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Statistical model
Statistical model
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A statistical model is a mathematical model that embodies a set of statistical assumptions concerning the generation of sample data (and similar data from a larger population). A statistical model represents, often in considerably idealized form, the data-generating process.[1] When referring specifically to probabilities, the corresponding term is probabilistic model. All statistical hypothesis tests and all statistical estimators are derived via statistical models. More generally, statistical models are part of the foundation of statistical inference. A statistical model is usually specified as a mathematical relationship between one or more random variables and other non-random variables. As such, a statistical model is "a formal representation of a theory" (Herman Adèr quoting Kenneth Bollen).[2]

Introduction

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Informally, a statistical model can be thought of as a statistical assumption (or set of statistical assumptions) with a certain property: that the assumption allows us to calculate the probability of any event. As an example, consider a pair of ordinary six-sided dice. We will study two different statistical assumptions about the dice.

The first statistical assumption is this: for each of the dice, the probability of each face (1, 2, 3, 4, 5, and 6) coming up is 1/6. From that assumption, we can calculate the probability of both dice coming up 5:  1/6 × 1/6 = 1/36.  More generally, we can calculate the probability of any event: e.g. (1 and 2) or (3 and 3) or (5 and 6). The alternative statistical assumption is this: for each of the dice, the probability of the face 5 coming up is 1/8 (because the dice are weighted). From that assumption, we can calculate the probability of both dice coming up 5:  1/8 × 1/8 = 1/64.  We cannot, however, calculate the probability of any other nontrivial event, as the probabilities of the other faces are unknown.

The first statistical assumption constitutes a statistical model: because with the assumption alone, we can calculate the probability of any event. The alternative statistical assumption does not constitute a statistical model: because with the assumption alone, we cannot calculate the probability of every event. In the example above, with the first assumption, calculating the probability of an event is easy. With some other examples, though, the calculation can be difficult, or even impractical (e.g. it might require millions of years of computation). For an assumption to constitute a statistical model, such difficulty is acceptable: doing the calculation does not need to be practicable, just theoretically possible.

Formal definition

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In mathematical terms, a statistical model is a pair (), where is the set of possible observations, i.e. the sample space, and is a set of probability distributions on .[3] The set represents all of the models that are considered possible. This set is typically parameterized: . The set defines the parameters of the model. If a parameterization is such that distinct parameter values give rise to distinct distributions, i.e. (in other words, the mapping is injective), it is said to be identifiable.[3]

In some cases, the model can be more complex.

  • In Bayesian statistics, the model is extended by adding a probability distribution over the parameter space .
  • A statistical model can sometimes distinguish two sets of probability distributions. The first set is the set of models considered for inference. The second set is the set of models that could have generated the data which is much larger than . Such statistical models are key in checking that a given procedure is robust, i.e. that it does not produce catastrophic errors when its assumptions about the data are incorrect.

An example

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Suppose that we have a population of children, with the ages of the children distributed uniformly, in the population. The height of a child will be stochastically related to the age: e.g. when we know that a child is of age 7, this influences the chance of the child being 1.5 meters tall. We could formalize that relationship in a linear regression model, like this: heighti = b0 + b1agei + εi, where b0 is the intercept, b1 is a parameter that age is multiplied by to obtain a prediction of height, εi is the error term, and i identifies the child. This implies that height is predicted by age, with some error.

An admissible model must be consistent with all the data points. Thus, a straight line (heighti = b0 + b1agei) cannot be admissible for a model of the data—unless it exactly fits all the data points, i.e. all the data points lie perfectly on the line. The error term, εi, must be included in the equation, so that the model is consistent with all the data points. To do statistical inference, we would first need to assume some probability distributions for the εi. For instance, we might assume that the εi distributions are i.i.d. Gaussian, with zero mean. In this instance, the model would have 3 parameters: b0, b1, and the variance of the Gaussian distribution. We can formally specify the model in the form () as follows. The sample space, , of our model comprises the set of all possible pairs (age, height). Each possible value of  = (b0, b1, σ2) determines a distribution on ; denote that distribution by . If is the set of all possible values of , then . (The parameterization is identifiable, and this is easy to check.)

In this example, the model is determined by (1) specifying and (2) making some assumptions relevant to . There are two assumptions: that height can be approximated by a linear function of age; that errors in the approximation are distributed as i.i.d. Gaussian. The assumptions are sufficient to specify —as they are required to do.

General remarks

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A statistical model is a special class of mathematical model. What distinguishes a statistical model from other mathematical models is that a statistical model is non-deterministic. Thus, in a statistical model specified via mathematical equations, some of the variables do not have specific values, but instead have probability distributions; i.e. some of the variables are stochastic. In the above example with children's heights, ε is a stochastic variable; without that stochastic variable, the model would be deterministic. Statistical models are often used even when the data-generating process being modeled is deterministic. For instance, coin tossing is, in principle, a deterministic process; yet it is commonly modeled as stochastic (via a Bernoulli process). Choosing an appropriate statistical model to represent a given data-generating process is sometimes extremely difficult, and may require knowledge of both the process and relevant statistical analyses. Relatedly, the statistician Sir David Cox has said, "How [the] translation from subject-matter problem to statistical model is done is often the most critical part of an analysis".[4]

There are three purposes for a statistical model, according to Konishi & Kitagawa:[5]

  1. Predictions
  2. Extraction of information
  3. Description of stochastic structures

Those three purposes are essentially the same as the three purposes indicated by Friendly & Meyer: prediction, estimation, description.[6]

Dimension of a model

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Suppose that we have a statistical model () with . In notation, we write that where k is a positive integer ( denotes the real numbers; other sets can be used, in principle). Here, k is called the dimension of the model. The model is said to be parametric if has finite dimension.[citation needed] As an example, if we assume that data arise from a univariate Gaussian distribution, then we are assuming that

.

In this example, the dimension, k, equals 2. As another example, suppose that the data consists of points (x, y) that we assume are distributed according to a straight line with i.i.d. Gaussian residuals (with zero mean): this leads to the same statistical model as was used in the example with children's heights. The dimension of the statistical model is 3: the intercept of the line, the slope of the line, and the variance of the distribution of the residuals. (Note the set of all possible lines has dimension 2, even though geometrically, a line has dimension 1.)

Although formally is a single parameter that has dimension k, it is sometimes regarded as comprising k separate parameters. For example, with the univariate Gaussian distribution, is formally a single parameter with dimension 2, but it is often regarded as comprising 2 separate parameters—the mean and the standard deviation. A statistical model is nonparametric if the parameter set is infinite dimensional. A statistical model is semiparametric if it has both finite-dimensional and infinite-dimensional parameters. Formally, if k is the dimension of and n is the number of samples, both semiparametric and nonparametric models have as . If as , then the model is semiparametric; otherwise, the model is nonparametric.

Parametric models are by far the most commonly used statistical models. Regarding semiparametric and nonparametric models, Sir David Cox has said, "These typically involve fewer assumptions of structure and distributional form but usually contain strong assumptions about independencies".[7]

Nested models

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Two statistical models are nested if the first model can be transformed into the second model by imposing constraints on the parameters of the first model. As an example, the set of all Gaussian distributions has, nested within it, the set of zero-mean Gaussian distributions: we constrain the mean in the set of all Gaussian distributions to get the zero-mean distributions. As a second example, the quadratic model

y = b0 + b1x + b2x2 + ε,    ε ~ 𝒩(0, σ2)

has, nested within it, the linear model

y = b0 + b1x + ε,    ε ~ 𝒩(0, σ2)

—we constrain the parameter b2 to equal 0.

In both those examples, the first model has a higher dimension than the second model (for the first example, the zero-mean model has dimension 1). Such is often, but not always, the case. As an example where they have the same dimension, the set of positive-mean Gaussian distributions is nested within the set of all Gaussian distributions; they both have dimension 2.

Comparing models

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Comparing statistical models is fundamental for much of statistical inference. Konishi & Kitagawa (2008, p. 75) state: "The majority of the problems in statistical inference can be considered to be problems related to statistical modeling. They are typically formulated as comparisons of several statistical models." Common criteria for comparing models include the following: R2, Bayes factor, Akaike information criterion, and the likelihood-ratio test together with its generalization, the relative likelihood.

Another way of comparing two statistical models is through the notion of deficiency introduced by Lucien Le Cam.[8]

See also

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Notes

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References

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Further reading

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Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
A statistical model is a mathematical framework that formalizes a set of assumptions about the probability distribution generating observed data, typically represented as a family of probability distributions on a sample space. Formally, it specifies a collection of possible distributions Φ\Phi that could have produced a data sample ξ\xi, viewed as a realization of an underlying random vector XiX_i, thereby restricting the infinite possibilities of data-generating processes to a manageable set for analysis. In parameterized forms, the model includes a parameter space Θ\Theta and a mapping P:ΘP(S)P: \Theta \to \mathcal{P}(S) that assigns a distribution PθP_\theta to each parameter value θ\theta, where SS is the sample space. Statistical models serve as essential tools for and across disciplines including sciences, , and social sciences, enabling the quantification of and relationships in . They support key tasks such as parameter estimation to infer unknown values from , hypothesis testing to evaluate assumptions about the underlying process, and to forecast unobserved outcomes based on fitted distributions. Central components include the , which maps experimental units to covariates; the , comprising all possible response outcomes; and the family of distributions, which must satisfy consistency conditions like marginalization over subsets of . Models are categorized primarily into parametric types, which assume a specific distributional form (e.g., normal or Poisson) defined by a finite number of parameters, and nonparametric types, which impose minimal structure on the distribution to allow greater flexibility at the cost of requiring larger samples. Effective use demands careful specification of assumptions—such as or homoscedasticity—which should be verified through diagnostics, alongside criteria to balance fit and complexity, ensuring robust and interpretable results.

Fundamentals

Introduction

A statistical model serves as a mathematical representation of real-world phenomena, incorporating elements of and to describe, predict, or explain observed patterns in . Unlike purely mathematical equations that assume fixed relationships, these models acknowledge variability inherent in natural processes, allowing for probabilistic outcomes rather than deterministic predictions. The primary purpose of a statistical model is to quantify surrounding observations, enabling inferences about broader populations based on limited samples and facilitating testing to evaluate competing explanations. For instance, consider the simple case of rolling two fair six-sided : the probability of both landing on 5 is 136\frac{1}{36}, a basic probabilistic calculation that models chance and variability in random events. This highlights how statistical models formalize such uncertainties to make reliable predictions beyond observed . Statistical models play a crucial role in data analysis across various domains, aiding decision-making under incomplete information. In economics, they forecast market behaviors and assess policy impacts; in biology, they interpret genetic sequences and population dynamics; and in machine learning, they underpin algorithms for pattern recognition and forecasting.

Historical development

The foundations of statistical modeling trace back to the 17th and 18th centuries, when early began addressing variability in data. Jacob Bernoulli's (1713) introduced the , establishing that the average of independent observations converges to the , providing a cornerstone for modeling random processes. Building on this, Abraham de Moivre's 1733 approximation of the to the normal curve offered a practical tool for handling large-scale variability, influencing subsequent probabilistic frameworks. In the , advancements shifted toward systematic estimation techniques. Carl Friedrich Gauss's Theoria Motus Corporum Coelestium (1809) formalized the method of for fitting linear models to observational , minimizing errors under a assumption and enabling precise astronomical predictions. Concurrently, developed precursors to through in works like his 1774 memoir and later expansions in 1781 and 1786, allowing updates to probabilities based on evidence and laying groundwork for modern inferential modeling. The 20th century marked the maturation of parametric and testing frameworks. Ronald Fisher's 1922 paper "On the Mathematical Foundations of Theoretical Statistics" advanced parametric models via , providing a unified approach to parameter inference and . In the 1930s, Jerzy Neyman and Egon Pearson's collaboration, notably their 1933 paper in Philosophical Transactions of the Royal Society, introduced hypothesis testing with Neyman-Pearson lemma, emphasizing power and error control for decision-making under uncertainty. Post-World War II, non-parametric methods emerged to relax distributional assumptions, with Frank Wilcoxon's 1945 rank-sum test exemplifying distribution-free alternatives for comparing groups. Computational advances in the expanded model complexity. From the 1980s, Bayesian networks, pioneered by Pearl's 1985 framework for evidential reasoning, integrated graphical structures with probabilistic inference for handling dependencies in complex systems. The 1990s and 2000s saw deeper integrations with , such as support vector machines (1995) and random forests (2001), blending statistical rigor with algorithmic scalability for high-dimensional data. In the , the rise of catalyzed a key shift from —summarizing past observations—to predictive modeling, leveraging vast datasets and computational power for forecasting, as seen in applications of to clinical and economic predictions.

Definition and Framework

Formal definition

A statistical model is formally defined as a pair (S,P)(S, \mathcal{P}), where SS is the consisting of all possible outcomes or observations from an experiment, and P\mathcal{P} is a family of probability measures defined on SS. This structure provides a mathematical framework for describing the in data generation processes. More precisely, the sample space SS is equipped with a σ\sigma-algebra F\mathcal{F} of measurable events, forming a measurable space (S,F)(S, \mathcal{F}), on which the probability measures in P\mathcal{P} are defined; these measures assign probabilities to subsets of events in F\mathcal{F}. In the parametric case, the family takes the form P={PθθΘ}\mathcal{P} = \{P_\theta \mid \theta \in \Theta \}, where ΘRk\Theta \subset \mathbb{R}^k is the parameter space indexing the distributions, and each PθP_\theta is a probability measure on (S,F)(S, \mathcal{F}). For the model to allow unique inference about parameters, it must satisfy the identifiability condition: if θθΘ\theta \neq \theta' \in \Theta, then PθPθP_\theta \neq P_{\theta'}. Unlike a fixed probability model, which specifies a single , a statistical model defines a class of distributions P\mathcal{P} from which the true generating mechanism is selected to fit observed data, enabling flexibility in . The , central to estimation within the model, is given in general form by the probability (or density) of the observed data under a specific value: L(θx)=P(X=xθ),L(\theta \mid x) = P(X = x \mid \theta), where xSx \in S is the observed realization and P(θ)P(\cdot \mid \theta) denotes the measure PθP_\theta.

Components and assumptions

A statistical model typically comprises several core components that formalize the probabilistic structure of the observed data. The primary elements include random variables representing the observations. In models that describe relationships between variables, such as regression models, these are often divided into response variables (often denoted as YY, the outcome) and covariates (denoted as XX, the predictors). Parameters, denoted collectively as θ\theta, quantify the model's characteristics and are treated as fixed unknowns in frequentist approaches or as random variables with prior distributions in Bayesian frameworks. In certain models with additive structure, error terms, often symbolized as ϵ\epsilon, capture unexplained variation or noise, assuming they arise from an underlying probability distribution. Central to the model's inferential framework are key assumptions that ensure the validity of statistical procedures. Observations are commonly assumed to be independent and identically distributed (i.i.d.), meaning each point is drawn from the same without influence from others. In many parametric models, such as , errors are further assumed to follow a with mean zero and constant variance (homoscedasticity), alongside or additivity in the relationship between predictors and the response. These assumptions underpin the model's ability to generalize from sample to inferences. The plays a pivotal role in linking these components to for parameter estimation and hypothesis testing. For i.i.d. observations x1,,xnx_1, \dots, x_n from a distribution parameterized by θ\theta, it is defined as L(θx)=i=1nP(xiθ),L(\theta \mid x) = \prod_{i=1}^n P(x_i \mid \theta), where P(xiθ)P(x_i \mid \theta) is the probability mass or function for each observation. This function quantifies the probability of the observed given the parameters, serving as the foundation for and other inferential methods. Violations of these assumptions can lead to serious inferential issues. For instance, dependence among observations or non-identical distributions may introduce in estimates, while heteroscedasticity—unequal error variances—results in inefficient estimators and invalid standard errors, potentially leading to incorrect hypothesis tests and confidence intervals. Such failures undermine the model's reliability, emphasizing the need for robust checks. To verify these assumptions, residual analysis is employed, where residuals (differences between observed and predicted values) are examined via plots such as residuals versus fitted values or normal probability plots. Deviations from randomness, such as patterns indicating non-linearity or heteroscedasticity, signal potential violations, guiding model refinement without delving into specific corrective techniques.

Examples and Illustrations

Basic examples

One of the simplest statistical models is the Bernoulli model, which describes outcomes of a single trial with two possible results, such as a coin flip where success (X=1) occurs with probability p and failure (X=0) with probability 1-p. The is given by: P(X=x)={pif x=11pif x=0P(X = x) = \begin{cases} p & \text{if } x = 1 \\ 1 - p & \text{if } x = 0 \end{cases} The Poisson model is used for counting the number of rare events occurring in a fixed interval, such as arrivals per hour, where the rate is λ. The is: P(X=k)=λkeλk!,k=0,1,2,P(X = k) = \frac{\lambda^k e^{-\lambda}}{k!}, \quad k = 0, 1, 2, \dots For continuous data, the normal distribution model assumes observations follow a Gaussian distribution, often applied to hypothetical height measurements with mean μ and variance σ². The is: f(x)=1σ2πexp((xμ)22σ2)f(x) = \frac{1}{\sigma \sqrt{2\pi}} \exp\left( -\frac{(x - \mu)^2}{2\sigma^2} \right)
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