# Unified neutral theory of biodiversity

Unified neutral theory of biodiversity

The unified neutral theory of biodiversity and biogeography (here "Unified Theory" or "UNTB") is a theory and the title of a monograph [http://www.pupress.princeton.edu/titles/7105.html] by ecologist Stephen Hubbell. The theory aims to explain the diversity and relative abundance of species in ecological communities, although like other neutral theories of ecology, Hubbell's theory assumes that the differences between members of an ecological community of trophically similar species are "neutral," or irrelevant to their success.

Overview

"Neutrality" is defined as per capita ecological equivalence among all individuals of every species at a given trophic level in a food web; "per capita equivalence" means that all species are held to behave (ie reproduce and die) in the same way as one another; and individuals of a particular species reproduce and die (behave) in the same way. Other neutral theories preceded Hubbell's. This author considers that the island biogeography theory by Robert MacArthur & E.O. Wilson was also an instance of neutral theory [Hubbell 2001] .

An "ecological community" is a group of trophically similar, sympatric species that actually or potentially compete in a local area for the same or similar resources (Hubbell 2001). Under the Unified Theory, complex ecological interactions are permitted among individuals of an ecological community (such as competition and cooperation), provided that all individuals obey the same rules. Asymmetric phenomena such as parasitism and predation are ruled out by the terms of reference; but cooperative strategies such as swarming, and negative interaction such as competing for limited food or light are allowed (so long as all individuals behave in the same way).

Although the Unified Theory makes a large number of falsifiable hypotheses, differences between predictions of the Unified Theory and observations are of very small magnitude.Fact|date=October 2007 The Unified Theory also makes predictions that have profound implications for the management of biodiversity, especially the management of rare species.Fact|date=November 2007

The neutral theory is an instance of dispersal assembly theory. In contrast, niche assembly theories are nonneutral, because they hold that different species behave in different ways from one another (e.g. Robert MacArthur's broken stick is a niche theory). A recent alternative to the neutral theory is the idiosyncratic theory of biodiversity [Pueyo et al. 2007] [http://www.blackwell-synergy.com/doi/pdf/10.1111/j.1461-0248.2007.01096.x] .

Under Hubbell's theory, species drift is allowed to occur via speciation, which would occur with a specific probability per birth. The neutrality of the Unified Theory implies that this probability would be independent of the parent's species (common species have a higher birth rate, and thus the UNTB predicts that speciation occurs more frequently for common species than rare species). [Leigh 2007] is a helpful recent review of the unified neutral theory, pinpointing its achievements and limitations.

The theory predicts the existence of a fundamental biodiversity constant, conventionally written "θ", that appears to govern species richness on a wide variety of spatial and temporal scales.

The Unified Theory and saturation

Although not strictly necessary for a neutral theory, many stochastic models of biodiversity assume a fixed, finite community size. There are unavoidable physical constraints on the total number of individuals that can be packed into a given space (although space "per se" isn't necessarily a resource, it is often a useful surrogate variable for a limiting resource that is distributed over the landscape; examples would include sunlight or hosts, in the case of parasites).

If a wide range of species is considered (say, giant sequoia trees and duckweed, two species that have very different saturation densities), then the assumption of constant community size might not be very good, because density would be higher if the smaller species were monodominant.

However, because the Unified Theory refers only to communities of trophically similar, competing species, it is unlikely that population density will vary too widely from one place to another.

Hubbell considers the fact that population densities are constant and interprets it as a general principle: "large landscapes are always biotically saturated with individuals". Hubbell thus treats communities as being of a fixed number of individuals, usually denoted by "J".

Exceptions to the saturation principle include disturbed ecosystems such as the Serengeti, where saplings are trampled by elephants and Blue wildebeests; or gardens, where certain species are systematically removed.

pecies abundances

When abundance data on natural populations are collected, two observations are almost universal:

* The most common species accounts for a substantial fraction of the individuals sampled;
* A substantial fraction of the species sampled are very rare. Indeed, a substantial fraction of the species sampled are singletons, that is, species which are sufficiently rare for only a single individual to have been sampled.

Such observations typically generate a large number of questions. Why are the rare species rare? Why is the most abundant species so much more abundant than the median species abundance?

A non neutral explanation for the rarity of rare species might suggest that rarity is a result of poor adaptation to local conditions. The UNTB implies that such considerations may be neglected from the perspective of population biology (because the explanation cited implies that the rare species behaves differently from the abundant species).

Species composition in any community will change randomly with time. However, any particular abundance structure will have an associated probability. The UNTB predicts that the probability of a community of "J" individuals composed of "S" distinct species with abundances $n_1$ for species 1, $n_2$ for species 2, and so on up to $n_S$ for species "S" is given by

:$Pr\left(n_1,n_2,ldots,n_S| heta, J\right)=frac\left\{J! heta^S\right\}\left\{ 1^\left\{phi_1\right\}2^\left\{phi_2\right\}cdots J^\left\{phi_J\right\} phi_1!phi_2!cdotsphi_J! Pi_\left\{k=1\right\}^J\left( heta+k-1\right)\right\}$

where $heta=2J u$ is the fundamental biodiversity number ($u$ is the speciation rate), and $phi_i$ is the number of species that have "i" individuals in the sample.

This equation shows that the UNTB implies a nontrivial dominance-diversity equilibrium between speciation and extinction.

As an example, consider a community with 10 individuals and three species "a", "b", and "c" with abundances 3, 6 and 1 respectively. Then the formula above would allow us to assess the likelihood of different values of "θ". There are thus "S" = 3 species and $phi_1=phi_3=phi_6=1$, all other $phi$'s being zero. The formula would give

:$Pr\left(3,6,1| heta,10\right)=frac\left\{10! heta^3\right\}\left\{1^1cdot 3^1cdot 6^1cdot1!1!1!cdot heta\left( heta+1\right)\left( heta+1\right)cdots\left( heta+9\right)\right\}$

which could be maximized to yield an estimate for "θ" (in practice, numerical methods are used). The maximum likelihood estimate for "θ" is about 1.1478.

We could have labelled the species another way and counted the abundances being 1,3,6 instead (or 3,1,6, etc etc). Logic tells us that the probability of observing a pattern of abundances will be the same observing any permutation of those abundances. Here we would have

: $Pr\left(3;3,6,1\right)=Pr\left(3;1,3,6\right)=Pr\left(3;3,1,6\right)$

and so on.

To account for this, it is helpful to consider only ranked abundances (that is, to sort the abundances before inserting into the formula). A ranked dominance-diversity configuration is usually written as $Pr\left(S;r_1,r_2,ldots,r_s,0,ldots,0\right)$ where $r_i$ is the abundance of the "i"th most abundant species: $r_1$ is the abundance of the most abundant, $r_2$ the abundance of the second most abundant species, and so on. For convenience, the expression is usually "padded" with enough zeros to ensure that there are "J" species (the zeros indicating that the extra species have zero abundance).

It is now possible to determine the expected abundance of the "i"th most abundant species:

:$E\left(r_i\right)=sum_\left\{k=1\right\}^Cr_i\left(k\right)cdot Pr\left(S;r_1,r_2,ldots,r_s,0,ldots,0\right)$

where "C" is the total number of configurations, $r_i\left(k\right)$ is the abundance of the "i"th ranked species in the "k"th configuration, and $Pr\left(ldots\right)$ is the dominance-diversity probability. This formula is difficult to manipulate mathematically, but relatively simple to simulate computationally.

The model discussed so far is a model of a regional community, which Hubbell calls the metacommunity. Hubbell also acknowledged that on a local scale, dispersal plays an important role. For example, seeds are more likely to come from nearby parents than from distant parents. Hubbell introduced the parameter m, which denotes the probability of immigration in the local community from the metacommunity. If m = 1, dispersal is unlimited; the local community is just a sample from the metacommunity and the formulas above apply. If m < 1, however, dispersal is limited and the local community is a dispersal-limited sample from the metacommunity for which different formulas apply.

In a paper in Nature in 2003, it is shown that $langle phi_n angle$, the expected number of species with abundance n, may be calculated by

:$hetafrac\left\{J!\right\}\left\{n!\left(J-n\right)!\right\}frac\left\{Gamma\left(gamma\right)\right\}\left\{Gamma\left(J+gamma\right)\right\}int_\left\{y=0\right\}^gammafrac\left\{Gamma\left(n+y\right)\right\}\left\{Gamma\left(1+y\right)\right\}frac\left\{Gamma\left(J-n+gamma-y\right)\right\}\left\{Gamma\left(gamma-y\right)\right\}exp\left(-y heta/gamma\right),dy$

where "θ" is the fundamental biodiversity number, "J" the community size, $Gamma$ is the gamma function, and $gamma=\left(J-1\right)m/\left(1-m\right)$. This formula is however an approximation. The correct formula is derived in a series of papers, reviewed and synthesized by Etienne & Alonso 2005 [http://www.blackwell-synergy.com/doi/abs/10.1111/j.1461-0248.2005.00817.x] :

:$frac\left\{ heta \right\}\left\{\left(I\right)_\left\{J \left\{J choose n\right\}int_\left\{0\right\}^\left\{1\right\}\left(Ix\right)_\left\{n\right\}\left(I\left(1-x\right)\right)_\left\{J-n\right\}frac\left\{\left(1-x\right)^\left\{ heta -1\left\{x\right\},dx$

where $I = \left(J - 1\right)*m/\left(1-m\right)$ is a parameter that measures dispersal limitation.

$langle phi_n angle$ is zero for "n" > "J", as there cannot be more species than individuals.

This formula is important because it allows a quick evaluation of the Unified Theory. It is not suitable for testing the theory. For this purpose, the approptiate likelihood function should be used. For the metacommunity this was given above. For the local community with dispersal limitation it is given by:

:$Pr\left(n_1,n_2,ldots,n_S| heta, m, J\right)=frac\left\{J!\right\}\left\{prod_\left\{i=1\right\}^\left\{S\right\}n_\left\{i\right\}prod_\left\{j=1\right\}^\left\{J\right\}Phi_\left\{j\right\}!\right\}frac\left\{ heta ^\left\{S\left\{\left(I\right)_\left\{Jsum_\left\{A=S\right\}^\left\{J\right\}K\left(overrightarrow\left\{D\right\},A\right)frac\left\{I^\left\{A\left\{\left( heta\right) _\left\{A$

Here, the $K\left(overrightarrow\left\{D\right\},A\right)$ for $A=S,...,J$ are coefficients fully determined by the data, being defined as

:$K\left(overrightarrow\left\{D\right\},A\right):=sum_\left\{\left\{a_\left\{1\right\},...,a_\left\{S\right\}|sum_\left\{i=1\right\}^\left\{S\right\}a_\left\{i\right\}=Aprod_\left\{i=1\right\}^\left\{S\right\}frac\left\{overline\left\{s\right\}left\left( n_\left\{i\right\},a_\left\{i\right\} ight\right) overline\left\{s\right\}left\left( a_\left\{i\right\},1 ight\right) \right\}\left\{overline\left\{s\right\}left\left( n_\left\{i\right\},1 ight\right) \right\}$

This seemingly complicated formula involves Stirling numbers and Pochhammer symbols, but can be easily calculated. See [http://www.blackwellpublishing.com/products/journals/suppmat/ELE/ELE717/ELE717sm.htm]

An example of a species abundance curve can be found here: [http://www.sciam.com/article.cfm?articleID=000656C3-8F00-1CDA-B4A8809EC588EEDF] .

tochastic modelling of species abundances under the UNTB

UNTB distinguishes between a dispersal-limited local community of size $J$ and a so called metacommunity from which species can (re)immigrate and which acts as a heat bath to the local community. The distribution of species in the metacommunity is given by a dynamic equilibrium of speciation and extinction. Both community dynamics are modelled by appropriate urn processes, where each individual is represented by a ball with a color corresponding to its species. With a certain rate $r$ randomly chosen individuals reproduce, i.e. add another ball of their own color to the urn. Since one basic assumption is saturation, this reproduction has to happen at the cost of another random individual from the urn which is removed. At a different rate $mu$ single individuals in the metacommunity are replaced by mutants of an entirely new species. Hubbell calls this simplified model for speciation a point mutation, using the terminology of the Neutral theory of molecular evolution. The urn scheme for the metacommunity of $J_M$ individuals is the following.

At each time step take one of the two possible actions :

# With probability $\left(1- u\right)$ draw an individual at random and replace another random individual from the urn with a copy of the first one.
# With probability $u$ draw an individual and replace it with an individual of a new species.

Note that the size $J_M$ of the metacommunity does not change. Note also that this is a point process in time. The length of the time steps is distributed exponentially. For simplicity one can, however, assume that each time step is as long as the mean time between two changes which can be derived from the reproduction and mutation rates $r$ and $mu$. The probability $u$ is given as $u=mu/\left(r+mu\right)$.

The species abundance distribution for this urn process is given by Ewens's sampling formula which was originally derived in 1972 for the distribution of allele under neutral mutations. The expected number $S_M\left(n\right)$ of species in the metacommunity having exactly $n$ individuals is [Vallade, Houchmandzadeh 2003 [http://prola.aps.org/abstract/PRE/v68/i6/e061902] ]

:$S_M\left(n\right) = frac\left\{ heta\right\}\left\{n\right\}frac\left\{Gamma\left(J_M+1\right)Gamma\left(J_M+ heta-n\right)\right\}\left\{Gamma\left(J_M+1-n\right)Gamma\left(J_M+ heta\right)\right\}$

where $heta=\left(J_M-1\right) u/\left(1- u\right)approx J_M u$ is called the fundamental biodiversity number. For largemetacommunities and $nll J_M$ one recovers the Fisher Log-Series as species distribution.

:$S_M\left(n\right) approx frac\left\{ heta\right\}\left\{n\right\} left\left( frac\left\{J_M\right\}\left\{J_M+ heta\right\} ight\right)^n$

The urn scheme for the local community of fixed size $J$ is very similar to the one for the metacommunity.

At each time step take one of the two actions :

# With probability $\left(1-m\right)$ draw an individual at random and replace another random individual from the urn with a copy of the first one.
# With probability $m$ replace a random individual with an immigrant drawn from the metacommunity.

The metacommunity is changing on a much larger timescale and is assumed to be fixed during the evolution of the local community. The resulting distribution of species in the local community and expected values depend on four parameters, $J$, $J_M$, $heta$ and $m$ (or $I$) and are derived in [Etienne, Alonso 2005 [http://www.blackwell-synergy.com/doi/full/10.1111/j.1461-0248.2005.00817.x] ] , including several simplifying limit cases like the one presented in the previous section (there called $langlephi_n angle$). The parameter $m$ is a dispersal parameter. If $m=1$ then the local community is just a sample from the metacommunity. For $m=0$ the local community is completely isolated from the metacommunity and all species will go extinct except one. This case has been analyzed by Hubbell himself [Hubbell 2001] . The case

Unified Theory and species-area relationships

The Unified Theory unifies "biodiversity", as measured by species-abundance curves, with "biogeography", as measured by species-area curves. Species-area relationships show the rate at which species diversity increases with area. The topic is of great interest to conservation biologists in the design of reserves, as it is often desired to harbour as many species as possible.

The most commonly encountered relationship is the power law given by

:$S=cA^z$

where "S" is the number of species found, "A" is the area sampled, and "c" and "z" are constants. This relationship, with different constants, has been found to fit a wide range of empirical data.

From the perspective of Unified Theory, it is convenient to consider "S" as a function of total community size "J". Then $S=kJ^z$ for some constant "k", and if this relationship were exactly true, the species area line would be straight on log scales. It is typically found that the curve is not straight, but the slope changes from being steep at small areas, shallower at intermediate areas, and steep at the largest areas.

The formula for species composition derived above (not done this bit yet) may be used to calculate the expected number of species present in a community under the assumptions of the Unified Theory. In symbols

:$Eleft\left\{S| heta,J ight\right\}=frac\left\{ heta\right\}\left\{ heta \right\}+frac\left\{ heta\right\}\left\{ heta+1\right\}+frac\left\{ heta\right\}\left\{ heta+2\right\}+cdots +frac\left\{ heta\right\}\left\{ heta+J-1\right\}$

where θ is the fundamental biodiversity number. This formula specifies the expected number of species sampled in a community of size "J". The last term, $heta/\left( heta+J-1\right)$, is the expected number of "new" species encountered when adding one new individual to the community. This is an increasing function of θ and a decreasing function of "J", as expected.

By making the substitution $J= ho A$ (see section on saturation above), then the expected number of species becomes $Sigma heta/\left( heta+ ho A-1\right)$.

The formula above may be approximated to an integral giving

:$S\left( heta\right)=1+ hetalnleft\left(1+frac\left\{J-1\right\}\left\{ heta\right\} ight\right).$

Example

Consider the following (synthetic) dataset, of 23 individuals:

a, a,a, a,a, a,a, a,a, a,b, b,b, b,c, c,c, c,d, d,d, d,e, f,g, h,i

There are thus 27 individuals of 9 species ("a" to "i") in the sample. Tabulating this would give:

a b c d e f g h i 10 4 4 4 1 1 1 1 1

indicating that species "a" is the most abundant with 10 individuals and species "d" to "i" are singletons. Tabulating the table gives:

species abundance 1 2 3 4 5 6 7 8 9 10 number of species 5 0 0 3 0 0 0 0 0 1

On the second row, the 5 in the first column means that five species, species "e" through "i", have abundance one. The following two zeros in columns 2 and 3 mean that zero species have abundance 2 or 3. The 3 in column 4 means that three species, species "b", "c", and "d", have abundance four. The final 1 in column 10 means that one species, species "a", has abundance 10.

This type of dataset is typical in biodiversity studies. Observe how more than half the biodiversity (as measured by species count) is due to singletons.

For real datasets, the species abundances are binned into logarithmic categories, usually using base 2, which gives bins of abundance 0-1, abundance 1-2, abundance 2-4, abundance 4-8, etc. Such abundance classes are called "octaves"; early developers of this concept included F. W. Preston and histograms showing number of species as a function of abundance octave are known as Preston diagrams.

These bins are not mutually exclusive: a species with abundance 4, for example, could be considered as lying in the 2-4 abundance class or the 4-8 abundance class. Species with an abundance of an exact power of 2 (ie 2,4,8,16, etc) are conventionally considered as having 50% membership in the lower abundance class 50% membership in the upper class. Such species are thus considered to be evenly split between the two adjacent classes (apart from singletons which are classified into the rarest category). Thus in the example above, the Preston abundances would be

abundance class 1 1-2 2-4 4-8 8-16 species 5 0 1.5 1.5 1

The three species of abundance four thus appear, 1.5 in abundance class 2-4, and 1.5 in 4-8.

The above method of analysis cannot account for species that are unsampled: that is, species sufficiently rare to have been recorded zero times. Preston diagrams are thus truncated at zero abundance Fisher called this the "veil line" and noted that the cutoff point would move as more individuals are sampled.

Proponents and critics of the UNTB

Notable proponents of the Unified Theory include Stephen Hubbell (UCLA) and Graham Bell (McGill University); notable critics include Brian McGill (University of Arizona) and J. Timothy Wootton (University of Chicago).

References

* (cite journal|title=Errata |journal=Ecology Letters|volume=9|pages=500|doi=10.1111/j.1461-0248.2006.00917.x|year=2006)
*cite journal|last=Gilbert|first=B |coauthor=Lechowicz MJ|date=2004|title=Neutrality, niches, and dispersal in a temperate forest understory|journal=PNAS|volume=101|pages=7651–7656|doi=10.1073/pnas.0400814101|pmid=15128948}
*
*
*
*
*

ee also

* Biodiversity Action Plan
* Warren Ewens
* Ewens's sampling formula
* Metabolic theory of ecology
* Neutral theory of molecular evolution
* [http://rss.acs.unt.edu/Rdoc/library/untb/html/00Index.html R package for implementing UNTB]

* [http://www.sciam.com/article.cfm?articleID=000D401A-8D9D-1CDA-B4A8809EC588EEDF Scientific American Interview with Steve Hubbell]

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