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Dispersion relations on lattices with an arithmetic Lorentz group

Status
Proved from the results of section 2 (Borel density, Benoist–Quint, Di Scala–Leistner–Neukirchner, Howe–Moore). Proposition 7 assumes a clustering condition, case 3 of Theorem 3(b) is open, and the packet-response values of section 6 are computed numerically. Broken symmetry, infinitely many fields and states centred on one point carry their own hypotheses (sections 7 and 10).
Excludes
Under exact lattice translations and an exactly preserved Zariski-dense arithmetic Lorentz group such as O(1,3;Z), a dispersion relation for translation-invariant operators on finitely many field components that commute with the group, and any momentum dependence of the two-point function of a positive scalar state other than periodic terms.
Revised

We ask whether a lattice theory with exact lattice translations and an exactly preserved discrete group Γ\Gamma of Lorentz transformations, such as the integer Lorentz group O(1,3;Z)O(1,3;\mathbb Z) acting on Z4\mathbb Z^4, can have a dispersion relation. The answer is no when Γ\Gamma is Zariski dense in the Lorentz group, that is, contained in no proper subgroup cut out by polynomial equations, as O(1,3;Z)O(1,3;\mathbb Z) and its finite-index subgroups are. A translation-invariant operator on finitely many field components that commutes with Γ\Gamma has the same characteristic polynomial at every momentum, so its bands are flat (Theorem 1). The two-point function of a positive translation- and Γ\Gamma-invariant state of a scalar field is uniform in momentum apart from periodic terms (Theorem 2), which covers interacting states because only the two-point function enters.

If Γ\Gamma is a symmetry of the action and the state breaks it, the conclusion persists as long as the unbroken translations have finite index in the lattice and the linear parts of the unbroken symmetries stay Zariski dense (Theorem 3(a)). When the linear parts are not Zariski dense and the unbroken translations have finite index, the remaining symmetry allows a Lorentz-violating quadratic term, in all but one case left open (Theorem 3(b)). A family of infinitely many fields permuted by Γ\Gamma propagates in a Γ\Gamma-invariant state (Example 1). With translations broken to infinite index, section 10 shows that under a clustering hypothesis the correlations of the centre, of spacelike points and of null points with most other points vanish, while pairs inside the cone are not constrained and a Lorentz-invariant field has a state with correlations there. Section 8 shows that the Lorentz action on a non-linear function of the lattice momentum, used in the literature to obtain covariant lattice wave equations, is not induced by any map of the lattice points, and section 9 shows that exact equivariance excludes spectral triples with compact resolvent on the Brillouin quotient.

Integral Lorentz transformations of Z4\mathbb Z^4 and the covariance of lattice wave equations under them were studied by Lorente [Lorente], who obtains covariance by letting the group act on non-linear functions of the lattice momentum. The proofs rest on the Borel density theorem for arithmetic groups, the Benoist–Quint classification of invariant measures and closed invariant sets on the torus [Benoist–Quint] (the proximal case is due to Bourgain, Furman, Lindenstrauss and Mozes [BFLM]), and the classification of irreducible connected groups preserving a Lorentzian form [Di Scala–Leistner–Neukirchner], all stated in section 2. Theorem 1 follows from the fact that every non-zero lattice vector has an infinite Γ\Gamma-orbit; Theorem 2 needs in addition the classification of Γ\Gamma-invariant measures on the Brillouin torus.

Random point sets with a Lorentz-invariant law are the subject of quantum sprinklings (quantum states whose counts are Poisson with a random intensity) and Lorentz-invariant point sets (Haar-random lattices). On kernel-scale kinematics of a single realisation, one realisation of a cocompact orbit lattice is shown to be a lattice with its own translations whose Lorentz stabiliser is a Zariski-dense lattice in SO+(1,3)SO^+(1,3), so Theorem 1 and Proposition 1 below apply to the bounded operators on it and the kernels supported on finitely many shells, with the hypotheses stated there.

1. Conventions

Write B(x,y)=x0y0−x⃗⋅y⃗B(x,y)=x_0y_0-\vec x\cdot\vec y and Q(x)=B(x,x)Q(x)=B(x,x), so the signature is (+,−,−,−)(+,-,-,-) and timelike vectors have Q>0Q>0. The lattice Λ⊂R4\Lambda\subset\mathbb R^4 has rank 4 and Γ⊂O(1,3)\Gamma\subset O(1,3) is a group with gΛ=Λg\Lambda=\Lambda for g∈Γg\in\Gamma, so that Γ\Gamma acts on Λ\Lambda through GL(Λ)≅GL(4,Z)GL(\Lambda)\cong GL(4,\mathbb Z). The Brillouin torus is T=R4/2πΛ∨\mathbb T=\mathbb R^4/2\pi\Lambda^\vee with Λ∨={k:k⋅v∈Z ∀v∈Λ}\Lambda^\vee=\{k: k\cdot v\in\mathbb Z\ \forall v\in\Lambda\}, and its characters are χv(k)=eik⋅v\chi_v(k)=e^{ik\cdot v}, v∈Λv\in\Lambda. The group acts on T\mathbb T by g⋅k=(g−1)Tkg\cdot k=(g^{-1})^{T}k, the action for which

χv(g⋅k)=χg−1v(k).(1)\chi_v(g\cdot k)=\chi_{g^{-1}v}(k). \tag{1}

For g∈O(1,3)g\in O(1,3) one has (g−1)T=ηgη(g^{-1})^T=\eta g\eta with η=diag(1,−1,−1,−1)\eta=\mathrm{diag}(1,-1,-1,-1), so the action on T\mathbb T is equivalent to the vector action.

The Fourier transform f^(k)=∑xf(x)e−ik⋅x\hat f(k)=\sum_xf(x)e^{-ik\cdot x} identifies ℓ2(Λ)⊗V\ell^2(\Lambda)\otimes V with L2(T;V)L^2(\mathbb T;V). Here V=CNV=\mathbb C^N is the space of field components and σ:Γ→GL(V)\sigma:\Gamma\to GL(V) a finite-dimensional representation, not necessarily unitary (for spinors, the spin representation). Translation (Taf)(x)=f(x−a)(T_af)(x)=f(x-a) becomes multiplication by e−ik⋅ae^{-ik\cdot a}, and the Lorentz action (Ugf)(x)=σ(g)f(g−1x)(U_gf)(x)=\sigma(g)f(g^{-1}x) becomes

(UgF)(k)=σ(g)F(g−1⋅k).(2)(U_gF)(k)=\sigma(g)F(g^{-1}\cdot k). \tag{2}

A symbol is a measurable map d:T→MN(C)d:\mathbb T\to M_N(\mathbb C), defining (DF)(k)=d(k)F(k)(DF)(k)=d(k)F(k). Every operator commuting with all TaT_a is of this form (proof of Theorem 1). The dispersion relations are the eigenvalues of d(k)d(k) as functions of kk.

Two hypotheses on Γ\Gamma are used.

(F) Every Γ\Gamma-orbit on Λ∖{0}\Lambda\setminus\{0\} is infinite.

(H1) The Zariski closure of Γ\Gamma in GL(4,R)GL(4,\mathbb R) contains the identity component SO(1,3)∘SO(1,3)^\circ of the Lorentz group.

The Zariski closure of a set of matrices is the smallest set, cut out by polynomial equations in the matrix entries, that contains it; Γ\Gamma satisfies (H1) when every polynomial that vanishes on Γ\Gamma vanishes on SO(1,3)∘SO(1,3)^\circ. A group that is Zariski dense in this sense is not contained in any proper algebraic subgroup, so it fixes no non-zero vector and no proper subspace that SO(1,3)∘SO(1,3)^\circ does not. Arithmetic groups such as O(1,3;Z)O(1,3;\mathbb Z), the integer matrices preserving QQ, are discrete subgroups of the Lorentz group and nevertheless Zariski dense; this is the content of the Borel density theorem (Theorem C1).

Lemma 1 below shows that (H1) implies (F). Condition (F) alone is used in Lemma 2, Theorem 1 and Theorem 4, and it makes sense in lower dimension too. For Λ=Z2\Lambda=\mathbb Z^2 with the form t2−x2t^2-x^2, an integer matrix preserving the form has first column (a,c)(a,c) with a2−c2=1a^2-c^2=1, so a=±1a=\pm1, c=0c=0, and Γ={diag(±1,±1)}\Gamma=\{\mathrm{diag}(\pm1,\pm1)\} is finite. The orbit of e0e_0 is {±e0}\{\pm e_0\}, (F) fails, and the usual lattice Klein–Gordon operator with a non-trivial dispersion relation is an invariant example. For the form t2−2x2t^2-2x^2, the matrix A=(3423)A=\begin{pmatrix}3&4\\2&3\end{pmatrix} preserves it, has eigenvalues 3±223\pm2\sqrt2, and no non-zero vector of Z2\mathbb Z^2 has a finite ⟨A⟩\langle A\rangle-orbit; (F) holds, and Theorem 1 forbids a dispersion relation even in 1+1 dimensions.

2. The cited theorems

The following results are used without proof, in the form in which they are applied.

Theorem C1 (Borel density; Borel–Harish-Chandra). If G\mathcal G is the group of real points of a semisimple algebraic group over Q\mathbb Q without compact factors, then G∩GL(n,Z)\mathcal G\cap GL(n,\mathbb Z) is a lattice in G\mathcal G (Borel and Harish-Chandra [BHC]), and every lattice in G\mathcal G is Zariski dense in G\mathcal G (Borel [Borel]). Consequently (H1) holds for every finite-index subgroup of O(1,3;Z)O(1,3;\mathbb Z) and, more generally, of the automorphism group of any integral quadratic form of signature (1,3)(1,3), such as 7x02−x12−x22−x327x_0^2-x_1^2-x_2^2-x_3^2. The same applies to signature (1,2)(1,2).

Theorem C2 (Benoist–Quint [Benoist–Quint], Theorem 1.3 and Corollary 1.4). Let Γ0\Gamma_0 be a subsemigroup of SL(d,Z)SL(d,\mathbb Z) acting strongly irreducibly on Rd\mathbb R^d, meaning that every finite-index subgroup of the group it generates acts irreducibly. On the torus Rd/Zd\mathbb R^d/\mathbb Z^d: (a) the only Γ0\Gamma_0-invariant Borel probability measure without atoms is the Haar measure; (b) the only closed infinite Γ0\Gamma_0-invariant subset is the whole torus. As recorded in that paper, part (b) for such groups is due to Muchnik and to Guivarc’h and Starkov, and part (a) under a proximality assumption to Bourgain, Furman, Lindenstrauss and Mozes [BFLM].

Theorem C3 (Di Scala, Leistner, Neukirchner [Di Scala–Leistner–Neukirchner]). A connected subgroup of GL(n,R)GL(n,\mathbb R) that acts irreducibly on Rn\mathbb R^n and leaves invariant a bilinear form of Lorentzian signature is conjugate to SO(1,n−1)∘SO(1,n-1)^\circ.

Theorem C4 (Howe–Moore [Howe–Moore]). If π\pi is a unitary representation of a connected non-compact simple Lie group with finite centre, such as SO+(1,3)≅PSL(2,C)SO^+(1,3)\cong PSL(2,\mathbb C), and π\pi has no non-zero invariant vector, then every matrix coefficient ⟨ψ,π(h)ψ′⟩\langle\psi,\pi(h)\psi'\rangle tends to 0 as h→∞h\to\infty in the group.

Under (H1) the group Γ+=Γ∩SL(4,Z)\Gamma^+=\Gamma\cap SL(4,\mathbb Z), of index at most 2, still has Zariski closure containing SO(1,3)∘SO(1,3)^\circ and acts strongly irreducibly: a finite-index subgroup has Zariski closure of finite index in that of Γ\Gamma, hence containing SO(1,3)∘SO(1,3)^\circ, which acts irreducibly because it contains boosts in every (0,j)(0,j)-plane and all rotations. So C2 applies to Γ+\Gamma^+ acting on T\mathbb T, and a fortiori to measures and sets invariant under Γ\Gamma.

C1 supplies (H1) for the arithmetic groups named above and is used again for the stabilisers of section 10. C2 enters Corollary 1, Proposition 1 and Theorem 2 (and Theorem 3(a) through Theorem 2), C3 enters Theorem 3(b), and C4 enters Proposition 8. The other statements are derived from (F) or (H1) alone.

3. No finite orbits, no finite-dimensional invariant subspaces

A Γ\Gamma-orbit on the Brillouin torus is either finite, in which case its points are torsion points, or infinite, and no finite-dimensional space of functions on the torus is invariant apart from the constants.

Lemma 1 (no finite orbits). Assume (H1). Then (F) holds. A point of T\mathbb T has a finite Γ\Gamma-orbit if and only if it is a torsion point, that is, a point of finite order in the group T\mathbb T.

Proof. If Γv\Gamma v is finite, a finite-index subgroup Γ′\Gamma' fixes vv. The condition gv=vgv=v is polynomial in gg, so the Zariski closure of Γ′\Gamma' also fixes vv. That closure contains SO(1,3)∘SO(1,3)^\circ, which fixes no non-zero vector: a vector with v0≠0v_0\ne0 is moved by a boost, and one with v0=0v_0=0, v⃗≠0\vec v\ne0 by a rotation about an axis orthogonal to v⃗\vec v. Hence v=0v=0.

Torsion points of a given order are finitely many and form a Γ\Gamma-invariant set, so they have finite orbits. Conversely, let kk have a finite orbit and let Γ′\Gamma' be the finite-index subgroup fixing it. The fixed set Fix(Γ′)∋k\mathrm{Fix}(\Gamma')\ni k is a closed subgroup of T\mathbb T whose identity component is a subtorus S=exp⁡sS=\exp\mathfrak s, s⊂R4\mathfrak s\subset\mathbb R^4. Since Γ′\Gamma' fixes SS pointwise, it fixes every vector of s\mathfrak s under the linear action g↦(g−1)T=ηgηg\mapsto(g^{-1})^T=\eta g\eta. By the argument of the first paragraph, applied to this equivalent representation, s=0\mathfrak s=0. A compact group with trivial identity component is finite, so kk has finite order. □\square

Lemma 2 (weak mixing and ergodicity). Assume (F). Let L02(T)L^2_0(\mathbb T) be the orthogonal complement of the constants in L2(T)L^2(\mathbb T), and (Kgf)(k)=f(g−1⋅k)(K_gf)(k)=f(g^{-1}\cdot k). (i) L02(T)L^2_0(\mathbb T) contains no non-zero finite-dimensional KK-invariant subspace. (ii) Every measurable function h:T→Ch:\mathbb T\to\mathbb C with h(g⋅k)=h(k)h(g\cdot k)=h(k) almost everywhere for each g∈Γg\in\Gamma is almost everywhere constant.

Proof. (i) By (1), the Fourier transform turns KgK_g into the permutation operator f↦f∘g−1f\mapsto f\circ g^{-1} on ℓ2(Λ)\ell^2(\Lambda), and L02L^2_0 into ℓ2(Λ∖{0})\ell^2(\Lambda\setminus\{0\}). Suppose F⊂ℓ2(Λ∖{0})F\subset\ell^2(\Lambda\setminus\{0\}) is a non-zero finite-dimensional invariant subspace. Pick f∈Ff\in F and v0v_0 with f(v0)≠0f(v_0)\ne0. By (F) there are gn∈Γg_n\in\Gamma with the points gnv0g_nv_0 pairwise distinct. The vectors f∘gn−1f\circ g_n^{-1} lie on a sphere in FF, which is compact, so a subsequence converges in norm. But (f∘gn−1)(gnv0)=f(v0)(f\circ g_n^{-1})(g_nv_0)=f(v_0), while for fixed mm the values (f∘gm−1)(gnv0)=f(gm−1gnv0)(f\circ g_m^{-1})(g_nv_0)=f(g_m^{-1}g_nv_0) tend to 0 as n→∞n\to\infty, because f∈ℓ2f\in\ell^2 and the points gm−1gnv0g_m^{-1}g_nv_0 are pairwise distinct. Passing inductively to a subsequence with ∣f(gm−1gnv0)∣≤∣f(v0)∣/2\lvert f(g_m^{-1}g_nv_0)\rvert \le\lvert f(v_0)\rvert /2 for m<nm<n gives ∥f∘gn−1−f∘gm−1∥≥∣f(v0)∣/2\lVert f\circ g_n^{-1}-f\circ g_m^{-1}\rVert \ge\lvert f(v_0)\rvert /2 for all m<nm<n, so no subsequence is Cauchy. This contradicts compactness.

(ii) The functions arctan⁡Re⁡h\arctan\operatorname{Re}h and arctan⁡Im⁡h\arctan\operatorname{Im}h are bounded, hence in L2L^2, and invariant. An invariant function u∈L2u\in L^2 gives the one-dimensional invariant subspace spanned by u−∫uu-\int u in L02L^2_0, which is zero by (i). Since arctan⁡\arctan is injective, hh is constant almost everywhere. □\square

4. Operators that commute with translations and with the group

Theorem 1 (constant symbols). Assume (F). Let DD be a bounded operator, or a self-adjoint operator, on ℓ2(Λ)⊗V\ell^2(\Lambda)\otimes V with V=CNV=\mathbb C^N, N<∞N<\infty, that commutes with every TaT_a, a∈Λa\in\Lambda, and every UgU_g, g∈Γg\in\Gamma. Then DD is the multiplication by a symbol dd with d(g⋅k)=σ(g)d(k)σ(g)−1d(g\cdot k)=\sigma(g)d(k)\sigma(g)^{-1} almost everywhere, and:

(a) if N=1N=1 (σ\sigma is then a character), dd is almost everywhere a constant d0d_0 and D=d0⋅1D=d_0\cdot1;

(b) for general NN, the characteristic polynomial of d(k)d(k) is almost everywhere independent of kk, so every band of the dispersion relation is flat;

(c) if DD is bounded, then dd is almost everywhere a constant matrix d0d_0, and d0=σ(g)d0σ(g)−1d_0=\sigma(g)d_0\sigma(g)^{-1} for all g∈Γg\in\Gamma.

Translation invariance turns the operator into a function on the torus, and invariance under Γ\Gamma makes that function constant on the orbits of an ergodic action. The input is (F); the remaining steps are routine.

Proof. The operators TaT_a generate, on L2(T)⊗VL^2(\mathbb T)\otimes V, the von Neumann algebra L∞(T)⊗1L^\infty(\mathbb T)\otimes1 of multiplications by characters and their limits. Its commutant is L∞(T)⊗MN(C)L^\infty(\mathbb T)\otimes M_N(\mathbb C), because L∞(T)L^\infty(\mathbb T) is maximal abelian on L2(T)L^2(\mathbb T). A bounded operator commuting with all TaT_a is therefore a bounded matrix symbol, and a self-adjoint one has its spectral projections in the commutant, so it is a multiplier by a measurable Hermitian symbol. Commutation with UgU_g and (2) give d(k)σ(g)F(g−1⋅k)=σ(g)d(g−1⋅k)F(g−1⋅k)d(k)\sigma(g)F(g^{-1}\cdot k)=\sigma(g)d(g^{-1}\cdot k)F(g^{-1}\cdot k) for all FF, which is the stated covariance.

(a) dd is a measurable function with d(g⋅k)=d(k)d(g\cdot k)=d(k), so it is constant by Lemma 2(ii).

(b) For each jj the function k↦tr⁡d(k)jk\mapsto\operatorname{tr}d(k)^j is measurable and invariant, hence constant by Lemma 2(ii). The coefficients of the characteristic polynomial are polynomials in these traces (Newton’s identities).

(c) The entries of dd are bounded, hence in L2(T)L^2(\mathbb T). By the covariance, the entries of d∘gd\circ g are linear combinations of the entries of dd, so the span of the entries is a finite-dimensional invariant subspace of L2(T)L^2(\mathbb T). Its projection onto L02L^2_0 is again finite-dimensional and invariant, hence zero by Lemma 2(i). □\square

For bounded DD and N=1N=1 there is a direct argument without ergodic theory: the kernel c=Dδ0c=D\delta_0 lies in ℓ2(Λ)\ell^2(\Lambda) and is constant on Γ\Gamma-orbits, and the orbits of non-zero vectors are infinite, so c=c(0)δ0c=c(0)\delta_0. The ergodic form covers unbounded operators and the matrix case.

Remark 1 (a sublattice of translations). Translation invariance under all of Λ\Lambda is used. Suppose only a Γ\Gamma-stable sublattice Λ′\Lambda' of finite index is a translation symmetry, and let DD be a bounded scalar operator (N=1N=1) commuting with the translations by Λ′\Lambda' and with Γ\Gamma, with kernel D(x,y)D(x,y). The column fy=Dδyf_y=D\delta_y is square summable. Let Γy⊂Γ\Gamma_y\subset\Gamma be the finite-index subgroup of elements gg with gy−y∈Λ′gy-y\in\Lambda'. For g∈Γyg\in\Gamma_y the affine map h(x)=gx−(gy−y)h(x)=gx-(gy-y) fixes yy and is a product of gg and a translation by Λ′\Lambda', so fy(y+z)f_y(y+z) is invariant under z↦gzz\mapsto gz for g∈Γyg\in\Gamma_y. Orbits of Γy\Gamma_y on Λ∖{0}\Lambda\setminus\{0\} are infinite, because the Γ\Gamma-orbit of a vector is a finite union of Γy\Gamma_y-orbits and is infinite by (F). A square-summable function that is constant on infinite orbits vanishes there, so fy=D(y,y)δyf_y=D(y,y)\delta_y. Hence DD is multiplication by a function of the class of xx modulo Λ′\Lambda', constant on Γ\Gamma-orbits of classes: a constant matrix, diagonal in the coset basis, and not in general a multiple of the identity. An example is the staggered mass for Λ=Z4\Lambda=\mathbb Z^4: since Q(x)≡x0+x1+x2+x3(mod2)Q(x)\equiv x_0+x_1+x_2+x_3\pmod2, the function m(x)=(−1)Q(x)m(x)=(-1)^{Q(x)} is Γ\Gamma-invariant, commutes with translations by the Γ\Gamma-stable even sublattice {Q even}\{Q\ \text{even}\}, and does not commute with translation by e0e_0. Operators that are Γ\Gamma-invariant without translation invariance exist (any multiplication by a function of Q(x)Q(x)).

Corollary 1 (low momenta are dense in the zone). Assume (H1). For every non-torsion k∈Tk\in\mathbb T the orbit Γ⋅k\Gamma\cdot k is dense in T\mathbb T.

Proof. By Lemma 1 the orbit is infinite, and so is the orbit under Γ+\Gamma^+, which satisfies (H1) as well. Its closure is a closed infinite Γ+\Gamma^+-invariant set, hence the whole torus by C2(b). □\square

A lattice momentum kk is non-torsion as soon as k⋅v/2πk\cdot v/2\pi is irrational for some v∈Λv\in\Lambda. For such a kk of small norm, some g∈Γg\in\Gamma maps it arbitrarily close to any prescribed point of the zone, the zone boundary included. A symmetry that identifies low momenta with momenta at the cutoff leaves no separate low-energy description. By Borel density a continuum effective action with Γ\Gamma-invariant polynomial coefficients has Lorentz-invariant coefficients, since an invariant tensor is fixed by the Zariski closure; Theorem 1 and Corollary 1 show that the lattice theory itself has no low-energy sector on which that protection could act.

Proposition 1 (shell sums have no dispersion on any open set). Assume (H1). Let c:Λ→Cc:\Lambda\to\mathbb C be a bounded Γ\Gamma-invariant function that vanishes outside finitely many shells {Q=q}\{Q=q\} and is non-zero at some v≠0v\ne0. Then its Fourier series c^\hat c, a distribution on T\mathbb T, coincides with an integrable function on no non-empty open subset of T\mathbb T.

The point is that invariance carries a local integrable representation of c^\hat c over the whole torus, where ergodicity makes it constant; what is left is supported on finitely many torsion points, where the Fourier coefficients are polynomials times periodic functions, and vanishing on all but finitely many shells then forces them to vanish.

Proof. Suppose c^=h\hat c=h on an open set U≠∅U\ne\emptyset with h∈Lloc1(U)h\in L^1_{\rm loc}(U). Since c^\hat c is Γ\Gamma-invariant, it equals h∘g−1h\circ g^{-1} on gUgU, and these local functions agree on overlaps because c^\hat c is one distribution; so c^=h~\hat c=\tilde h on the open invariant set ΓU\Gamma U, with h~∈Lloc1\tilde h\in L^1_{\rm loc} invariant. The indicator of ΓU\Gamma U is invariant, hence almost everywhere constant by Lemma 2(ii), and equal to 1 since UU has positive measure; so ΓU\Gamma U is conull and h~\tilde h is almost everywhere a constant κ\kappa. The closed invariant set Z=T∖ΓUZ=\mathbb T\setminus\Gamma U is not the whole torus, so by C2(b) it is finite, and by Lemma 1 it consists of torsion points. The distribution c^−κ\hat c-\kappa is supported on ZZ, hence is a finite sum of derivatives of delta functions at points of ZZ. Inverting the Fourier series, c(v)=κδv,0+∑z∈Zpz(v)eiz⋅vc(v)=\kappa\delta_{v,0}+\sum_{z\in Z}p_z(v)e^{iz\cdot v} with polynomials pzp_z.

Let v0≠0v_0\ne0 have c(v0)≠0c(v_0)\ne0. Let M≥2M\ge2 be an integer such that Mz∈2πΛ∨Mz\in2\pi\Lambda^\vee for all z∈Zz\in Z and v0∉MΛv_0\notin M\Lambda. On the coset v0+MΛv_0+M\Lambda, which does not contain 0, each factor eiz⋅ve^{iz\cdot v} is constant, so cc coincides there with a single polynomial pp. The points of the coset outside the finitely many shells form a Zariski-dense subset of R4\mathbb R^4 (a polynomial vanishing on them, multiplied by ∏q(Q−q)\prod_q(Q-q), vanishes on the whole coset, which is Zariski dense), and pp vanishes on them. So p≡0p\equiv0 and c(v0)=0c(v_0)=0, a contradiction. □\square

The proposition applies to the kernels of causal-set-inspired lattice operators that sum interior-count weights over finitely many shells; on a lattice with a Zariski-dense Γ\Gamma such a kernel is a distribution that is not a function.

5. Invariant states

Section 4 concerns operators. A state, free or interacting, gives a two-point function, and the next theorem applies to that function directly; it covers interacting and non-perturbative states.

Theorem 2 (invariant two-point functions are flat plus periodic). Assume (H1). Let ω\omega be a positive linear functional on a ∗\ast-algebra containing elements ϕ(x)\phi(x), x∈Λx\in\Lambda, and set W(x,y)=ω(ϕ(x)∗ϕ(y))W(x,y)=\omega(\phi(x)^\ast\phi(y)). Suppose W(x+a,y+a)=W(x,y)W(x+a,y+a)=W(x,y) for a∈Λa\in\Lambda and W(gx,gy)=W(x,y)W(gx,gy)=W(x,y) for g∈Γg\in\Gamma. Then

W(x,y)=a0 δx,y+∑ObO 1∣O∣∑k∈Oeik⋅(y−x),(3)W(x,y)=a_0\,\delta_{x,y}+\sum_{O}b_O\,\frac1{\lvert O\rvert }\sum_{k\in O}e^{ik\cdot(y-x)}, \tag{3}

where a0≥0a_0\ge0, the sum runs over the countably many finite Γ\Gamma-orbits OO of torsion points of T\mathbb T, bO≥0b_O\ge0, and a0+∑ObO=W(0,0)<∞a_0+\sum_Ob_O=W(0,0)<\infty.

The spectral measure of the two-point function is a multiple of Haar measure plus atoms at torsion points. The Haar part is the same at every momentum, and the atoms at rational wave vectors give correlations that do not decay with distance; no part has a non-trivial dependence on kk.

Proof. Positivity gives ∑λˉxλyW(x,y)=ω((∑λxϕ(x))∗(∑λyϕ(y)))≥0\sum\bar\lambda_x\lambda_yW(x,y)=\omega\big((\sum\lambda_x\phi(x))^\ast(\sum\lambda_y\phi(y))\big)\ge0. Put w(v)=W(0,v)w(v)=W(0,v); translation invariance gives W(x,y)=w(y−x)W(x,y)=w(y-x), and ww is a positive-definite function on Λ\Lambda. By Bochner’s theorem for the discrete group Λ\Lambda, w(v)=∫Teik⋅vdμ(k)w(v)=\int_{\mathbb T}e^{ik\cdot v}d\mu(k) for a unique finite positive measure μ\mu with μ(T)=w(0)\mu(\mathbb T)=w(0). From w(gv)=W(g0,gv)=w(v)w(gv)=W(g0,gv)=w(v) and (1), the measure g∗μg_\ast\mu has the same Fourier coefficients as μ\mu, so μ\mu is Γ\Gamma-invariant.

Decompose μ=μc+μp\mu=\mu_{\rm c}+\mu_{\rm p} into non-atomic and purely atomic parts; both are Γ\Gamma-invariant because Γ\Gamma acts by homeomorphisms. By C2(a), μc=a0⋅Haar\mu_{\rm c}=a_0\cdot\text{Haar} (Haar normalised to total mass 1). The atomic part is ∑kmkδk\sum_km_k\delta_k with mkm_k constant on orbits and summable, so an orbit carrying positive mass is finite, and by Lemma 1 its points are torsion. With bO=∣O∣mkb_O=\lvert O\rvert m_k for k∈Ok\in O this is (3), and evaluation at x=yx=y gives the sum rule. □\square

If only a Γ\Gamma-stable finite-index sublattice Λ′\Lambda' is a translation symmetry, the theorem applies to the sub-algebra generated by ϕ(x)\phi(x), x∈Λ′x\in\Lambda'.

Positivity is used in an essential way. The shell function c=1{Q=1}c=\mathbf 1_{\{Q=1\}} is Γ\Gamma-invariant, defines a translation-invariant kernel, and has c(0)=0c(0)=0; in (3) this would force a0=bO=0a_0=b_O=0 and so w≡0w\equiv0. It is therefore the two-point function of no positive state, and a kernel of this kind can arise only from a state on an indefinite-metric space. For such kernels Proposition 1 still forbids a dispersion relation on an open set of momenta.

For a field with several components in a non-unitary representation σ\sigma the trace of the matrix-valued spectral measure is only quasi-invariant, and the argument above does not apply as written; Theorem 1 covers such fields for operators.

Remark 2 (infinite invariant measures). The finiteness of μ\mu is essential. Infinite Γ\Gamma-invariant measures on T\mathbb T exist, for example counting measure on a dense orbit, but they are not Radon on the compact torus and cannot be spectral measures of a state, for which μ(T)=W(0,0)\mu(\mathbb T)=W(0,0).

6. Packet response of shell kernels

Section 4 shows that a Γ\Gamma-invariant lattice operator has no symbol to expand in momentum. One can ask instead what a localised probe sees. A finite-norm packet ϕ(x)=eip⋅xf(x)\phi(x)=e^{ip\cdot x}f(x), with ff real, decaying and normalised to ∥f∥=1\lVert f\rVert=1, is what a dispersion relation is read off from. A kernel supported on a shell {Q=q}\{Q=q\} sums over infinitely many lattice vectors, so the sum has to be cut off, and here the packet envelope cuts it off. Let DD have kernel cc with c(−v)=c(v)c(-v)=c(v), so ⟨ϕ,Dϕ⟩=∑x,vϕˉ(x)c(v)ϕ(x+v)\langle\phi,D\phi\rangle=\sum_{x,v}\bar\phi(x)c(v)\phi(x+v). Summing over xx gives

⟨ϕ,Dϕ⟩=∑vc(v)cos⁡(p⋅v)E(v),E(v)=∑xf(x)f(x+v),(4)\langle\phi,D\phi\rangle=\sum_{v}c(v)\cos(p\cdot v)E(v),\qquad E(v)=\sum_xf(x)f(x+v), \tag{4}

where EE is the envelope autocorrelation, E(0)=1E(0)=1. For the Gaussian envelope f(x)∝e−∣x∣E2/2L2f(x)\propto e^{-\lvert x\rvert_{\rm E}^2/2L^2} of width LL in the Euclidean norm, E(v)∝e−∣v∣E2/4L2E(v)\propto e^{-\lvert v\rvert _{\rm E}^2/4L^2} up to corrections exponentially small in L2L^2, with the constant fixed by E(0)=1E(0)=1; this form is used below. Expanding the cosine, the packet sees S0−12pμpνΠμν+O(p4)S_0-\tfrac12p_\mu p_\nu \Pi^{\mu\nu}+O(p^4) with

Πμν=∑vc(v)E(v) vμvν,S0=∑vc(v)E(v).(5)\Pi^{\mu\nu}=\sum_vc(v)E(v)\,v^\mu v^\nu,\qquad S_0=\sum_vc(v)E(v). \tag{5}

A Lorentz-invariant low-energy dispersion requires Πμν∝ημν\Pi^{\mu\nu}\propto\eta^{\mu\nu}, that is ρ:=Π00/(−Π11)=+1\rho:=\Pi^{00}/(-\Pi^{11})=+1 with the three spatial entries equal.

Proposition 2 (positive kernels give an elliptic packet response). Let c(−v)=c(v)c(-v)=c(v) and E>0E>0. (i) If c≥0c\ge0 and c(v)≠0c(v)\ne0 for some v≠0v\ne0, then Π\Pi is positive semidefinite and non-zero, hence not proportional to ημν\eta^{\mu\nu}, and ρ≤0\rho\le0 where defined. (ii) For a shell kernel c=1{Q=q}c=\mathbf 1_{\{Q=q\}} on a lattice for which cc and EE are symmetric under permutations of the three spatial axes,

ρ=−3⟨t2⟩⟨t2⟩−q,⟨t2⟩=∑vc(v)E(v)v02S0,(6)\rho=-\frac{3\langle t^2\rangle}{\langle t^2\rangle-q},\qquad \langle t^2\rangle=\frac{\sum_{v}c(v)E(v)v_0^2}{S_0}, \tag{6}

exactly. (iii) Let Λ=Z4\Lambda=\mathbb Z^4 with the standard form, E=ELE=E_L the Gaussian above, and let the shell {Q=q}\{Q=q\} contain a non-zero vector. Then ρ→−3\rho\to-3 as L→∞L\to\infty. For q=0q=0, ρ=−3\rho=-3 for every LL.

Proof. (i) xTΠx=∑cE (x⋅v)2≥0x^T\Pi x=\sum cE\,(x\cdot v)^2\ge0 for every real xx, and the trace ∑cE ∣v∣E2\sum cE\,\lvert v\rvert _{\rm E}^2 is positive. A non-zero positive semidefinite form is not proportional to the indefinite ημν\eta^{\mu\nu}. Moreover Π00≥0\Pi^{00}\ge0 and Π11≥0\Pi^{11}\ge0, so ρ=−Π00/Π11≤0\rho=-\Pi^{00}/\Pi^{11}\le0 where Π11≠0\Pi^{11}\ne0.

(ii) On the shell v02=q+∣v⃗∣2v_0^2=q+\lvert \vec v\rvert ^2, and by the permutation symmetry Π11=13∑cE ∣v⃗∣2=13(Π00−qS0)\Pi^{11}=\tfrac13\sum cE\,\lvert \vec v\rvert ^2=\tfrac13(\Pi^{00}-qS_0). Hence ρ=−3Π00/(Π00−qS0)\rho=-3\Pi^{00}/(\Pi^{00}-qS_0), which is (6).

(iii) The symmetry hypotheses of (ii) hold for Z4\mathbb Z^4 and the Euclidean Gaussian. Let T0>0T_0>0 and let n(T0)n(T_0) be the number of shell points with ∣v0∣≤T0\lvert v_0\rvert \le T_0; it is finite because ∣v⃗∣2=v02−q\lvert \vec v\rvert ^2=v_0^2-q. The shell is infinite by (F), which holds for Γ=O(1,3;Z)\Gamma=O(1,3;\mathbb Z), and EL→1E_L\to1 pointwise as L→∞L\to\infty, so S0→∞S_0\to\infty by Fatou’s lemma. The weight carried by ∣v0∣≤T0\lvert v_0\rvert \le T_0 is at most n(T0)n(T_0), so ⟨t2⟩≥T02(1−n(T0)/S0)→T02\langle t^2\rangle\ge T_0^2(1-n(T_0)/S_0)\to T_0^2. As T0T_0 is arbitrary, ⟨t2⟩→∞\langle t^2\rangle\to\infty and (6) gives ρ→−3\rho\to-3. For q=0q=0, (6) equals −3-3 identically. □\square

The tensor tends to Π00 diag(1,13,13,13)\Pi^{00}\,\mathrm{diag}(1,\tfrac13,\tfrac13,\tfrac13), that of null dust: boosted copies of the shell lie almost along the light cone and dominate the sum. In the rest frame of the envelope, with time direction uu, the packet sees the elliptic quadratic form p02+∣p⃗∣2/3p_0^2+\lvert\vec p\rvert^2/3 instead of p02−∣p⃗∣2p_0^2-\lvert \vec p\rvert ^2. A packet boosted by a different rapidity sees a different Π\Pi, so the envelope picks a frame, and the Lorentz-violating coefficient is of order one. How a frame in a regulator enters low-energy coefficients is the subject of Where a preferred frame leaks into low-energy physics.

Direct summation of (4) and (5) for Λ=Z4\Lambda=\mathbb Z^4 and the shell Q=1Q=1, truncated where the weight is below 10−1210^{-12}, gives the following values, which show the rate of approach to −3-3 in Proposition 2(iii).

LL 4 8 16
ρ\rho −3.0931-3.0931 −3.0232-3.0232 −3.0059-3.0059

For kernels with weights of both signs, such as retuned d’Alembertians, part (i) does not apply. Whether ρ\rho is then near −3-3 depends on cancellations between shells, and Proposition 2 does not determine the value of ρ\rho for them.

7. Spontaneous breaking of the discrete Lorentz group

Theorem 2 assumes an invariant state. Suppose instead that the action is invariant under Γ⋉Λ\Gamma\ltimes\Lambda, the group of affine maps x↦gx+ax\mapsto gx+a with g∈Γg\in\Gamma, a∈Λa\in\Lambda, and that the state is invariant only under a subgroup SS. Let Λ′=S∩Λ\Lambda'=S\cap\Lambda be the unbroken translations and

H={g∈Γ: (g,a)∈S for some a∈Λ}H=\{g\in\Gamma:\ (g,a)\in S\ \text{for some }a\in\Lambda\}

the group of linear parts of the unbroken symmetries. An unbroken symmetry can be a linear map composed with a translation that is not itself a symmetry, so HH can be larger than S∩ΓS\cap\Gamma.

The statement of Theorem 3 uses Λ′\Lambda', HH, S∩ΓS\cap\Gamma and the identity component H0H_0 of the Zariski closure of HH (defined below). The action of HH on Λ/Λ′\Lambda/\Lambda' serves only to compare S∩ΓS\cap\Gamma with HH.

The group HH preserves Λ′\Lambda', because (g,a) tb (g,a)−1=tgb(g,a)\,t_b\,(g,a)^{-1}=t_{gb}. For h∈Hh\in H choose aha_h with (h,ah)∈S(h,a_h)\in S; it is determined modulo Λ′\Lambda', and ahk≡hak+aha_{hk}\equiv ha_k+a_h. So HH acts on the quotient Λ/Λ′\Lambda/\Lambda' by h⋅[x]=[hx+ah]h\cdot[x]=[hx+a_h], and S∩Γ={h:(h,0)∈S}S\cap\Gamma=\{h:(h,0)\in S\} is the stabiliser of the class [0][0]. If Λ′\Lambda' has finite index in Λ\Lambda, S∩ΓS\cap\Gamma therefore has finite index in HH, at most [Λ:Λ′][\Lambda:\Lambda']. If Λ′\Lambda' has infinite index the two can differ completely: for a state centred at a lattice point pp, S=tpΓtp−1S=t_p\Gamma t_p^{-1}, so H=ΓH=\Gamma while S∩Γ=StabΓ(p)S\cap\Gamma=\mathrm{Stab}_\Gamma(p) is finite when pp is timelike.

Write Hˉ\bar H for the Zariski closure of HH in GL(4,R)GL(4,\mathbb R) and H0H_0 for the identity component, in the Lie-group topology, of its real points. Since H⊂O(1,3)H\subset O(1,3) and Hˉ\bar H is algebraic, H0⊂SO(1,3)∘H_0\subset SO(1,3)^\circ. A real algebraic group has finitely many connected components, so H0H_0 has finite index in Hˉ(R)\bar H(\mathbb R) and H∩H0H\cap H_0 has finite index in HH. Conjugation by h∈Hh\in H preserves Hˉ(R)\bar H(\mathbb R), so HH normalises H0H_0. Finally H0=SO(1,3)∘H_0=SO(1,3)^\circ if and only if Hˉ⊃SO(1,3)∘\bar H\supset SO(1,3)^\circ, which is (H1) for HH.

An effective quadratic action for the fluctuations about the state is invariant under SS. When Λ′\Lambda' has finite index it is invariant under translations by Λ′\Lambda', so its gradient term has coefficients that are periodic modulo Λ′\Lambda', and an affine map (g,a)(g,a) acts on a term with constant coefficients through gg alone. The term Θμν∂μϕ ∂νϕ\Theta^{\mu\nu}\partial_\mu\phi\,\partial_\nu\phi with constant Θ\Theta for a scalar ϕ\phi is therefore invariant under SS exactly when Θ\Theta is invariant under HH. Since HH preserves η\eta, an HH-invariant symmetric bilinear form on R4\mathbb R^4 corresponds to an HH-invariant symmetric tensor by raising indices with η\eta, and the two are not distinguished below.

Theorem 3 (dichotomy for the unbroken group). (a) Assume that Λ′\Lambda' has finite index in Λ\Lambda and that HH satisfies (H1). Then the two-point function of a positive state on an algebra containing the fields ϕ(x)\phi(x), x∈Λ′x\in\Lambda', has the form (3) with Λ′\Lambda' and S∩ΓS\cap\Gamma in place of Λ\Lambda and Γ\Gamma. This applies when SS has finite index in Γ⋉Λ\Gamma\ltimes\Lambda, since (H1) for HH then follows from (H1) for Γ\Gamma.

(b) Let HH be any subgroup of Γ\Gamma with H0≠SO(1,3)∘H_0\ne SO(1,3)^\circ. Then exactly one of the following holds.

  1. H0H_0 leaves invariant a non-degenerate subspace YY with 0≠Y≠R40\ne Y\ne\mathbb R^4.
  2. H0H_0 leaves invariant no such subspace; it then leaves invariant exactly one null line n\mathfrak n, and n\mathfrak n contains a non-zero lattice vector.
  3. As in 2, but n\mathfrak n contains no non-zero lattice vector.

In cases 1 and 2 there is an HH-invariant symmetric tensor Θμν\Theta^{\mu\nu} that is not a multiple of ημν\eta^{\mu\nu}, so the term Θμν∂μϕ ∂νϕ\Theta^{\mu\nu}\partial_\mu\phi\,\partial_\nu\phi is invariant under all unbroken symmetries when Λ′\Lambda' has finite index. Cases 2 and 3 occur only if H0H_0 does not act completely reducibly.

For (a), a finite-index subgroup of a Zariski-dense group is again Zariski dense, so Theorem 2 applies to the unbroken symmetries. For (b), Theorem C3 forces H0H_0 to be reducible, and an invariant subspace or an invariant null line then supplies a symmetric tensor other than ημν\eta^{\mu\nu}. Whether the quadratic action is Lorentz invariant at low energy then depends on couplings that the symmetry leaves free.

Proof. (a) If Λ′\Lambda' has finite index, S∩ΓS\cap\Gamma has finite index in HH by the paragraph above, and so inherits (H1): the Zariski closure of a finite-index subgroup has finite index in that of the group, hence contains SO(1,3)∘SO(1,3)^\circ. Both Λ′\Lambda' and S∩ΓS\cap\Gamma preserve Λ′\Lambda', and the restricted two-point function is invariant under translations by Λ′\Lambda' and under S∩ΓS\cap\Gamma. Theorem 2 applies to Λ′\Lambda' and S∩ΓS\cap\Gamma. If SS has finite index in Γ⋉Λ\Gamma\ltimes\Lambda, then [Λ:Λ′]≤[Γ⋉Λ:S][\Lambda:\Lambda']\le[\Gamma\ltimes\Lambda:S] and [Γ:H]≤[Γ⋉Λ:S][\Gamma:H]\le[\Gamma\ltimes\Lambda:S], since HH is the image of SS under the projection to Γ\Gamma; so HH has finite index in Γ\Gamma and inherits (H1).

(b) First, H0H_0 is reducible. It is a connected subgroup of SO(1,3)∘SO(1,3)^\circ and preserves the Lorentzian form. If it acted irreducibly, C3 would make it conjugate to SO(1,3)∘SO(1,3)^\circ, and a connected Lie subgroup of SO(1,3)∘SO(1,3)^\circ of the same dimension is open, hence equal to SO(1,3)∘SO(1,3)^\circ; this is excluded. So H0H_0 preserves a subspace Y0Y_0 with 0≠Y0≠R40\ne Y_0\ne\mathbb R^4.

Suppose H0H_0 preserves two distinct null lines. They span a plane on which the Gram matrix has the form (0ββ0)\begin{pmatrix}0&\beta\\\beta&0\end{pmatrix} with β≠0\beta\ne0, since a totally null plane does not exist in R1,3\mathbb R^{1,3}; the plane is Lorentzian and non-degenerate. So two invariant null lines imply case 1. If case 1 fails, Y0Y_0 is degenerate, and its radical Y0∩Y0⊥Y_0\cap Y_0^\perp is a non-zero totally null subspace, hence a null line, invariant under H0H_0. By the previous sentence it is the only invariant null line n\mathfrak n.

Case 1. Let YY be as in case 1 and bY(p,q)=B(PYp,PYq)b_Y(p,q)=B(P_Yp,P_Yq), with PYP_Y the orthogonal projection onto YY, so that bY+bY⊥=Bb_Y+b_{Y^\perp}=B. A non-degenerate subspace of R1,3\mathbb R^{1,3} is negative definite, or its orthogonal complement is. For h∈Hh\in H the subspace hYhY is again H0H_0-invariant, because HH normalises H0H_0, and bhY=bY(h−1⋅,h−1⋅)b_{hY}=b_Y(h^{-1}\cdot,h^{-1}\cdot). The orbit HYHY is finite, since the stabiliser of YY contains H∩H0H\cap H_0, of finite index in HH. Put Θ=∑Y′∈HYbY′\Theta=\sum_{Y'\in HY}b_{Y'}, which is HH-invariant. If YY is negative definite, every bY′b_{Y'} is negative semidefinite and non-zero, so Θ\Theta is also, and it cannot be a multiple of the indefinite BB. Otherwise Y⊥Y^\perp is negative definite, bY′=B−bY′⊥b_{Y'}=B-b_{Y'^\perp} with −bY′⊥-b_{Y'^\perp} positive semidefinite and non-zero, and Θ=∣HY∣ B+P\Theta=\lvert HY\rvert \,B+P with PP positive semidefinite and non-zero. If Θ=αB\Theta=\alpha B then P=(α−∣HY∣)BP=(\alpha-\lvert HY\rvert )B, which is impossible for a non-zero positive semidefinite PP and an indefinite BB.

Cases 2 and 3. The group HH maps n\mathfrak n to an H0H_0-invariant null line, hence to n\mathfrak n. If n=Rn0\mathfrak n=\mathbb Rn_0 with n0∈Λn_0\in\Lambda primitive, then H⊂GL(Λ)H\subset GL(\Lambda) preserves the rank-one lattice n∩Λ\mathfrak n\cap\Lambda and acts on it by ±1\pm1, so Θ=n0⊗n0\Theta=n_0\otimes n_0 is HH-invariant. It is not a multiple of ημν\eta^{\mu\nu}: Θ00>0\Theta^{00}>0 and Θ11≥0\Theta^{11}\ge0, while a multiple αημν\alpha\eta^{\mu\nu} has Θ00\Theta^{00} and Θ11\Theta^{11} of opposite sign unless α=0\alpha=0. This gives the tensor in case 2. If n\mathfrak n contains no lattice vector, we are in case 3.

Finally, suppose H0H_0 acts completely reducibly and preserves a null line n\mathfrak n. An invariant complement CC of n\mathfrak n gives an invariant two-dimensional subspace C∩n⊥C\cap\mathfrak n^\perp complementary to n\mathfrak n in n⊥\mathfrak n^\perp; it is negative definite, since n⊥/n\mathfrak n^\perp/\mathfrak n is. Its orthogonal complement is an invariant Lorentzian plane containing n\mathfrak n, which contains a second null line, also invariant because H0H_0 is connected. So case 1 holds. Hence cases 2 and 3 require that H0H_0 does not act completely reducibly. □\square

The very special relativity groups of Cohen and Glashow [Cohen–Glashow], such as SIM(2)SIM(2), fix a null direction up to scale. A boost along that direction rescales it, so n0⊗n0n_0\otimes n_0 is not invariant under such a group. The group HH here is discrete, and it cannot rescale a primitive lattice vector, which is why case 2 carries the invariant tensor n0⊗n0n_0\otimes n_0. For an irrational null line, case 3, this argument is unavailable, and whether an HH-invariant tensor other than η\eta exists is not decided here.

Example 1 (infinitely many fields). Let Γ=O+(1,3;Z)\Gamma=O^+(1,3;\mathbb Z) and Λ=Z4\Lambda=\mathbb Z^4, and let O=Γe0\mathcal O=\Gamma e_0 be the orbit of e0e_0, an infinite set. For u∈Ou\in\mathcal O choose γu∈Γ\gamma_u\in\Gamma with γue0=u\gamma_ue_0=u, so that fμu=γueμf^u_\mu=\gamma_ue_\mu is a basis of Z4\mathbb Z^4 with Q(fμu)=ημμQ(f^u_\mu)=\eta_{\mu\mu} and f0u=uf^u_0=u. The model has one real scalar field ϕu\phi^{u} for each u∈Ou\in\mathcal O and the action ∑uAu[ϕu]\sum_u\mathcal A_u[\phi^u] with

Au[ϕ]=12∑x∈Λ[(ϕ(x+f0u)−ϕ(x))2−ν∑i=13(ϕ(x+fiu)−ϕ(x))2−m2ϕ(x)2],\mathcal A_u[\phi]=\tfrac12\sum_{x\in\Lambda}\Big[(\phi(x+f^u_0)-\phi(x))^2-\nu\sum_{i=1}^3(\phi(x+f^u_i)-\phi(x))^2-m^2\phi(x)^2\Big],

a nearest-neighbour action in the frame fuf^u with the same coefficient ν\nu for the three spatial directions. An element (g,a)(g,a) of Γ⋉Λ\Gamma\ltimes\Lambda acts by ϕu(x)↦ϕgu(gx+a)\phi^u(x)\mapsto\phi^{gu}(gx+a), permuting the labels. The action is invariant: γgu−1gγu\gamma_{gu}^{-1}g\gamma_u lies in StabΓ(e0)\mathrm{Stab}_\Gamma(e_0), the finite group of signed spatial permutations, so gg maps the neighbour directions ±fiu\pm f^u_i to ±fπ(i)gu\pm f^{gu}_{\pi(i)} for a permutation π\pi, and the equal coefficients ν\nu are mapped to each other.

Let ν>0\nu>0 and m>0m>0 satisfy 12ν+m2<412\nu+m^2<4. The frame-uu dispersion relation

4sin⁡2(ω/2)=4ν∑i=13sin⁡2(pi/2)+m24\sin^2(\omega/2)=4\nu\sum_{i=1}^3\sin^2(p_i/2)+m^2

then has a unique solution ωp∈(0,π)\omega_p\in(0,\pi) for every p∈[−π,π]3p\in[-\pi,\pi]^3, because the right side lies in (0,4)(0,4); its maximum 12ν+m212\nu+m^2 is attained at p=(π,π,π)p=(\pi,\pi,\pi). For 12ν+m2≥412\nu+m^2\ge4 some modes have no frequency in (0,π)(0,\pi) (at equality ωp=π\omega_p=\pi at p=(π,π,π)p=(\pi,\pi,\pi), where the weight below diverges), and the action has no positive-frequency vacuum. Since fμu=γueμf^u_\mu=\gamma_ue_\mu, the difference of two lattice points is x−y=γuzx-y=\gamma_uz with z∈Z4z\in\mathbb Z^4 and z⃗=(z1,z2,z3)\vec z=(z_1,z_2,z_3). Let

Wu(x,y)=∫[−π,π]3d3p(2π)3 e−iωpz0+ip⃗⋅z⃗2sin⁡ωp,z=γu−1(x−y).W_u(x,y)=\int_{[-\pi,\pi]^3}\frac{d^3p}{(2\pi)^3}\,\frac{e^{-i\omega_pz_0+i\vec p\cdot\vec z}}{2\sin\omega_p},\qquad z=\gamma_u^{-1}(x-y).

This is the two-point function of the vacuum of Au\mathcal A_u: it solves the equation of motion in both arguments, and the weight 1/(2sin⁡ωp)1/(2\sin\omega_p) is fixed by the commutator [ϕ(x),ϕ(x+f0u)]=i[\phi(x),\phi(x+f^u_0)]=i that the action defines. It is positive, because ∑λˉxλyWu(x,y)\sum\bar\lambda_x\lambda_yW_u(x,y) is the integral of ∣∑yλyeiωpa(y)0−ip⃗⋅a⃗(y)∣2\lvert\sum_y\lambda_ye^{i\omega_pa(y)_0-i\vec p\cdot\vec a(y)}\rvert^2, with a(y)=γu−1ya(y)=\gamma_u^{-1}y, against a positive density, and it is invariant under translations and under StabΓ(u)\mathrm{Stab}_\Gamma(u), which permutes the three spatial axes of the frame up to signs and leaves the density unchanged. Put W((u,x),(u′,y))=δuu′Wu(x,y)W((u,x),(u',y))=\delta_{uu'}W_u(x,y). This is the two-point function of the product of the vacua of the independent sectors, a state on the algebra of all the fields, and it is invariant under Γ⋉Λ\Gamma\ltimes\Lambda by the same frame argument as for the action. For small mm and pp the sector has ωp2≈m2+ν∣p⃗∣2\omega_p^2\approx m^2+\nu\lvert\vec p\rvert^2, a speed ν\sqrt\nu in the units of the frame lattice. The stability condition forces ν<1/3\nu<1/3, so a speed equal to 1, which leading-order Lorentz invariance would need, is not available with this action. The residual symmetry of a single sector is the finite group StabΓ(u)\mathrm{Stab}_\Gamma(u), which imposes no relation on ν\nu or mm.

The example has propagation, a symmetric action and a symmetric state with a Zariski-dense Γ\Gamma. It does not contradict the theorems because the field has infinitely many components. Theorem 2 concerns a single field ϕ(x)\phi(x), and the single field ϕu\phi^u is invariant only under StabΓ(u)\mathrm{Stab}_\Gamma(u). Theorem 1 requires V=CNV=\mathbb C^N with N<∞N<\infty; here V=ℓ2(O)V=\ell^2(\mathcal O), the symbol is an operator-valued function with dgu(g⋅k)=du(k)d_{gu}(g\cdot k)=d_u(k), and this covariance does not force it to be constant, because Γ\Gamma acts on T×O\mathbb T\times\mathcal O with non-constant invariant functions.

8. Cayley-momentum covariance is not a symmetry of a point set

Lorente obtains a covariant lattice Klein–Gordon operator by letting Lorentz transformations act on the variables φ(k)μ=2tan⁡(kμ/2)\varphi(k)_\mu=2\tan(k_\mu/2), which we call the Cayley momentum, through g~=φ−1∘g∘φ\tilde g=\varphi^{-1}\circ g\circ\varphi for g∈O(1,3)g\in O(1,3) [Lorente]. The symbol η(φ(k),φ(k))−m2\eta(\varphi(k),\varphi(k))-m^2 is invariant under this action. The question is whether the action is induced by a transformation of the points of a lattice.

Proposition 3 (point maps induce only automorphisms). Let ψ\psi be a bijection of Z4\mathbb Z^4. Suppose that on a connected neighbourhood UU of 00 in R4\mathbb R^4 there are a continuous map ψ~:U→R4\tilde\psi:U\to\mathbb R^4 with ψ~(0)=0\tilde\psi(0)=0 and unit complex numbers ϵ(k)\epsilon(k) such that eik⋅ψ−1(x)=ϵ(k) eiψ~(k)⋅xe^{ik\cdot\psi^{-1}(x)}=\epsilon(k)\,e^{i\tilde\psi(k)\cdot x} for all k∈Uk\in U and x∈Z4x\in\mathbb Z^4; that is, the composition operator of ψ\psi maps each character of small momentum to a multiple of a character. Then ψ\psi is affine with linear part in GL(4,Z)GL(4,\mathbb Z), and ψ~\tilde\psi is linear on UU.

Proof. Evaluating at x=0x=0 gives ϵ(k)=eik⋅ψ−1(0)\epsilon(k)=e^{ik\cdot\psi^{-1}(0)}. With ψ′(x)=ψ−1(x)−ψ−1(0)\psi'(x)=\psi^{-1}(x)-\psi^{-1}(0) we get eik⋅ψ′(x)=eiψ~(k)⋅xe^{ik\cdot\psi'(x)}=e^{i\tilde\psi(k)\cdot x}. For fixed xx the function k↦ψ~(k)⋅x−k⋅ψ′(x)k\mapsto\tilde\psi(k)\cdot x-k\cdot\psi'(x) is continuous on the connected set UU, takes values in 2πZ2\pi\mathbb Z and vanishes at k=0k=0, so it vanishes identically. Taking x=ejx=e_j gives ψ~(k)j=k⋅ψ′(ej)\tilde\psi(k)_j=k\cdot\psi'(e_j), so ψ~\tilde\psi is linear, ψ~(k)=Ak\tilde\psi(k)=Ak with Aji=ψ′(ej)iA_{ji}=\psi'(e_j)_i. Then k⋅ψ′(x)=k⋅ATxk\cdot\psi'(x)=k\cdot A^Tx for all k∈Uk\in U, so ψ′(x)=ATx\psi'(x)=A^Tx. Since ψ′\psi' is a bijection of Z4\mathbb Z^4 (a translate of the bijection ψ−1\psi^{-1}), AT∈GL(4,Z)A^T\in GL(4,\mathbb Z). □\square

Proposition 4 (g~\tilde g is additive only for monomial gg). Let g∈O(1,3)g\in O(1,3). Then g~(k+k′)=g~(k)+g~(k′)\tilde g(k+k')=\tilde g(k)+\tilde g(k') for all small k,k′k,k' if and only if gg has exactly one non-zero entry in each row and column.

Proof. Expand φ(k)=k+k(3)/12+O(k5)\varphi(k)=k+k^{(3)}/12+O(k^5) and φ−1(y)=y−y(3)/12+O(y5)\varphi^{-1}(y)=y-y^{(3)}/12+O(y^5), where (⋅)(3)(\cdot)^{(3)} is the componentwise cube. Then g~(k)=gk+Δ(k)+O(k5)\tilde g(k)=gk+\Delta(k)+O(k^5) with Δ(k)=112(gk(3)−(gk)(3))\Delta(k)=\tfrac1{12}\big(gk^{(3)}-(gk)^{(3)}\big), homogeneous of degree 3. If g~\tilde g is additive then g~(2k)=2g~(k)\tilde g(2k)=2\tilde g(k), and the cubic terms give 6Δ(k)=06\Delta(k)=0, that is gk(3)=(gk)(3)gk^{(3)}=(gk)^{(3)} for all kk. If some row ii of gg has two non-zero entries gij,gilg_{ij},g_{il}, the coefficient of kj2klk_j^2k_l in (gk)i3(gk)_i^3 is 3gij2gil≠03g_{ij}^2g_{il}\ne0, while (gk(3))i=∑jgijkj3(gk^{(3)})_i=\sum_jg_{ij}k_j^3 has no such monomial. So gg is monomial (a matrix in O(1,3)O(1,3) is invertible, so no row or column vanishes, and a monomial matrix has one non-zero entry in each). Conversely, a monomial gg is a signed permutation, which commutes with the odd componentwise function φ\varphi, so g~=g\tilde g=g is linear. □\square

The map g~=φ−1∘g∘φ\tilde g=\varphi^{-1}\circ g\circ\varphi is defined and continuous on the open cube (−π,π)4(-\pi,\pi)^4, with g~(0)=0\tilde g(0)=0. If a non-monomial gg, such as a boost, had g~\tilde g induced by a bijection of Z4\mathbb Z^4 in the sense of Proposition 3, then g~\tilde g would be linear near 00, hence additive, which Proposition 4 excludes. So g~\tilde g is induced by no point map for such gg: it is a symmetry of the dispersion relation only.

Proposition 5 (vertices). Let g∈O(1,3)g\in O(1,3) be non-monomial. Then there are small momenta k,k′k,k' with k+k′+(−k−k′)=0k+k'+(-k-k')=0 such that g~(k)+g~(k′)+g~(−k−k′)≠0\tilde g(k)+\tilde g(k')+\tilde g(-k-k')\ne0 modulo 2π2\pi. Consequently no three-point vertex that conserves ∑jkj\sum_jk_j modulo 2π2\pi is covariant under g~\tilde g.

Proof. The map g~=φ−1gφ\tilde g=\varphi^{-1}g\varphi is odd, because φ\varphi and φ−1\varphi^{-1} are odd and gg is linear; hence g~(0)=0\tilde g(0)=0 and g~(−k−k′)=−g~(k+k′)\tilde g(-k-k')=-\tilde g(k+k'). By Proposition 4 there are small k,k′k,k' with g~(k+k′)≠g~(k)+g~(k′)\tilde g(k+k')\ne \tilde g(k)+\tilde g(k'), so g~(k)+g~(k′)+g~(−k−k′)=g~(k)+g~(k′)−g~(k+k′)≠0\tilde g(k)+\tilde g(k')+\tilde g(-k-k')=\tilde g(k)+\tilde g(k')-\tilde g(k+k')\ne0. This vector is small by continuity of g~\tilde g at 0, so it is non-zero modulo 2π2\pi. A vertex supported on the triples with zero sum would be mapped by a covariant action to a vertex supported on the images, which do not have zero sum. □\square

Remark 3 (the covariant alternative). A vertex that is covariant must instead conserve ∑jφ(kj)\sum_j\varphi(k_j), and it cannot conserve ∑jkj\sum_jk_j as well, because φ\varphi is not additive. The composition law k⊕k′=φ−1(φ(k)+φ(k′))k\oplus k'=\varphi^{-1}(\varphi(k)+\varphi(k')) is commutative, associative and covariant. It has the structure of the composition laws of the doubly special relativity models of Judes and Visser [Judes–Visser], which are obtained from a non-linear realisation of the Lorentz group by a change of variables. Identifying φ(k)\varphi(k) with the conserved momentum turns the theory into one with continuous translations and the linear Lorentz action; we do not prove this identification in detail. It follows the distinction between momentum and translation generator emphasised by Mignemi [Mignemi]. Under this identification the covariant theory is a continuum theory in a non-linear parametrisation of momentum, and the lattice is a labelling of a basis.

If the lattice translations are kept as symmetries, covariance fails at the vertex and the lattice theory is Lorentz violating. The free massless dispersion obtained from φ(ω)=∣φ(k⃗)∣\varphi(\omega)=\lvert \varphi(\vec k)\rvert follows from ω+ω3/12=∣k⃗∣+∣k⃗∣3∑ini4/12\omega+\omega^3/12=\lvert\vec k\rvert+\lvert\vec k\rvert^3\sum_in_i^4/12 with n=k⃗/∣k⃗∣n=\vec k/\lvert \vec k\rvert, and is, to cubic order, ω=∣k⃗∣−∣k⃗∣312(1−∑ini4)\omega=\lvert \vec k\rvert -\frac{\lvert \vec k\rvert ^3}{12}\big(1-\sum_in_i^4\big), a direction-dependent correction that vanishes along the axes.

Proposition 6 (automorphic actions are linear lattice actions or continuum actions). Let M\mathcal M be a connected four-dimensional Lie group, the group on which momenta (or translations) live, and let a subgroup Γ\Gamma of O(1,3)O(1,3) satisfying (H1) act on it by group automorphisms, with differential at the identity equal to the vector representation. Then M≅R4\mathcal M\cong\mathbb R^4 or M≅T4\mathcal M\cong\mathbb T^4.

Proof. The Lie bracket on m≅R4\mathfrak m\cong\mathbb R^4 is a Γ\Gamma-equivariant linear map ∧2R4→R4\wedge^2\mathbb R^4\to\mathbb R^4. Equivariance under gg is a polynomial condition, so the set of gg for which the bracket is equivariant is Zariski closed and contains Γ\Gamma, hence SO(1,3)∘SO(1,3)^\circ. As a representation of SO(1,3)∘SO(1,3)^\circ, ∧2R4=so(1,3)\wedge^2\mathbb R^4=\mathfrak{so}(1,3) is the adjoint representation of a simple real Lie algebra, hence irreducible of dimension 6. It contains no copy of the four-dimensional vector representation, so by Schur’s lemma the equivariant bracket vanishes. Thus M=R4/ker⁡exp⁡\mathcal M=\mathbb R^4/\ker\exp with ker⁡exp⁡\ker\exp discrete. Its real span is a Γ\Gamma-invariant, hence SO(1,3)∘SO(1,3)^\circ-invariant, subspace, so it is 00 or R4\mathbb R^4, and a discrete subgroup spanning R4\mathbb R^4 is a lattice. □\square

In the torus case Γ\Gamma acts linearly through GL(4,Z)GL(4,\mathbb Z), which is the setting of Theorems 1 and 2. In the R4\mathbb R^4 case there is no discreteness. What remains is a Lorentz action on momentum space that is not by group automorphisms, as in κ\kappa-Poincaré constructions, which are not realised on a point set.

9. Spectral triples on the Brillouin quotient

A spectral triple, in the sense of non-commutative geometry, is an algebra acting on a Hilbert space together with a self-adjoint operator DD with compact resolvent whose commutators with the algebra are bounded. The operator DD plays the role of a Dirac operator, and the dimension of the geometry is read from the growth of its spectrum: for a Dirac operator on a compact dd-dimensional manifold the number ND(R)\mathcal N_D(R) of eigenvalues in [−R,R][-R,R] grows like RdR^d. A triple is called pp-summable when ND(R)≤C(1+R)p\mathcal N_D(R)\le C(1+R)^p, and θ\theta-summable when Tr⁡e−tD2<∞\operatorname{Tr}e^{-tD^2}<\infty for every t>0t>0.

Proposition 6 leaves open whether the Brillouin torus modulo the integral Lorentz group could carry a geometry of finite spectral dimension. The quotient is not a Hausdorff space: under (H1), by Corollary 1, the orbit of every non-torsion point is dense. In non-commutative geometry the quotient is replaced by the crossed product C(Tn)⋊ΓC(\mathbb T^n)\rtimes\Gamma, the algebra generated by the continuous functions on the torus and unitaries UgU_g that satisfy UgfUg−1=f∘g−1U_gfU_g^{-1}=f\circ g^{-1}. On H=L2(Tn)⊗V\mathcal H=L^2(\mathbb T^n)\otimes V it is generated by the translation unitaries TxT_x (multiplication by characters) and the operators UgU_g of (2), taken with σ\sigma unitary. A covariant Brillouin triple is a self-adjoint DD with compact resolvent on H\mathcal H such that TeiT_{e_i} and UgU_g, for gg in a finite generating set of Γ\Gamma, and their inverses, preserve dom D\mathrm{dom}\,D and have bounded commutators with DD. It is exactly equivariant if UgDUg−1=DU_gDU_g^{-1}=D for all g∈Γg\in\Gamma.

Theorem 4 (exact equivariance excludes compact resolvent). Assume (F) for Γ\Gamma acting on Λ=Zn\Lambda=\mathbb Z^n. There is no self-adjoint operator DD with compact resolvent on L2(Tn)⊗VL^2(\mathbb T^n)\otimes V, with VV finite-dimensional and σ\sigma a representation of Γ\Gamma on VV (not necessarily unitary), that satisfies UgDUg−1=DU_gDU_g^{-1}=D for all g∈Γg\in\Gamma.

Proof. Let E\mathcal E be an eigenspace of DD; it is finite-dimensional because the resolvent is compact, and invariant under every UgU_g. Let F⊂L2(Tn)F\subset L^2(\mathbb T^n) be the span of the components (id⊗e∗)(ϑ)(\mathrm{id}\otimes e^\ast)(\vartheta), ϑ∈E\vartheta\in\mathcal E, e∗∈V∗e^\ast\in V^\ast; it is finite-dimensional. For f=(id⊗e∗σ(g))ϑf=(\mathrm{id}\otimes e^\ast\sigma(g))\vartheta one has Kgf=(id⊗e∗)(Ugϑ)∈FK_gf=(\mathrm{id}\otimes e^\ast)(U_g\vartheta)\in F, and as e∗e^\ast ranges over V∗V^\ast so does e∗σ(g)e^\ast\sigma(g), because σ(g)\sigma(g) is invertible; so FF is KK-invariant. Its projection onto L02L^2_0 is invariant and finite-dimensional, hence zero by Lemma 2(i). Thus every component of every eigenvector is constant, E⊂1⊗V\mathcal E\subset1\otimes V. The eigenvectors of a self-adjoint operator with compact resolvent span H\mathcal H, so H=1⊗V\mathcal H=1\otimes V is finite-dimensional, which contradicts dim⁡L2(Tn)=∞\dim L^2(\mathbb T^n)=\infty. □\square

The Dirac-type operator γμxμ\gamma^\mu x_\mu in position space is covariant in form, but it is not self-adjoint, because the spatial γi\gamma^i are anti-Hermitian, and its square is the multiplication by Q(x)Q(x), which takes each non-zero value on an infinite orbit. It therefore has no compact resolvent, in line with the theorem.

If covariance is only required up to bounded terms, the obstruction is a different one: the translations are exponentially distorted in G=Λ⋊ΓG=\Lambda\rtimes\Gamma. Fix a finite generating set of GG, and write ∣x∣G\lvert x\rvert _G for the word length of the translation txt_x, x∈Λx\in\Lambda.

Lemma 3 (exponential distortion of translations). (i) Let A∈SL(2,Z)A\in SL(2,\mathbb Z) with tr⁡A>2\operatorname{tr}A>2 and GA=Z2⋊⟨A⟩G_A=\mathbb Z^2\rtimes\langle A\rangle. There is CC with ∣x∣GA≤Clog⁡(2+∣x∣)\lvert x\rvert _{G_A}\le C\log(2+\lvert x\rvert ) for all x∈Z2x\in\mathbb Z^2. (ii) Let Γ\Gamma be a subgroup of finite index in O(1,3;Z)O(1,3;\mathbb Z) and G=Z4⋊ΓG=\mathbb Z^4\rtimes\Gamma. Then ∣x∣G≤Clog⁡(2+∣x∣)\lvert x\rvert _G\le C\log(2+\lvert x\rvert ) for all x∈Z4x\in\mathbb Z^4.

The difficulty is that a translation by a large vector costs a long word in the translation generators alone. Conjugation by AA stretches one eigendirection by λ>1\lambda>1, so a large vector can be written as a short sum of integer vectors from a bounded set, each conjugated by a power of AA, in the manner of a base-λ\lambda expansion.

Proof. (i) Let λ>1\lambda>1 be the larger eigenvalue of AA. Write x=u(x)eu+s(x)esx=u(x)e_u+s(x)e_s in the eigenbasis, so that AA acts by (u,s)↦(λu,s/λ)(u,s)\mapsto(\lambda u,s/\lambda). Let rcr_c be the covering radius of Z2\mathbb Z^2 in the sup norm of these coordinates and τ0=λrc\tau_0=\lambda r_c.

Step 1 (points near the unstable axis). Suppose ∣s(y)∣≤τ0\lvert s(y)\rvert \le\tau_0. The rectangle {∣u∣≤rc, ∣s−s(y)∣≤τ0/λ}\{\lvert u\rvert \le r_c,\ \lvert s-s(y)\rvert \le\tau_0/\lambda\} contains a ball of sup-radius rcr_c, hence a lattice point vv of the finite set F={v∈Z2:∣u(v)∣≤rc, ∣s(v)∣≤τ0+τ0/λ}F=\{v\in\mathbb Z^2:\lvert u(v)\rvert \le r_c,\ \lvert s(v)\rvert \le\tau_0+\tau_0/\lambda\}. Put y′=A−1(y−v)y'=A^{-1}(y-v), an integer vector because det⁡A=1\det A=1. Then ∣s(y′)∣=λ∣s(y)−s(v)∣≤τ0\lvert s(y')\rvert =\lambda\lvert s(y)-s(v)\rvert \le\tau_0 and ∣u(y′)∣≤(∣u(y)∣+rc)/λ\lvert u(y')\rvert \le(\lvert u(y)\rvert +r_c)/\lambda. Iterating, after kk steps ∣u∣≤∣u(y)∣λ−k+rc/(λ−1)\lvert u\rvert \le\lvert u(y)\rvert \lambda^{-k}+r_c/(\lambda-1), so after k=log⁡λ(2+∣u(y)∣)+O(1)k=\log_\lambda(2+\lvert u(y)\rvert )+O(1) steps the point lies in a fixed finite set B0\mathcal B_0. This gives y=∑j<kAjvj+Akyky=\sum_{j<k}A^jv_j+A^ky_k with vj∈Fv_j\in F and yk∈B0y_k\in \mathcal B_0.

Step 2 (the word). Let aa be the generator acting as AA, so a tza−1=tAza\,t_za^{-1}=t_{Az}. Then t∑j<kAjvj=tv0 a tv1 a tv2⋯a tvk−1 a−(k−1)t_{\sum_{j<k}A^jv_j}=t_{v_0}\,a\,t_{v_1}\,a\,t_{v_2}\cdots a\,t_{v_{k-1}}\,a^{-(k-1)} and tAkyk=aktyka−kt_{A^ky_k}=a^kt_{y_k}a^{-k}. The elements tvt_v with v∈F∪B0v\in F\cup \mathcal B_0 have bounded length, so ∣ty∣GA≤C1k+C2\lvert t_y\rvert _{G_A}\le C_1k+C_2.

Step 3 (general xx). The same construction with A−1A^{-1} treats points with ∣u∣≤τ0\lvert u\rvert \le\tau_0 and large ∣s∣\lvert s\rvert. Given x∈Z2x\in\mathbb Z^2, choose a lattice point pp within sup-distance rcr_c of u(x)euu(x)e_u, then a lattice point qq within rcr_c of the stable-axis point of x−px-p. Then x=p+q+rx=p+q+r with ∣s(p)∣≤rc\lvert s(p)\rvert \le r_c, ∣u(q)∣≤rc\lvert u(q)\rvert \le r_c, rr in a finite set, and ∣p∣,∣q∣≤C∣x∣\lvert p\rvert ,\lvert q\rvert \le C\lvert x\rvert. Hence ∣x∣GA≤Clog⁡(2+∣x∣)\lvert x\rvert _{G_A}\le C\log(2+\lvert x\rvert ).

(ii) Let A=(3423)A=\begin{pmatrix}3&4\\2&3\end{pmatrix}, which preserves a2−2b2a^2-2b^2 since (3a+4b)2−2(2a+3b)2=a2−2b2(3a+4b)^2-2(2a+3b)^2=a^2-2b^2. Let g0∈GL(4,R)g_0\in GL(4,\mathbb R) act as AA on the coordinates (a,b)(a,b) of ae0+b(e1+e2)ae_0+b(e_1+e_2) and trivially on e1−e2e_1-e_2 and e3e_3. These vectors are mutually orthogonal, with Q(e0)=1Q(e_0)=1, Q(e1+e2)=Q(e1−e2)=−2Q(e_1+e_2)=Q(e_1-e_2)=-2, so g0g_0 preserves QQ. It maps e1e_1 to 2e0+2e1+e22e_0+2e_1+e_2 and e2e_2 to 2e0+e1+2e22e_0+e_1+2e_2, so g0∈O+(1,3;Z)g_0\in O^+(1,3;\mathbb Z), and some power h=g0j0h=g_0^{j_0}, j0≥1j_0\ge1, lies in the finite-index subgroup Γ\Gamma (two of the powers g0jg_0^j lie in the same coset of Γ\Gamma). Put P=Re0+R(e1+e2)P=\mathbb R e_0+\mathbb R(e_1+e_2) and P0=Z4∩P=Ze0+Z(e1+e2)P_0=\mathbb Z^4\cap P=\mathbb Ze_0+\mathbb Z(e_1+e_2). For γ∈Γ\gamma\in\Gamma the element γhγ−1∈Γ\gamma h\gamma^{-1}\in\Gamma preserves γP\gamma P and acts on γP0=Z4∩γP\gamma P_0=\mathbb Z^4\cap\gamma P as a hyperbolic element of SL(2,Z)SL(2,\mathbb Z) in the basis γ(e0,e1+e2)\gamma(e_0,e_1+e_2). Part (i) applies on each such plane, with the translations of γP0\gamma P_0 and the element γhγ−1\gamma h\gamma^{-1} as generators, whose lengths in GG are bounded; the relation a tza−1=taza\,t_za^{-1}=t_{az} holds in GG for all z∈Z4z\in\mathbb Z^4. So ∣z∣G≤Clog⁡(2+∣z∣)\lvert z\rvert _G\le C\log(2+\lvert z\rvert ) for z∈P0∪γP0z\in P_0\cup\gamma P_0.

The condition P⊕γP=R4P\oplus\gamma P=\mathbb R^4 is the non-vanishing of a determinant, a polynomial in the entries of γ\gamma. It is not identically zero on SO(1,3)∘SO(1,3)^\circ: take γ\gamma to be a boost of rapidity s≠0s\ne0 in the e0e3e_0e_3 plane composed with a rotation by π/2\pi/2 in the e1e2e_1e_2 plane, so that γe0=cosh⁡s e0+sinh⁡s e3\gamma e_0=\cosh s\,e_0+\sinh s\,e_3 and γ(e1+e2)=−(e1−e2)\gamma(e_1+e_2)=-(e_1-e_2). The four vectors e0e_0, e1+e2e_1+e_2, γe0\gamma e_0, γ(e1+e2)\gamma(e_1+e_2) are independent. By (H1) some γ∈Γ\gamma\in\Gamma satisfies the condition. Then P0⊕γP0P_0\oplus\gamma P_0 has finite index in Z4\mathbb Z^4, and every xx is x1+x2+rx_1+x_2+r with x1∈P0x_1\in P_0, x2∈γP0x_2\in\gamma P_0, ∣xi∣≤C∣x∣\lvert x_i\rvert \le C\lvert x\rvert and rr in a finite set of coset representatives. Then ∣x∣G≤∣x1∣G+∣x2∣G+∣r∣G\lvert x\rvert _G\le\lvert x_1\rvert _G+\lvert x_2\rvert _G+\lvert r\rvert _G. □\square

Theorem 5 (exponential Weyl law). Let G=Zn⋊ΓG=\mathbb Z^n\rtimes\Gamma with either n=2n=2 and Γ=⟨A⟩\Gamma=\langle A\rangle as in Lemma 3(i), or n=4n=4 and Γ\Gamma of finite index in O(1,3;Z)O(1,3;\mathbb Z). Let DD be a covariant Brillouin triple on L2(Tn)⊗VL^2(\mathbb T^n)\otimes V with σ\sigma unitary. Then there are c,κ,R0>0c,\kappa,R_0>0 with

ND(R):=rank⁡1[−R,R](D) ≥ c eκR(R≥R0).(7)\mathcal N_D(R):=\operatorname{rank}\mathbf 1_{[-R,R]}(D)\ \ge\ c\,e^{\kappa R}\qquad(R\ge R_0). \tag{7}

In particular DD is pp-summable for no p<∞p<\infty.

Bounded commutators with the generators give a commutator with a word of length mm that grows only linearly in mm, so exponentially many translates of one vector fit into a spectral window of width linear in mm. Lemma 3 supplies the exponential count.

Proof. The vectors ζx=Txζ\zeta_x=T_x\zeta, x∈Λx\in\Lambda, with ζ=1⊗v0\zeta=1\otimes v_0 and ∥v0∥=1\lVert v_0\rVert =1, are orthonormal. Let CDC_D bound the commutators of DD with the generators and their inverses. For a product uu of mm generators or inverses, all partial products preserve dom D\mathrm{dom}\,D, and the Leibniz rule gives ∥[D,u]∥≤CDm\lVert [D,u]\rVert \le C_Dm. Choose ξ∈dom D\xi\in\mathrm{dom}\,D with ∥ξ−ζ∥≤14\lVert \xi-\zeta\rVert \le\tfrac14. For ∣x∣G≤m\lvert x\rvert _G\le m, ∥DTxξ∥≤∥TxDξ∥+∥[D,Tx]ξ∥≤∥Dξ∥+54CDm\lVert DT_x\xi\rVert \le\lVert T_xD\xi\rVert +\lVert [D,T_x]\xi\rVert \le \lVert D\xi\rVert+\tfrac54C_Dm. Put R=4∥Dξ∥+5CDmR=4\lVert D\xi\rVert+5C_Dm and P=1[−R,R](D)P=\mathbf 1_{[-R,R]}(D). Then ∥(1−P)Txξ∥≤∥DTxξ∥/R≤14\lVert (1-P)T_x\xi\rVert \le\lVert DT_x\xi\rVert /R\le\tfrac14, so ∥(1−P)ζx∥≤14+∥ζ−ξ∥≤12\lVert (1-P)\zeta_x\rVert \le\tfrac14+\lVert \zeta-\xi\rVert \le\tfrac12 and ⟨ζx,Pζx⟩=1−∥(1−P)ζx∥2≥34\langle\zeta_x,P\zeta_x\rangle=1-\lVert (1-P)\zeta_x\rVert ^2\ge\tfrac34. Bessel’s inequality for the orthonormal family gives rank⁡P≥∑x⟨ζx,Pζx⟩≥34 #{x:∣x∣G≤m}\operatorname{rank}P\ge\sum_x\langle\zeta_x,P\zeta_x\rangle\ge\tfrac34\,\#\{x:\lvert x\rvert _G\le m\}. By Lemma 3 every xx with ∣x∣∞≤r\lvert x\rvert _\infty\le r has ∣x∣G≤Clog⁡(2+r)+c0\lvert x\rvert _G\le C\log(2+r)+c_0, so for r=e(m−c0)/C−2r=e^{(m-c_0)/C}-2 the count is at least (2r+1)n≥en(m−c0)/C(2r+1)^n\ge e^{n(m-c_0)/C}. Since RR is affine in mm, this is (7) with κ=n/(5CDC)\kappa=n/(5C_DC). A pp-summable DD has ND(R)≤C′(1+R)p\mathcal N_D(R)\le C'(1+R)^p, which (7) violates. □\square

The estimate is sharp in the following sense. The operator D=∣x∣GD=\lvert x\rvert _G acting by multiplication in position space has bounded commutators with all generators (since ∣x+a∣G≤∣x∣G+∣a∣G\lvert x+a\rvert _G\le\lvert x\rvert _G+\lvert a\rvert _G and ∣gx∣G≤∣x∣G+2∣g∣G\lvert gx\rvert _G\le\lvert x\rvert _G+2\lvert g\rvert _G), compact resolvent, and Tr⁡e−tD2=∑xe−t∣x∣G2<∞\operatorname{Tr}e^{-tD^2}=\sum_xe^{-t\lvert x\rvert _G^2}<\infty for every t>0t>0, because the number of elements of GG of length at most RR is at most exponential in RR. It is therefore θ\theta-summable, and by Theorem 5 not finitely summable.

Whittaker has built finitely summable spectral triples for the stable-groupoid algebras of Smale spaces such as a hyperbolic toral automorphism [Whittaker]. These replace C(Tn)⋊ΓC(\mathbb T^n)\rtimes\Gamma by a different algebra and are not covered by the theorems above.

10. States centred on one lattice point

Theorem 2 assumes exact translations. Take instead Γ\Gamma to fix the origin of Λ=Z4\Lambda=\mathbb Z^4 and impose no translation symmetry. A positive Γ\Gamma-invariant state is then the lattice analogue of the Milne universe about the origin, the open future cone foliated by the hyperboloids Q=constQ=\text{const}, whose isometry group is the Lorentz group.

Two facts about stabilisers in Γ\Gamma, a finite-index subgroup of O+(1,3;Z)O^+(1,3;\mathbb Z), are used. They are consequences of Theorem C1.

(S1) For a primitive spacelike v∈Λv\in\Lambda, StabΓ(v)\mathrm{Stab}_\Gamma(v) acts faithfully on v⊥≅R1,2v^\perp\cong\mathbb R^{1,2}, its Zariski closure there contains SO(v⊥)∘≅SO(1,2)∘SO(v^\perp)^\circ\cong SO(1,2)^\circ, and it contains a hyperbolic element, that is, one with null eigenvectors of eigenvalues λ±1\lambda^{\pm1}, λ>1\lambda>1. Indeed, StabO(1,3;Z)(v)\mathrm{Stab}_{O(1,3;\mathbb Z)}(v) acts on the lattice Λ∩v⊥\Lambda\cap v^\perp with the integral form of signature (1,2)(1,2) induced by QQ; it is contained in the automorphism group of L=Λ∩v⊥L=\Lambda\cap v^\perp and contains the finite-index subgroup of automorphisms that act trivially on the finite discriminant group L∨/LL^\vee/L. Such an automorphism, extended by the identity on vv, maps every coset of Zv⊕L\mathbb Zv\oplus L in Λ\Lambda to itself, because Λ\Lambda lies between Zv⊕L\mathbb Zv\oplus L and its dual lattice, so it preserves Λ\Lambda. That automorphism group is a lattice by C1, hence StabΓ(v)\mathrm{Stab}_\Gamma(v), of finite index in StabO+(1,3;Z)(v)\mathrm{Stab}_{O^+(1,3;\mathbb Z)}(v), is a lattice in the automorphism group of LL and its Zariski closure contains SO(1,2)∘SO(1,2)^\circ. Let Δ\Delta be its subgroup of finite index that lies in SO(1,2)∘SO(1,2)^\circ; its Zariski closure still contains SO(1,2)∘SO(1,2)^\circ, so Δ\Delta is Zariski dense in SO(1,2)∘SO(1,2)^\circ. A Zariski-dense discrete subgroup of SO(1,2)∘≅PSL(2,R)SO(1,2)^\circ\cong PSL(2,\mathbb R) is non-elementary (an elementary group lies in a proper algebraic subgroup: the stabiliser of a point of the closed hyperbolic disc or of a pair of boundary points), and a non-elementary Fuchsian group contains hyperbolic elements.

(S2) For a primitive null v∈Λv\in\Lambda and b∈Λ∩v⊥b\in\Lambda\cap v^\perp, the null rotation Xb(y)=y+B(y,v)b−B(y,b)v−12Q(b)B(y,v)vX_b(y)=y+B(y,v)b-B(y,b)v-\tfrac12Q(b)B(y,v)v (an isometry fixing vv, with XbXb′=Xb+b′X_bX_{b'}=X_{b+b'}) has X2bX_{2b} integral, so X2b∈O+(1,3;Z)X_{2b}\in O^+(1,3;\mathbb Z) and a power of it lies in Γ\Gamma.

Proposition 7 (clustering forces vanishing correlations of the centre, spacelike points and null points). Let Γ\Gamma be a finite-index subgroup of O+(1,3;Z)O^+(1,3;\mathbb Z), Λ=Z4\Lambda=\mathbb Z^4, and let W(x,y)=ω(ϕ(x)∗ϕ(y))W(x,y)=\omega(\phi(x)^\ast\phi(y)) for a positive state ω\omega on a ∗\ast-algebra containing the fields ϕ(x)\phi(x), x∈Λx\in\Lambda, with W(gx,gy)=W(x,y)W(gx,gy)=W(x,y), g∈Γg\in\Gamma. Assume

(WC) if y∈Λy\in\Lambda and γn∈Γ\gamma_n\in\Gamma satisfy ∣B(y,γny)∣→∞\lvert B(y,\gamma_ny)\rvert \to\infty, then W(y,γny)→0W(y,\gamma_ny)\to0.

Then:

(a) W(0,y)=0W(0,y)=0 for all y∈Λ∖{0}y\in\Lambda\setminus\{0\};

(b) W(v,y)=0W(v,y)=0 for spacelike v∈Λv\in\Lambda and all y∈Λ∖Rvy\in\Lambda\setminus\mathbb Rv;

(c) W(v,y)=0W(v,y)=0 for null v∈Λv\in\Lambda and all y∈Λy\in\Lambda with B(v,y)≠0B(v,y)\ne0.

Proof. Let ξx=ϕ(x)Ω\xi_x=\phi(x)\Omega be the vectors of the Gelfand–Naimark–Segal construction, so W(x,y)=⟨ξx,ξy⟩W(x,y)=\langle\xi_x,\xi_y\rangle. Since WW is Γ\Gamma-invariant, U(g)ξx=ξgxU(g)\xi_x=\xi_{gx} defines an isometry on the closed span of the ξx\xi_x.

Let ℓ∈Γ\ell\in\Gamma fix vv (in (a) take v=0v=0, fixed by every ℓ\ell), so U(ℓ)ξv=ξvU(\ell)\xi_v=\xi_v. By the mean ergodic theorem for isometries on a Hilbert space, 1N∑k<NU(ℓ)kξy→Pξy\frac1N\sum_{k<N}U(\ell)^k\xi_y\to P\xi_y, with PP the projection onto the fixed vectors of U(ℓ)U(\ell). If ∣B(y,ℓky)∣→∞\lvert B(y,\ell^ky)\rvert \to\infty, then (WC) gives ⟨ξy,U(ℓ)kξy⟩=W(y,ℓky)→0\langle\xi_y,U(\ell)^k\xi_y\rangle=W(y,\ell^ky)\to0, so ∥Pξy∥2=lim⁡1N∑k⟨ξy,U(ℓ)kξy⟩=0\lVert P\xi_y\rVert ^2=\lim\frac1N\sum_k\langle\xi_y,U(\ell)^k\xi_y\rangle=0. As ξv\xi_v is fixed, W(v,y)=⟨Pξv,ξy⟩=⟨ξv,Pξy⟩=0W(v,y)=\langle P\xi_v,\xi_y\rangle=\langle\xi_v,P\xi_y\rangle=0. It remains to find, in each case, ℓ\ell fixing vv with ∣B(y,ℓky)∣→∞\lvert B(y,\ell^ky)\rvert \to\infty.

In (a), let ℓ0∈Γ\ell_0\in\Gamma be hyperbolic (the element hh of Lemma 3(ii) is one), with null eigenvectors w±w_\pm of eigenvalues λ±1\lambda^{\pm1}; it acts as a rotation on the plane {w+,w−}⊥\{w_+,w_-\}^\perp. For γ∈Γ\gamma\in\Gamma, ℓ=γℓ0γ−1\ell=\gamma\ell_0\gamma^{-1} has eigenvectors γw±\gamma w_\pm. Write y=αγw++βγw−+y0y=\alpha\gamma w_++\beta\gamma w_-+y_0 with y0⊥γw±y_0\perp\gamma w_\pm; then α∝B(y,γw−)\alpha\propto B(y,\gamma w_-), β∝B(y,γw+)\beta\propto B(y,\gamma w_+), and B(y,ℓky)=αβ(λk+λ−k)B(γw+,γw−)+B(y0,ℓky0)B(y,\ell^ky)=\alpha\beta(\lambda^k+\lambda^{-k})B(\gamma w_+,\gamma w_-)+B(y_0,\ell^ky_0) tends to ±∞\pm\infty if αβ≠0\alpha\beta\ne0, because the last term is bounded. The function γ↦B(γ−1y,w+)B(γ−1y,w−)\gamma\mapsto B(\gamma^{-1}y,w_+)B(\gamma^{-1}y,w_-) is a polynomial on SO(1,3)SO(1,3) that is not identically zero: if B(⋅,w+)B(\cdot,w_+) vanished on the orbit of yy, which spans R4\mathbb R^4 by irreducibility, then w+=0w_+=0. Since Γ+\Gamma^+ is Zariski dense in SO(1,3)∘SO(1,3)^\circ, some γ\gamma gives αβ≠0\alpha\beta\ne0.

In (b), write y=cv+y′y=cv+y' with y′∈v⊥y'\in v^\perp; y′≠0y'\ne0 because y∉Rvy\notin\mathbb Rv. The same argument inside v⊥≅R1,2v^\perp\cong\mathbb R^{1,2} with the Zariski-dense subgroup Δ⊂StabΓ(v)\Delta\subset\mathrm{Stab}_\Gamma(v) of (S1) gives a hyperbolic ℓ\ell fixing vv with B(y′,ℓky′)→∞B(y',\ell^ky')\to\infty, and B(y,ℓky)=c2Q(v)+B(y′,ℓky′)B(y,\ell^ky)=c^2Q(v)+B(y',\ell^ky').

In (c), take b∈Λ∩v⊥b\in\Lambda\cap v^\perp not proportional to vv; since v⊥/Rvv^\perp/\mathbb Rv is negative definite, Q(b)<0Q(b)<0. We have B(y,Xkby)=Q(y)−12k2Q(b)B(y,v)2B(y,X_{kb}y)=Q(y)-\tfrac12k^2Q(b)B(y,v)^2, which tends to +∞+\infty when B(y,v)≠0B(y,v)\ne0. By (S2) take ℓ=X2bm∈Γ\ell=X_{2b}^m\in\Gamma for a suitable m≥1m\ge1. □\square

Under (WC), a Γ\Gamma-invariant state has no correlation between the centre and any other point (a), between a spacelike point and any point off its line (b), and between a null point and any point not orthogonal to it (c). Correlations between points inside the light cone of the centre are not constrained: timelike vectors have finite stabilisers in Γ\Gamma (they lie in a compact O(3)O(3)), and the argument gives nothing for them. Condition (WC) is a hypothesis on the state and does not follow from positivity and invariance.

Proposition 8 (a state that propagates inside the cone). Let Φ\Phi be a free massive scalar field on Minkowski space with Fock vacuum Ω\Omega, let f0f_0 be a real Schwartz function on R4\mathbb R^4 invariant under spatial rotations, let Ξx\Xi_x be a boost taking e0e_0 to u(x)=x/Q(x)u(x)=x/\sqrt{Q(x)}, and put fx(y)=f0(Ξx−1(y−x))f_x(y)=f_0(\Xi_x^{-1}(y-x)) for xx in the open future cone. The functional ω(ϕ(x)ϕ(y))=⟨Ω,Φ(fx)Φ(fy)Ω⟩\omega(\phi(x)\phi(y))=\langle\Omega,\Phi(f_x)\Phi(f_y)\Omega\rangle on Λ∩{Q>0, x0>0}\Lambda\cap\{Q>0,\ x_0>0\} is positive and invariant under O+(1,3)O^+(1,3), hence under Γ\Gamma; its spectral support is the mass shell; and it satisfies (WC) on pairs of points in the open cone.

Proof. Positivity: WW is the Gram matrix of the vectors Φ(fx)Ω\Phi(f_x)\Omega. Invariance: for g∈O+(1,3)g\in O^+(1,3), u(gx)=gu(x)u(gx)=gu(x), so Ξgx=gΞxR\Xi_{gx}=g\Xi_xR with RR a spatial rotation, and since f0f_0 is rotation invariant, fgx=fx∘g−1f_{gx}=f_x\circ g^{-1}. The vacuum is invariant, so ⟨Φ(fgx)Φ(fgy)⟩=⟨Φ(fx)Φ(fy)⟩\langle\Phi(f_{gx})\Phi(f_{gy})\rangle=\langle\Phi(f_x)\Phi(f_y)\rangle. The spectral support is that of the vacuum two-point function, the mass shell. For (WC), let ψy=Φ(fy)Ω\psi_y=\Phi(f_y)\Omega, a vector of the one-particle space L2L^2 of the mass shell, on which O+(1,3)O^+(1,3) acts unitarily by π\pi. Since fγy=fy∘γ−1f_{\gamma y}=f_y\circ\gamma^{-1}, W(y,γny)=⟨ψy,π(γn)ψy⟩W(y,\gamma_ny)=\langle\psi_y,\pi(\gamma_n)\psi_y\rangle. The function g↦B(y,gy)g\mapsto B(y,gy) is continuous, so ∣B(y,γny)∣→∞\lvert B(y,\gamma_ny)\rvert\to\infty forces γn→∞\gamma_n\to\infty in the group. The representation has no non-zero SO+(1,3)SO^+(1,3)-invariant vector, because such a vector would be constant on the mass shell, whose invariant measure is infinite. Write γn=hnPϵn\gamma_n=h_nP^{\epsilon_n} with hn∈SO+(1,3)h_n\in SO^+(1,3), PP a spatial reflection and ϵn∈{0,1}\epsilon_n\in\{0,1\}; then hn→∞h_n\to\infty, and C4 applied to ψy\psi_y and π(P)ψy\pi(P)\psi_y gives ⟨ψy,π(hn)π(P)ϵnψy⟩→0\langle\psi_y,\pi(h_n)\pi(P)^{\epsilon_n}\psi_y\rangle\to0. □\square

This state is defined on the open cone only, not on all of Λ\Lambda, so it does not meet the hypothesis of Proposition 7; it shows that the inside of the cone can carry correlations of a Lorentz-invariant field.

In the Milne frame u(x)u(x) the symmetry fixing the point xx is the compact O(3)u(x)O(3)_{u(x)} only, so a separate (u⋅∂ϕ)2(u\cdot\partial\phi)^2 term is allowed for each field species without breaking the symmetry. The unit timelike field u(x)=x/Q(x)u(x)=x/\sqrt{Q(x)} then plays the role of the aether of Einstein–aether theories.

11. Point sets without a fixed translation lattice and open cases

The theorems of sections 3 to 5 do not cover an ensemble whose realisations have different translation groups, nor a generic lattice gZ4g\mathbb Z^4 with g∈SL(4,R)g\in SL(4,\mathbb R), whose Lorentz stabiliser is finite, so that (F) fails. Random lattices are treated in Lorentz-invariant point sets.

Radiative stability of the allowed tensor

The tensor Θμν\Theta^{\mu\nu} allowed by cases 1 and 2 of Theorem 3(b) is left free by the unbroken symmetry. Whether a value of Θ\Theta that makes the low-energy dispersion Lorentz invariant is stable under radiative corrections would be settled by the running of the coefficients of the invariant tensors in an explicit model; no such computation is given here.

Correlations of states centred on one point

Proposition 8 gives a state on the open cone with correlations inside it, and Proposition 7 constrains states on all of Λ\Lambda that cluster. Whether a state on all of Λ\Lambda can combine the correlations of Proposition 8 with the vanishing correlations of Proposition 7 is unsettled, as is whether a null-rotation argument controls the pairs (v,y)(v,y) with B(v,y)=0B(v,y)=0 in (c).

Distortion of translations in other arithmetic groups

Lemma 3(ii) is proved for finite-index subgroups of O(1,3;Z)O(1,3;\mathbb Z). For other Zariski-dense arithmetic groups, such as the automorphism group of an anisotropic form, it is not proved, and Theorem 5 for them is open.

References

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