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Discrete Lomax Distribution

Updated 20 January 2026
  • The discrete Lomax distribution is a two-parameter discrete model defined by closed-form pmf, cdf, survival, and hazard functions, capturing overdispersed count data with heavy right tails.
  • It effectively models phenomena with extra-Poisson variability, such as accident counts or industrial strike data, thanks to its flexibility in handling a mass at zero and extreme events.
  • Parameter estimation is carried out through frequency methods and maximum likelihood, with goodness-of-fit assessed via chi-square and discrete KS tests for reliable inference.

The discrete Lomax distribution is a two-parameter discrete probability model that arises as the “zero-vertex” (μ=0\mu=0) specialization of the discrete generalized Pareto distribution. Its pmf, cumulative, survival, quantile, and hazard functions all admit closed-form expressions. The distribution is suitable for overdispersed count data typically featuring a substantial mass at zero and heavy right tails. Its flexibility and tractability make it effective in modeling phenomena such as the annual number of deaths at road-accident blackspots and count data exhibiting extra-Poisson variability (Prieto et al., 2013, &&&1&&&).

1. Definition and Fundamental Properties

The discrete Lomax distribution, denoted DL(α,λ)\operatorname{DL}(\alpha, \lambda), is defined for x=0,1,2,x=0,1,2,\dotsc by its cumulative distribution function (cdf): F(x)=Pr[Xx]=1[1+λ(x+1)]α,α>0,λ>0F(x) = \Pr[X \leq x] = 1 - [1+\lambda(x+1)]^{-\alpha}, \quad \alpha>0,\, \lambda>0 Here α\alpha is a shape parameter and λ\lambda a scale parameter. The pmf follows as the difference: p(x)=F(x)F(x1)=[1+λx]α[1+λ(x+1)]αp(x) = F(x)-F(x-1) = [1+\lambda x]^{-\alpha} - [1+\lambda(x+1)]^{-\alpha} The survival function (tail probability) is

S(x)=Pr[Xx]=[1+λx]αS(x) = \Pr[X \geq x] = [1+\lambda x]^{-\alpha}

These closed-form expressions imply computational tractability for evaluation and sampling via inversion.

The discrete Lomax arises as the a=1a=1 special case of the more general discrete gamma-Lomax distribution (DGLD). For c>0c>0 and θ>0\theta>0, the DGLD has pmf

g1(x)=(1+x/θ)1/c(1+(x+1)/θ)1/cg_1(x) = (1 + x/\theta)^{-1/c} - (1 + (x+1)/\theta)^{-1/c}

which matches the Lomax form under the identification c=1/αc = 1/\alpha, θ=1/λ\theta = 1/\lambda (Ghosh et al., 2018).

2. Moments and Tail Behavior

The rrth moment of the discrete Lomax exists for α>r\alpha > r and is expressible via a tail sum: E[Xr]=x=1[xr(x1)r][1+λx]α\mathbb{E}[X^r] = \sum_{x=1}^{\infty} \left[ x^r - (x-1)^r \right][1+\lambda x]^{-\alpha} The mean exists for α>1\alpha > 1, and the variance for α>2\alpha > 2. Closed-form solution is not available, but the convergent sum is practical for numerical computation.

The distribution possesses heavy right tails. As xx \to \infty, p(x)xα1p(x) \sim x^{-\alpha - 1}. This tail behavior enables the model to capture extreme count events.

Overdispersion is inherent: Var(X)>E[X]\operatorname{Var}(X) > \mathbb{E}[X] for a broad parameter range. This makes the discrete Lomax suitable for data where classical Poisson models severely understate the empirical variance (Prieto et al., 2013, Ghosh et al., 2018).

3. Quantile and Hazard Functions

The quantile function (inverse cdf) for level γ(0,1)\gamma \in (0,1) is given by

xγ=(1γ)1/α1λ1x_\gamma = \left\lceil \frac{(1-\gamma)^{-1/\alpha} - 1}{\lambda} - 1 \right\rceil

This operation facilitates efficient random variate generation via inversion.

The discrete hazard function is

r(x)=p(x)S(x)=1(1+λx1+λ(x+1))αr(x) = \frac{p(x)}{S(x)} = 1 - \left( \frac{1+\lambda x}{1+\lambda(x+1)} \right)^{\alpha}

This function is strictly decreasing in xx, reflecting a decreasing-failure-rate (DFR): the risk of observing an exact count xx declines as xx increases (Prieto et al., 2013, Ghosh et al., 2018).

4. Parameter Estimation

Two inference approaches are common: the (μ,μ+1)(\mu, \mu+1)-frequency method and maximum likelihood estimation (MLE).

Frequency method: For sample proportions p^0\hat p_0 (zero count) and p^1\hat p_1 (one count), equations

p^0=1[1+λ]α,p^1=[1+λ]α[1+2λ]α\hat p_0 = 1 - [1+\lambda]^{-\alpha},\qquad \hat p_1 = [1+\lambda]^{-\alpha} - [1+2\lambda]^{-\alpha}

are solved by first eliminating α\alpha: log(1+2λ)log(1+λ)=p^0+p^11p^01\frac{\log(1+2\lambda)}{\log(1+\lambda)} = \frac{\hat p_0 + \hat p_1 - 1}{\hat p_0 - 1} Numerical root finding for λ\lambda yields λ^\hat \lambda, and then

α^=log(1p^0)/log(1+λ^)\hat \alpha = -\log(1-\hat p_0) / \log(1+\hat \lambda)

The resulting estimates supply initial values for MLE.

Maximum likelihood estimation: For data x1,,xnx_1,\ldots,x_n, the log-likelihood is

(α,λ)=i=1nlog([1+λxi]α[1+λ(xi+1)]α)\ell(\alpha, \lambda) = \sum_{i=1}^n \log\left( [1+\lambda x_i]^{-\alpha} - [1+\lambda(x_i+1)]^{-\alpha} \right)

Parameter optimization requires numerical maximization, typically initialized at the frequency-based estimates. The asymptotic normality of MLEs enables standard error computation via the observed information matrix (Prieto et al., 2013, Ghosh et al., 2018).

5. Model Assessment and Goodness-of-Fit

Goodness-of-fit is conventionally assessed by Chi-square or Kolmogorov–Smirnov (KS) tests adapted for discrete data.

  • Chi-square test: Data are binned with expected counts Ei5E_i \geq 5, and the statistic

χ2=i=1k(OiEi)2Ei\chi^2 = \sum_{i=1}^k \frac{(O_i - E_i)^2}{E_i}

is compared to the χ2\chi^2 quantile with k21k-2-1 degrees of freedom under the null model fit.

  • Discrete KS test by parametric bootstrap: The empirical cdf Fn(k)F_n(k) is compared to the fitted model cdf F(k;α^,λ^)F(k; \hat \alpha, \hat \lambda): Kn=nmax0kmaxxiFn(k)F(k;α^,λ^)K_n = \sqrt{n} \max_{0 \leq k \leq \max x_i} | F_n(k) - F(k; \hat \alpha, \hat \lambda) | A large number of synthetic samples are generated, re-fitted, and used to compute a bootstrap p-value as the proportion of simulated KnK_n^\ast exceeding the observed KnK_n. Rejection occurs for p<0.05p < 0.05 (Prieto et al., 2013).

6. Applications and Empirical Studies

Prieto et al. (2014) modeled annual counts of deaths on Spanish road accident blackspots (2003–2007) using the discrete Lomax. Maximum likelihood estimates and standard errors for each year are summarized as follows:

Year α^\hat \alpha (s.e.) λ^\hat \lambda (s.e.)
2003 6.55 (2.07) 0.314 (0.118)
2004 13.86 (9.90) 0.129 (0.100)
2005 5.49 (1.68) 0.381 (0.144)
2006 4.34 (1.16) 0.536 (0.186)
2007 10.83 (5.88) 0.204 (0.125)

Goodness-of-fit tests (both chi-square and KS with bootstrap) yielded p-values above the $0.05$ significance level in all years (e.g., 2003: χ2=3.64\chi^2=3.64 with df=1df=1, p=0.056p=0.056; KS =0.136=0.136, bootstrap p=0.261p=0.261), indicating the discrete Lomax model was not rejected at conventional levels (Prieto et al., 2013).

Additionally, the discrete Lomax arises as a special case (a=1a=1) of the discrete gamma-Lomax, which has been fitted to blockades and strike counts in UK industrial data, demonstrating its capacity to model overdispersed, heavy-tailed count processes (Ghosh et al., 2018).

The discrete Lomax is embedded within the general class of discrete generalized Pareto distributions (DGP), parameterized by location μ\mu, shape, and scale. Setting μ=0\mu = 0 yields the Lomax as a two-parameter reduction. It is also a limiting form of the discrete gamma-Lomax for a=1a=1, characterized via Poisson–Gamma mixtures discretized by the cdf-difference scheme.

A notable property is unification of heavy-tailed count models with closed-form expressions for likelihoods and moments. The decreasing failure rate property for a1a \leq 1 (and thus for the discrete Lomax) distinguishes it from other popular models such as the Poisson and negative binomial, especially in settings with many zeros and high dispersion (Ghosh et al., 2018).

The discrete Lomax and its generalizations are readily implemented in likelihood-based inferential frameworks using standard statistical software, and offer interpretable parameters controlling both dispersion and tail heaviness.

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