Abstract

Within i.i.d. multiplicative cascades, a single axiom—the hierarchical symmetry, a linear contraction on incremental scaling exponents—is shown to be necessary and sufficient for the cascade multiplier to be log-Poisson. We prove: (1) a characterization theorem determining the log-Poisson law with explicit parameters, within the class of all multipliers with finite lattice moments; (2) a classification theorem locating the log-Poisson class inside the log-infinitely-divisible family and identifying the mechanism by which every rival sub-family fails the symmetry; (3) a stability theorem with sharp constants—(1+β)1/2(1+\beta)^{1/2} when the limiting increment is known, 2\sqrt{2} when it is fitted—and (4) an unconditional propagation theorem transferring the bound to the multiplier distribution at the sharp rate Θ(ε)\Theta(\sqrt{\varepsilon}), with a matching lower bound. Beyond independence, the classification is shown to extend exactly at the level of asymptotic statistics (limiting cumulant generating function, large deviations, multifractal spectrum) and provably not at the level of laws: an explicit stationary ergodic Markov multiplier satisfies the symmetry exactly with a non-log-Poisson marginal, while exchangeable multipliers collapse to the i.i.d. log-Poisson cascade and finite-state Markov multipliers cannot satisfy the symmetry at all. In the continuous category of exactly scale-invariant log-infinitely-divisible multifractal random measures, no finite moment window of structure-function exponents identifies the cascade class, whereas at the level of the scale-invariance generator the symmetry selects exactly the Barral–Mandelbrot compound Poisson cascade, with scale-ratio-free stability constants. The proofs reduce to second-moment identities on [0,1][0,1] via the change of variables u=ekxu = e^{kx}, boundedness of the multiplier (esssupW=rγ\mathop{\mathrm{ess\,sup}} W = r^\gamma), and multiplicative couplings.

2020 Mathematics Subject Classification. 60G57, 60E10, 60G51, 60F10, 28A80, 76F55.

Key words and phrases. Multiplicative cascades, log-Poisson distribution, hierarchical symmetry, multifractal spectrum, Hausdorff moment problem, multifractal random measures, large deviations.

1. Introduction

Multiplicative cascades model the successive fragmentation of a conserved quantity across scales and arise in fully developed turbulence [13, 14], rainfall, finance, and other settings exhibiting intermittent, scale-invariant fluctuations. The mathematical foundations of multiplicative cascades were established by Kahane and Peyrière [10]; see Barral and Mandelbrot [4] and Bacry and Muzy [2] for the modern discrete and continuous theories. The statistical properties of a cascade are encoded in the scaling exponents ζp\zeta_p of the structure functions Sp()=Φ()pζpS_p(\ell) = \langle |\Phi(\ell)|^p \rangle \sim \ell^{\zeta_p}. A central question is: which probability distributions on the cascade multiplier W are compatible with observed scaling laws?

Kolmogorov [13] proposed log-normal multipliers, leading to quadratic scaling exponents. Z.-S. She and Lévêque [16] introduced a hierarchical symmetry for the scaling exponents and derived a different, log-Poisson exponent formula that has since shown excellent agreement with experimental data. Dubrulle [7] independently identified the log-Poisson form. Z.-S. She and Waymire [17] used the Lévy–Khintchine representation to argue that this symmetry selects log-Poisson within the log-infinitely-divisible family; Dubrulle and Graner [8] reached a similar conclusion via symmetry groups. These works provided compelling physical arguments but did not supply rigorous proofs. Z.-S. She and Zhang [18] subsequently proposed that the hierarchical symmetry is universal—applicable not only to turbulence but to general multi-scale fluctuation systems including MHD turbulence, natural image statistics, and biological signals—and should serve as a standard analytical framework. The present paper supplies the rigorous mathematical foundation for this program.

We formalize the hierarchical symmetry as a single axiom (A1) and prove the following.

Characterization (Theorem 3). A1 uniquely determines the cascade multiplier WW to be log-Poisson, with parameters (a=γlnr,  b=(lnβ)/k,  λ=Clnr)(a = \gamma\ln r,\; b = (\ln\beta)/k,\; \lambda = -C\ln r) expressed in terms of the observable scaling exponents. No other distribution—infinitely divisible or not—is compatible with A1.

Classification (Theorem 7). Within the full log-infinitely-divisible family, A1 selects exactly the log-Poisson class, and the proof stratifies the exclusion: Gaussian components, positive jumps, and stable generators of index α[1,2)\alpha \in [1,2) are eliminated by divergence of the incremental exponents; all remaining generators are eliminated by a second-moment rigidity.

Stability (Theorem 10). If A1 holds only approximately, with residuals bounded by ε\varepsilon, then the (tilted, compactified) Lévy measure of the generator is within KεK\sqrt{\varepsilon} of a Dirac mass in the Wasserstein-1 metric, with the sharp constant K=((1+β)lnr/A)1/2K = ((1+\beta)|\ln r|/|A|)^{1/2} when the limiting increment δ\delta_\infty is known, and the sharp constant (2lnr/A)1/2(2|\ln r|/|A|)^{1/2} when δ\delta_\infty is fitted along with β\beta.

Propagation at the sharp rate (Theorems 11 and 12). Closeness of the Lévy measure transfers to closeness of the multiplier distribution at rate O(ε)O(\sqrt{\varepsilon}) unconditionally—no finite-activity or minimum-jump hypothesis—with an explicit constant; and an explicit family shows the rate Θ(ε)\Theta(\sqrt{\varepsilon}) is exact.

Beyond independence (Section 6). For stationary ergodic multipliers, A1 is equivalent to the limiting cumulant generating function—hence the large-deviation rate and the multifractal spectrum—being exactly log-Poisson (Theorem 13); but it provably does not determine the multiplier law: an explicit stationary ergodic countable-state Markov multiplier satisfies A1 exactly with a non-log-Poisson marginal (Theorem 14). Exchangeable multipliers with exact scaling collapse to the i.i.d. log-Poisson cascade (Corollary 15), and finite-state Markov multipliers cannot satisfy A1 at all with nontrivial intermittency (Theorem 16).

Continuous cascades (Section 7). In the Bacry–Muzy category of exactly scale-invariant log-infinitely-divisible multifractal random measures, structure-function exponents exist only on a finite moment window, and no finite window identifies the cascade class (Theorem 17); at the level of the scale-invariance generator—magnitude statistics, observable at all orders—A1 selects exactly the Barral–Mandelbrot compound Poisson cascade (Theorem 18), with stability constants that are native and scale-ratio-free (Corollary 19).

The converse—that log-Poisson multipliers imply A1—is established in Proposition 5, yielding a biconditional equivalence (Corollary 6).

Relation to prior work. The exponent formula (\ast\ast) (Lemma 1) and the log-Poisson identification are due to Z.-S. She and Lévêque [16] and Dubrulle [7]. Z.-S. She and Waymire [17] gave the first argument connecting A1 to the Lévy–Khintchine classification. The compound Poisson cascades appear in Barral–Mandelbrot [4]; the log-ID multifractal random measures in Bacry–Muzy [2, 15]; magnitude-cumulant analysis in Delour–Muzy–Arneodo [5]. The following results are new: the boundedness and moment-determinacy lemma (Lemma 2); the converse and biconditional (Proposition 5, Corollary 6); the classification with stratified exclusion (Theorem 7); the determinacy dichotomy (Proposition 9); the stability theorem with sharp constants under both readings (Theorem 10); the unconditional sharp-rate propagation theory (Theorems 11, 12); the beyond-i.i.d. classification and its impossibility boundary (Theorems 13, 14, 16, Corollary 15); and the continuous-cascade results (Theorems 17, 18).

Method. The change of variables u=ekxu = e^{kx} maps the Lévy measure from (,0](-\infty,0] to the compact interval [0,1][0,1], where a second-moment identity against the candidate atom decides the classification and its stability. A1 forces the multiplier to be essentially bounded with esssupW=rγ\mathop{\mathrm{ess\,sup}} W = r^\gamma, which yields moment determinacy directly and eliminates all tail estimates from the propagation argument; the propagation itself is a multiplicative coupling in which jumps near the identity are costed by their multiplicative deviation rather than counted. Beyond independence the arguments run at the level of limiting cumulant generating functions; in the continuous category they transfer through the dictionary lnr1\ln r \mapsto -1.

Throughout this paper, log\log denotes the natural logarithm.

2. Setup

Let r(0,1)r \in (0,1) be a scale ratio. A multiplicative cascade generates a random positive measure μ\mu on nested sets B0B1B_0 \supset B_1 \supset \cdots via

μ(Bn+1)=Wn+1μ(Bn),\mu(B_{n+1}) = W_{n+1} \cdot \mu(B_n),

where {Wn}\{W_n\} are i.i.d. positive random variables with E[W]=1\mathbb{E}[W] = 1 (conservation of mean; a normalization convention—none of the proofs below depend on it, cf. Corollary 20). Sections 6 and 7 relax, respectively, the independence assumption and the discrete setting.

Let Φ()\Phi(\ell) be the cascade observable at scale =rn\ell = r^n. Define the structure functions

Sp()=Φ()p=ζp,S_p(\ell) = \langle |\Phi(\ell)|^p \rangle = \ell^{\zeta_p},

where ζp\zeta_p are the scaling exponents, with ζ0=0\zeta_0 = 0; all moments of WW are assumed finite, so that ζp\zeta_p is finite for every p0p \ge 0. The relation E[Wp]=rζp\mathbb{E}[W^p] = r^{\zeta_p} identifies the single-step moment structure of the multiplier with the observable's scaling.

For a fixed integer k1k \geq 1 (the hierarchy step), define the moment ratios

Hp()=Sp+k()Sp()=δp,H_p(\ell) = \frac{S_{p+k}(\ell)}{S_p(\ell)} = \ell^{\delta_p},

where δp=ζp+kζp\delta_p = \zeta_{p+k} - \zeta_p are the incremental exponents at step kk.

3. The Axiom

Axiom (A1: Hierarchical Symmetry). There exist β(0,1)\beta \in (0,1) and LRL \in \mathbb{R} such that for all pkN0p \in k\mathbb{N}_0 (non-negative integer multiples of kk), the incremental exponents satisfy

δp+k=(1β)L+βδp.(∗)\delta_{p+k} = (1 - \beta)\,L + \beta\,\delta_p. \tag{∗}

Since (\ast) is a contraction, it forces δmkL\delta_{mk} \to L as mm \to \infty; we write δ:=L\delta_\infty := L. (Stating the axiom with a free constant LL, rather than defining δ\delta_\infty as a limit inside the equation that uses it, matters only for the approximate version in Theorem 10, where the distinction between the true limit and a fitted constant is quantitatively significant.)

A1 determines the full parameter set from the observable exponents:

Parameter Determined by Meaning
β\beta Contraction ratio of (\ast) Coupling strength
γ\gamma δ/k\delta_\infty / k Linear drift
CC (δ0δ)/(1β)(\delta_0 - \delta_\infty)/(1 - \beta) Concentration amplitude

Edge case (C=0C = 0). If δ0=δ\delta_0 = \delta_\infty, then C=0C = 0 and ζp=γp\zeta_p = \gamma p (monofractal scaling). The cascade multiplier W=rγW = r^\gamma is deterministic. A1 is trivially satisfied for any β(0,1)\beta \in (0,1). The classification and stability theorems assume C>0C > 0 (nontrivial intermittency).

4. Results: The i.i.d. Cascade

Lemma 1 (Exponent Form)

If the incremental exponents {δp}\{\delta_p\} satisfy the A1 recurrence (\ast) with β(0,1)\beta \in (0,1), then with ζ0=0\zeta_0 = 0:

ζp=γp+C(1βp/k),(∗∗)\zeta_p = \gamma p + C\bigl(1 - \beta^{p/k}\bigr), \tag{∗∗}

where γ=δ/k\gamma = \delta_\infty / k and C=(δ0δ)/(1β)C = (\delta_0 - \delta_\infty)/(1 - \beta).

We emphasize that this lemma is purely algebraic and involves no probabilistic content.

Proof.

(1) The recurrence (\ast) is first-order linear with fixed point δ\delta_\infty:

δp+kδ=β(δpδ).\delta_{p+k} - \delta_\infty = \beta\,(\delta_p - \delta_\infty).

(2) At p=mkp = mk (integer multiples of kk), iteration gives

δmkδ=(δ0δ)βm.\delta_{mk} - \delta_\infty = (\delta_0 - \delta_\infty)\,\beta^m.

Replacing m=p/km = p/k:

δp=δ+(δ0δ)βp/k.\delta_p = \delta_\infty + (\delta_0 - \delta_\infty)\,\beta^{p/k}.

(This formula is derived at pkN0p \in k\mathbb{N}_0. For general p0p \geq 0, we define ζp\zeta_p by (\ast\ast); the function βp/k\beta^{p/k} is well-defined for all real p0p \geq 0 since β>0\beta > 0. The moment-based arguments in Lemma 2 and Theorem 3 use only the lattice pkN0p \in k\mathbb{N}_0, where the formula is proved.)

(3) With ζ0=0\zeta_0 = 0, sum the step-kk increments using the geometric series:

ζp=pkδ+δ0δ1β(1βp/k).\zeta_p = \frac{p}{k}\,\delta_\infty + \frac{\delta_0 - \delta_\infty}{1 - \beta}\,\bigl(1 - \beta^{p/k}\bigr).

Identifying γ=δ/k\gamma = \delta_\infty/k and C=(δ0δ)/(1β)C = (\delta_0 - \delta_\infty)/(1-\beta):

ζp=γp+C(1βp/k).\zeta_p = \gamma p + C\bigl(1 - \beta^{p/k}\bigr). \qquad\square

Lemma 2 (Boundedness and Moment Determinacy)

Let {Wn}\{W_n\} be an i.i.d. multiplicative cascade whose lattice scaling exponents satisfy ζkm=γkm+C(1βm)\zeta_{km} = \gamma km + C(1-\beta^{m}) for all mN0m \in \mathbb{N}_0, as produced by A1 via Lemma 1. Then:

(i) WW is essentially bounded, with esssupW=rγ\mathop{\mathrm{ess\,sup}} W = r^{\gamma};

(ii) the law of WW is uniquely determined by the lattice moments {E[Wkm]}m0\{\mathbb{E}[W^{km}]\}_{m \ge 0}.

Proof. Set V=Wk0V = W^k \ge 0. By independence across cascade levels, E[(W1Wn)p]=(E[Wp])n\mathbb{E}[(W_1\cdots W_n)^p] = (\mathbb{E}[W^p])^n; combined with Sp()=rnζpS_p(\ell) = r^{n\zeta_p} this gives, for a single step, E[Vm]=E[Wkm]=rζkm\mathbb{E}[V^m] = \mathbb{E}[W^{km}] = r^{\zeta_{km}} for every mN0m \in \mathbb{N}_0—these are exactly the moments constrained by A1. Then

(E[Vm])1/m=rζkm/m=rγk+C(1βm)/mrγk(m).\bigl(\mathbb{E}[V^m]\bigr)^{1/m} = r^{\zeta_{km}/m} = r^{\,\gamma k + C(1-\beta^m)/m} \longrightarrow r^{\gamma k} \qquad (m \to \infty).

On a probability space the norms VLm\|V\|_{L^m} are nondecreasing in mm and converge to VL\|V\|_{L^\infty}; hence VV is essentially bounded with V=rγk\|V\|_\infty = r^{\gamma k}, and W=V1/kW = V^{1/k} is bounded with W=rγ\|W\|_\infty = r^{\gamma}, proving (i).

For (ii): a probability law supported in the compact interval [0,rγk][0, r^{\gamma k}] is uniquely determined by its integer moments. (Hausdorff moment problem: polynomials are uniformly dense in C([0,rγk])C([0,r^{\gamma k}]) by the Weierstrass approximation theorem, so two laws with equal moments integrate every continuous function equally and coincide by the Riesz representation theorem.) Hence the law of VV is determined by {E[Vm]}\{\mathbb{E}[V^m]\}; since xx1/kx \mapsto x^{1/k} is a Borel bijection of [0,)[0,\infty), the law of WW is determined as well. \square

Remark. A Carleman-condition argument [1] is available here only along the lattice (applied to V=WkV = W^k), since A1 constrains no other moments when k2k \ge 2. The boundedness route above is shorter and stronger: statement (i) identifies the essential supremum of the multiplier with the most-singular scaling factor rγr^\gamma, a fact used again in Theorem 11.

Theorem 3 (Characterization)

Let {Wn}\{W_n\} be an i.i.d. multiplicative cascade whose incremental scaling exponents satisfy A1. Then:

(i) Scaling exponents.

ζp=γp+C(1βp/k),\zeta_p = \gamma p + C\bigl(1 - \beta^{p/k}\bigr),

where γ=δ/k\gamma = \delta_\infty/k and C=(δ0δ)/(1β)C = (\delta_0 - \delta_\infty)/(1-\beta).

(ii) Uniqueness. The cascade multiplier WW is uniquely determined to be log-Poisson:

logW=a+bN,NPoisson(λ),\log W = a + bN, \qquad N \sim \mathrm{Poisson}(\lambda),
a=γlnr,b=lnβk,λ=Clnr.a = \gamma \ln r, \quad b = \frac{\ln\beta}{k}, \quad \lambda = -C\ln r.

No other probability distribution on WW is compatible with A1.

(iii) Multifractal spectrum. Let dd denote the spatial dimension of the cascade support. Then

f(h)=dC+Cx(1lnx),x=k(hγ)Clnβ,f(h) = d - C + Cx(1 - \ln x), \qquad x = \frac{k(h - \gamma)}{C|\ln\beta|},

defined for h[γ,  γ+(C/k)lnβ]h \in [\gamma,\; \gamma + (C/k)|\ln\beta|].

Proof.

(i) Immediate from Lemma 1.

(ii) Set a=γlnra = \gamma\ln r, b=(lnβ)/kb = (\ln\beta)/k, λ=Clnr>0\lambda = -C\ln r > 0. For logW=a+bN\log W = a + bN with NPoisson(λ)N \sim \mathrm{Poisson}(\lambda):

E[Wp]=eapexp[λ(ebp1)]for all real p0,\mathbb{E}[W^p] = e^{ap} \cdot \exp\bigl[\lambda(e^{bp} - 1)\bigr] \qquad\text{for all real } p \ge 0,

and since ebp=βp/ke^{bp} = \beta^{p/k}, the choice λ=Clnr\lambda = -C\ln r gives λ(βp/k1)=Clnr(1βp/k)\lambda(\beta^{p/k}-1) = C\ln r\,(1-\beta^{p/k}), so that

E[Wkm]=e(γlnr)kmeClnr(1βm)=rζkmfor every mN0.\mathbb{E}[W^{km}] = e^{(\gamma\ln r) km}\, e^{C\ln r\,(1-\beta^{m})} = r^{\zeta_{km}} \qquad\text{for every } m \in \mathbb{N}_0.

Thus the log-Poisson law realizes exactly the lattice moments of the cascade multiplier. By Lemma 2(ii) the lattice moments uniquely determine the law; hence WW is log-Poisson, and no other distribution is possible. (The same matching holds at every real p0p \ge 0, so the extension of (\ast\ast) off the lattice is consistent.)

(iii) The singularity spectrum f(h)=infp[phζp+d]f(h) = \inf_p\,[ph - \zeta_p + d]. Setting the derivative to zero:

hγ+Ck(lnβ)βp/k=0hγ=Clnβkβp/k.h - \gamma + \frac{C}{k}(\ln\beta)\,\beta^{p/k} = 0 \quad\Longrightarrow\quad h - \gamma = \frac{C|\ln\beta|}{k}\,\beta^{p/k}.

Define x=βp/k=k(hγ)/(Clnβ)x = \beta^{p/k} = k(h-\gamma)/(C|\ln\beta|). Then p=klnx/lnβp = -k\ln x / |\ln\beta| and

p(hγ)=klnxlnβClnβkx=Cxlnx.p(h - \gamma) = \frac{-k\ln x}{|\ln\beta|} \cdot \frac{C|\ln\beta|}{k}\,x = -Cx\ln x.

Therefore

f(h)=dC+Cx(1lnx),x=k(hγ)Clnβ.f(h) = d - C + Cx(1 - \ln x), \qquad x = \frac{k(h-\gamma)}{C|\ln\beta|}.

Boundary checks: p=0x=1f=dp = 0 \Rightarrow x = 1 \Rightarrow f = d; px0fdCp \to \infty \Rightarrow x \to 0 \Rightarrow f \to d - C. Concavity: ζp=(C/k2)(lnβ)2βp/k<0\zeta_p'' = -(C/k^2)(\ln\beta)^2\beta^{p/k} < 0. \square

Corollary 4 (Most-singular branch)

Under A1, WrγW \le r^\gamma almost surely, and the bound is attained with positive probability: P(W=rγ)=eλ\mathbb{P}(W = r^\gamma) = e^{-\lambda}. The probability that a cascade trajectory takes the maximal factor for nn consecutive levels is

eλn=rCn=Cat scale =rn:e^{-\lambda n} = r^{Cn} = \ell^{\,C} \qquad\text{at scale } \ell = r^n :

the set of always-maximal cascade paths carries codimension exactly CC, in agreement with f(hmin)=dCf(h_{\min}) = d - C in Theorem 3(iii).

Proof. By Theorem 3(ii), W=rγβN/kW = r^\gamma \beta^{N/k} with NPoisson(λ)N \sim \mathrm{Poisson}(\lambda), so WrγW \le r^\gamma with equality iff N=0N = 0, an event of probability eλe^{-\lambda}. By independence across levels, nn consecutive maximal factors have probability eλn=e(Clnr)n=rCne^{-\lambda n} = e^{(C\ln r) n} = r^{Cn}. \square

Remark (Scope of Theorem 3). No infinite-divisibility assumption enters Theorem 3: A1 characterizes the log-Poisson law within the class of all nonnegative multipliers with finite lattice moments. Theorem 7 below is therefore not a larger uniqueness statement but an anatomical one: it locates the log-Poisson class inside the Lévy–Khintchine parameterization and identifies the mechanism by which each rival sub-family fails A1. Its proof technique—the compactifying substitution u=ekxu = e^{kx}—is also the engine of the stability and propagation theory.

Remark (Conservation). The setup assumes E[W]=1\mathbb{E}[W] = 1, which requires ζ1=0\zeta_1 = 0. Substituting into (\ast\ast): γ+C(1β1/k)=0\gamma + C(1 - \beta^{1/k}) = 0, giving γ=C(1β1/k)\gamma = -C(1-\beta^{1/k}). This is a constraint relating γ\gamma to CC and β\beta, reducing the free parameters from three to two.

Proposition 5 (Converse)

If the cascade multiplier WW is log-Poisson—that is, logW=a+bN\log W = a + bN with NPoisson(λ)N \sim \mathrm{Poisson}(\lambda), b<0b < 0, λ>0\lambda > 0—then the incremental scaling exponents satisfy A1 with β=ebk(0,1)\beta = e^{bk} \in (0,1).

Proof. The moment generating function gives E[Wp]=exp(ap+λ(ebp1))\mathbb{E}[W^p] = \exp(ap + \lambda(e^{bp} - 1)), so ζp=(ap+λ(ebp1))/lnr\zeta_p = \bigl(ap + \lambda(e^{bp} - 1)\bigr)/\ln r. The step-kk increments are

δp=ak+λebp(ebk1)lnr.\delta_p = \frac{ak + \lambda e^{bp}(e^{bk}-1)}{\ln r}.

Setting β=ebk(0,1)\beta = e^{bk} \in (0,1) (since b<0b < 0, k1k \geq 1):

δp=aklnr+λ(β1)lnrβp/k.\delta_p = \frac{ak}{\ln r} + \frac{\lambda(\beta - 1)}{\ln r}\,\beta^{p/k}.

As pp \to \infty: βp/k0\beta^{p/k} \to 0, so δ=ak/lnr\delta_\infty = ak/\ln r. The deviation is

δpδ=λ(β1)lnrβp/k.\delta_p - \delta_\infty = \frac{\lambda(\beta - 1)}{\ln r}\,\beta^{p/k}.

At p+kp + k:

δp+kδ=λ(β1)lnrβ(p+k)/k=β(δpδ).\delta_{p+k} - \delta_\infty = \frac{\lambda(\beta-1)}{\ln r}\,\beta^{(p+k)/k} = \beta\,(\delta_p - \delta_\infty).

Therefore δp+k=(1β)δ+βδp\delta_{p+k} = (1-\beta)\delta_\infty + \beta\delta_p, which is exactly A1. \square

Corollary 6 (Biconditional)

Within i.i.d. multiplicative cascades, A1 is necessary and sufficient for log-Poisson:

A1 holds        W is log-Poisson (with b<0).\text{A1 holds} \;\;\Longleftrightarrow\;\; W \text{ is log-Poisson (with } b < 0\text{).}

The forward direction is Theorem 3(ii); the reverse is Proposition 5.

Theorem 7 (Log-ID Classification)

Let {Wn}\{W_n\} be an i.i.d. multiplicative cascade with nontrivial intermittency (C>0C > 0), whose generator logW\log W is infinitely divisible with Lévy triplet (a,σ2,ν)(a, \sigma^2, \nu). Then A1 holds with β(0,1)\beta \in (0,1) if and only if σ2=0\sigma^2 = 0 and ν=λδb\nu = \lambda\delta_b for some b<0b < 0, λ>0\lambda > 0. That is:

A1 selects exactly the log-Poisson class from the full log-infinitely-divisible family.

No other log-ID cascade—log-normal, log-stable, or any intermediate—satisfies A1.

Proof.

Reverse direction. If ν=λδb\nu = \lambda\delta_b with b<0b < 0 and σ2=0\sigma^2 = 0, then logW=a+bN\log W = a + bN with NPoisson(λ)N \sim \mathrm{Poisson}(\lambda), and A1 holds by Proposition 5.

Forward direction. Assume A1 holds. We show σ2=0\sigma^2 = 0 and ν=λδb\nu = \lambda\delta_b.

Step 1 (unsplit form). The cumulant generating function of logW\log W is

ψ(p)=ap+σ2p22+(epx1px1x1)ν(dx),\psi(p) = ap + \frac{\sigma^2 p^2}{2} + \int\bigl(e^{px} - 1 - px\,\mathbf{1}_{|x|\leq 1}\bigr)\,\nu(dx),

finite for all p0p \ge 0 since all moments of WW are finite. With ζp=ψ(p)/lnr\zeta_p = \psi(p)/\ln r and δp=(ψ(p+k)ψ(p))/lnr\delta_p = (\psi(p+k) - \psi(p))/\ln r, define ϕ(p)=ψ(p+k)ψ(p)\phi(p) = \psi(p+k) - \psi(p). Then

ϕ(p)=ak+σ2k ⁣(p+k2)+gp(x)ν(dx),gp(x):=epx(ekx1)kx1x1,\phi(p) = ak + \sigma^2 k\!\left(p + \tfrac{k}{2}\right) + \int g_p(x)\,\nu(dx), \qquad g_p(x) := e^{px}\bigl(e^{kx}-1\bigr) - kx\,\mathbf{1}_{|x|\leq 1},

where gpg_p is ν\nu-integrable for each pp, being the difference of the two compensated Lévy–Khintchine integrands. No splitting of the integral is performed at this stage.

Step 1′ (sign inventory). For every p0p \ge 0:

  • on (0,1](0,1]: epx1e^{px} \ge 1 gives gp(x)(ekx1)kx0g_p(x) \ge (e^{kx}-1) - kx \ge 0, and gp(x)g_p(x) \uparrow \infty pointwise as pp \to \infty;
  • on (1,)(1,\infty): gp(x)=epx(ekx1)0g_p(x) = e^{px}(e^{kx}-1) \ge 0, increasing to ++\infty pointwise;
  • on [1,0)[-1,0): epx(ekx1)1ekxkx|e^{px}(e^{kx}-1)| \le 1 - e^{kx} \le k|x|, so 0gp(x)kx0 \le g_p(x) \le k|x|, with gp(x)kxg_p(x) \to k|x| pointwise as pp \to \infty;
  • on (,1)(-\infty,-1): 1gp(x)0-1 \le g_p(x) \le 0, with gp(x)0g_p(x) \to 0 pointwise.

In particular gpdνν((,1))\int g_p\,d\nu \ge -\nu((-\infty,-1)), uniformly in pp.

Step 2 (σ2=0\sigma^2 = 0). If σ2>0\sigma^2 > 0 then, by Step 1′,

ϕ(p)    ak+σ2k(p+k2)ν((,1))    +,\phi(p) \;\ge\; ak + \sigma^2 k\Bigl(p + \tfrac{k}{2}\Bigr) - \nu\bigl((-\infty,-1)\bigr) \;\longrightarrow\; +\infty,

so δp=ϕ(p)/lnr\delta_p = \phi(p)/\ln r \to -\infty, contradicting the finite limit δ\delta_\infty forced by A1. Hence σ2=0\sigma^2 = 0. This eliminates all log-normal and mixed Gaussian-jump generators.

Step 3 (supp(ν)(,0]\mathrm{supp}(\nu) \subseteq (-\infty,0]). If ν\nu has mass on (0,)(0,\infty) then, since gp0g_p \ge 0 there and gpg_p \uparrow \infty pointwise, monotone convergence gives (0,)gpdν\int_{(0,\infty)} g_p\,d\nu \to \infty, while (,0)gpdνν((,1))\int_{(-\infty,0)} g_p\,d\nu \ge -\nu((-\infty,-1)); again ϕ(p)\phi(p) \to \infty and δp\delta_p \to -\infty, a contradiction. Therefore supp(ν)(,0]\mathrm{supp}(\nu) \subseteq (-\infty,0]. This eliminates all generators with positive jumps.

Step 3½ (integrability near 00). We claim A1 forces [1,0)xν(dx)<\int_{[-1,0)} |x|\,\nu(dx) < \infty. With σ2=0\sigma^2 = 0 and suppν(,0]\mathrm{supp}\,\nu \subseteq (-\infty,0], apply Fatou's lemma on [1,0)[-1,0) (integrand gp0g_p \ge 0 by Step 1′, pointwise limit kxk|x|) and dominated convergence on (,1)(-\infty,-1) (bounded by 11, finite mass):

lim infpϕ(p)    ak+k[1,0)xν(dx)ν((,1)).\liminf_{p\to\infty} \phi(p) \;\ge\; ak + k\int_{[-1,0)} |x|\,\nu(dx) - \nu\bigl((-\infty,-1)\bigr).

If [1,0)xdν=\int_{[-1,0)}|x|\,d\nu = \infty then ϕ(p)\phi(p) \to \infty and δp\delta_p \to -\infty, contradicting A1. Hence x1xdν<\int_{|x|\le1}|x|\,d\nu < \infty, the compensator integral kx1x1dνk\int x\,\mathbf{1}_{|x|\le1}\,d\nu is finite, and only now may the integral be split:

ϕ(p)=c0+(,0)epx(ekx1)ν(dx),c0=akk ⁣x1x1ν(dx).\phi(p) = c_0 + \int_{(-\infty,0)} e^{px}\bigl(e^{kx}-1\bigr)\,\nu(dx), \qquad c_0 = ak - k\!\int x\,\mathbf{1}_{|x|\leq 1}\,\nu(dx).

The remaining integrand is dominated by 1ekxmin(1,kx)L1(ν)1 - e^{kx} \le \min(1, k|x|) \in L^1(\nu) and tends to 00 pointwise, so by dominated convergence ϕ(p)c0\phi(p) \to c_0 as pp \to \infty; thus ϕ=c0\phi_\infty = c_0 and δ=c0/lnr\delta_\infty = c_0/\ln r.

Step 4 (ν\nu is a single Dirac mass). A1 at p=mkp = mk gives, by Lemma 1(2), δmkδ=(δ0δ)βm\delta_{mk} - \delta_\infty = (\delta_0-\delta_\infty)\beta^m; multiplying by lnr\ln r,

(,0)emkx(ekx1)ν(dx)=Aβmfor all m0,(1)\int_{(-\infty,0)} e^{mkx}\bigl(e^{kx}-1\bigr)\,\nu(dx) = A\beta^m \qquad\text{for all } m \geq 0, \tag{1}

where A=(δ0δ)lnr<0A = (\delta_0 - \delta_\infty)\ln r < 0 (nontrivial intermittency and lnr<0\ln r < 0). Substitute u=ekxu = e^{kx}, mapping (,0)(0,1)(-\infty,0) \to (0,1); let ν~\tilde\nu be the pushforward of ν\nu and set

η:=(1u)dν~    0,μm:=(0,1)umdη.\eta := (1-u)\,d\tilde\nu \;\ge\; 0, \qquad \mu_m := \int_{(0,1)} u^m \, d\eta.

Then (1) reads μm=Aβm\mu_m = |A|\,\beta^m for all m0m \ge 0; the case m=0m=0 shows η\eta is a finite positive measure of total mass A|A|. Only m{0,1,2}m \in \{0,1,2\} are needed:

(0,1)(uβ)2dη=μ22βμ1+β2μ0=A(β22β2+β2)=0.\int_{(0,1)} (u-\beta)^2 \, d\eta = \mu_2 - 2\beta\mu_1 + \beta^2\mu_0 = |A|\bigl(\beta^2 - 2\beta^2 + \beta^2\bigr) = 0.

Since (uβ)2>0(u-\beta)^2 > 0 on (0,1){β}(0,1)\setminus\{\beta\} and η0\eta \ge 0, we conclude η((0,1){β})=0\eta\bigl((0,1)\setminus\{\beta\}\bigr) = 0 and η({β})=A\eta(\{\beta\}) = |A|. Because u10u - 1 \neq 0 on (0,1)(0,1), the tilt is invertible:

ν~=A1βδβ=λδβ,λ=A1β>0.\tilde\nu = \frac{|A|}{1-\beta}\,\delta_\beta = \lambda\,\delta_\beta, \qquad \lambda = \frac{|A|}{1-\beta} > 0.

Therefore ν=λδb\nu = \lambda\delta_b with b=(lnβ)/k<0b = (\ln\beta)/k < 0 and λ>0\lambda > 0. The generator logW\log W is compound Poisson with deterministic jump size bb and rate λ\lambda: this is the log-Poisson distribution. \square

Remark (Alternative identification; minimality). The conclusion of Step 4 can also be reached from the full moment sequence: a finite signed measure on a compact interval is determined by its moments (Weierstrass approximation and the Riesz representation theorem), and AδβA\delta_\beta realizes the moments (1). The second-moment argument given above is preferred because it (a) uses only m{0,1,2}m \in \{0,1,2\} of (1), so that A1 restricted to p{0,k,2k}p \in \{0, k, 2k\}, together with Steps 2–3½, already pins the distribution; and (b) is exactly the computation that the stability theorem quantifies (see the Remark closing Section 5).

Remark (Which families die where). The exclusion mechanism stratifies. Gaussian components (Step 2), positive jumps (Step 3), and negative-support Lévy measures with x1xdν=\int_{|x|\le1}|x|\,d\nu = \infty—in particular totally skewed stable generators of index α[1,2)\alpha \in [1,2)—all fail A1 by divergence: δ=\delta_\infty = -\infty (Step 3½). All remaining log-ID generators have bounded incremental exponents but fail the geometric rigidity of Step 4: e.g. for a stable generator of index α<1\alpha < 1 the moments μm\mu_m decay like the power law mα1m^{\alpha-1}, which cannot equal Aβm|A|\beta^m for any β(0,1)\beta \in (0,1).

Corollary 8 (Principal cascade classes)

The log-ID cascade family is partitioned by A1:

Class Lévy data A1 Failure mode Determinate
Log-Poisson σ2=0\sigma^2=0, ν=λδb\nu=\lambda\delta_b, b<0b<0 Holds Yes (bounded WW)
Log-normal σ2>0\sigma^2>0 Fails δ=\delta_\infty=-\infty (Step 2) No
Log-stable, α[1,2)\alpha\in[1,2) ν\nu power-law Fails δ=\delta_\infty=-\infty (Step 3½)
Log-stable, α<1\alpha<1 ν\nu power-law Fails non-geometric decay (Step 4) Yes (bounded WW)
General log-ID any other Fails Step 3 or Step 4

Determinacy in this family tracks boundedness of the multiplier, equivalently boundedness of {δp}\{\delta_p\} (Lemma 2(i)): every negative-support generator with finite δ\delta_\infty has compactly supported WW, hence is moment-determinate. The operative dichotomy is bounded versus unbounded, with A1 strictly on the bounded side.

Proposition 9 (Determinacy Dichotomy)

The two principal cascade exponent laws are distinguished by moment determinacy:

(a) If A1 holds within a cascade (log-Poisson regime), then the scaling exponents uniquely determine the multiplier law (Theorem 3(ii)); indeed WW is bounded and moment-determinate (Lemma 2).

(b) If the exponents are quadratic, ζp=c1p+c2p2\zeta_p = c_1 p + c_2 p^2 with c2<0c_2 < 0 ([13]/log-normal regime), then E[Wp]=exp(μp+σ2p2/2)\mathbb{E}[W^p] = \exp(\mu p + \sigma^2 p^2/2) with μ=c1lnr\mu = c_1\ln r and σ2=2c2lnr>0\sigma^2 = 2c_2\ln r > 0, and this moment sequence is indeterminate: uncountably many distinct laws realize it. Under quadratic scaling, the exponents cannot identify the multiplier law.

Proof.

Part (a) is contained in Lemma 2 and Theorem 3(ii).

Part (b). We exhibit the family (Heyde [9]). Let ff be the log-normal density with parameters (μ,σ2)(\mu, \sigma^2) and, for c1|c| \le 1, define

fc(x)=f(x)[1+csin ⁣(2π(lnxμ)σ2)],x>0.f_c(x) = f(x)\,\Bigl[\,1 + c\,\sin\!\Bigl(\tfrac{2\pi(\ln x - \mu)}{\sigma^2}\Bigr)\Bigr], \qquad x > 0.

Substituting lnx=μ+σz\ln x = \mu + \sigma z with ZZ standard normal, for every nN0n \in \mathbb{N}_0:

0xnf(x)sin ⁣(2π(lnxμ)σ2)dx=enμE[enσZsin ⁣(2πZσ)]=enμe(n2σ24π2/σ2)/2sin(2πn)=0,\int_0^\infty x^n f(x)\sin\!\Bigl(\tfrac{2\pi(\ln x-\mu)}{\sigma^2}\Bigr)\,dx = e^{n\mu}\,\mathbb{E}\Bigl[e^{n\sigma Z}\sin\!\Bigl(\tfrac{2\pi Z}{\sigma}\Bigr)\Bigr] = e^{n\mu}\, e^{(n^2\sigma^2 - 4\pi^2/\sigma^2)/2}\,\sin(2\pi n) = 0,

using E[e(α+iβ)Z]=e(α+iβ)2/2\mathbb{E}[e^{(\alpha+i\beta')Z}] = e^{(\alpha+i\beta')^2/2}, whose imaginary part is e(α2β2)/2sin(αβ)e^{(\alpha^2-\beta'^2)/2}\sin(\alpha\beta'), with α=nσ\alpha = n\sigma, β=2π/σ\beta' = 2\pi/\sigma, αβ=2πn\alpha\beta' = 2\pi n. The case n=0n = 0 shows each fcf_c is a probability density (and fc0f_c \ge 0 since c1|c| \le 1); the cases n1n \ge 1 show all fcf_c share the log-normal moments exp(nμ+n2σ2/2)\exp(n\mu + n^2\sigma^2/2). Hence uncountably many distinct laws realize the moment sequence. \square

Remark. Indeterminacy cannot be inferred from the convergence of the Carleman sum: Carleman's condition is sufficient for determinacy but not necessary, so its failure proves nothing. The explicit family above is the classical argument.

Theorem 10 (Stability)

Let {Wn}\{W_n\} be an i.i.d. multiplicative cascade with log-infinitely-divisible generator, all moments finite, and nontrivial intermittency. Suppose there exist β(0,1)\beta \in (0,1), dRd^\ast \in \mathbb{R} and ε>0\varepsilon > 0 such that

δp+k(1β)dβδp<εfor all pkN0.\bigl|\delta_{p+k} - (1-\beta)\,d^\ast - \beta\,\delta_p\bigr| < \varepsilon \qquad\text{for all } p \in k\mathbb{N}_0.

Then σ2=0\sigma^2 = 0, suppν(,0]\mathrm{supp}\,\nu \subseteq (-\infty,0], (x1)dν<\int(|x|\wedge1)\,d\nu < \infty, the limit δ:=limpδp\delta_\infty := \lim_{p\to\infty}\delta_p exists finitely, and (1β)dδε(1-\beta)\,|d^\ast - \delta_\infty| \le \varepsilon. Moreover, with u=ekxu = e^{kx}, η=(1u)dν~\eta = (1-u)\,d\tilde\nu, and A=(δ0δ)lnrA = (\delta_0 - \delta_\infty)\ln r:

(i) if d=δd^\ast = \delta_\infty (the true limit is known),

W1 ⁣(ηη,  δβ)    ((1+β)lnrA) ⁣1/2 ⁣ε;W_1\!\left(\frac{\eta}{\|\eta\|},\;\delta_\beta\right) \;\leq\; \left(\frac{(1+\beta)\,|\ln r|}{|A|}\right)^{\!1/2}\!\sqrt{\varepsilon}\,;

(ii) in general (fitted dd^\ast),

W1 ⁣(ηη,  δβ)    (2lnrA) ⁣1/2 ⁣ε.W_1\!\left(\frac{\eta}{\|\eta\|},\;\delta_\beta\right) \;\leq\; \left(\frac{2\,|\ln r|}{|A|}\right)^{\!1/2}\!\sqrt{\varepsilon}\,.

Both constants are sharp in their respective settings. In particular, the cascade multiplier distribution converges to log-Poisson as ε0\varepsilon \to 0, at the sharp rate Θ(ε)\Theta(\sqrt{\varepsilon}) (Theorems 11 and 12).

Proof.

Step 0 (reduction and existence of the limit). From the hypothesis, δ(m+1)kβδmk+(1β)d+ε|\delta_{(m+1)k}| \le \beta|\delta_{mk}| + (1-\beta)|d^\ast| + \varepsilon, so the lattice sequence {δmk}\{\delta_{mk}\} is bounded: lim supmδmkd+ε/(1β)\limsup_m |\delta_{mk}| \le |d^\ast| + \varepsilon/(1-\beta). But by Steps 2, 3 and 3½ of the proof of Theorem 7—none of which used the exact form of A1, only the finiteness of lim inf\liminf of {δp}\{\delta_p\}—each of the conditions σ2>0\sigma^2 > 0, ν((0,))>0\nu((0,\infty)) > 0, x1xdν=\int_{|x|\le1}|x|\,d\nu = \infty forces δmk\delta_{mk} \to -\infty, a contradiction. Hence σ2=0\sigma^2 = 0, suppν(,0]\mathrm{supp}\,\nu \subseteq (-\infty,0], (x1)dν<\int(|x|\wedge1)\,d\nu < \infty; the split form of ϕ\phi is valid, dominated convergence gives ϕ(p)c0\phi(p) \to c_0, and δ=c0/lnr\delta_\infty = c_0/\ln r exists finitely. Letting mm \to \infty in the hypothesis,

δ(1β)dβδε(1β)dδε.\bigl|\delta_\infty - (1-\beta)d^\ast - \beta\delta_\infty\bigr| \le \varepsilon \quad\Longrightarrow\quad (1-\beta)\,|d^\ast - \delta_\infty| \le \varepsilon.

Step 1 (exact moment identities and residuals). As in Step 4 of Theorem 7 (now with no approximation in the identity itself),

μm:=(0,1)umdη=(δmkδ)lnr    0for all m0,\mu_m := \int_{(0,1)} u^m\,d\eta = \bigl(\delta_{mk} - \delta_\infty\bigr)\,|\ln r| \;\ge\; 0 \qquad\text{for all } m \ge 0,

in particular η=μ0=(δ0δ)lnr=A\|\eta\| = \mu_0 = (\delta_0 - \delta_\infty)|\ln r| = |A| exactly. Define the signed residuals

ϵm:=δ(m+1)k(1β)δβδmk=μm+1βμmlnr,\epsilon_m := \delta_{(m+1)k} - (1-\beta)\,\delta_\infty - \beta\,\delta_{mk} = \frac{\mu_{m+1} - \beta\,\mu_m}{|\ln r|},

and let hmh_m denote the hypothesis residuals (with dd^\ast in place of δ\delta_\infty), hm<ε|h_m| < \varepsilon. Setting t:=(1β)(dδ)t := (1-\beta)(d^\ast - \delta_\infty), tε|t| \le \varepsilon by Step 0, one has ϵm=hm+t\epsilon_m = h_m + t. Under reading (i), t=0t = 0 and ϵm<ε|\epsilon_m| < \varepsilon.

Step 2 (variance identity). Telescoping,

(0,1)(uβ)2dη=μ22βμ1+β2μ0=(μ2βμ1)β(μ1βμ0)=lnr(ϵ1βϵ0).\int_{(0,1)} (u-\beta)^2\,d\eta = \mu_2 - 2\beta\mu_1 + \beta^2\mu_0 = (\mu_2 - \beta\mu_1) - \beta(\mu_1 - \beta\mu_0) = |\ln r|\,\bigl(\epsilon_1 - \beta\,\epsilon_0\bigr).

Under reading (i): ϵ1βϵ0<(1+β)ε|\epsilon_1 - \beta\epsilon_0| < (1+\beta)\varepsilon. Under reading (ii): ϵ1βϵ0=(h1βh0)+(1β)t\epsilon_1 - \beta\epsilon_0 = (h_1 - \beta h_0) + (1-\beta)t, so ϵ1βϵ0<(1+β)ε+(1β)ε=2ε|\epsilon_1 - \beta\epsilon_0| < (1+\beta)\varepsilon + (1-\beta)\varepsilon = 2\varepsilon. Hence

0    (0,1)(uβ)2dη    {(1+β)lnrε(i),2lnrε(ii).0 \;\le\; \int_{(0,1)}(u-\beta)^2\,d\eta \;\le\; \begin{cases} (1+\beta)\,|\ln r|\,\varepsilon & \text{(i)},\\ 2\,|\ln r|\,\varepsilon & \text{(ii)}. \end{cases}

Step 3 (Wasserstein bound). For a Dirac target the W1W_1 distance is the first absolute moment: W1(η/η,δβ)=η1uβdηW_1(\eta/\|\eta\|, \delta_\beta) = \|\eta\|^{-1}\int|u-\beta|\,d\eta. By Cauchy–Schwarz and η=A\|\eta\| = |A|,

W1 ⁣(ηη,δβ)    (1A(uβ)2dη)1/2    {((1+β)lnr/A)1/2ε(i),(2lnr/A)1/2ε(ii).W_1\!\left(\frac{\eta}{\|\eta\|},\,\delta_\beta\right) \;\le\; \Bigl(\frac{1}{|A|}\int (u-\beta)^2\,d\eta\Bigr)^{1/2} \;\le\; \begin{cases} \bigl((1+\beta)\,|\ln r|/|A|\bigr)^{1/2}\sqrt{\varepsilon} & \text{(i)},\\ \bigl(2\,|\ln r|/|A|\bigr)^{1/2}\sqrt{\varepsilon} & \text{(ii)}. \end{cases} \qquad\square

Remark (Sharpness; a warning about per-moment transfer).

(a) The constant in reading (i) is attained in the limit by the two-atom family η=c0δu0+c1δv\eta = c_0\delta_{u_0} + c_1\delta_v with u00u_0 \downarrow 0, v(β,1)v \in (\beta,1), c1v(vβ)=εlnrc_1 v(v-\beta) = \varepsilon|\ln r| and c0=(εlnr/β)(1+1/v)c_0 = (\varepsilon|\ln r|/\beta)(1 + 1/v): then ϵ0ε\epsilon_0 \to -\varepsilon, ϵ1=+ε\epsilon_1 = +\varepsilon, ϵm=εvm1ε|\epsilon_m| = \varepsilon v^{m-1} \le \varepsilon for m2m \ge 2, and (uβ)2dη(1+β)lnrε\int(u-\beta)^2 d\eta \to (1+\beta)|\ln r|\varepsilon.

(b) The constant in reading (ii) is likewise attained: choose moment residuals (ϵ0,ϵ1)(0,2ε)(\epsilon_0, \epsilon_1) \to (0, 2\varepsilon) realized by two atoms (one near 00, one in (β,1)(\beta,1)) and the offset tεt \to \varepsilon; all hypothesis residuals hm=ϵmth_m = \epsilon_m - t then stay below ε\varepsilon in absolute value. For β<21\beta < \sqrt{2} - 1 one has 2>(1+β)22 > (1+\beta)^2: the distinction between the two readings is quantitatively real, and a constant valid in reading (i)—even the non-sharp (1+β)2(1+\beta)^2—can fail outright in reading (ii).

(c) A tempting route passes through the per-moment estimate μmAβmlnrε|\mu_m - |A|\beta^m| \le |\ln r|\,\varepsilon for all mm. That estimate is false in general: recurrence errors accumulate to μmAβmlnrε1βm1β|\mu_m - |A|\beta^m| \le |\ln r|\,\varepsilon\,\tfrac{1-\beta^m}{1-\beta}, and the bound is attained in the limit by η=(Ac)δβ+cδv\eta = (|A|-c)\delta_\beta + c\,\delta_v with c(vβ)=εlnrc(v-\beta) = \varepsilon|\ln r|, v1v \to 1, for which supmμmAβm/(lnrε)1/(1β)\sup_m |\mu_m - |A|\beta^m| / (|\ln r|\varepsilon) \to 1/(1-\beta). It is also unnecessary: only ϵ0\epsilon_0 and ϵ1\epsilon_1 enter the variance identity.

5. Propagation: The Sharp Rate

We now transfer the bound of Theorem 10 from the Lévy measure to the multiplier distribution, at a rate that is exact: O(ε)O(\sqrt{\varepsilon}) with no further hypotheses (Theorem 11), and no better (Theorem 12).

Throughout this section the hypotheses are those of Theorem 10, reading (i) (for reading (ii) replace (1+β)(1+\beta) by 22 in every constant), so that Step 0 there gives σ2=0\sigma^2 = 0, suppν(,0]\mathrm{supp}\,\nu \subseteq (-\infty,0], (x1)dν<\int(|x|\wedge1)\,d\nu < \infty, and Steps 2–3 give, with Vε:=(1+β)lnrεV_\varepsilon := (1+\beta)|\ln r|\,\varepsilon and S:=((1+β)Alnr)1/2S := \bigl((1+\beta)\,|A|\,|\ln r|\bigr)^{1/2},

(0,1)(uβ)2dη    Vε,(0,1)uβdη    Sε.(2)\int_{(0,1)}(u-\beta)^2\,d\eta \;\le\; V_\varepsilon, \qquad \int_{(0,1)}|u-\beta|\,d\eta \;\le\; S\sqrt{\varepsilon}. \tag{2}

The Lévy measure may have infinite total mass, accumulating only at u=1u = 1 where the tilt (1u)(1-u) vanishes; the multiplier is the a.s.-convergent product over the Poisson point process {Ui}\{U_i\} of intensity ν~\tilde\nu,

W=eaεiUi1/k,i(1Ui1/k)2ki(1Ui)  of finite mean 2kηW = e^{a_\varepsilon}\prod_i U_i^{1/k}, \qquad \sum_i\bigl(1 - U_i^{1/k}\bigr) \le \tfrac{2}{k}\sum_i(1-U_i) \ \text{ of finite mean } \tfrac{2}{k}\|\eta\|

(Campbell's formula [12]). Under E[W]=1\mathbb{E}[W]=1 the drift is aε=(1u1/k)dν~<a_\varepsilon = \int(1-u^{1/k})\,d\tilde\nu < \infty. The comparison target W0W_0 is the log-Poisson multiplier with jump factor β1/k\beta^{1/k}, rate λ=A/(1β)\lambda = |A|/(1-\beta), and drift a0a_0 fixed by the same normalization.

Theorem 11 (Unconditional propagation)

Under the hypotheses of Theorem 10 alone—no finite-activity or minimum-jump assumption—there exist ε0>0\varepsilon_0 > 0 and an explicit constant K=K(β,C,r,k)K_\infty = K_\infty(\beta, C, r, k) such that for all εε0\varepsilon \le \varepsilon_0,

W1(law(W), law(W0))    Kε.W_1\bigl(\mathrm{law}(W),\ \mathrm{law}(W_0)\bigr) \;\le\; K_\infty\,\sqrt{\varepsilon}.

One admissible (not optimized) choice is

K=4ea0+1(Lk1β+1(1β)2)(1+β)Alnr,Lk=1k(β2)(1k)/k,K_\infty = 4\,e^{a_0+1}\Bigl(\frac{L_k}{1-\beta} + \frac{1}{(1-\beta)^2}\Bigr)\sqrt{(1+\beta)\,|A|\,|\ln r|}\,, \qquad L_k = \tfrac{1}{k}\bigl(\tfrac{\beta}{2}\bigr)^{(1-k)/k},

absorbing O(ε)O(\varepsilon) terms via εε\varepsilon \le \sqrt{\varepsilon}.

Proof. Fix the ε\varepsilon-independent split height

h0:=1β2,u0:=1h0=1+β2,h_0 := \tfrac{1-\beta}{2}, \qquad u_0 := 1 - h_0 = \tfrac{1+\beta}{2},

and call a jump small if u(u0,1)u \in (u_0, 1), macroscopic if u(0,u0]u \in (0, u_0].

Step 1 (small jumps: individually cheap, collectively O(ε)). Every u(u0,1)u \in (u_0,1) lies at distance >h0> h_0 from β\beta, so by Chebyshev's inequality against (2),

η((u0,1))    Vεh02  =  4(1+β)lnr(1β)2ε.\eta\bigl((u_0,1)\bigr) \;\le\; \frac{V_\varepsilon}{h_0^{\,2}} \;=\; \frac{4(1+\beta)|\ln r|}{(1-\beta)^2}\,\varepsilon.

Leave the small-jump points of WW unpaired and cost them multiplicatively: for factors in (0,1](0,1], telescoping gives isi1i(1si)|\prod_i s_i - 1| \le \sum_i(1-s_i) (valid for infinite products by monotone limits), and 1u1/k2k(1u)1 - u^{1/k} \le \tfrac{2}{k}(1-u) for u12u \ge \tfrac{1}{2} (derivative bound; u012u_0 \ge \tfrac{1}{2}). By Campbell's formula,

EsmallUi1/k1    2k(u0,1)(1u)dν~  =  2kη((u0,1))    8(1+β)lnrk(1β)2ε.\mathbb{E}\Bigl|\prod_{\text{small}} U_i^{1/k} - 1\Bigr| \;\le\; \frac{2}{k}\int_{(u_0,1)}(1-u)\,d\tilde\nu \;=\; \frac{2}{k}\,\eta\bigl((u_0,1)\bigr) \;\le\; \frac{8(1+\beta)|\ln r|}{k(1-\beta)^2}\,\varepsilon.

This is the step that controls infinite activity: a near-1 jump's cost is its multiplicative deviation ≍(1−u)—already η-weighted—not the count 1.

Step 2 (the macroscopic part is automatically finite-activity, with a fixed de-tilting constant). On (0,u0](0,u_0]: 11u1h0=21β\tfrac{1}{1-u} \le \tfrac{1}{h_0} = \tfrac{2}{1-\beta}, so λmac:=ν~((0,u0])2A1β<\lambda_{\mathrm{mac}} := \tilde\nu((0,u_0]) \le \tfrac{2|A|}{1-\beta} < \infty. Comparing rates against λ=A/(1β)=dη1β\lambda = |A|/(1-\beta) = \int\tfrac{d\eta}{1-\beta}, and using 11u11β=uβ(1u)(1β)2uβ(1β)2\bigl|\tfrac{1}{1-u} - \tfrac{1}{1-\beta}\bigr| = \tfrac{|u-\beta|}{(1-u)(1-\beta)} \le \tfrac{2|u-\beta|}{(1-\beta)^2} on (0,u0](0,u_0],

λmacλ    2(1β)2Sε  +  η((u0,1))1β,\bigl|\lambda_{\mathrm{mac}} - \lambda\bigr| \;\le\; \frac{2}{(1-\beta)^2}\,S\sqrt{\varepsilon} \;+\; \frac{\eta((u_0,1))}{1-\beta},

the second term being O(ε)O(\varepsilon) by Step 1.

Step 3 (macroscopic jump cost). The map uu1/ku \mapsto u^{1/k} is LkL_k-Lipschitz on [β/2,1][\beta/2,1] and bounded by 11 below β/2\beta/2; on (0,β/2)(0,\beta/2), 11u11β/22\tfrac{1}{1-u} \le \tfrac{1}{1-\beta/2} \le 2, so ν~((0,β/2))2η((0,β/2))2Vε(β/2)2\tilde\nu((0,\beta/2)) \le 2\eta((0,\beta/2)) \le 2V_\varepsilon(\beta/2)^{-2} by Chebyshev. Hence

(0,u0]u1/kβ1/kdν~    2Lk1βSε  +  8Vεβ2.\int_{(0,u_0]}\bigl|u^{1/k} - \beta^{1/k}\bigr|\,d\tilde\nu \;\le\; \frac{2L_k}{1-\beta}\,S\sqrt{\varepsilon} \;+\; \frac{8\,V_\varepsilon}{\beta^2}.

Step 4 (assembly). Couple the macroscopic Poisson count with W0W_0's count by thinning (shared count Poisson(λλmac)\mathrm{Poisson}(\lambda\wedge\lambda_{\mathrm{mac}}), excess independent; [3], Theorem 10.A), shared jump pairs optimally in the multiplier coordinate against the constant target β1/k\beta^{1/k}, and leave the small jumps unpaired. Writing W=eaεPmacPsmallW = e^{a_\varepsilon}P_{\mathrm{mac}}P_{\mathrm{small}} and W0=ea0P0W_0 = e^{a_0}P_0 with all products in [0,1][0,1], the telescoping inequality and Wald's identity give

EPmacPsmallP0    (0,u0] ⁣u1/kβ1/kdν~Step 3  +  λmacλStep 2  +  EPsmall1Step 1,\mathbb{E}\bigl|P_{\mathrm{mac}}P_{\mathrm{small}} - P_0\bigr| \;\le\; \underbrace{\int_{(0,u_0]}\!\bigl|u^{1/k}-\beta^{1/k}\bigr|\,d\tilde\nu}_{\text{Step 3}} \;+\; \underbrace{\bigl|\lambda_{\mathrm{mac}} - \lambda\bigr|}_{\text{Step 2}} \;+\; \underbrace{\mathbb{E}\bigl|P_{\mathrm{small}} - 1\bigr|}_{\text{Step 1}},

each excess jump on either side changing a product by at most 11. The drift difference obeys the same bound: under E[W]=1\mathbb{E}[W]=1, aεa0=(1u1/k)dν~λ(1β1/k)a_\varepsilon - a_0 = \int(1-u^{1/k})\,d\tilde\nu - \lambda(1-\beta^{1/k}) decomposes into the same three pieces. Both multipliers are bounded by eae^{a_\cdot} (Lemma 2(i)), so for εε0\varepsilon \le \varepsilon_0 with aεa01|a_\varepsilon - a_0| \le 1,

W1EWW0ea0+1(EPmacPsmallP0+aεa0)2ea0+1[Step 1+Step 2+Step 3].W_1 \le \mathbb{E}|W - W_0| \le e^{a_0+1}\Bigl(\mathbb{E}|P_{\mathrm{mac}}P_{\mathrm{small}} - P_0| + |a_\varepsilon - a_0|\Bigr) \le 2e^{a_0+1}\bigl[\text{Step 1} + \text{Step 2} + \text{Step 3}\bigr].

Substituting the three displays and absorbing every O(ε)O(\varepsilon) term via εε\varepsilon \le \sqrt{\varepsilon} yields the stated KK_\infty. \square

Remark (Why no hypotheses are needed). A coupling built in log-space would require finite activity and a minimum jump size—a Poisson count must be finite, and a de-tilting factor must be bounded—and an ε\varepsilon-dependent shell decomposition for the small jumps would surrender a logarithmic factor, O(εlog(1/ε))O(\sqrt{\varepsilon}\log(1/\varepsilon)). In the multiplicative coupling both holes close themselves: infinite activity can only accumulate at u=1u = 1, where multiplicative cost vanishes at exactly the rate η\eta measures, and the de-tilting factor appears only on (0,u0](0,u_0], where it is the fixed constant 2/(1β)2/(1-\beta). The flatness of the exponential map at -\infty, fatal to couplings of jump distributions in xx-space, is the resource here.

Theorem 12 (Lower bound: the rate √ε is exact)

Fix (β,C,r)(\beta, C, r), k=1k = 1, and conservation E[W]=1\mathbb{E}[W]=1. For d(0,d0]d \in (0, d_0], d0=d0(β)d_0 = d_0(\beta) small, let W(d)W_{(d)} be the compound-Poisson multiplier with tilted measure

ηd=A2(δβd+δβ+d)\eta_d = \tfrac{|A|}{2}\bigl(\delta_{\beta-d} + \delta_{\beta+d}\bigr)

(jump atoms β±d\beta\pm d with Lévy masses A/21(β±d)\tfrac{|A|/2}{1-(\beta\pm d)}, drift by conservation). Then:

(i) its A1 residual satisfies

Alnrd2    ε(d)    c2(β)Alnrd2,\dfrac{|A|}{|\ln r|}\,d^2 \;\le\; \varepsilon(d) \;\le\; c_2(\beta)\,\dfrac{|A|}{|\ln r|}\,d^2,

where c2(β)=[eminρ[β,(1+β)/2]ρlnρ]11c_2(\beta) = \bigl[e\min_{\rho\in[\beta,(1+\beta)/2]}\rho|\ln\rho|\bigr]^{-1} \vee 1;

(ii) with λd=ν~d=λ/(1d2(1β)2)\lambda_d = \|\tilde\nu_d\| = \lambda/(1 - d^2(1-\beta)^{-2}) and a=Aa = |A|,

W1(lawW(d), lawW0)    λdeλdead    c1(β,C,r)ε(d).W_1\bigl(\mathrm{law}\,W_{(d)},\ \mathrm{law}\,W_0\bigr) \;\ge\; \lambda_d\,e^{-\lambda_d}\,e^{a}\,d \;\ge\; c_1(\beta, C, r)\,\sqrt{\varepsilon(d)}\,.

Hence no propagation bound of order o(ε)o(\sqrt{\varepsilon}) is possible: combined with Theorem 11, the exact rate is Θ(ε)\Theta(\sqrt{\varepsilon}).

Proof.

(i) The moments are μm=A2[(βd)m+(β+d)m]\mu_m = \tfrac{|A|}{2}[(\beta-d)^m + (\beta+d)^m], so the signed residuals are

ϵm=μm+1βμmlnr=Ad2lnr[(β+d)m(βd)m]  0,\epsilon_m = \frac{\mu_{m+1} - \beta\mu_m}{|\ln r|} = \frac{|A|\,d}{2\,|\ln r|}\bigl[(\beta+d)^m - (\beta-d)^m\bigr] \;\ge 0,

with ϵ0=0\epsilon_0 = 0 and ϵ1=Ad2/lnr\epsilon_1 = |A|d^2/|\ln r| exactly, giving the lower bound on ε(d)=supmϵm\varepsilon(d) = \sup_m \epsilon_m. For the upper bound, the mean value theorem gives (β+d)m(βd)m2dm(β+d)m1(\beta+d)^m - (\beta-d)^m \le 2dm(\beta+d)^{m-1}, and supx0xρx1=(eρlnρ)1\sup_{x\ge0} x\rho^{x-1} = (e\rho|\ln\rho|)^{-1} for ρ=β+d(1+β)/2\rho = \beta+d \le (1+\beta)/2.

(ii) For k=1k=1 the conservation drift is a(d)=(1u)dν~d=ηd=Aa_{(d)} = \int(1-u)\,d\tilde\nu_d = \|\eta_d\| = |A|, identical to a0=λ(1β)=Aa_0 = \lambda(1-\beta) = |A|: the family is drift-rigid. The support of law(W0)\mathrm{law}(W_0) is the geometric set G={eaβj:j0}G = \{e^{a}\beta^j : j \ge 0\}. Take the 1-Lipschitz test function

f(w):=min(dist(w,G), eaβ(1β)2)    0,f(w) := \min\Bigl(\mathrm{dist}\bigl(w,\,G\bigr),\ \tfrac{e^a\beta(1-\beta)}{2}\Bigr) \;\ge\; 0,

which vanishes on GG, so Ef(W0)=0\mathbb{E}f(W_0) = 0. On the one-jump event of W(d)W_{(d)} (probability λdeλd\lambda_d e^{-\lambda_d}), W(d)=ea(β±d)W_{(d)} = e^{a}(\beta\pm d), whose distance to the nearest point of GG is exactly eade^a d for d<β(1β)/2d < \beta(1-\beta)/2 (the neighbors eae^a and eaβ2e^a\beta^2 are farther, and eade^ad is below the cap); all other events contribute 0\ge 0. By Kantorovich–Rubinstein duality [19],

W1    Ef(W(d))Ef(W0)    λdeλdead,W_1 \;\ge\; \mathbb{E}f(W_{(d)}) - \mathbb{E}f(W_0) \;\ge\; \lambda_d e^{-\lambda_d}\,e^{a}\,d,

and substituting d(lnrε(d)/(c2(β)A))1/2d \ge \bigl(|\ln r|\,\varepsilon(d) / (c_2(\beta)|A|)\bigr)^{1/2} from (i) gives the c1εc_1\sqrt{\varepsilon} form. (The same construction works for k>1k > 1 on the lattice {eaβj/k}\{e^{a}\beta^{j/k}\}; k=1k = 1 is stated for cleanliness.) \square

Remark (The stability theory is elementary and now complete). The change of variables u=ekxu = e^{kx} maps the Lévy measure to the compact interval [0,1][0,1], where a second-moment test against the candidate atom decides everything: the classification is the ε=0\varepsilon = 0 case of the variance identity in Theorem 10, Step 2; the stability constant is read off two residuals and is sharp; and the propagation to the multiplier law is a telescoped multiplicative coupling with no tail estimates (boundedness, Lemma 2(i)), sharp in rate by Theorem 12. Every quantitative statement in the package—variance constant (1+β)(1+\beta), Wasserstein constant, propagation rate Θ(ε)\Theta(\sqrt{\varepsilon})—is attained by an explicit family. In particular the log-Poisson class is an open set, with exactly computed modulus, in the space of cascade multiplier distributions metrized by A1 residuals.

6. Beyond Independence: Stationary and Markov Multipliers

The i.i.d. assumption enters the preceding sections through the identity E[(W1Wn)p]=(E[Wp])n\mathbb{E}[(W_1\cdots W_n)^p] = (\mathbb{E}[W^p])^n, which converts scaling data into one-step moment data. This section determines exactly what survives without it. Let (Wn)(W_n) be stationary ergodic, Xn=lnWnX_n = \ln W_n, Sn=X1++XnS_n = X_1 + \cdots + X_n, and define exponents asymptotically:

Standing assumptions (S). For each lattice pp: mn(p):=E[epSn]<m_n(p) := \mathbb{E}[e^{pS_n}] < \infty for all nn, and

Λ(p):=limn1nlnmn(p)exists and is finite;ζp:=Λ(p)/lnr.\Lambda(p) := \lim_{n\to\infty}\tfrac{1}{n}\ln m_n(p) \quad\text{exists and is finite}; \qquad \zeta_p := \Lambda(p)/\ln r.

A1 is imposed on δp=ζp+kζp\delta_p = \zeta_{p+k}-\zeta_p as before. Write ΛLP(p)=ap+λ(ebp1)\Lambda_{\mathrm{LP}}(p) = ap + \lambda(e^{bp}-1) for the log-Poisson limiting cumulant function with the parameter dictionary of Theorem 3.

Theorem 13 (Asymptotic-statistics classification)

Under (S), A1 holds on the lattice if and only if Λ=ΛLP\Lambda = \Lambda_{\mathrm{LP}} on the lattice. Consequently, under A1 every observable computed from lattice exponents—structure-function exponents, moment ratios, and (under the regularity below) the large-deviation rate function and multifractal spectrum—coincides exactly with that of the i.i.d. log-Poisson cascade with parameters (β,γ,C)(\beta, \gamma, C).

Proof. Lemma 1 is purely algebraic, so A1 gives Λ(km)=akm+λ(ebkm1)\Lambda(km) = a\,km + \lambda(e^{b\,km}-1) for all mm; the converse is the computation of Proposition 5. \square

Remark. If Λ\Lambda exists, is finite and differentiable on a neighborhood of [0,)[0,\infty), the Gärtner–Ellis theorem [6] yields a large-deviation principle for Sn/nS_n/n with rate I(h)=supp[phΛ(p)]I(h) = \sup_p[ph - \Lambda(p)] on the exposed range—the Legendre structure of Theorem 3(iii). Off-lattice, Λ\Lambda is pinned between consecutive lattice values by convexity.

Theorem 13 is deliberately easy; the substantive question is whether A1 still determines the multiplier law. It does not:

Theorem 14 (Interleaved cascade: the law is not determined)

There exists a stationary ergodic multiplier sequence (Wn)(W_n)—realizable as a function of a stationary, irreducible, positive-recurrent countable-state Markov chain—such that:

(i) mn(p)=rnζpLPm_n(p) = r^{n\zeta^{\mathrm{LP}}_p} exactly for every even nn and every real p0p \ge 0; hence (S) holds, Λ=ΛLP\Lambda = \Lambda_{\mathrm{LP}} on all of [0,)[0,\infty), and A1 holds exactly, in its strongest (real-pp) form;

(ii) the one-step marginal of lnW1\ln W_1 is not log-Poisson;

(iii) the sequence is not i.i.d., and is not equal in law to any i.i.d. cascade.

Consequently the law-level conclusion of Theorem 3 does not extend beyond independence, by any proof.

Proof.

Construction. With (a,b,λ)(a, b, \lambda) as in Theorem 3 and λ:=2λ\lambda' := 2\lambda, let A1,A2,A_1, A_2, \ldots be i.i.d. Poisson(λ)\mathrm{Poisson}(\lambda'), define

Y2j1=a+bAj,Y2j=a(j1),Y_{2j-1} = a + bA_j, \qquad Y_{2j} = a \qquad (j \ge 1),

draw a phase θUnif{0,1}\theta \sim \mathrm{Unif}\{0,1\} independent of everything, and set Xn:=Yn+θX_n := Y_{n+\theta}, Wn:=eXnW_n := e^{X_n}: jump slots of doubled intensity alternate with deterministic slots.

Stationarity and Markov realization. The pair Zn:=((n+θ)mod2,Xn)Z_n := ((n+\theta)\bmod 2,\, X_n) is a Markov chain on {0,1}×(a+bN0)\{0,1\}\times(a+b\mathbb{N}_0): from phase-1 states the next value is a+bAa + bA with fresh APoisson(λ)A \sim \mathrm{Poisson}(\lambda') and the phase flips; from phase-0 states the next value is aa and the phase flips. The chain is irreducible on its reachable set and positive recurrent; the phase-uniform stationary law makes (Zn)(Z_n) stationary and WnW_n a function of it.

Ergodicity. Let P0,P1P_0, P_1 be the path laws given θ=0,1\theta = 0,1, so the law is 12(P0+P1)\tfrac{1}{2}(P_0+P_1) with P1=P0T1P_1 = P_0\circ T^{-1} (TT = shift). If EE is TT-invariant, it is T2T^2-invariant, and under P0P_0 the double shift is ergodic (the blocks (Y2j1,Y2j)(Y_{2j-1}, Y_{2j}) are i.i.d.), so P0(E){0,1}P_0(E) \in \{0,1\}; and P1(E)=P0(T1E)=P0(E)P_1(E) = P_0(T^{-1}E) = P_0(E). Hence P(E){0,1}\mathbb{P}(E) \in \{0,1\}.

Exact exponents. For even n=2mn = 2m the window {1,,2m}\{1,\ldots,2m\} contains exactly mm jump slots under either phase, carrying mm distinct i.i.d. AjA_j's; hence, exactly, for every real pp,

m2m(p)=e2mapexp[mλ(ebp1)]=exp[2m(ap+λ(ebp1))]=exp[2mΛLP(p)].m_{2m}(p) = e^{2map}\exp\bigl[m\lambda'(e^{bp}-1)\bigr] = \exp\bigl[2m\bigl(ap + \lambda(e^{bp}-1)\bigr)\bigr] = \exp\bigl[2m\,\Lambda_{\mathrm{LP}}(p)\bigr].

For odd nn the window covers mm or m+1m+1 jump slots depending on the phase, and 1nlnmn(p)ΛLP(p)\tfrac{1}{n}\ln m_n(p) \to \Lambda_{\mathrm{LP}}(p). Theorem 13 then gives A1 exactly.

Non-log-Poisson marginal. P(X1=a)=12(1+e2λ)\mathbb{P}(X_1 = a) = \tfrac{1}{2}(1 + e^{-2\lambda}), whereas the log-Poisson(λ\lambda) marginal has P(X=a)=eλ\mathbb{P}(X = a) = e^{-\lambda}; for She–Lévêque dissipation parameters (λ=2ln2\lambda = 2\ln 2): 0.5310.531 versus 0.2500.250. The marginal is the mixture 12δa+12law(a+bPoisson(2λ))\tfrac{1}{2}\delta_a + \tfrac{1}{2}\,\mathrm{law}(a + b\,\mathrm{Poisson}(2\lambda)).

Non-i.i.d. Given XnaX_n \ne a the next multiplier is deterministic: P(Xn+1=aXna)=1P(Xn+1=a)\mathbb{P}(X_{n+1} = a \mid X_n \ne a) = 1 \ne \mathbb{P}(X_{n+1} = a). \square

Remark. The construction generalizes freely (blocks of length LL, arbitrary allocation of the total jump intensity across slots, Markov-modulated loads): A1 is compatible with an infinite-dimensional family of mutually singular stationary ergodic processes, all sharing the log-Poisson asymptotics—exactly as Theorem 13 says they must.

Two rigidity results delimit the boundary of Theorem 14.

Corollary 15 (Exchangeable rigidity)

Let (Wn)(W_n) be exchangeable with mn(p)=rnζpm_n(p) = r^{n\zeta_p} holding exactly for n{1,2}n \in \{1,2\} and all lattice pp, with ζ\zeta satisfying A1. Then (Wn)(W_n) is i.i.d. log-Poisson with parameters (β,γ,C)(\beta, \gamma, C).

Proof. By de Finetti's theorem [11], (Wn)(W_n) is conditionally i.i.d. given a random directing measure; let Mp:=E[W1pdirecting measure]M_p := \mathbb{E}[W_1^p \mid \text{directing measure}]. Conditional independence gives m1(p)=E[Mp]m_1(p) = \mathbb{E}[M_p] and m2(p)=E[Mp2]m_2(p) = \mathbb{E}[M_p^2], so exactness at n=1,2n = 1,2 reads E[Mp]=rζp\mathbb{E}[M_p] = r^{\zeta_p}, E[Mp2]=r2ζp\mathbb{E}[M_p^2] = r^{2\zeta_p}, whence Var(Mp)=0\mathrm{Var}(M_p) = 0: Mp=rζpM_p = r^{\zeta_p} a.s., for every lattice pp simultaneously. Almost every directing measure therefore has exactly the A1 lattice moments, hence equals the log-Poisson law by Lemma 2 and Theorem 3(ii); the mixture is degenerate. \square

Theorem 16 (Finite-state impossibility)

Let ξ\xi be an irreducible finite-state Markov chain, stationary, and Wn=ef(ξn)W_n = e^{f(\xi_n)} with ff non-constant. Then the cascade cannot satisfy A1 in its real-pp form with nontrivial intermittency: there are no parameters (β,γ,C)(\beta, \gamma, C) with C>0C > 0 and ζp=γp+C(1βp/k)\zeta_p = \gamma p + C(1-\beta^{p/k}) for all real p0p \ge 0.

Proof. For finite irreducible chains, Λ(p)=lnρ(M(p))\Lambda(p) = \ln\rho(M(p)) with M(p)xy=Pxyepf(y)M(p)_{xy} = P_{xy}e^{pf(y)} and ρ\rho the Perron root—a simple eigenvalue for every real pp, hence real-analytic on R\mathbb{R}. If the closed form held on [0,)[0,\infty), then Λ(p)=ap+λ(ebp1)\Lambda(p) = ap + \lambda(e^{bp}-1) there with λ=Clnr>0\lambda = -C\ln r > 0; both sides are real-analytic on R\mathbb{R} and agree on an interval, hence agree everywhere (identity theorem). Now let pp \to -\infty. Since fmin=minsf(s)>f_{\min} = \min_s f(s) > -\infty, every row sum of M(p)M(p) is at most epfmine^{pf_{\min}} for p0p \le 0, so Λ(p)pfmin\Lambda(p) \le pf_{\min}: a linear upper bound. But with b<0b < 0,

ΛLP(p)pfmin    λebpλ+p(afmin)    +:\Lambda_{\mathrm{LP}}(p) - pf_{\min} \;\ge\; \lambda e^{|b||p|} - \lambda + p(a - f_{\min}) \;\longrightarrow\; +\infty :

contradiction. \square

Remark (The boundary, and what A1 really is). The mechanism of Theorem 16 is that finite alphabets make lnW\ln W bounded below, while the log-Poisson generator is intrinsically unbounded below (lnWa+bN0\ln W \in a + b\mathbb{N}_0): A1 forces multipliers with arbitrarily severe attenuation events, and the counterexample of Theorem 14 necessarily has unbounded-below lnW\ln W. Assembled, this section says: A1 is an asymptotic-statistics axiom. It pins the limiting cumulant function, the spectrum, and the large deviations to the log-Poisson cascade (Theorem 13); it cannot pin the per-step law (Theorem 14); and the i.i.d. log-Poisson cascade is the canonical realization—unique under exchangeability (Corollary 15), with finite-state Markov realizations impossible (Theorem 16). Whether Theorem 16 persists under lattice-only A1 remains open (the identity-theorem step is unavailable on a discrete set; see Section 9).

7. Continuous Cascades: Log-Infinitely-Divisible Multifractal Measures

We now place the theory in the continuous category of Bacry–Muzy multifractal random measures [2, 15], which contains the log-normal multifractal random walk, log-stable measures, and the Barral–Mandelbrot compound Poisson cascades [4] as special cases. We use two structural properties of the class as axioms:

(M1) Exact stochastic scale invariance. For every σ(0,1)\sigma \in (0,1) and tTt \le T (the integral scale),

(M(σt))t  =d  σeΩσ(M(t))t,\bigl(M(\sigma t)\bigr)_t \;\stackrel{d}{=}\; \sigma\,e^{\Omega_\sigma}\bigl(M(t)\bigr)_t,

with Ωσ\Omega_\sigma infinitely divisible, independent of MM, and E[eqΩσ]=σψ(q)\mathbb{E}[e^{q\Omega_\sigma}] = \sigma^{-\psi(q)}, where ψ\psi is the Lévy exponent of the generator per unit logarithmic scale.

(M2) Conservation. E[eΩσ]=1\mathbb{E}[e^{\Omega_\sigma}] = 1, i.e. ψ(1)=0\psi(1) = 0.

(S_c) ψ(q)<\psi(q) < \infty for all q0q \ge 0 (the continuous analogue of finite multiplier moments).

From (M1), wherever E[M([0,t])q]<\mathbb{E}[M([0,t])^q] < \infty,

E[M([0,t])q]tζq,ζq=qψ(q),\mathbb{E}\bigl[M([0,t])^q\bigr] \propto t^{\zeta_q}, \qquad \zeta_q = q - \psi(q),

and moments of the total mass are finite (for q>1q > 1) precisely on the window where ζq>1\zeta_q > 1 [2]. Since ζ\zeta is concave with ζ1=1\zeta_1 = 1, structure functions see only a finite window [0,q)[0, q^\ast)—a hard information barrier with no discrete counterpart (there the log-Poisson multiplier is bounded and all moments exist). The hierarchical symmetry A1 is imposed on δq=ζq+kζq\delta_q = \zeta_{q+k} - \zeta_q as before.

The dictionary to the discrete theory is one line: with ϕc(q):=ψ(q+k)ψ(q)\phi_c(q) := \psi(q+k) - \psi(q) one has δq=kϕc(q)\delta_q = k - \phi_c(q), and A1 gives, by Lemma 1,

ϕc(mk)ϕc,=Acβm,Ac=(δ0δ)=C(1β)<0:\phi_c(mk) - \phi_{c,\infty} = A_c\,\beta^m, \qquad A_c = -(\delta_0 - \delta_\infty) = -C(1-\beta) < 0 :

formally the discrete identities with lnr1\ln r \mapsto -1, so Ac=C(1β)|A_c| = C(1-\beta) and the rate λ=Clnr\lambda = -C\ln r becomes the intensity CC per unit log-scale. Every lnr|\ln r| in the discrete constants disappears.

Theorem 17 (No finite moment window identifies the class)

Fix the She–Lévêque exponent curve ζqSL=γq+C(1βq/k)\zeta^{\mathrm{SL}}_q = \gamma q + C(1-\beta^{q/k}) normalized by (M2), and any finite lattice window FkN0F \subset k\mathbb{N}_0. Then there is a continuum of exactly scale-invariant log-ID multifractal random measures whose generators are not compound Poisson with a single atom—in particular are not the compound Poisson cascade—yet whose exponents satisfy ζq=ζqSL\zeta_q = \zeta^{\mathrm{SL}}_q for every qFq \in F. Structure-function data on a finite moment window, even exact and noise-free, cannot certify the log-Poisson class.

Proof. We give the construction for k=1k = 1 and the physically typical window F={0,1,2}F = \{0,1,2\} (i.e. 2<q32 < q^\ast \le 3); larger windows are identical with more atoms. In the tilted coordinates u=exu = e^{x}, the CPC generator (Theorem 18) has Π~=Cδβ\tilde\Pi = C\delta_\beta. Perturb:

Π~s=(Csc)δβ+s(w1δv1+w2δv2),0<v1<β<v2<1,\tilde\Pi_s = (C - sc)\,\delta_\beta + s\,(w_1\delta_{v_1} + w_2\delta_{v_2}), \qquad 0 < v_1 < \beta < v_2 < 1,

with the drift re-fixed by (M2) for each ss, and impose

i=1,2wi(vim1)  =  c(βm1),m=1,2.\sum_{i=1,2} w_i\,(v_i^m - 1) \;=\; c\,(\beta^m - 1), \qquad m = 1, 2.

The m=1m=1 equation makes the (M2)-drifts of Π~s\tilde\Pi_s and Π~0\tilde\Pi_0 coincide; the m=2m=2 equation then matches ζ2\zeta_2; ζ0=0\zeta_0 = 0 and ζ1=1\zeta_1 = 1 are automatic. At (β,v1,v2)=(2/3,0.3,0.9)(\beta, v_1, v_2) = (2/3,\,0.3,\,0.9), c=1c = 1, the 2×22\times2 system gives w1=0.1852w_1 = 0.1852, w2=2.0370w_2 = 2.0370, both positive, so Π~s0\tilde\Pi_s \ge 0 for all s[0,C/c]s \in [0, C/c]: a one-parameter family of genuine Lévy measures, none a single atom for s>0s > 0, all matching ζSL\zeta^{\mathrm{SL}} exactly on FF (and differing beyond: at m=3m = 3 the perturbed exponent differs by +0.0143+0.0143 at s=12s = \tfrac{1}{2}). For general finite FF, the same ansatz with more atoms imposes finitely many linear constraints on infinitely many degrees of freedom, with positivity maintained by anchoring the negative part on the CPC atom. \square

Remark. Theorem 17 does not contradict the discrete classification: there A1 was available at all lattice orders—the divergence steps of Theorem 7 need qq \to \infty, and on a finite window even σ02>0\sigma_0^2 > 0 survives (a quadratic log-normal exponent interpolates any three-point window with the correct convexity). Identifiability requires constraints of unbounded order, which structure functions cannot supply. The scale-invariance factor Ωσ\Omega_\sigma can: under (S_c) it has all exponential moments, at every σ\sigma, and its statistics ("magnitude" statistics, in the language of [5]) are observable at all orders.

Theorem 18 (Generator-level classification: A1 selects the compound Poisson cascade)

Let MM satisfy (M1), (M2), (S_c), with nontrivial intermittency C>0C > 0, and define the generator exponents ζq=qψ(q)\zeta_q = q - \psi(q) for all q0q \ge 0. Then A1 on the full lattice kN0k\mathbb{N}_0 holds if and only if

σ02=0,Π=Cδb,b=lnβk<0,\sigma_0^2 = 0, \qquad \Pi = C\,\delta_b, \qquad b = \frac{\ln\beta}{k} < 0,

with drift a~=C(1β1/k)\tilde a = C(1-\beta^{1/k}) fixed by (M2); equivalently

Ωσ  =d  a~ln(1/σ)  +  bPoisson(Cln(1/σ))for every σ(0,1),\Omega_\sigma \;\stackrel{d}{=}\; \tilde a\,\ln(1/\sigma) \;+\; b\,\mathrm{Poisson}\bigl(C\ln(1/\sigma)\bigr) \qquad\text{for every } \sigma \in (0,1),

log-Poisson at every scale ratio simultaneously, and MM is the Barral–Mandelbrot compound Poisson cascade [4] with fixed multiplier atom eb=β1/ke^b = \beta^{1/k} and Poisson intensity CC on the time–log-scale cone. No other member of the Bacry–Muzy class—log-normal, log-stable, or any intermediate—satisfies A1.

Proof.

Reverse: with Π=Cδb\Pi = C\delta_b, ψ(q)=a~q+C(ebq1)\psi(q) = \tilde aq + C(e^{bq}-1), so ζq=qψ(q)=(1a~)q+C(1βq/k)\zeta_q = q - \psi(q) = (1-\tilde a)q + C(1-\beta^{q/k}), which satisfies A1 by Proposition 5 with γ=1a~\gamma = 1 - \tilde a; (M2) gives a~=C(1β1/k)\tilde a = C(1-\beta^{1/k}), the continuous conservation constraint (ζ1=1\zeta_1 = 1).

Forward: ψ\psi is a Lévy–Khintchine exponent, finite for all q0q \ge 0, and ϕc(q)=ψ(q+k)ψ(q)\phi_c(q) = \psi(q+k)-\psi(q) has a finite limit under A1: exactly the hypothesis configuration of Theorem 7's proof under the dictionary lnr1\ln r \mapsto -1. Steps 2, 3, 3½ and 4 of that proof apply verbatim: a Gaussian component, positive jumps, or x1xdΠ=\int_{|x|\le1}|x|\,d\Pi = \infty each force δq=kϕc(q)\delta_q = k - \phi_c(q) \to -\infty; then with η=(1u)dΠ~\eta = (1-u)\,d\tilde\Pi, u=ekxu = e^{kx}, A1 gives umdη=Acβm\int u^m\,d\eta = |A_c|\beta^m and the variance identity yields η=Acδβ\eta = |A_c|\delta_\beta, i.e. Π~=Ac1βδβ=Cδβ\tilde\Pi = \frac{|A_c|}{1-\beta}\delta_\beta = C\delta_\beta and Π=Cδb\Pi = C\delta_b. The identification of the compound-Poisson member of the Bacry–Muzy class with the Barral–Mandelbrot cascade is [2]. \square

Corollary 19 (Stability with native constants)

In the setting of Theorem 18, if A1 holds to within ε\varepsilon on the generator lattice—with dd^\ast the true limit (reading (i)) or fitted (reading (ii))—then σ02=0\sigma_0^2 = 0, Π\Pi is supported on (,0](-\infty,0], and with η=(1u)dΠ~\eta = (1-u)\,d\tilde\Pi, η=Ac=C(1β)\|\eta\| = |A_c| = C(1-\beta) exactly:

W1 ⁣(ηη,δβ)    1+βC(1β)  ε(i),  2C(1β)  ε(ii),W_1\!\Bigl(\frac{\eta}{\|\eta\|},\,\delta_\beta\Bigr) \;\le\; \sqrt{\frac{1+\beta}{C(1-\beta)}}\;\sqrt{\varepsilon} \quad\text{(i)}, \qquad \le\; \sqrt{\frac{2}{C(1-\beta)}}\;\sqrt{\varepsilon} \quad\text{(ii)},

both sharp; for She–Lévêque values (β,C)=(2/3,2)(\beta, C) = (2/3, 2): 1.58ε1.58\sqrt{\varepsilon} and 1.73ε1.73\sqrt{\varepsilon}. The propagation to the law of the per-octave factor eΩ1/2e^{\Omega_{1/2}} holds at the unconditional sharp rate Θ(ε)\Theta(\sqrt{\varepsilon}) of Theorems 11–12 (whose proofs nowhere used finite activity—the natural situation here).

Proof. Theorem 10, Steps 0–3, under the dictionary lnr1\ln r \mapsto -1, AAc=C(1β)|A| \mapsto |A_c| = C(1-\beta); the sharpness families transfer symbol-for-symbol, as does the propagation argument of Section 5. \square

Remark (What the two theorems mean together). Theorems 17 and 18 are two halves of one statement about observability: structure functions cannot identify the cascade class even in principle (a finiteness barrier, not a statistical one), while magnitude statistics classify it completely, with quantitative stability. This places a theorem under the long-standing practical preference for magnitude-cumulant analysis over high-order structure functions [5]. Note also that the continuous category is more rigid than the discrete one: infinite divisibility, an assumption in Theorem 7, is automatic here (consistency of Ωσσ=dΩσ+Ωσ\Omega_{\sigma\sigma'} \stackrel{d}{=} \Omega_\sigma + \Omega'_{\sigma'}), so the classification needs no distributional hypothesis beyond membership in the class. Finally, the most-singular-branch geometry (Corollary 4) reads natively: the probability that the cone above a point carries no Poisson point down to scale \ell is C\ell^{\,C}—codimension CC, with no discretization anywhere.

8. Corollaries

Corollary 20 (Conservation constraint). If there exists an index k0>0k_0 > 0 such that ζk0=z0\zeta_{k_0} = z_0 for a known constant z0z_0 fixed by an exact conservation law, then

γ=z0C(1βk0/k)k0.\gamma = \frac{z_0 - C(1-\beta^{k_0/k})}{k_0}.

This reduces the observable parameters from two to one.

Corollary 21 (Codimension identification). If the most singular structures have Hausdorff codimension CgeomC_{\mathrm{geom}} and C=CgeomC = C_{\mathrm{geom}}, then β\beta alone determines the full exponent curve, the multifractal spectrum, and the cascade distribution.

Corollary 22 (Spectrum width). The width of the multifractal spectrum is

Δh=hmaxhmin=Cklnβ,\Delta h = h_{\max} - h_{\min} = \frac{C}{k}\,|\ln\beta|,

where hmax=γ+(C/k)lnβh_{\max} = \gamma + (C/k)|\ln\beta| (at p=0p = 0, most regular) and hmin=γh_{\min} = \gamma (at pp \to \infty, most singular).

Corollary 23 (Parameter-free stability constant). Since A=C(1β)lnr|A| = C(1-\beta)\,|\ln r|, the scale ratio cancels in Theorem 10:

W1 ⁣(ηη,δβ)    1+βC(1β)  ε(i),  2C(1β)  ε(ii),W_1\!\left(\frac{\eta}{\|\eta\|},\,\delta_\beta\right) \;\le\; \sqrt{\frac{1+\beta}{C(1-\beta)}}\;\sqrt{\varepsilon} \quad\text{(i)}, \qquad \le\; \sqrt{\frac{2}{C(1-\beta)}}\;\sqrt{\varepsilon} \quad\text{(ii)},

independent of rr and kk (and identical to the native continuous constants of Corollary 19). For fully developed turbulence (β=2/3\beta = 2/3, C=2C = 2, in either the dissipation form k=1k=1 or the velocity form k=3k=3) the constants are 5/21.58\sqrt{5/2} \approx 1.58 and 31.73\sqrt{3} \approx 1.73: a measured violation ε\varepsilon of hierarchical symmetry confines the normalized tilted jump measure within 1.58ε1.58\sqrt{\varepsilon} (resp. 1.73ε1.73\sqrt{\varepsilon}) of δ2/3\delta_{2/3} in Wasserstein-1 distance.

9. Concluding Remarks

The results of this paper show that the hierarchical symmetry A1 carries considerably more force than might be expected from its appearance as a simple linear recurrence. Within i.i.d. multiplicative cascades it is equivalent to the log-Poisson class, with sharp stability constants and the exact propagation rate Θ(ε)\Theta(\sqrt{\varepsilon}); beyond independence it pins all asymptotic statistics (and provably nothing more); and in the continuous category it selects exactly the compound Poisson cascade at the generator level, while no finite moment window of structure functions can do so. The following directions remain open.

  1. Lattice-only finite-state rigidity. Theorem 16 assumes the closed exponent form for all real p0p \ge 0; under lattice-only A1 the identity-theorem step is unavailable, and Carlson-type interpolation is blocked by possible complex eigenvalue crossings of the tilted transfer matrix. We expect the conclusion to persist.

  2. Determination of k, and the joint-in-k test. The hierarchy step kk is treated as given; in applications it must be estimated. A1 at several steps simultaneously imposes the compatibility constraint lnβ(k)k\ln\beta(k) \propto k, and the statistical gain from the joint test is unquantified.

  3. Boundary cases. The log-normal class is the β1\beta \to 1 closure point of the log-Poisson family (b0b \to 0, λb2σ2\lambda b^2 \to \sigma^2): quantifying the degeneration of identifiability as β1\beta \uparrow 1 would unify the classification with its principal rival. The maximal-intermittency limit β0\beta \to 0 likewise deserves analysis.

  4. Statistics of the A1 test. The present results are exact-population statements. A finite-sample theory—error bars on (β^,d^)(\hat\beta, \hat d^\ast), power against log-normal and log-stable alternatives, with the reading-(ii) constants of Theorem 10 and Corollary 19 as the operative null band—is the missing link between the classification and data; the window obstruction of Theorem 17 dictates that such a theory be built on magnitude statistics rather than high-order structure functions.

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