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Fisher Threshold Theorem Overview

Updated 8 October 2025
  • Fisher Threshold Theorem is a framework identifying critical parameters where qualitative transitions occur in diverse systems such as probability, physics, and genetics.
  • It quantifies thresholds in limit theorems via Fisher information decay, spectral gap analysis, and cumulant vanishings in i.i.d. sum models.
  • The theorem also delineates error thresholds in population genetics, phase transitions in statistical physics, and optimal bounds in combinatorial designs and signal detection.

The Fisher Threshold Theorem encapsulates a collection of threshold phenomena in probability, statistical physics, combinatorics, information theory, and population genetics, each emerging from the interplay between Fisher’s metrics (e.g., Fisher information, partition function zeros, genetic variance, combinatorial intersection bounds) and structural or dynamical constraints on the underlying systems. The term is used to denote the existence of critical parameters or rates at which qualitative changes occur in convergence, phase transitions, population stability, combinatorial design bounds, or signal detection. Across mathematical biology, probability theory, combinatorics, and quantum/statistical physics, this threshold governs transitions in system behavior, criticality, and optimality.

1. Fisher Thresholds in Probability and Information Theory

Central to statistical limit theorems, the Fisher Threshold Theorem characterizes how Fisher information decays in sum sequences of independent (or nonlinear) random variables. Let X1,,XnX_1,\dots,X_n be i.i.d. with mean zero and variance σ2\sigma^2, and let Zn=(X1++Xn)/nZ_n = (X_1+\cdots+X_n)/\sqrt{n}. The relative Fisher information is

I(ZnN)=I(Zn)I(N),I(Z_n\|\mathcal{N}) = I(Z_n) - I(\mathcal{N}),

where N\mathcal{N} denotes the normal law. Via Edgeworth-type expansions, it is established that

I(ZnN)=c1n+c2n2++o(n(s2)/2(logn)(s3)/2),I(Z_n\|\mathcal{N}) = \frac{c_1}{n} + \frac{c_2}{n^2} + \cdots + o\left(n^{-(s-2)/2}(\log n)^{(s-3)/2}\right),

with cjc_j determined by the cumulants of X1X_1 beyond order two (Bobkov et al., 2012). If all lower cumulants vanish, the leading coefficients are zero until the first nonzero cjc_j (“Fisher threshold” phenomenon).

Further, via spectral analysis of the convolution operator and maximal correlation (Hirschfeld-Gebelein-Rényi), the standardized Fisher information Jst(Zn)J_{st}(Z_n) obeys

Jst(Zn)Jst(X1)1+ε(2)(n1),J_{st}(Z_n) \leq \frac{J_{st}(X_1)}{1+\varepsilon(2)(n-1)},

where the spectral gap ε(2)\varepsilon(2) linked to the second-largest eigenvalue controls the O(1/n)O(1/n) convergence rate and monotonicity (Johnson, 2019). This establishes a quantitative threshold for Gaussianization in information-theoretic CLTs.

Recent work extends decomposition techniques (martingale or approximation by independent components) to nonlinear statistics FF, yielding new bounds:

I(FN)2E[(1OFOF)2]+2E[(OF,FOF)2],I(F\|\mathcal{N}) \leq 2\,\mathbb{E}\left[\left(\frac{1-O_F}{O_F}\right)^2\right] + 2\,\mathbb{E}\left[\left(\frac{O_{F,F}}{O_F}\right)^2\right],

providing explicit O(1/n)O(1/n) rates for quadratic forms and functions of sample means, generalizing the Fisher threshold to broader settings (Dung, 2022).

Setting Threshold Parameter Rate/Transition
i.i.d. sums CLT moment-based cumulant vanishings faster than $1/n$
Maximal correlation spectral gap 2nd-largest eigenvalue ε(2)\varepsilon(2) O(1/n)O(1/n) bound
Nonlinear statistics deviation of score from linearity info-threshold

2. Fisher Zeros and Thresholds in Statistical Physics

In the theory of phase transitions, the Fisher Threshold Theorem refers to the locus of Fisher zeros—roots of the partition function in a complexified temperature (or coupling) parameter—approaching the real axis, thereby revealing thermodynamic or quantum critical points (Liu et al., 27 Jun 2024, Liu et al., 2018). For the one-dimensional transverse field Ising model (1DTFIM), the partition function

Z(β,g)=12[k=1L2cosh(βϵ2k)+sign(gcg)k=1L2sinh(βϵ2k)+]Z(\beta, g) = \frac{1}{2}\left[\prod_{k=1}^L 2\cosh(\beta \epsilon_{2k}) + \text{sign}(g_c - g)\prod_{k=1}^L 2\sinh(\beta \epsilon_{2k}) + \ldots\right]

has zeros (Fisher zeros) which, for large LL, form open or closed lines in the complex β\beta plane. The topology of these lines changes at the quantum critical point g=gcg = g_c:

  • For g<1g < 1: open lines associated with ferromagnetic domain walls
  • At g=gcg = g_c: open lines vanish, closed loops persist (disordered phase)
  • Fishers zeros serve as dynamical (quantum) or thermodynamic phase transition indicators

Algorithmic studies of the Ising model on graphs of bounded degree reveal that, in the correlation decay (uniqueness) region for β\beta, the partition function is analytic, and Fisher zeros are absent in a complex neighborhood (Liu et al., 2018). This absence signals no phase transition and enables efficient deterministic approximations.

Model/Class Fisher Threshold Physical Transition
1DTFIM and spin models Topology of Fisher zeros quantum/thermal criticality
General Ising graphs Absence of zeros in region analyticity, no transition

3. Thresholds in Population Genetics

In evolutionary dynamics, the Fisher Threshold Theorem denotes the conditions under which genetic information (e.g., high-fitness “master sequences”) is maintained in the face of stochastic effects (mutation, drift). In the finite population Wright-Fisher model (Cerf, 2012), the critical threshold is expressed as

αψ(a)=lnκ\alpha\,\psi(a) = \ln \kappa

where α=m/\alpha = m/\ell (scaled population size), ψ(a)\psi(a) (cost function via Freidlin-Wentzell large deviations), and κ\kappa (alphabet size) demarcate regimes:

  • αψ(a)<lnκ\alpha\,\psi(a) < \ln\kappa: error catastrophe, random population
  • αψ(a)>lnκ\alpha\,\psi(a) > \ln\kappa: stability, quasispecies formation

In classical infinite-population quasispecies (Eigen model), the error threshold appears as σea=1\sigma e^{-a} = 1. These results rigorously connect deterministic threshold phenomena to stochastic finite-population effects through large deviation theory.

4. Fisher Thresholds in Combinatorics and Design Theory

The combinatorial Fisher Threshold Theorem generalizes Fisher’s inequality to set systems and its q-analogues (Dey, 21 May 2025, Das et al., 2014). For sets (or subspaces) with prescribed intersection properties:

  • Classical: any family F\mathcal{F} on [n][n] with F|\mathcal{F}| subsets such that AB=k|A \cap B| = k for any ABA \neq B in F\mathcal{F} satisfies Fn|\mathcal{F}| \leq n
  • qq-analogue: for F\mathcal{F} a family of subspaces of Fqn\mathbb{F}_q^n with dim(AB)=kdim(A \cap B) = k, F[n]q|\mathcal{F}| \leq [n]_q

Relaxing intersection conditions (allowing up to kk exceptions per set) increases the maximum attainable family size:

  • For kk-almost λ\lambda-Fisher families, bounds interpolate between nn and $2n-2$ with the “Hadamard construction” optimal when λ=n/4\lambda = n/4 (Das et al., 2014)
Setting Threshold Parameter(s) Max Family Size Bound
Sets, AB=k|A\cap B|=k nn Fn|\mathcal{F}|\leq n
qq-analogues qq, nn F[n]q|\mathcal{F}| \leq [n]_q
kk-almost Fisher families k,n,λk, n, \lambda Linear in kk, tight @ Hadamard

5. Thresholds in Signal Detection and Meta-Analysis

Statistical thresholding appears in the optimal design of pp-value combination methods. The TFisher framework generalizes Fisher’s method by truncating and weighting pp-values (Zhang et al., 2018).

  • For sparse signals, hard or soft thresholding (e.g., inclusion of only pp-values below a data-adaptive cutoff τ\tau) is optimal
  • The Bahadur Efficiency (BE) and Asymptotic Power Efficiency (APE) metrics reveal that soft-thresholding (τ1=τ2\tau_1 = \tau_2) often achieves maximal power
  • Adaptive thresholding, as in the omnibus oTFisher test, achieves near-optimal detection even without prior signal proportion knowledge
Approach Threshold Mechanism Signal Detection Context
Fisher combination none (all pp-values) dense signal, less selective
TFisher soft/hard adaptive cutoff τ\tau sparse signal, optimal power
oTFisher (omnibus) grid of thresholds robust across regimes

6. Thresholds in Evolution and Dynamical Systems

The original Fisher’s Fundamental Theorem (as interpreted in (Frank, 2011)) partitions evolutionary change in mean fitness as

ΔW=ΔWNS+ΔWE,\Delta W = \Delta W_{NS} + \Delta W_E,

where ΔWNS\Delta W_{NS} (due to natural selection) equals the genetic variance in fitness, and ΔWE\Delta W_E captures environmental deterioration. The “Fisher threshold” corresponds to the dynamic equilibrium where improvement via selection is counterbalanced by environmental or competitive effects, leading to near-constancy of mean population fitness over time.

This invariance law is juxtaposed with Wright’s dynamical models, revealing a conceptual threshold between universal conservation principles and context-dependent evolutionary trajectories.

7. Thresholds Characterizing Criticality and Phase Transitions

Across disciplines, the Fisher threshold serves as a diagnostic or bifurcation point, signifying transitions in system behavior:

  • Convergence to Gaussianity (probability/information theory)
  • Emergence or disappearance of genetic information (population biology)
  • Existence or absence of phase transitions (quantum/statistical physics)
  • Maximal configuration numbers under combinatorial constraints (design theory)
  • Statistical power optimality under signal sparsity (meta-analysis)

These threshold phenomena are unified by the role of Fisher’s conceptual or quantitative metrics in structuring the space of possible behaviors, often expressed as sharp inequalities, spectral parameters, or topological transitions in zeros or maxima.


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