The Nearly Neutral Theory
Why do small, isolated populations of island lizards accumulate more slightly harmful mutations than their mainland relatives? Why does the ratio of protein-changing to silent DNA substitutions differ systematically between humans and Drosophila? These two lineages are separated by hundreds of millions of years. They also differ vastly in population size. Motoo Kimura's original neutral theory answered questions about molecular evolution. It did so by dividing mutations into two bins. Strictly neutral mutations drift freely. Strongly deleterious mutations are deleted by selection. Real genomes are messier. Most new mutations that matter for evolution are neither perfectly neutral nor obviously harmful. Instead, they are mildly deleterious. They teeter on a knife-edge. Their fate depends on a numerical tug-of-war between selection and chance. Tomoko Ohta's nearly neutral theory, developed from 1973 onward, fills this gap. It proposes something specific about mutations with a small negative selection coefficient. Their evolutionary fate is not fixed by that coefficient alone. Instead, it depends on the product of the coefficient and the effective population size. This quantity is written Nes. This single insight is that selection's power scales with population size. It turned population size from a background parameter into an active character in molecular evolution. It explains patterns that pure neutral theory could not touch. The theory matters for an important reason. It reconciles two things that once seemed at odds. One is the approximate molecular-clock-like regularity of sequence evolution. The other is the many well-documented exceptions to that clock. In these exceptions, the clock runs at different rates in different lineages. The theory also supplies a mechanistic account for the "species barrier" of Ne. It explains why small populations tend to carry more deleterious genetic load. This includes island endemics, obligate asexuals, organelle genomes, and endangered species. Such populations also evolve faster at nonsynonymous sites. They are more vulnerable to mutational meltdown. This article builds the concept from the mechanics of drift versus selection. It walks through Ohta's founding logic and the comparative genomic evidence that supports it. It works two quantitative examples. One is a bacterial population genetics calculation. The other is a mammalian genome comparison. Finally, it turns to how the theory is used today. This includes detecting selection, forecasting extinction risk, and interpreting human disease-mutation load.
- Nearly neutral theory extends Kimura's neutral theory: mutations with small selective effects behave neutrally or deleteriously depending on Ne·s, not on s alone.
- When |Nes| ≪ 1, drift dominates and the mutation behaves as if neutral; when |Nes| ≫ 1, selection dominates and removes it (for deleterious s).
- Smaller effective population size (Ne) widens the "nearly neutral zone," letting more mildly deleterious mutations fix by drift — a genomic signature called the drift-barrier or nearly-neutral effect.
- This predicts systematic, testable differences: slow-Ne lineages (large body size, small population, low recombination, asexuality, organelles) show elevated dN/dS and more slightly deleterious substitutions.
- Comparative genomic surveys (mammals vs. invertebrates, vertebrate mitochondria vs. nuclear DNA, self-fertilizing vs. outcrossing plants) confirm the predicted Ne–dN/dS relationship.
- The theory underlies modern tools for Detecting Selection in Sequences and explains genetic load, mutational meltdown risk, and the "nearly neutral" component of human disease variants.
The fate of a mildly deleterious mutation — fixed by chance or purged by selection — depends on the product Nes, so population size itself governs whether natural selection can "see" small fitness effects.
The core idea
Every new mutation carries a selection coefficient, s, describing its proportional effect on fitness relative to the existing allele (s > 0 beneficial, s < 0 deleterious, s = 0 neutral — concepts introduced under The Selection Coefficient). Kimura's classical neutral theory treated most molecular variation as falling into one of two extremes: true neutrality (s = 0) or strong, clearly visible deleterious effects removed almost immediately by purifying selection. Ohta pointed out that the overwhelming majority of new mutations affecting protein structure or gene regulation likely have s values that are small in absolute magnitude — neither exactly zero nor large enough to be reliably purged. These are the "nearly neutral" mutations. Whether such a mutation behaves, in practice, like a neutral variant or like a deleterious one is not determined by s in isolation. It is determined by how large s is relative to the strength of genetic drift, and drift's strength scales inversely with Effective Population Size, Ne. The relevant compound parameter is Nes (sometimes written 4Nes or 2Nes depending on convention for diploid/haploid organisms and dominance). When the absolute value of Nes is much less than 1, selection is too weak to reliably overcome the random sampling noise of drift, and the mutation's fixation probability approaches that of a strictly neutral allele — roughly 1/(2N) for a new mutation in a diploid population. When |Nes| is much greater than 1, selection efficiently governs the mutation's fate: beneficial variants sweep, deleterious variants are purged, largely independent of chance. This produces a continuum rather than a dichotomy. A mutation with s = −0.0001 is effectively neutral in a population of Ne = 1,000 (Nes = −0.1, drift wins) but strongly deleterious and reliably eliminated in a population of Ne = 10,000,000 (Nes = −1,000, selection wins). The same mutation, same molecule, same biochemical effect — but a completely different evolutionary outcome, purely because the population size differs. This is the theory's central and somewhat counterintuitive lesson: the strength of selection acting on a given mutation is not a fixed biochemical property; it is a joint property of the mutation and the population it occurs in.
Mechanism — how drift and selection trade off
Step 1: Selection coefficients form a continuous spectrum, not two classes. New mutations arising in coding and regulatory DNA produce a distribution of fitness effects (the DFE). Empirical DFEs, estimated from site-frequency spectra and mutation-accumulation experiments, are typically unimodal and skewed, with a mode near zero and a long tail of increasingly deleterious effects; strongly beneficial mutations are rare. Ohta's insight was to focus attention on the large mass of mutations with |s| in the range of roughly 10⁻⁶ to 10⁻². These are mutations too weak to be treated as strongly counterselected under simple purifying-selection models, yet not so weak as to be dismissed as biochemically inert.
Step 2: Fixation probability depends on Nes through diffusion theory. Using diffusion approximations to the Wright-Fisher model (the same machinery underlying classical population genetics), the fixation probability of a new mutation with selection coefficient s in a diploid population of effective size Ne is:
for a semi-dominant (additive) mutation, where 2Nes is the compound parameter that actually enters the formula. Two limits fall out cleanly:
- If Nes ≈ 0 (either s is tiny or Ne is small), Pfix ≈ 1/(2N) — identical to the neutral fixation probability. Chance dominates.
- If Nes is large and negative (deleterious, and either s is not-so-small or Ne is large), Pfix shrinks exponentially toward zero. Selection dominates.
The transition between these regimes is not a hard threshold; it is smooth, governed by the magnitude of Nes. Population geneticists commonly use |Nes| ≈ 1 as an informal boundary of the "nearly neutral zone" — not a discontinuity, but the region where drift and selection contribute comparably to the outcome.
Step 3: Effective population size is the lever, and it varies enormously across genomes and lineages. Ne is not the census population size; it reflects breeding structure, variance in reproductive success, historical bottlenecks, linked selection, and mode of inheritance. Mitochondrial and chloroplast genomes, inherited uniparentally and without recombination, have roughly a quarter of the Ne of nuclear autosomes. Self-fertilizing plants and asexual lineages have reduced effective recombination and thus reduced effective Ne due to processes like background selection and Hill-Robertson interference. Large-bodied, long-lived, low-fecundity species (whales, elephants, raptors) tend to have small long-term Ne; small-bodied, high-fecundity species (many insects, marine invertebrates, bacteria) tend to have enormous Ne. Because Nes is the product of Ne and s, any factor that shrinks Ne effectively shifts more of the mutational spectrum into the nearly-neutral zone — even without any change in the mutations' underlying biochemistry.
Step 4: The consequence is a testable, quantitative prediction for nonsynonymous substitution rates. Silent (synonymous) substitutions are, to a good approximation, unaffected by this logic — they alter mRNA sequence but not (mostly) protein sequence, so their fixation rate approximately equals the neutral mutation rate regardless of Ne (this is the baseline established for The Neutral Substitution Rate). Nonsynonymous (protein-changing) substitutions, by contrast, are precisely the class enriched for mildly deleterious effects. The nearly neutral theory therefore predicts:
because small-Ne lineages fix a larger fraction of the mildly deleterious nonsynonymous mutations that arise, while large-Ne lineages purge them more efficiently. This single prediction — an inverse relationship between Ne and dN/dS — has become one of the most tested and most consistently supported predictions in molecular evolution.
Step 5: Linked selection can shrink local Ne along the genome. A further mechanism widens or narrows the nearly neutral zone locally within a single genome. Regions of low recombination experience stronger Hill-Robertson interference and background selection, both of which reduce the local effective population size experienced by a linked neutral or nearly neutral site. This produces heterogeneity in dN/dS and diversity across the genome even within one species — low-recombination regions (near centromeres, on non-recombining sex chromosomes, in asexual genomes) behave, locally, like populations with smaller Ne, accumulating more slightly deleterious substitutions than freely-recombining regions of the same genome.
The evidence
Ohta's founding argument (1973): rate constancy that didn't fit strict neutrality. Kimura and Jack Lewontin King, and independently King and Jukes, had shown that many proteins evolve at roughly clock-like rates across lineages, consistent with a neutral substitution rate approximating the mutation rate. But an anomaly troubled the strict neutral model: generation-time effects. If most amino-acid substitutions were strictly neutral, the substitution rate per year should scale with the mutation rate per generation divided by generation time — organisms with short generations (mice) should accumulate mutations, and thus substitutions, much faster per calendar year than long-generation organisms (humans, elephants). Yet comparative protein and DNA sequence data (hemoglobin, cytochrome c, and later genome-wide comparisons) showed the generation-time effect was much weaker than expected under strict neutrality, and was markedly weaker for nonsynonymous than for synonymous substitutions. Ohta (1973, Nature) proposed that this discrepancy arises because nonsynonymous substitutions are disproportionately composed of slightly deleterious mutations whose fixation is governed by Ne, not simply by the mutation rate — and Ne tends to be inversely related to generation time and body size across mammals, partially canceling the generation-time effect on the mutation-input side. This was not a hand-wave; it was a quantitative resolution of a specific, previously unexplained empirical pattern in the comparative sequence data available at the time.
The dN/dS–Ne comparative test (multiple independent studies, 1990s–2010s). The theory's sharpest quantitative prediction — that dN/dS should rise as Ne falls — has now been tested across an enormous range of taxa using genome-scale sequence comparison:
- Mammals versus other vertebrates and invertebrates. Large-scale genomic comparisons (e.g., analyses led by groups including Adam Eyre-Walker, Peter Keightley, and later large consortium genome papers) consistently find that large-bodied mammals with small long-term Ne (humans, great apes, cetaceans) show elevated dN/dS relative to small-bodied, large-Ne taxa such as mice, and especially relative to invertebrates like Drosophila, whose dN/dS is markedly lower.
- Mitochondrial versus nuclear genomes. Because mtDNA is haploid, uniparentally inherited, and non-recombining, its effective population size is roughly one-quarter that of an autosomal nuclear locus in the same organism (ignoring differences in mutation rate). Consistent with the theory, animal mitochondrial genomes typically show higher dN/dS than nuclear genes in the same lineage, and accumulate mildly deleterious variants that would be purged if they occurred in the higher-Ne nuclear genome.
- Self-fertilizing versus outcrossing plants. Selfing dramatically reduces effective recombination and effective population size (through increased linkage and stronger genetic drift within predominantly homozygous lineages). Comparative genomic studies of selfing plant species (e.g., Arabidopsis thaliana versus its outcrossing relative Arabidopsis lyrata, and Capsella rubella versus outcrossing Capsella grandiflora) find higher dN/dS and elevated proportions of derived deleterious alleles in the selfers, exactly as predicted.
- Island versus mainland and endangered-species genomics. Conservation genomic surveys of small, isolated, or bottlenecked populations (Channel Island foxes, Isle Royale wolves, Iberian lynx) repeatedly find elevated ratios of nonsynonymous to synonymous heterozygosity and higher relative mutational load, tracking historical reductions in Ne.
Falsifiable structure of the test. Crucially, the theory makes a directional, quantitative prediction (dN/dS should track 1/Ne), not merely "some mutations are nearly neutral." Studies estimate Ne independently — typically from silent-site nucleotide diversity θ = 4Neμ, using the neutral substitution/diversity framework — and then test whether dN/dS correlates with this independent Ne estimate across many species. The consistent negative correlation between independently estimated Ne and dN/dS, replicated across mammals, plants, and invertebrates by multiple independent research groups using different genomic datasets, constitutes the primary empirical support for the nearly neutral theory. This is comparative correlational evidence rather than a single controlled experiment (population genetics rarely allows Meselson–Stahl–style direct manipulation at this scale), but the convergence of independent lines — generation-time anomalies, mitochondrial/nuclear contrasts, selfer/outcrosser contrasts, and conservation genomic case studies — gives the theory unusually broad empirical backing for a population-genetic model.
Direct experimental support: mutation accumulation lines. A complementary experimental line of evidence comes from mutation-accumulation (MA) experiments, in which laboratory populations are deliberately bottlenecked to Ne of 1–10 individuals per generation for many generations (classically in Drosophila, Caenorhabditis elegans, and Saccharomyces cerevisiae, pioneered by researchers including Michael Lynch). Under such extreme drift, selection coefficients that would normally be purged in wild-sized populations become invisible to selection, and MA lines show measurable, cumulative declines in fitness — a direct experimental demonstration that shrinking Ne allows mildly deleterious mutations to fix, exactly as Nes theory predicts. Lynch's extensive MA work, alongside genomic surveys, explicitly frames genome architecture (intron size, gene density, repetitive DNA content) as partly a product of long-term differences in Ne acting on nearly-neutral insertions and deletions — organisms with small Ne (many eukaryotes) tolerate more "junk," while organisms with enormous Ne (many bacteria, some yeast) have more streamlined genomes because slightly deleterious non-functional DNA is efficiently purged.
Worked examples
Example 1 — A bacterial population genetics calculation. Suppose a bacterial species has an effective population size of Ne = 10⁸ (fairly typical for a free-living bacterium with a large, well-mixed population and no strong recent bottleneck). A new mutation in a regulatory region reduces fitness by s = −2 × 10⁻⁸ per generation — an extremely small effect, biochemically almost undetectable in the lab. Compute Nes:
Since |Nes| = 2, this mutation sits just past the boundary of the nearly neutral zone — selection is weak but non-negligible; the mutation is somewhat more likely to be lost than a strictly neutral variant, though not overwhelmingly so. Now compare the same mutation (same s) occurring in a small, bottlenecked bacterial population, say a chronic-infection population within a single host with Ne = 10⁴ (a scenario documented in some persistent infections, such as Pseudomonas aeruginosa in cystic fibrosis lungs):
Here |Nes| ≪ 1: the mutation is, for practical evolutionary purposes, neutral. It can drift to fixation within the host population with essentially the same probability as a truly neutral allele, ≈ 1/(2Ne). This is not a hypothetical curiosity — it is precisely the logic used to explain why bacterial populations undergoing chronic, bottlenecked infection (or serial single-colony transfer in evolution experiments) accumulate more slightly deleterious mutations, including loss-of-function changes in genes still under weak selection, than the same species does in a large, well-mixed free-living population. The compound parameter Nes, not s alone, decided the outcome.
Example 2 — Reading a comparative genomic dataset. A researcher compares four mammal species' genome-wide average dN/dS ratios (nonsynonymous divergence over synonymous divergence, a standard proxy for the relative efficacy of purifying selection) alongside independent estimates of long-term effective population size from synonymous-site nucleotide diversity (θS = 4Neμ):
| Species | Estimated Ne | Genome-wide dN/dS |
|---|---|---|
| House mouse (Mus musculus) | ~500,000 | 0.13 |
| Domestic dog (Canis familiaris) | ~45,000 | 0.22 |
| Human (Homo sapiens) | ~10,000 | 0.30 |
| Killer whale (Orcinus orca) | ~2,500 | 0.38 |
(Figures are illustrative, order-of-magnitude representative of published comparative estimates, not exact published values.) Reading this table through the nearly neutral lens: as Ne falls roughly 200-fold from mouse to killer whale, dN/dS nearly triples. This is the qualitative signature the theory predicts — smaller Ne widens the nearly neutral zone, so a larger fraction of nonsynonymous mutations that arise are fixed rather than purged, inflating dN/dS even though the underlying distribution of fitness effects (the DFE) may be similar across these related mammals. A student should resist two wrong readings of this table. First, it does not mean killer whales are "evolving faster" in an adaptive sense — the higher dN/dS mostly reflects relaxed purifying selection (drift fixing mildly deleterious variants), not more frequent positive selection; distinguishing the two requires methods that separate a genuinely elevated rate of adaptive substitution from an elevated rate of deleterious fixation, a key motivation for later methods used in Detecting Selection in Sequences such as the McDonald–Kreitman test. Second, it does not mean mice are somehow "more perfect" — mice simply have a larger Ne, so selection more efficiently screens out the same class of mildly harmful mutations that drift permits to fix in whales.
Common misconceptions & traps
| Misconception | Correction |
|---|---|
| "Nearly neutral theory says mutations are neutral or not — same as Kimura." | It replaces the sharp dichotomy with a continuum governed by Nes; the same s can behave as effectively neutral or effectively deleterious depending on Ne. |
| "High dN/dS always means positive/adaptive selection." | Elevated dN/dS can equally reflect relaxed purifying selection in a small-Ne lineage; distinguishing drift-driven fixation of mildly deleterious sites from genuine positive selection requires additional tests (e.g., polymorphism-vs-divergence methods). |
| "Ne is just the census population size." | Ne reflects breeding structure, variance in offspring number, linked selection, and inheritance mode; mitochondrial Ne is typically ~1/4 of nuclear Ne even in the same organism. |
| "Selection coefficients are fixed properties of a mutation." | The evolutionary outcome of a given s depends jointly on s and Ne — the same mutation is effectively neutral in a small population and effectively deleterious in a large one. |
| "Nearly neutral theory contradicts the neutral theory." | It is a refinement and generalization, not a rejection — synonymous-site behavior and the basic logic of drift are retained; the extension concerns mildly selected sites specifically. |
| "Small populations evolve 'better' because drift lets them explore more phenotypes." | Small-Ne populations accumulate more deleterious substitutions on average (increased genetic load), a liability, not an innovation engine, in the standard nearly-neutral framework. |
The scientist behind it
Tomoko Ohta (b. 1933) is a Japanese population geneticist who worked for most of her career at the National Institute of Genetics in Mishima, Japan, closely alongside Motoo Kimura, the architect of the neutral theory. Trained originally in agricultural science and later in population genetics (including graduate work in the United States), Ohta brought a quantitative, model-building rigor to a question that Kimura's framework had left partly unresolved: why did the molecular clock show systematic irregularities, especially tied to generation time and taxon, that pure neutrality struggled to explain? Rather than abandoning the neutral framework, she extended it, publishing her foundational nearly neutral model in a short but consequential 1973 paper in Nature, and then developing its mathematical and empirical implications across several decades of subsequent work, including influential treatments of gene duplication, multigene family evolution, and the role of population size in genome architecture. Ohta's career is notable for having built one of the field's most durable theoretical frameworks from a relatively narrow starting anomaly — an inconsistency in generation-time scaling of substitution rates — and generalizing it into a broadly applicable principle connecting molecular evolution, population size, and genome structure. Her work has been recognized with major honors including the Crafoord Prize in Biosciences (2015, shared with Richard Lewontin), the Prize often considered biology's counterpart to fields lacking a Nobel category, along with membership in the U.S. National Academy of Sciences and Japan's Academy.
Origins · 1 minTomoko Ohta and how this was discovered
Where this matters today
Conservation genomics. Endangered and historically bottlenecked populations — Iberian lynx, Isle Royale wolves, Channel Island foxes, mountain gorillas — show elevated ratios of nonsynonymous to synonymous variation and increased homozygosity for putatively deleterious alleles, exactly as nearly neutral theory predicts for reduced Ne. Conservation geneticists now use genomic estimates of "realized" and "masked" genetic load, grounded in this framework, to help decide whether genetic rescue (introducing migrants to restore Ne and heterozygosity) is warranted, and to forecast extinction risk from mutational meltdown — a process in which shrinking Ne and rising deleterious fixation reinforce each other in a downward spiral.
Human medical genetics. Human Ne is modest by mammalian standards (on the order of 10,000), which the theory predicts should leave humans carrying a comparatively high burden of mildly deleterious coding variants relative to species with larger Ne. Large human sequencing projects (gnomAD, UK Biobank, and earlier 1000 Genomes analyses) confirm exactly this: every human genome carries thousands of predicted-damaging missense variants, most rare and individually mildly deleterious, consistent with a population too small (in evolutionary terms) to purge them all efficiently. This framework helps interpret why rare disease variants persist at low but non-zero frequency and informs models of complex-disease genetic architecture.
Livestock, crop, and captive-breeding management. Domesticated and captive populations routinely experience severe Ne reductions from founder effects and selective breeding. Nearly neutral logic predicts, and genomic surveys confirm, elevated deleterious mutation load in many domesticated lineages relative to wild ancestors — a consideration actively used in breeding-program design to manage inbreeding depression and maintain genetic diversity in both agricultural and zoo populations.
Foundational tool for detecting selection. Perhaps the theory's broadest modern legacy is methodological: because it specifies exactly how drift and weak selection jointly shape dN/dS and the site-frequency spectrum, it supplies the null expectation against which genuine positive selection must be distinguished. Tests such as the McDonald–Kreitman test, extensions estimating the distribution of fitness effects (DFE-alpha and related methods), and genome scans for adaptive substitution all build on the nearly neutral baseline — making this theory the conceptual bridge into the modern toolkit covered under Detecting Selection in Sequences.
Ask the tutor: How does the nearly neutral theory's Nes framework connect to the McDonald–Kreitman test used for detecting positive selection in sequences?
Is the nearly neutral theory a rejection of Kimura's neutral theory?
No — it is an extension, not a refutation. Kimura's core claims about synonymous-site evolution and the general importance of drift in molecular evolution remain intact. Ohta added a more realistic treatment of nonsynonymous and regulatory mutations, most of which have small but non-zero selection coefficients, showing that their fate depends jointly on s and Ne rather than falling neatly into "strictly neutral" or "strongly deleterious" bins. The two frameworks share the same mathematical toolkit (diffusion approximations, fixation probability formulas) and the same conclusion that drift is a major evolutionary force; nearly neutral theory simply makes the boundary between "selected" and "neutral" a function of population size rather than a fixed property of the mutation.
How large does |Nes| need to be for selection to "win" against drift?
There is no sharp cutoff, but |Nes| ≈ 1 is the conventional reference point where drift and selection contribute comparably to a mutation's fate. When |Nes| is around 5–10 or more, selection dominates strongly and the fixation probability of a deleterious mutation becomes very small (exponentially suppressed). When |Nes| is well below 1 (say, 0.01), the mutation's fixation probability is nearly indistinguishable from a strictly neutral allele's 1/(2Ne). Because real DFEs are continuous, real genomes contain mutations spanning this entire spectrum simultaneously, which is why "nearly neutral" is better understood as a zone than a category.
Does a small effective population size make a species evolve "worse" or is this value-neutral?
It is value-neutral in the sense that natural selection has no foresight or goal, but it does have a measurable fitness consequence: smaller Ne allows more mildly deleterious mutations to fix, which on average increases genetic load (a population-wide reduction in mean fitness relative to a hypothetical mutation-free genotype). This is a real, quantifiable cost seen in mutation accumulation experiments and in elevated deleterious variant burden in bottlenecked wild populations. It is not "worse" in any teleological sense — it is simply a predictable statistical consequence of weaker selection efficacy at small Ne, and it is central to concerns about long-term viability (mutational meltdown) in critically endangered species.
How do biologists estimate Ne independently, so the dN/dS prediction can actually be tested without circularity?
The standard approach uses synonymous-site nucleotide diversity, θS = 4Neμ (for diploids), where μ is estimated from mutation rate studies (pedigree sequencing, mutation accumulation lines) and θS is measured directly from population sequence data at silent sites assumed to be nearly free of selection. Because this Ne estimate comes from silent-site diversity and an independently measured mutation rate — not from dN/dS itself — comparing this Ne against dN/dS avoids circular reasoning. This is exactly the logic used in the comparative mammal, plant, and mitochondrial/nuclear studies described in the evidence section.
Can nearly neutral theory explain adaptive evolution, or is it only about deleterious mutations?
The theory as classically framed emphasizes the fate of mildly deleterious mutations, but the same Nes logic applies symmetrically to mildly beneficial mutations: a weakly beneficial mutation (small positive s) can also be effectively invisible to selection in a small population and lost by drift, just as a weakly deleterious one can fix. This means small-Ne populations not only accumulate more mild deleterious load but may also fail to fix weakly beneficial mutations that a larger population would capture — a cost sometimes called reduced "adaptive potential" at the nearly-neutral margin, distinct from, but related to, the loss of standing genetic variation from drift more generally.
Why does dN/dS matter more than just counting amino acid differences between two species?
Raw amino-acid differences confound two very different things: the mutation rate (how many changes arise) and the strength of selection (how many changes are tolerated). Dividing nonsynonymous divergence (dN) by synonymous divergence (dS) cancels out most of the mutation-rate and time-since-divergence effects, because synonymous sites are assumed to evolve at close to the neutral mutation rate. The resulting ratio isolates, approximately, the fraction of amino-acid-changing mutations that are tolerated (fixed) relative to the neutral expectation — precisely the quantity that nearly neutral theory predicts should track 1/Ne.
Does the nearly neutral theory apply only to protein-coding DNA?
No. The same Nes logic applies to any site under weak selection, including regulatory regions, splice sites, untranslated regions, and even genome architecture features like intron size or transposable element content, where small fitness costs (e.g., from slightly increased replication burden or slightly altered expression) can be effectively invisible to selection in small-Ne genomes. Michael Lynch and colleagues have argued this extended logic helps explain large-scale genome architecture differences between lineages with very different long-term effective population sizes, such as the generally larger, more repeat-rich genomes of many eukaryotes with modest Ne compared to the leaner genomes of many bacteria with enormous Ne.