{-\xi}p_v) and Ωξ=diag(eξ/2,e−ξ/2)\Omega_\xi=\mathrm{diag}(e^{\xi/2},e^{-\xi/2}). Here Λξ\Lambda_\xi is the action on momenta of the boost that multiplies (U,V)(U,V) by (e−ξ,eξ)(e^{-\xi},e^{\xi}), so that puU+pvVp_uU+p_vV is invariant. Then on the half-lines pv=0p_v=0 only the entry D21D_{21} can be non-zero and it is linear in pup_u; on the half-lines pu=0p_u=0 only D12D_{12} can be non-zero and it is linear in pvp_v. Every other zero set of det⁡D\det D is a union of boost orbits, that is of hyperbolas pupv=const≠0p_up_v=\mathrm{const}\neq0.

Proof. Conjugation by Ωξ\Omega_\xi leaves the diagonal entries unchanged, multiplies D12D_{12} by eξe^{\xi} and D21D_{21} by e−ξe^{-\xi}. On the ray p=κ(1,0)p=\kappa(1,0) one has Λξp=eξp\Lambda_\xi p=e^{\xi}p. Covariance gives D11(eξp)=D11(p)D_{11}(e^{\xi}p)=D_{11}(p), and the left side tends to D11(0)=0D_{11}(0)=0 as ξ→−∞\xi\to-\infty, so D11=0D_{11}=0 on the ray; the same holds for D22D_{22}. It gives D12(eξp)=e−ξD12(p)D_{12}(e^{\xi}p)=e^{-\xi}D_{12}(p), whose left side tends to 00 as ξ→−∞\xi\to-\infty while the right side diverges unless D12(p)=0D_{12}(p)=0. It gives D21(eξp)=eξD21(p)D_{21}(e^{\xi}p)=e^{\xi}D_{21}(p), which is linearity along the ray. The other null ray is treated with ξ→+∞\xi\to+\infty, and exchanges the roles of D12D_{12} and D21D_{21}. The determinant is boost invariant, so its zero set is a union of orbits, and the orbits of the boost group in the plane are the hyperbolas pupv=constp_up_v=\mathrm{const}, the four open null half-lines and the origin. □\square

The symbol of Definition 1, D(k)=(0ikvhikuh0)D(k)=\begin{pmatrix}0&ik_vh\\ ik_uh&0\end{pmatrix} with hh evaluated at −2kukv/ρ-2k_uk_v/\rho, satisfies the hypotheses (the invariant kukvk_uk_v is unchanged by Λξ\Lambda_\xi), with D21∝kuD_{21}\propto k_u surviving on kv=0k_v=0 and D12∝kvD_{12}\propto k_v on ku=0k_u=0. Its determinant kukvh2k_uk_vh^2 vanishes only on the two null lines, because hh has no zero (Proposition 1). Doubling is therefore not what obstructs chirality for this kernel. The Nielsen–Ninomiya theorem [NN] forces extra zeros through the periodicity of the Brillouin zone of a lattice, and the symbol of a frame-free kernel is not periodic.

Positive covariant weights cannot be used instead. A function ϕ(Δ2)\phi(\Delta^2) of the invariant interval alone is never integrable over the plane unless it vanishes: in rapidity coordinates d2Δ=12 dσ dθd^2\Delta=\tfrac12\,d\sigma\,d\theta with σ=Δ2\sigma=\Delta^2 and θ∈R\theta\in\mathbb R, so ∫∣ϕ∣ d2Δ=∞\int\lvert \phi\rvert \,d^2\Delta=\infty whenever ϕ≠0\phi\ne0. The same holds on every hyperboloid in higher dimensions. A covariant kernel therefore has a symbol only through cancellations, and the layer weights (1,−2,1)(1,-2,1) are such a cancellation.

2. The overlap operator and its index

Let XX be a linear operator on a finite-dimensional space V=VR⊕VL\mathcal V=\mathcal V_R\oplus\mathcal V_L with grading γ5=±1\gamma_5=\pm1 on VR/L\mathcal V_{R/L}, and let m0>0m_0>0 be a real number. Put

H=γ5 (X−m0),Dov=m0 (1+γ5 Σ),Σ=sgn H.(2)H=\gamma_5\,(X-m_0),\qquad D_{\rm ov}=m_0\,\big(1+\gamma_5\,\Sigma\big),\qquad \Sigma=\mathrm{sgn}\,H . \tag{2}

For a matrix HH with no eigenvalue on the imaginary axis, sgn H=P+−P−\mathrm{sgn}\,H=P_+-P_- where P±P_\pm are the spectral projections onto the generalised eigenspaces with Re λ>0\mathrm{Re}\,\lambda>0 and <0<0. Then Σ2=1\Sigma^2=1, Σ\Sigma commutes with HH, Tr Σ=N+−N−\mathrm{Tr}\,\Sigma=N_+-N_- is the difference of the numbers of eigenvalues (counted with algebraic multiplicity) in the two half planes, and for Hermitian HH it is the usual sign function. Here XX is the sum of a Dirac part and an optional Wilson term, and m0m_0 plays the role of the Wilson mass. When V=C2⊗Cn\mathcal V=\mathbb C^2\otimes\mathbb C^n with γ5=σz⊗1\gamma_5=\sigma_z\otimes1, a Wilson term is called chirally even if it has the form 1⊗W1\otimes W, that is, if it acts by the same matrix on the RR and LL components. We call the integer

ind Dov=−12 Tr sgn H(3)\mathrm{ind}\,D_{\rm ov}=-\tfrac12\,\mathrm{Tr}\,\mathrm{sgn}\,H \tag{3}

the overlap index. It is defined exactly when HH has no purely imaginary eigenvalue, and it is an integer because N++N−=dim⁡VN_++N_-=\dim\mathcal V is even when Tr γ5=0\mathrm{Tr}\,\gamma_5=0.

Lemma 1 (Ginsparg–Wilson relation and index). (a) For every XX for which Σ\Sigma is defined, DovD_{\rm ov} satisfies γ5Dov+Dovγ5=m0−1Dovγ5Dov\gamma_5D_{\rm ov}+D_{\rm ov}\gamma_5=m_0^{-1}D_{\rm ov}\gamma_5D_{\rm ov}. (b) If dim⁡VR=dim⁡VL\dim\mathcal V_R=\dim\mathcal V_L and HH is Hermitian, then ind Dov=ν+−ν−\mathrm{ind}\,D_{\rm ov}=\nu_+-\nu_-, where ν±\nu_\pm is the number of zero modes of DovD_{\rm ov} with γ5=±1\gamma_5=\pm1. (c) If Tr γ5=0\mathrm{Tr}\,\gamma_5=0, then for every XX for which Σ\Sigma is defined, Tr γ5(1−Dov/2m0)=−12Tr Σ\mathrm{Tr}\,\gamma_5(1-D_{\rm ov}/2m_0)=-\tfrac12\mathrm{Tr}\,\Sigma.

Proof. (a) Using only Σ2=1\Sigma^2=1, m0−1Dovγ5Dov=m0(1+γ5Σ)γ5(1+γ5Σ)=m0(2γ5+γ5Σγ5+Σ)m_0^{-1}D_{\rm ov}\gamma_5D_{\rm ov}=m_0(1+\gamma_5\Sigma)\gamma_5(1+\gamma_5\Sigma)=m_0(2\gamma_5+\gamma_5\Sigma\gamma_5+\Sigma), and γ5Dov+Dovγ5=m0(2γ5+Σ+γ5Σγ5)\gamma_5D_{\rm ov}+D_{\rm ov}\gamma_5=m_0(2\gamma_5+\Sigma+\gamma_5\Sigma\gamma_5).

(c) Tr γ5(1−Dov/2m0)=Tr γ5−12Tr γ5(1+γ5Σ)=−12Tr Σ\mathrm{Tr}\,\gamma_5(1-D_{\rm ov}/2m_0)=\mathrm{Tr}\,\gamma_5-\tfrac12\mathrm{Tr}\,\gamma_5(1+\gamma_5\Sigma)=-\tfrac12\mathrm{Tr}\,\Sigma, because Tr γ5=0\mathrm{Tr}\,\gamma_5=0.

(b) Let T=γ5ΣT=\gamma_5\Sigma. For Hermitian HH, Σ\Sigma is Hermitian, so TT is unitary and Dov=m0(1+T)D_{\rm ov}=m_0(1+T) is normal, with γ5Dovγ5=Dov†\gamma_5D_{\rm ov}\gamma_5=D_{\rm ov}^\dagger. Its eigenvalues lie on the circle ∣λ−m0∣=m0\lvert \lambda-m_0\rvert =m_0, so a real eigenvalue is 00 or 2m02m_0. The map γ5\gamma_5 takes the eigenspace of a non-real λ\lambda to that of λˉ\bar\lambda, which is orthogonal to it, so every eigenvector with non-real eigenvalue has ⟨γ5⟩=0\langle\gamma_5\rangle=0. Therefore Tr γ5(1−Dov/2m0)\mathrm{Tr}\,\gamma_5(1-D_{\rm ov}/2m_0) receives a contribution only from the eigenvalue 00, namely ν+−ν−\nu_+-\nu_-, and by (c) it equals −12Tr Σ-\tfrac12\mathrm{Tr}\,\Sigma. □\square

For a Hermitian HH the index therefore counts the net chirality of exact zero modes, and Lemma 1(a) is why the construction is exactly chiral at finite cutoff. For a non-Hermitian HH only (a) and (c) survive. The integer (3) is then the trace of the chiral density γ5(1−Dov/2m0)\gamma_5(1-D_{\rm ov}/2m_0), and it need not count zero modes: in the zero-diagonal case of Theorem 1 below DovD_{\rm ov} is nilpotent, so every vector is annihilated by some power of it, while (3) vanishes. The theorems of Sections 3 and 4 concern this trace, which is the quantity that equals the flux in the Hermitian Euclidean case.

Example 1 (the Euclidean overlap on Poisson points). Take a unit-density Poisson process on the torus of side L=NL=\sqrt N with antiperiodic spinors, Pauli matrices γ1=σ1\gamma_1=\sigma_1, γ2=σ2\gamma_2=\sigma_2, γ5=σ3\gamma_5=\sigma_3, and the Gaussian-kernel Wilson–Dirac operator

DW[x,y]=w(Δxy)[γ⋅ΔxyZ1−rZ0]Φxy,DW[x,x]=rZ0∑y≠xw(Δxy),(4)D_W[x,y]=w(\Delta_{xy})\Big[\frac{\gamma\cdot\Delta_{xy}}{Z_1}-\frac{r}{Z_0}\Big]\Phi_{xy},\quad D_W[x,x]=\frac{r}{Z_0}\sum_{y\ne x}w(\Delta_{xy}), \tag{4}

where Δxy\Delta_{xy} is the displacement from xx to the nearest image of yy, w(Δ)=e−∣Δ∣2/2s2w(\Delta)=e^{-\lvert \Delta\rvert ^2/2s^2} for ∣Δ∣<6s\lvert \Delta\rvert <6s, Z1=2πs4Z_1=2\pi s^4, Z0=2πs2Z_0=2\pi s^2, and Φxy\Phi_{xy} are the link phases of a background U(1) field. The field is uniform, F12=∂1A2−∂2A1=2πQ/L2F_{12}=\partial_1\mathcal A_2-\partial_2\mathcal A_1=2\pi Q/L^2 with total flux 2πQ2\pi Q, given in Landau gauge A=(0,F12x1)\mathcal A=(0,F_{12}x_1) with transition functions, and Φxy=exp⁡(i∫yxA⋅dl)\Phi_{xy}=\exp(i\int_y^x\mathcal A\cdot dl) along the straight segment, the parallel transport for D=∂−iAD=\partial-i\mathcal A. The mean symbol of DWD_W is iγ⋅p e−s2p2/2+r(1−e−s2p2/2)i\gamma\cdot p\,e^{-s^2p^2/2}+r(1-e^{-s^2p^2/2}). The operator uses the Euclidean metric ∣Δ∣\lvert \Delta\rvert, which is a choice of Euclidean time axis (a Wick axis; see below). With s=1.5s=1.5, r=1r=1, m0=12m_0=\tfrac12 we built DovD_{\rm ov} by (2) with X=DWX=D_W at N=300N=300 for three point sets and Q=0,1,2,−1Q=0,1,2,-1 each. In every one of the twelve cases HH had no eigenvalue of modulus below 0.100.10 and the index was +Q+Q in this convention, carried by exactly ∣Q∣\lvert Q\rvert zero modes, all of chirality sgn Q\mathrm{sgn}\,Q (none for Q=0Q=0). Reversing the orientation of the flux, or the sign of the link phase, gives −Q-Q.

These twelve cases are a numerical observation. Lüscher’s lattice index theorem [L] is proved for local, gauge-covariant, doubler-free operators on regular lattices with smooth admissible fields. We prove no analogue for the Gaussian kernel on Poisson points, only integrality and the Ginsparg–Wilson relation (Lemma 1).

The unit-density Poisson law is invariant under every volume-preserving affine map, because the image of a Poisson process under such a map is Poisson with the image intensity, which is again Lebesgue measure. A boost is such a map, and it carries the Euclidean metric attached to one unit timelike vector ee to the one attached to the boosted vector. The metric attached to ee is ∣Δ∣e2=2(Δ⋅e)2−Δ2\lvert \Delta\rvert _e^2=2(\Delta\cdot e)^2-\Delta^2, the Minkowski interval with the sign of its spatial part reversed, which equals t2+x2t^2+x^2 in the frame where e=(1,0)e=(1,0); a Poisson set in the plane with this metric is what Example 1 places on a torus. So the law of DWD_W built with the Euclidean metric of ee is the same for every unit timelike ee: the frame is a choice of Wick axis, which the points do not carry. Frames, Wilson terms and reflection positivity reports that the Gaussian-kernel Wilson term of Example 1 and its overlap fail a one-particle reflection-positivity test on mirror-symmetric sets in two dimensions, a numerical result, so that the Euclidean operator is not shown to define a Lorentzian theory. The operator DWD_W has γ5\gamma_5-Hermiticity, DW†=γ5DWγ5D_W^\dagger=\gamma_5D_W\gamma_5, which makes H=γ5(DW−m0)H=\gamma_5(D_W-m_0) Hermitian. The retarded operators of Section 3 lack it, and so does the symmetrised operator of Section 4 built from Definition 1, because their two off-diagonal blocks do not satisfy D21=−D12†D_{21}=-D_{12}^\dagger. The operators of Corollary 1 have it, with a Hermitian or anti-Hermitian Weyl block, and their index vanishes. What separates the Euclidean overlap of Example 1 from them is the pairing of the two blocks: the adjoint of ∂z\partial_z is −∂zˉ-\partial_{\bar z} in Euclidean signature, so the blocks approximate two different derivatives, whereas a block AA and −A†-A^\dagger with AA (anti-)Hermitian approximate the same derivative twice.

3. Retarded operators carry no index

An operator of the form of Definition 1, with any weights, links and gauge phases and in any dimension, is retarded, and Theorem 1 applies to it.

Theorem 1 (retarded operators). Let C\mathcal C be a finite partially ordered set with a linear extension x1,…,xNx_1,\dots,x_N, and let the space V\mathcal V be the direct sum of spaces Vx\mathcal V_x, x∈Cx\in\mathcal C, each graded by γ5\gamma_5. Assume

(R1) XX is block lower triangular for this ordering: the block XxyX_{xy} vanishes unless y⪯xy\preceq x in the linear extension. The diagonal blocks XxxX_{xx} are arbitrary.

(R2) m0>0m_0>0 is such that no Hxx=γ5(Xxx−m0)H_{xx}=\gamma_5(X_{xx}-m_0) has a purely imaginary eigenvalue.

Then H=γ5(X−m0)H=\gamma_5(X-m_0) is block lower triangular, its spectrum is the union of the spectra of the HxxH_{xx}, the overlap operator (2) exists, satisfies the Ginsparg–Wilson relation exactly, and

ind Dov=−12∑xTr sgn Hxx.(5)\mathrm{ind}\,D_{\rm ov}=-\tfrac12\sum_{x}\mathrm{Tr}\,\mathrm{sgn}\,H_{xx}. \tag{5}

In particular, if each diagonal block is chirally even, Xxx=1⊗axX_{xx}=1\otimes a_x on Vx=C2⊗Cℓx\mathcal V_x=\mathbb C^2\otimes\mathbb C^{\ell_x}, then ind Dov=0\mathrm{ind}\,D_{\rm ov}=0. If the diagonal blocks vanish, HH has the two eigenvalues ±m0\pm m_0 only, and DovD_{\rm ov} is strictly block lower triangular, hence nilpotent. The index does not depend on any off-diagonal block, so it is independent of the weights, the links and the background gauge field.

Proof. Since γ5\gamma_5 is block diagonal, HH is block lower triangular with diagonal blocks HxxH_{xx}. The characteristic polynomial of a block triangular matrix is the product of those of the diagonal blocks, so the eigenvalues of HH, with algebraic multiplicity, are those of the HxxH_{xx}, and (R2) says none lies on the imaginary axis. Then Tr sgn H=N+−N−\mathrm{Tr}\,\mathrm{sgn}\,H=N_+-N_- is the sum of the same numbers for the blocks, which is (5). Lemma 1(a) is algebra and applies.

For a chirally even diagonal block, Hxx=σz⊗(ax−m0)H_{xx}=\sigma_z\otimes(a_x-m_0) has the eigenvalues ±λ\pm\lambda for each eigenvalue λ\lambda of ax−m0a_x-m_0, so N+=N−N_+=N_- and the block contributes zero to (5).

For vanishing diagonal blocks, Hxx=−m0γ5H_{xx}=-m_0\gamma_5 has the eigenvalue −m0-m_0 on Vx,R\mathcal V_{x,R} and +m0+m_0 on Vx,L\mathcal V_{x,L}. Let P+P_+ be the Riesz projection 12πi∮(z−H)−1dz\frac1{2\pi i}\oint(z-H)^{-1}dz around +m0+m_0. The resolvent (z−H)−1(z-H)^{-1} is block lower triangular with diagonal blocks (z+m0γ5)−1(z+m_0\gamma_5)^{-1}, so P+P_+ is block lower triangular with diagonal blocks 12(1−γ5)\tfrac12(1-\gamma_5). Hence Σ=2P+−1\Sigma=2P_+-1 is block lower triangular with diagonal blocks −γ5-\gamma_5, and Dov=m0(1+γ5Σ)D_{\rm ov}=m_0(1+\gamma_5\Sigma) has diagonal blocks m0(1−γ5γ5)=0m_0(1-\gamma_5\gamma_5)=0. A block lower triangular matrix with zero diagonal blocks satisfies DovN=0D_{\rm ov}^N=0. □\square

A triangular matrix has the spectrum of its diagonal, and the trace of a sign function depends only on the spectrum, so the off-diagonal part cannot enter. The Ginsparg–Wilson relation holds, so the operator is exactly chiral, but formula (5) is a sum of on-site contributions that see neither the order nor the gauge field. A nonzero index of a retarded operator therefore requires a chirally asymmetric on-site term. For scalar diagonal blocks Xxx=diag(cR,cL)X_{xx}=\mathrm{diag}(c_R,c_L) with real cR,cL≠m0c_R,c_L\neq m_0, the contribution of the site to (5) is −12[sgn(cR−m0)−sgn(cL−m0)]-\tfrac12[\mathrm{sgn}(c_R-m_0)-\mathrm{sgn}(c_L-m_0)], which is ∓1\mp1 when m0m_0 lies between cRc_R and cLc_L and zero otherwise.

The theorem covers more than the signed-BD kernel. It applies to every retarded operator in every dimension: a Weyl block ∑yaxy σˉ⋅(x−y)\sum_y a_{xy}\,\bar\sigma\cdot(x-y) with y≺xy\prec x, any weights axya_{xy}, any link variables, and a retarded Wilson term. A retarded Wilson term whose diagonal is chirally even (in particular zero) keeps the index at zero. The theorem applies to advanced operators by reversing the order.

Numerically, the sign function of such a defective HH is ill conditioned, and eigenvalues from a numerical eigensolver are accurate only to a fractional power of machine precision, so formula (5) is the reliable way to evaluate the index of a retarded operator.

4. Self-adjointness for a chirality-exchanging involution

For the signed-BD kernel the adjoint of the retarded operator is advanced and has the same functional form: since the entries are real,

D+†[x,y]=D+[y,x]=ρ wnyx(uy−ux)(x≺y),soD+†=−D~+,(6)D_+^\dagger[x,y]=D_+[y,x]=\rho\,w_{n_{yx}}(u_y-u_x)\quad(x\prec y),\qquad\text{so}\qquad D_+^\dagger=-\widetilde D_+ , \tag{6}

where D~+[x,y]=ρ wnxy(ux−uy)\widetilde D_+[x,y]=\rho\,w_{n_{xy}}(u_x-u_y) for y≻xy\succ x is the advanced kernel of the same type. The sum D++D~+=D+−D+†D_++\widetilde D_+=D_+-D_+^\dagger is the symmetrised ∂v\partial_v kernel on all causally related pairs (the Pauli–Jordan type), and it is anti-Hermitian. In Lorentzian signature the formal adjoint of ∂v\partial_v is −∂v-\partial_v, whereas in Euclidean signature the adjoint of ∂z\partial_z is −∂zˉ-\partial_{\bar z}. A γ5\gamma_5-Hermitian Dirac operator (0A−A†0)\begin{pmatrix}0&A\\-A^\dagger&0\end{pmatrix} assembled from a frame-free block A≈∂vA\approx\partial_v therefore has the same derivative in both off-diagonal blocks when AA is anti-Hermitian: the second block is −A†=A-A^\dagger=A, not an approximation to ∂u\partial_u. Theorem 2 treats this case together with the larger class of operators that are self-adjoint for a matrix exchanging the two chiralities.

Theorem 2 (Krein-self-adjoint operators). Let γ5\gamma_5 be the grading on V\mathcal V and let JJ be a matrix with

(K1) J=J†J=J^\dagger, J2=1J^2=1 and Jγ5=−γ5JJ\gamma_5=-\gamma_5J (an involution that exchanges the two chiralities).

Let XX be a matrix that is JJ-self-adjoint, that is, self-adjoint for the indefinite form ⟨w,Jw′⟩\langle w,Jw'\rangle:

(K2) JX†J=XJX^\dagger J=X.

Let m0m_0 be real and put H=γ5(X−m0)H=\gamma_5(X-m_0) and J′=iJγ5J'=iJ\gamma_5. Then J′J' is a Hermitian involution and J′H†J′=−HJ'H^\dagger J'=-H. Consequently the spectrum of HH satisfies spec H=−spec H‾\mathrm{spec}\,H=-\overline{\mathrm{spec}\,H} with equal algebraic multiplicities. If HH has no purely imaginary eigenvalue then Tr sgn H=0\mathrm{Tr}\,\mathrm{sgn}\,H=0 and ind Dov=0\mathrm{ind}\,D_{\rm ov}=0. Otherwise the index (3) is undefined.

Proof. Since Jγ5=−γ5JJ\gamma_5=-\gamma_5J, (iJγ5)†=−iγ5J=iJγ5(iJ\gamma_5)^\dagger=-i\gamma_5J=iJ\gamma_5 and (iJγ5)2=−Jγ5Jγ5=J2γ52=1(iJ\gamma_5)^2=-J\gamma_5J\gamma_5=J^2\gamma_5^2=1. Because m0m_0 is real, Xm=X−m0X_m=X-m_0 also satisfies JXm†J=XmJX_m^\dagger J=X_m, and H=γ5XmH=\gamma_5X_m. Then

J′H†J′=−Jγ5Xm†γ5Jγ5=Jγ5Xm†J=−γ5JXm†J=−γ5Xm=−H,J'H^\dagger J'=-J\gamma_5X_m^\dagger\gamma_5J\gamma_5=J\gamma_5X_m^\dagger J=-\gamma_5JX_m^\dagger J=-\gamma_5X_m=-H ,

where we used γ5Jγ5=−J\gamma_5J\gamma_5=-J, then Jγ5=−γ5JJ\gamma_5=-\gamma_5J, then (K2) for XmX_m. So H†H^\dagger is similar to −H-H and the two have the same eigenvalues with multiplicity. The eigenvalues of H†H^\dagger are the conjugates of those of HH, which gives the symmetry. If no eigenvalue is purely imaginary, the map λ↦−λˉ\lambda\mapsto-\bar\lambda exchanges the eigenvalues in Re λ>0\mathrm{Re}\,\lambda>0 with those in Re λ<0\mathrm{Re}\,\lambda<0, so N+=N−N_+=N_-. □\square

The involution J′=iJγ5J'=iJ\gamma_5 turns the exchange of chiralities into a symmetry of HH itself. The symmetry of the spectrum is of the kind familiar from Krein-space theory, in which Dirac operators are self-adjoint for an indefinite form [S].

Corollary 1 (Hermitian and anti-Hermitian Weyl blocks). Let AA be any square matrix with A†=−AA^\dagger=-A or A†=AA^\dagger=A, let WW be any Hermitian matrix, and let m0m_0 be real. Let V=C2⊗Cℓ\mathcal V=\mathbb C^2\otimes\mathbb C^\ell with γ5=σz⊗1\gamma_5=\sigma_z\otimes1, and put

H=σz⊗(W−m0)+{iσy⊗A,A†=−A,σx⊗A,A†=A.H=\sigma_z\otimes(W-m_0)+\begin{cases}i\sigma_y\otimes A,&A^\dagger=-A,\\ \sigma_x\otimes A,&A^\dagger=A.\end{cases}

This is γ5(X−m0)\gamma_5(X-m_0) for the Dirac operator (0A−A†0)\begin{pmatrix}0&A\\-A^\dagger&0\end{pmatrix} with a chirally even Hermitian Wilson term WW. Then HH is Hermitian, spec H=−spec H\mathrm{spec}\,H=-\mathrm{spec}\,H and, if HH is invertible, ind Dov=0\mathrm{ind}\,D_{\rm ov}=0 for every m0m_0 and WW.

Proof. Both σx⊗1\sigma_x\otimes1 and σy⊗1\sigma_y\otimes1 anticommute with γ5=σz⊗1\gamma_5=\sigma_z\otimes1, so (K1) holds for either. For A†=−AA^\dagger=-A the Dirac operator is σx⊗A\sigma_x\otimes A, X=1⊗W+σx⊗AX=1\otimes W+\sigma_x\otimes A, X†=1⊗W−σx⊗AX^\dagger=1\otimes W-\sigma_x\otimes A, and with J=σy⊗1J=\sigma_y\otimes1 one has JX†J=XJX^\dagger J=X because σyσxσy=−σx\sigma_y\sigma_x\sigma_y=-\sigma_x. For A†=AA^\dagger=A the Dirac operator is iσy⊗Ai\sigma_y\otimes A, X†X^\dagger contains −iσy⊗A-i\sigma_y\otimes A, and with J=σx⊗1J=\sigma_x\otimes1 one has σx(−iσy)σx=iσy\sigma_x(-i\sigma_y)\sigma_x=i\sigma_y, so again JX†J=XJX^\dagger J=X. Thus (K2) holds and Theorem 2 applies, with J′=−σx⊗1J'=-\sigma_x\otimes1 for J=σy⊗1J=\sigma_y\otimes 1 and J′=σy⊗1J'=\sigma_y\otimes1 for J=σx⊗1J=\sigma_x\otimes1; in both cases J′J' anticommutes with HH. Because HH is Hermitian its spectrum is real, and the symmetry of the spectrum gives Tr sgn H=0\mathrm{Tr}\,\mathrm{sgn}\,H=0 whenever HH is invertible. □\square

Corollary 1 uses that WW is Hermitian and chirally even. Conjugation by either J=σx⊗1J=\sigma_x\otimes1 or J=σy⊗1J=\sigma_y\otimes1 exchanges WRW_R and WLW_L, so J diag(WR,WL)†J=diag(WL†,WR†)J\,\mathrm{diag}(W_R,W_L)^\dagger J=\mathrm{diag}(W_L^\dagger,W_R^\dagger). A Hermitian Wilson term diag(WR,WL)\mathrm{diag}(W_R,W_L) with WR≠WLW_R\ne W_L therefore fails (K2) for these two JJ, and Theorem 2 makes no statement about it. For a general chirality-exchanging JJ the condition on diag(WR,WL)\mathrm{diag}(W_R,W_L) differs, and we do not treat it. A non-Hermitian one with WL=WR†W_L=W_R^\dagger satisfies the Wilson-term part of (K2), and Theorem 2 then applies when the Dirac part does as well.

Corollary 1 does not exhaust Theorem 2. The retarded operator DD of Definition 1 is not JJ-self-adjoint, but for J=σxJ=\sigma_x the JJ-self-adjoint part of iDiD is i2(0D+−D+†D−−D−†0)\tfrac i2\begin{pmatrix}0&D_+-D_+^\dagger\\D_--D_-^\dagger&0\end{pmatrix}, the symmetrised kernel of (6) in both blocks. Its two off-diagonal blocks are different Hermitian matrices, so Theorem 2 applies while Corollary 1 (which needs equal blocks up to sign) does not. In four dimensions the same holds for a Weyl block A[x,y]=cxy σˉ⋅(x−y)A[x,y]=c_{xy}\,\bar\sigma\cdot(x-y) with real weights cxyc_{xy}, where σˉμ=(1,−σ⃗)\bar\sigma^\mu=(1,-\vec\sigma). Since each σˉμ\bar\sigma^\mu is Hermitian, A†[x,y]=−cyx σˉ⋅(x−y)A^\dagger[x,y]=-c_{yx}\,\bar\sigma\cdot(x-y), so AA is anti-Hermitian when the weights are symmetric, cxy=cyxc_{xy}=c_{yx}, and Hermitian when they are antisymmetric. A retarded kernel is neither, but its symmetrisation Aret−Aret†A_{\rm ret}-A_{\rm ret}^\dagger is anti-Hermitian and falls under Corollary 1, as in two dimensions. The retarded block alone falls under Theorem 1. We did not compute four-dimensional spectra of these operators.

For the Krein-self-adjoint operator built from the signed-BD kernel, the mean symbols of Proposition 1 show why the spectrum meets the imaginary axis. Let the chirally even Wilson term have symbol rW^(k)r\widehat W(k) and put α(k)=rW^(k)−m0\alpha(k)=r\widehat W(k)-m_0. The symbol of D+−D+†D_+-D_+^\dagger is 2i Im S=2ikvRe h2i\,\mathrm{Im}\,S=2ik_v\mathrm{Re}\,h, so the symbol of HH is (α−kvRe hkuRe h−α)\begin{pmatrix}\alpha&-k_v\mathrm{Re}\,h\\k_u\mathrm{Re}\,h&-\alpha\end{pmatrix} and its eigenvalues satisfy λ2=α2−kukv(Re h)2\lambda^2=\alpha^2-k_uk_v(\mathrm{Re}\,h)^2. At timelike momenta with kukv(Re h)2>α2k_uk_v(\mathrm{Re}\,h)^2>\alpha^2 the eigenvalues are purely imaginary, so the sign function is undefined on that open set of momenta. The set is non-empty only if α2\alpha^2 is below the maximum of kukv(Re h)2k_uk_v(\mathrm{Re}\,h)^2 over the timelike momenta, which is 1.009 ρ1.009\,\rho (reached at −2kukv/ρ≃−1.9-2k_uk_v/\rho\simeq-1.9, from a numerical evaluation of Re h\mathrm{Re}\,h on the cut), so it requires ∣rW^(k)−m0∣≲ρ\lvert r\widehat W(k)-m_0\rvert\lesssim\sqrt\rho at the momenta concerned. In Euclidean signature λ2=α2+∣k∣2>0\lambda^2=\alpha^2+\lvert k\rvert ^2>0 and there is no such set. This is a derivation from mean symbols, and an individual sprinkling is not covered by it.

On a two-dimensional causal diamond of 7272 points, with W=12(B+B†)W=\tfrac12(B+B^\dagger) for BB the signed-BD scalar kernel with random link phases and (r,m0)=(1,0.45),(−1,0.45),(0.6,1.3)(r,m_0)=(1,0.45),(-1,0.45),(0.6,1.3), the Krein-self-adjoint operator above has a few to about twenty of the 144144 eigenvalues of HH within 10−610^{-6} of the imaginary axis, depending on the sprinkling and the parameters, so the index is undefined for these sprinklings. Such eigenvalues also occur for some sprinklings at (r,m0)=(0,6)(r,m_0)=(0,6), where the set of momenta defined above is empty, so the mean-symbol estimate does not account for them.

5. Finite Atiyah–Patodi–Singer indices

In the continuum, the Dirac operator on a Lorentzian region between two Cauchy surfaces is Fredholm when the data on each surface are restricted to a spectral subspace of a boundary Dirac operator, with complementary subspaces on the two surfaces (which one goes with the initial surface depends on the sign convention of the boundary operator), and its index is the Atiyah–Patodi–Singer expression [BS]. A discrete analogue replaces the surfaces by antichains. In the simplest finite definition the index is a dimension count that does not involve the bulk operator, and it is generally nonzero.

Proposition 3 (finite APS reduction; any dimension). Let D:CN→CND:\mathbb C^N\to\mathbb C^N be any linear map. Let B0,B1B_0,B_1 be disjoint subsets of the NN points, with Hermitian operators Θ0\Theta_0 on CB0\mathbb C^{B_0} and Θ1\Theta_1 on CB1\mathbb C^{B_1}. Let D={ψ∈CN:P<0(Θ0)ψ ⁣↾B0=0, P>0(Θ1)ψ ⁣↾B1=0}\mathcal D=\{\psi\in\mathbb C^N: P_{<0}(\Theta_0)\psi\!\upharpoonright_{B_0}=0,\ P_{>0}(\Theta_1)\psi\!\upharpoonright_{B_1}=0\} and indAPS=dim⁡ker⁡(D ⁣↾D)−dim⁡coker(D ⁣↾D)\mathrm{ind}_{\rm APS}=\dim\ker(D\!\upharpoonright_{\mathcal D})-\dim\mathrm{coker}(D\!\upharpoonright_{\mathcal D}), the cokernel being taken in the full codomain CN\mathbb C^N. Write ν±(Θ)\nu_\pm(\Theta) for the numbers of positive and negative eigenvalues, ν0(Θ)=dim⁡ker⁡Θ\nu_0(\Theta)=\dim\ker\Theta and η(Θ)=ν+−ν−\eta(\Theta)=\nu_+-\nu_-. Then

(a) indAPS=−ν−(Θ0)−ν+(Θ1)\mathrm{ind}_{\rm APS}=-\nu_-(\Theta_0)-\nu_+(\Theta_1), independent of DD.

(b) indAPS+12(∣B0∣+∣B1∣)=12[η(Θ0)−η(Θ1)]+12[ν0(Θ0)+ν0(Θ1)]\mathrm{ind}_{\rm APS}+\tfrac12(\lvert B_0\rvert+\lvert B_1\rvert)=\tfrac12[\eta(\Theta_0)-\eta(\Theta_1)]+\tfrac12[\nu_0(\Theta_0)+\nu_0(\Theta_1)].

(c) Exchanging the roles of B0B_0 and B1B_1 (order reversal) changes the sign of the η\eta terms.

(d) Suppose Θi\Theta_i is a function of link variables Φ\Phi on a neighbourhood Ni\mathcal N_i of BiB_i that is covariant, Θi(Φg)=gΘi(Φ)g−1\Theta_i(\Phi^g)=g\Theta_i(\Phi)g^{-1} for diagonal unitary gg, and that the background field is pure gauge on N0∪N1\mathcal N_0\cup\mathcal N_1 (every closed path there has trivial holonomy). Then the spectra of Θ0\Theta_0 and Θ1\Theta_1, and hence indAPS\mathrm{ind}_{\rm APS}, are independent of the flux QQ through the region between them.

Proof. (a) The conditions defining D\mathcal D are ν−(Θ0)+ν+(Θ1)\nu_-(\Theta_0)+\nu_+(\Theta_1) linear constraints, each a nonzero linear functional supported on B0B_0 or B1B_1. The supports are disjoint and, within each set, the functionals are orthonormal eigenvectors, so the constraints are independent and dim⁡D=N−ν−(Θ0)−ν+(Θ1)\dim\mathcal D=N-\nu_-(\Theta_0)-\nu_+(\Theta_1). For any linear map from a space of dimension N−jN-j to CN\mathbb C^N, rank–nullity gives dim⁡ker⁡−dim⁡coker=(N−j)−N=−j\dim\ker-\dim\mathrm{coker}=(N-j)-N=-j, here with j=ν−(Θ0)+ν+(Θ1)j=\nu_-(\Theta_0)+\nu_+(\Theta_1). (b) Substitute ∣Bi∣=ν++ν−+ν0\lvert B_i\rvert=\nu_++\nu_-+\nu_0 for each set. (c) Reversal imposes P<0(Θ1)P_{<0}(\Theta_1) and P>0(Θ0)P_{>0}(\Theta_0). (d) Pure gauge on Ni\mathcal N_i means that on each connected component the link variables are those of the trivial field transformed by a diagonal unitary gg, which exists because every holonomy is trivial (define gg by transport from a base point in each component). Covariance gives Θi(Φ)=gΘi(1)g−1\Theta_i(\Phi)=g\Theta_i(1)g^{-1}, which has the spectrum of Θi(1)\Theta_i(1). □\square

The proposition concerns this definition, with the boundary condition imposed on the domain only and the full space as the codomain. It does not show that no discrete APS-type index exists. It shows that for this definition on finite antichains the index counts boundary eigenvalues and does not see the bulk, so a bulk-sensitive index needs an additional ingredient. In the continuum that ingredient is the evolution operator, which identifies two infinite-dimensional boundary spaces through the bulk. A closed loop of Hermitian matrices also has zero spectral flow in finite dimension, so the continuum relation between index and spectral flow cannot be reproduced by a finite family. A boundary operator whose spectrum depends on QQ, chosen by hand, would put QQ into (a), and by the independence of DD it would do so equally with the bulk block replaced by zero.

The lattice index of [F] is the eta invariant of a domain-wall Dirac operator, a spectral asymmetry of a Hermitian operator. If that operator has the form of Corollary 1 for some chirally even WW, its spectrum is symmetric and the eta invariant vanishes. Whether the domain-wall operator can be given that form with a frame-free kernel, and the variant with a non-Hermitian retarded block, are open.

6. An internal compact index

A chirality index can be carried by an internal compact space YY, as in Kaluza–Klein compactification: the index of the Dirac operator on YY in a flux fixes how many one-handed zero modes the external space sees. Take C\mathcal C a causal set with a retarded block DCD_{\mathcal C} odd under a grading γC\gamma_{\mathcal C}, and YY a point set with a Ginsparg–Wilson operator DYD_Y and grading γY\gamma_Y, for instance the operator of Example 1 on a flux torus. Define

D=DC⊗1+γC⊗DY,Γ=γC⊗γY.(7)D=D_{\mathcal C}\otimes1+\gamma_{\mathcal C}\otimes D_Y,\qquad \Gamma=\gamma_{\mathcal C}\otimes\gamma_Y . \tag{7}

Proposition 4 (exact reduction; any dimension). Assume γYDY+DYγY=m0−1DYγYDY\gamma_YD_Y+D_Y\gamma_Y=m_0^{-1}D_Y\gamma_YD_Y and γCDC=−DCγC\gamma_{\mathcal C}D_{\mathcal C}=-D_{\mathcal C}\gamma_{\mathcal C}. Then ker⁡DY\ker D_Y is invariant under γY\gamma_Y, so it splits into ν+\nu_+ and ν−\nu_- modes of chirality +1+1 and −1-1. The subspace VC⊗ker⁡DY\mathcal V_{\mathcal C}\otimes\ker D_Y is invariant under DD, and on it D=DC⊗1D=D_{\mathcal C}\otimes1. On VC⊗ker⁡DY\mathcal V_{\mathcal C}\otimes\ker D_Y the operator Γ\Gamma acts as ±γC\pm\gamma_{\mathcal C} on the γY=±1\gamma_Y=\pm1 modes. Hence this sector consists of ν+\nu_+ copies of DCD_{\mathcal C} with Γ=γC\Gamma=\gamma_{\mathcal C} and ν−\nu_- copies of DCD_{\mathcal C} with Γ=−γC\Gamma=-\gamma_{\mathcal C}, in every realisation, and ν+−ν−=ind DY\nu_+-\nu_-=\mathrm{ind}\,D_Y when DYD_Y is the overlap operator (2) of an operator XYX_Y for which HY=γY(XY−m0)H_Y=\gamma_Y(X_Y-m_0) is Hermitian (Lemma 1(b)).

Proof. If DYϕ=0D_Y\phi=0 the Ginsparg–Wilson relation gives DYγYϕ=−γYDYϕ+m0−1DYγYDYϕ=0D_Y\gamma_Y\phi=-\gamma_YD_Y\phi+m_0^{-1}D_Y\gamma_YD_Y\phi=0, so γYϕ∈ker⁡DY\gamma_Y\phi\in\ker D_Y and γY\gamma_Y is diagonalisable there. On ψ⊗ϕ\psi\otimes\phi with ϕ∈ker⁡DY\phi\in\ker D_Y the second term of DD vanishes, leaving (DCψ)⊗ϕ(D_{\mathcal C}\psi)\otimes\phi; Γ\Gamma acts as γC⊗γY\gamma_{\mathcal C}\otimes\gamma_Y and for γYϕ=±ϕ\gamma_Y\phi=\pm\phi this is ±γC⊗1\pm\gamma_{\mathcal C}\otimes1. □\square

The sector VC⊗ker⁡DY\mathcal V_{\mathcal C}\otimes\ker D_Y is not the whole kernel of DD, which also contains the kernel of DCD_{\mathcal C} in other sectors. In the basis γC=±1\gamma_{\mathcal C}=\pm1 write DC=(0D+D−0)D_{\mathcal C}=\begin{pmatrix}0&D_+\\D_-&0\end{pmatrix}, as in Definition 1. A zero mode of a copy has D−ψR=0D_-\psi_R=0 and D+ψL=0D_+\psi_L=0, so the Γ=+1\Gamma=+1 components obey D−ψ=0D_-\psi=0 in the ν+\nu_+ copies with Γ=γC\Gamma=\gamma_{\mathcal C} and D+ψ=0D_+\psi=0 in the ν−\nu_- copies with Γ=−γC\Gamma=-\gamma_{\mathcal C}. For ν−=0\nu_-=0 the sector contains ν+\nu_+ copies of a single Weyl block. For YY a flux torus carrying QQ units, YY contributes ∣Q∣\lvert Q\rvert zero modes of one chirality in the cases computed in Example 1.

Proposition 4 moves the question of chirality to C\mathcal C: the multiplicity and the handedness are fixed by DYD_Y, and the propagation of the mode along C\mathcal C is governed by the one-handed block D+D_+ or D−D_- of the retarded operator. The retarded operator DCD_{\mathcal C} has overlap index zero by Theorem 1, so in this construction the chirality of the product theory is carried by YY. Whether D+D_+ propagates a massless one-handed mode is a question about the two-dimensional block, which Section 7 addresses for the signed-BD kernel. By the symmetry u↔vu\leftrightarrow v the statements for D−D_- are the same.

7. Noise and smearing of the two-dimensional kernel

Proposition 1 gives the mean of D+D_+. A single sprinkling gives a random operator whose entries fluctuate, because nxyn_{xy} does. This section computes the fluctuation of one row, and the effect of smearing, for the kernel of Definition 1. The computation is two-dimensional and specific to the layer weights (1,−2,1)(1,-2,1).

Take ρ=1\rho=1 and a rectangular region, and let xx be a point whose past in the region is the rectangle [0,a]×[0,b][0,a]\times[0,b] in the displacements (U,V)(U,V). Given points at xx and yy, the entry D+ε[x,y]=ε2f(nxy,ε)UD^\varepsilon_+[x,y]=\varepsilon^2f(n_{xy},\varepsilon)U is a function of nxy∼Poisson(UV/2)n_{xy}\sim\mathrm{Poisson}(UV/2). Let Fε(x)2=∫Var(D+ε[x,y]∣x,y∈P) 12 dU dVF_\varepsilon(x)^2=\int\mathrm{Var}\big(D_+^\varepsilon[x,y]\mid x,y\in\mathcal P\big)\,\tfrac12\,dU\,dV be the total variance carried by the entries of the row, and Mε(x)2M_\varepsilon(x)^2 the squared norm of the mean row, ∫(E[D+ε[x,y] ∣ x,y])212 dU dV\int\big(\mathbb E[D_+^\varepsilon[x,y]\,\lvert \,x,y]\big)^2\tfrac12\,dU\,dV.

Proposition 5 (row noise; two dimensions). As b→∞b\to\infty with aa fixed,

E ∥rowx∥2=12ε3 6(2−ε)5 a2+O(b−2),Mε2=12ε3 316 a2+O(b−2),Fε2=12ε3[6(2−ε)5−316]a2+O(b−2).(8)\mathbb E\,\lVert{\rm row}_x\rVert^2=\tfrac12\varepsilon^3\,\frac{6}{(2-\varepsilon)^5}\,a^2+O(b^{-2}),\qquad M_\varepsilon^2=\tfrac12\varepsilon^3\,\frac{3}{16}\,a^2+O(b^{-2}),\qquad F_\varepsilon^2=\tfrac12\varepsilon^3\Big[\frac{6}{(2-\varepsilon)^5}-\frac3{16}\Big]a^2+O(b^{-2}). \tag{8}

For ε=1\varepsilon=1 these are 3a23a^2, 332a2\tfrac3{32}a^2 and 9332a2\tfrac{93}{32}a^2; for small ε\varepsilon, Fε2≃1564ε4a2F_\varepsilon^2\simeq\tfrac{15}{64}\varepsilon^4a^2.

Proof. By the Mecke formula E∥rowx∥2=12ε4∫0adU U2∫0bdV E[f(n,ε)2]\mathbb E\lVert {\rm row}_x\rVert ^2=\tfrac12\varepsilon^4\int_0^a dU\,U^2\int_0^b dV\,\mathbb E[f(n,\varepsilon)^2], with n∼Poisson(UV/2)n\sim\mathrm{Poisson}(UV/2). The substitution λ=UV/2\lambda=UV/2 turns the VV integral into (2/U)∫0Ub/2E[f2](λ) dλ(2/U)\int_0^{Ub/2}\mathbb E[f^2](\lambda)\,d\lambda, and for b→∞b\to\infty the upper limit may be removed with an error of order b−2b^{-2}, since E[f2](λ)\mathbb E[f^2](\lambda) decays exponentially. Because ∫0∞e−λλnn!dλ=1\int_0^\infty\frac{e^{-\lambda}\lambda^n}{n!}d\lambda=1, ∫0∞E[f2](λ) dλ=∑nf(n,ε)2\int_0^\infty\mathbb E[f^2](\lambda)\,d\lambda=\sum_nf(n,\varepsilon)^2. Writing q=1−εq=1-\varepsilon, f(n,ε)=qn−2(q2−2nεq+12n(n−1)ε2)f(n,\varepsilon)=q^{n-2}\big(q^2-2n\varepsilon q+\tfrac12 n(n-1)\varepsilon^2\big) for 0<ε<20<\varepsilon<2 (at ε=1\varepsilon=1 read ff as the weights wnw_n), the sum is a combination of ∑nnj‾q2n=j! q2j/(1−q2)j+1\sum_n n^{\underline j}q^{2n}=j!\,q^{2j}/(1-q^2)^{j+1}, where nj‾n^{\underline j} is the falling factorial. Expanding f2f^2 in falling factorials and summing gives ∑nf2=6/[ε(2−ε)5]\sum_nf^2=6/[\varepsilon(2-\varepsilon)^5] exactly. Then ∫0adU U=a2/2\int_0^adU\,U=a^2/2 gives the first formula. For the mean row, E[f(n,ε)]=f0(ελ)\mathbb E[f(n,\varepsilon)]=f_0(\varepsilon\lambda) with f0(z)=e−z(1−2z+z2/2)f_0(z)=e^{-z}(1-2z+z^2/2), and ∫0∞f0(z)2dz=316\int_0^\infty f_0(z)^2dz=\tfrac3{16} gives the second. The variance is the difference. □\square

The numbers 33 and 332\tfrac3{32} are sums over the weights, and the geometry of the region only supplies the factor a2/2a^2/2. At ε=1\varepsilon=1 the entries of a row have a total variance about thirty times the squared norm of the mean row. The ratio Fε2/Mε2=32/(2−ε)5−1F_\varepsilon^2/M_\varepsilon^2=32/(2-\varepsilon)^5-1 decreases to zero like 5ε/25\varepsilon/2 as ε→0\varepsilon\to0.

A plane wave of unit amplitude and wave number k∼π/ak\sim\pi/a has mean action of order kk. If correlations between entries are ignored, the fluctuation of (D+εψ)(x)(D_+^\varepsilon\psi)(x) is of order Fε≃15/64 ε2aF_\varepsilon\simeq\sqrt{15/64}\,\varepsilon^2a for small ε\varepsilon, so the ratio of fluctuation to signal is of order ε2a2\varepsilon^2a^2 in units of the discreteness length. This comparison is heuristic: it keeps only the diagonal part of the variance and drops the correlations between entries that share interval points. Requiring this ratio to be at most one gives ε≲1/a\varepsilon\lesssim 1/a, that is a nonlocality length (ερ)−1/2(\varepsilon\rho)^{-1/2} of order a1/2a^{1/2} discreteness lengths, which grows with the region.

Proposition 6 (smearing squeeze; two dimensions). Fix κ>0\kappa>0 and δ>0\delta>0. The fraction of the box [−κ,κ]2[-\kappa,\kappa]^2 of momenta (in units ρ=1\rho=1) on which ∣Sε(k)∣<δ\lvert S_\varepsilon(k)\rvert <\delta tends to 11 as ε→0\varepsilon\to0.

Proof. By Proposition 1, ∣Sε(k)∣=∣kv∣ ∣h(−2kukv/ε)∣≤C∣kv∣ ε2/(4ku2kv2)\lvert S_\varepsilon(k)\rvert =\lvert k_v\rvert \,\lvert h(-2k_uk_v/\varepsilon)\rvert \le C\lvert k_v\rvert \,\varepsilon^2/(4k_u^2k_v^2) as soon as 2∣kukv∣/ε≥12\lvert k_uk_v\rvert /\varepsilon\ge1, which tends to zero at every point off the axes. The indicator of {∣Sε∣<δ}\{\lvert S_\varepsilon\rvert <\delta\} is bounded by 11 and tends to 11 almost everywhere; dominated convergence gives the claim. □\square

Smearing at a fixed momentum resolution therefore removes the noise of Proposition 5 only by sending the mean symbol to zero over the whole resolved box. The statement depends on the box being held at the discreteness scale. If momenta are resolved only down to the nonlocality scale (ερ)−1/2(\varepsilon\rho)^{-1/2}, the box is rescaled with ε\varepsilon and the squeeze disappears.

Section 6 needs to know whether the unsmeared block D+D_+ annihilates a function of uu alone, as the continuum ∂v\partial_v does. To test this we applied D+D_+, with its prefactor ρ\rho, on two-dimensional sprinklings of the square [0,30]2[0,30]^2 in (u,v)(u,v) to two Gaussian packets, χu(u)\chi_u(u) and χv(v)\chi_v(v), both centred at 1515 with standard deviation 30/830/8. The first is annihilated by ∂v\partial_v and the second is not. The table gives the ratio of the sum of ∣D+ϕ∣2\lvert D_+\phi\rvert^2 over the points to the sum of ∣ϕ∣2\lvert\phi\rvert^2, averaged over five sprinklings (three at ρ=4\rho=4).

ρ\rho χu\chi_u χv\chi_v
1 722±39722\pm39 1092±1391092\pm139
2 2856±1972856\pm197 3886±3473886\pm347
4 10946±50810946\pm508 14667±113214667\pm1132

The continuum values are 00 and 1/(2⋅(30/8)2)=0.0361/(2\cdot(30/8)^2)=0.036, so the squared norm for χv\chi_v is between 3×1043\times10^4 and 4×1054\times10^5 times its continuum value. It exceeds the continuum contrast between the packets by orders of magnitude, since χv\chi_v gives a value larger than χu\chi_u only by a factor between 1.31.3 and 1.51.5, and it grows roughly like ρ2\rho^2. We interpret this as the noise of Proposition 5 acting on the packet. The numbers depend on the packet width and on the normalisation.

8. Whether a bulk-sensitive frame-free index exists

A γ5\gamma_5-Hermitian completion (0A−A†0)\begin{pmatrix}0&A\\-A^\dagger&0\end{pmatrix} of a retarded block A=D+A=D_+ has an advanced block of the same type in the second slot. It is not retarded, its Weyl block is not (anti-)Hermitian, and it is not Krein-self-adjoint for J=σxJ=\sigma_x or σy\sigma_y, so none of the theorems constrains its index. In four dimensions the literal pairing of a σˉ⋅Δ\bar\sigma\cdot\Delta block with a σ⋅Δ\sigma\cdot\Delta block falls under Theorem 1 when both blocks are retarded and under Corollary 1 when the blocks are (anti-)Hermitian.

By formula (5), a retarded operator with a chirally asymmetric on-site term can have a nonzero index. For Theorem 2 the Wilson term must satisfy (K2) together with the rest of the operator, and a non-Hermitian term with WL=WR†W_L=W_R^\dagger does. A construction of either kind of asymmetric term from the causal order and the invariant interval, with a mean symbol that has the correct limit, would settle whether such terms exist.

An involution that commutes with γ5\gamma_5 is outside Theorem 2, which needs Jγ5=−γ5JJ\gamma_5=-\gamma_5J. With J=γ5J=\gamma_5 one has γ5\gamma_5-Hermiticity, the structure of the Euclidean overlap of Example 1. Corollary 1 is the case of this structure in which AA is (anti-)Hermitian, and its index vanishes. The open case is a frame-free kernel AA, built from the causal order and the invariant interval, with AA approximating ∂v\partial_v and −A†-A^\dagger approximating ∂u\partial_u.

Two indices of another kind remain: a non-Hermitian time-domain-wall variant, and an APS-type index in which the bulk identifies infinite-dimensional boundary spaces. Proposition 3 covers only the finite definition with constraints on the domain, and a discrete definition of the second kind across a causal interval of a sprinkling is not known to us.

The Euclidean overlap of Example 1 uses a Wick axis. A frame in the regulator of the scalar line of a Yukawa model shifts the fermion speed at one loop by an amount independent of the cutoff when the scalar mass is small compared with the cutoff (frame leakage), and the reflection-positivity status of the Gaussian-kernel overlap on a Poisson process is described in frames, Wilson terms and reflection positivity.

The estimates of Section 7 hold for a fixed momentum resolution. With a nonlocality scale that grows like ε∼1/a\varepsilon\sim1/a, the fraction of momenta on which the mean symbol is small, and the propagation of a one-handed packet, remain to be determined. Proposition 4 is exact for a product of two point sets; a Poisson process on C×Y\mathcal C\times Y and a smeared DCD_{\mathcal C} fall outside it.

A frame-free operator on a sprinkling with a nonzero bulk-sensitive index would lie outside the classes treated here. No theorem excludes it, and no example is known.

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