This tutorial comes with a recorded video walkthrough. The video corresponding to each section of the exercise is linked next to the section title. The full playlist is available here:
This tutorial covers the first protocol from Höhna et al. (2017), which demonstrates how to set up and perform analyses using common nucleotide substitution models. The substitution models used in molecular evolution are continuous time Markov models, which are fully characterized by their instantaneous-rate matrix:
where $\mu_{ij}$ represents the instantaneous rate of substitution from state $i$ to state $j$. The diagonal elements $\mu_i$ are the rates of not changing out of state $i$, equal to the sum of the elements in the corresponding row. Given the instantaneous-rate matrix, $Q$, we can compute the corresponding transition probabilities for a branch of length $t$, $P(t)$, by exponentiating the rate matrix:
Each of the named substitution models (e.g., HKY or GTR) has a uniquely defined instantaneous-rate matrix, $Q$.
In this tutorial you will perform phylogeny inference under common models of DNA sequence evolution: JC, F81, HKY85, GTR, GTR+Gamma and GTR+Gamma+I. For all of these substitution models, you will perform a Markov chain Monte Carlo (MCMC) analysis to estimate phylogeny and other model parameters. The estimated trees will be unrooted trees with independent branch-length parameters. We will provide comments on how to modify the tutorial if you wish to estimate rooted, clock-like trees. All the assumptions will be covered in more detail later in this tutorial.
Model | Reference | Function | Parameters |
---|---|---|---|
Jukes-Cantor | (Jukes and Cantor 1969) | fnJC | - |
K80 (a.k.a. K2P) | (Kimura 1980) | fnK80 | $\kappa$ |
Felsenstein-81 | (Felsenstein 1981) | fnF81 | $\pi$ |
T92 | (Tamura 1992) | fnT92 | $\pi_{GC}$, $\kappa$ |
HKY | (Hasegawa et al. 1985) | fnHKY | $\pi$, $\kappa$ |
GTR | (Tavaré 1986) | fnGTR | $\pi$, $\epsilon$ |
The first section of this exercise involves:
We first consider the simplest substitution model described by Jukes and Cantor (1969). The instantaneous-rate matrix for the JC substitution model is defined as
which has the advantage that the transition probability matrix can be computed analytically
where $t$ is the branch length in units of time, and $r$ is the rate (clock) for the process. In the later exercises you will be asked to specify more complex substitution models. Don’t worry, you won’t have to calculate all of the transition probabilities, because RevBayes will take care of all the computations for you. Here we only provide some of the equations for the models in case you might be interested in the details. You will be able to complete the exercises without understanding the underlying math.
The files for this example analysis are provided for you (mcmc_JC.Rev
).
If you download this file and place it in a directory called scripts
inside your main tutorial directory,
you can
easily execute this analysis using the source()
function in the RevBayes console:
source("scripts/mcmc_JC.Rev")
If everything loaded properly, then you should see the program initiate the Markov chain Monte Carlo analysis that estimates the posterior distribution. If you continue to let this run, then you will see it output the states of the Markov chain once the MCMC analysis begins.
Ultimately, this is how you will execute most analyses in RevBayes, with the full specification of the model and analyses contained in the sourced files. You could easily run this entire analysis on your own data by substituting your data file name for that in the model-specification file. However, it is important to understand the components of the model to be able to take full advantage of the flexibility and richness of RevBayes. Furthermore, without inspecting the Rev scripts sourced in mcmc_JC.Rev
, you may end up inadvertently performing inappropriate analyses on your dataset, which would be a waste of your time and CPU cycles. The next steps will walk you through the full specification of the model and MCMC analyses.
First create a directory for this tutorial and name it
RB_CTMC_Tutorial
, or any name you like.Navigate to this new directory and create a new folder called
data
inside of it.Download the data file called
primates_and_galeopterus_cytb.nex
and save it to thedata
directory.Now start RevBayes from your working directory (
RB_CTMC_Tutorial
).
Checking and Changing Your Working Directory
For this tutorial and much of the work you will do in RevBayes, you will need to access files. It is important that you are aware of your current working directory if you use relative file paths in your Rev scripts or in the RevBayes console.
To check your current working directory, use the function
getwd()
.getwd()
/Users/tombayes/Work
If you want to change the directory, enter the path to your directory in the arguments of the function
setwd()
.setwd("Tutorials/RB_CTMC_Tutorial")
Now check your directory again to make sure you are where you want to be:
getwd()
/Users/tombayes/Work/Tutorials/RB_CTMC_Tutorial
First load in the sequences using the readDiscreteCharacterData()
function.
data <- readDiscreteCharacterData("data/primates_and_galeopterus_cytb.nex")
Executing these lines initializes the data matrix as the respective
Rev variables. To report the current value of any variable, simply
type the variable name and press enter. For the data
matrix, this
provides information about the alignment:
data
DNA character matrix with 23 taxa and 1141 characters
=====================================================
Origination: primates_and_galeopterus_cytb.nex
Number of taxa: 23
Number of included taxa: 23
Number of characters: 1141
Number of included characters: 1141
Datatype: DNA
Next we will specify some useful variables based on our dataset. The variable data
has member functions
that we can use to retrieve information about the dataset. These include, for example,
the number of species and the taxa. We will need that taxon information for setting up different parts of our model.
num_taxa <- data.ntaxa()
num_branches <- 2 * num_taxa - 3
taxa <- data.taxa()
Additionally, we set up a (vector) variable that holds all the moves for our analysis. Recall that moves are algorithms used to propose new parameter values during the MCMC simulation. Similarly, we set up a variable for the monitors. Monitors print the values of model parameters to the screen and/or log files during the MCMC analysis.
moves = VectorMoves()
monitors = VectorMonitors()
You may have noticed that we used the =
operator to create the move index.
This simply means that the variable is not part of the model.
You will later see that we use this operator more often, e.g., when we create moves and monitors.
With the data loaded, we can now proceed to specify our specifying the model.
Estimating an unrooted tree under the JC model requires specification of two main components: (1) the and (2) the .
A given substitution model is defined by its corresponding
instantaneous-rate matrix, $Q$. The Jukes-Cantor substitution model does
not have any free parameters (as the substitution rates are all assumed
to be equal, and there is a separate parameter that scales their overall
magnitude), so we can define it as a constant variable. The function
fnJC(n)
will create an instantaneous-rate matrix for a character with
$n$ states. Since we use DNA data here, we create a 4x4
instantaneous-rate matrix:
Q <- fnJC(4)
You can see the rates of the $Q$ matrix by typing
Q
[ [ -1.0000, 0.3333, 0.3333, 0.3333 ] ,
0.3333, -1.0000, 0.3333, 0.3333 ] ,
0.3333, 0.3333, -1.0000, 0.3333 ] ,
0.3333, 0.3333, 0.3333, -1.0000 ] ]
As you can see, all substitution rates are equal.
The tree topology and branch lengths are stochastic nodes in our phylogenetic model. In , the tree topology is denoted $\Psi$ and the length of the branch leading to node $i$ is $bl_i$.
We will assume that all possible labeled, unrooted tree topologies have equal probability.
This is the dnUniformTopology()
distribution in RevBayes.
Note that in RevBayes it is advisable to specify the outgroup for your study system
if you use an unrooted tree prior, whereas other software, e.g.,
MrBayes uses the first taxon in the data matrix file as the outgroup.
Providing RevBayes with an outgroup clade will enable the monitor writing the trees
to file to orient the topologies with the outgroup clade at the base,
thus making the trees easier to visualize.
Specify the topology
stochastic node by passing in the list of taxa
to the dnUniformTopology()
distribution:
out_group = clade("Galeopterus_variegatus")
topology ~ dnUniformTopology(taxa, outgroup=out_group)
Some types of stochastic nodes can be updated by a number of alternative moves.
Different moves may explore parameter space in different ways,
and it is possible to use multiple different moves for a given parameter to improve mixing
(the efficiency of the MCMC simulation).
In the case of our unrooted tree topology, for example, we can use both a nearest-neighbor interchange move (mvNNI
) and a subtree-prune and regrafting move (mvSPR
). These moves do not have tuning parameters associated with them, thus you only need to pass in the topology
node and proposal weight
.
moves.append( mvNNI(topology, weight=num_taxa) )
moves.append( mvSPR(topology, weight=num_taxa/10.0) )
The weight specifies how often the move will be applied either on average per iteration or relative to all other moves. Have a look at the MCMC Diagnosis tutorial for more details about moves and MCMC strategies (found in Tutorials).
Next we have to create a stochastic node representing the length of each of the $2N - 3$ branches in our tree (where $N=$ n_species
). We can do this using a for
loop — this is a plate in our graphical model. In this loop, we can create each of the branch-length nodes and assign each move. Copy this entire block of Rev code into the console:
for (i in 1:num_branches) {
br_lens[i] ~ dnExponential(10.0)
moves.append( mvScale(br_lens[i]) )
}
It is convenient for monitoring purposes to add the tree length as deterministic variable. The tree length is simply the sum of all branch lengths. Accordingly, the tree length can be computed using the sum()
function, which calculates the sum of any vector of values.
TL := sum(br_lens)
Finally, we can create a phylogram (a phylogeny in which the branch lengths are proportional to the expected number of substitutions/site) by combining the tree topology and branch lengths. We do this using the treeAssembly()
function, which applies the value of the $i^{th}$ member of the br_lens
vector to the branch leading to the $i^{th}$ node in topology
. Thus, the psi
variable is a deterministic node:
psi := treeAssembly(topology, br_lens)
Alternative tree priors
For large phylogenetic trees, i.e., with more than 200 taxa, it might be easier to specify a combined topology and branch length prior distribution. We can achieve this by simple using the distribution
dnUniformTopologyBranchLength()
.br_len_lambda <- 10.0 psi ~ dnUniformTopologyBranchLength(taxa, branchLengthDistribution=dnExponential(br_len_lambda)) moves.append( mvNNI(psi, weight=num_taxa) ) moves.append( mvSPR(psi, weight=num_taxa/10.0) ) moves.append( mvBranchLengthScale(psi, weight=num_branches) )
You might think that this approach is in fact simpler than the
for
loop that we explained above. We still think that it is pedagogical to specify the prior on each branch length separately in this tutorial to emphasize all components of the model.
Alternative branch-length priors
Some studies, e.g. Brown et al. (2010), Rannala et al. (2012), have criticized the exponential prior distribution for branch lengths because it induces a gamma-distributed tree-length and the mean of this gamma distribution grows with the number of taxa. As an alternative, we can instead use a specific gamma prior distribution (or any other distribution defined on a positive real variable) for the tree length, and then use a Dirichlet prior distribution to break the tree length into the corresponding branch lengths (Zhang et al. 2012).
First, specify a prior distribution on the tree length with your desired mean. For example, we use a gamma distribution as our prior on the tree length.
TL ~ dnGamma(2,4) moves.append( mvScale(TL) )
Now we create a random variable for the relative branch lengths.
rel_branch_lengths ~ dnDirichlet( rep(1.0,num_branches) ) moves.append( mvBetaSimplex(rel_branch_lengths, weight=num_branches) ) moves.append( mvDirichletSimplex(rel_branch_lengths, weight=num_branches/10.0) )
Finally, transform the relative branch lengths into actual branch lengths
br_lens := rel_branch_lengths * TL
Alternative Prior on Time-Trees: Tree Topology and Node Ages
Alternatively, you may want to specify a prior on time-trees. Here we will briefly indicate how to specify such an prior which will lead to inference of time trees.
The tree (the topology and node ages) is a stochastic node in our phylogenetic model. For simplicity, we will assume a uniform prior on both topologies and node ages. The distribution in RevBayes is
dnUniformTimeTree()
.Fore more information on tree priors, such as birth-death processes, please read the Relaxed Clocks & Time Trees.
First, we need to specify the age of the tree:
root_age <- 10.0
Here we simply assumed that the tree is 10.0 time units old. We could also specify a prior on the root age if we have fossil calibrations (see Relaxed Clocks & Time Trees). Next, we specify the
tree
stochastic variable by passing in the taxon informationtaxa
to thednUniformTimeTree()
distribution:psi ~ dnUniformTimeTree(rootAge=root_age, taxa=taxa)
Some types of stochastic nodes can be updated by a number of alternative moves. Different moves may explore parameter space in different ways,and it is possible to use multiple different moves for a given parameter to improve mixing (the efficiency of the MCMC simulation). In the case of our rooted tree, for example, we can use both a nearest-neighbor interchange move without and with changing the node ages (
mvNarrow
andmvNNI
) and a fixed-node-height subtree-prune and regrafting move (mvFNPR
) and its Metropolized-Gibbs variant (mvGPR
) (Höhna et al. 2008; Höhna and Drummond 2012). We also need moves that change the ages of the internal nodes, for example,mvSubtreeScale
andmvNodeTimeSlideUniform
. These moves do not have tuning parameters associated with them, thus you only need to pass in thepsi
node and proposalweight
.moves.append( mvNarrow(psi, weight=num_taxa) ) moves.append( mvNNI(psi, weight=num_taxa/5.0) ) moves.append( mvFNPR(psi, weight=num_taxa/5.0) ) moves.append( mvGPR(psi, weight=num_taxa/30.0) ) moves.append( mvSubtreeScale(psi, weight=num_taxa/3.0) ) moves.append( mvNodeTimeSlideUniform(psi, weight=num_taxa) )
The weight specifies how often the move will be applied either on average per iteration or relative to all other moves. Have a look at the Introduction to Markov chain Monte Carlo (MCMC) Sampling for more details about moves and MCMC strategies.
Molecular Clock
Additionally, in the case of time-calibrated trees, we need to add a molecular clock rate parameter. For example, we know from empirical estimates that the molecular clock rate is about 0.01 (=1%) per million years per site. Nevertheless, we can estimate it here because we fixed the root age. We use a uniform prior on the log-transform clock rate. This specifies our lack of prior knowledge on the magnitude of the clock rate.
log_clock_rate ~ dnUniform(-6,1) moves.append( mvSlide(log_clock_rate, weight=2.0) ) clock_rate := 10^log_clock_rate
Instead, you could also fix the clock rate and estimate the root age. For more information on molecular clocks please read the Relaxed Clocks & Time Trees tutorial.
We have fully specified all of the parameters of our phylogenetic
model—the tree topology with branch lengths, and the substitution model
that describes how the sequence data evolved over the tree with branch
lengths. Collectively, these parameters comprise a distribution called
the phylogenetic continuous-time Markov chain, and we use the
dnPhyloCTMC
constructor function to create this node. This
distribution requires several input arguments:
tree
with branch lengths;Q
;type
of character data.Build the random variable for the character data (sequence alignment).
seq ~ dnPhyloCTMC(tree=psi, Q=Q, type="DNA")
Once the PhyloCTMC
model has been created, we can attach our sequence
data to the tip nodes in the tree.
seq.clamp(data)
Note that although we assume that our sequence data are random variables—they are realizations of our phylogenetic model—for the purposes of inference, we assume that the sequence data are “clamped” to their observed values. When this function is called, RevBayes sets each of the stochastic nodes representing the tips of the tree to the corresponding nucleotide sequence in the alignment. This essentially tells the program that we have observed data for the sequences at the tips.
Finally, we wrap the entire model in a single object to provide convenient access to the
DAG. To do this, we only need to give the model()
function a single
node. With this node, the model()
function can find all of the other
nodes by following the arrows in the graphical model:
mymodel = model(Q)
Now we have specified a simple phylogenetic analysis—each parameter of
the model will be estimated from every site in our alignment. If we
inspect the contents of mymodel
we can review all of the nodes in the
DAG:
mymodel
For our MCMC analysis, we need to set up a vector of monitors to
record the states of our Markov chain. The monitor functions are all
called mn\*
, where \*
is the wild-card representing the monitor type.
First, we will initialize the model monitor using the mnModel
function. This creates a new monitor variable that will output the
states for all model parameters when passed into a MCMC function.
monitors.append( mnModel(filename="output/primates_cytb_JC.log", printgen=10) )
The mnFile
monitor will record the states for only the parameters
passed in as arguments. We use this monitor to specify the output for
our sampled trees and branch lengths.
monitors.append( mnFile(filename="output/primates_cytb_JC.trees", printgen=10, psi) )
Finally, create a screen monitor that will report the states of
specified variables to the screen with mnScreen
:
monitors.append( mnScreen(printgen=100, TL) )
This monitor mostly helps us to see the progress of the MCMC run.
With a fully specified model, a set of monitors, and a set of moves, we
can now set up the MCMC algorithm that will sample parameter values in
proportion to their posterior probability. The mcmc()
function will
create our MCMC object:
mymcmc = mcmc(mymodel, monitors, moves)
Now, run the MCMC:
mymcmc.run(generations=20000)
When the analysis is complete, you will have the monitored files in your output directory.
Saving and restarting analyses
MCMC analyses can take a long time to converge, and it is usually difficult to predict how many generations will be needed to obtain results. In addition, many analyses are run on computer clusters with time limits, and so may be stopped by the cluster partway through. For all of these reasons, it is useful to save the state of the chain regularly through the analysis.
mymcmc.run(generations=100000000, checkpointInterval=100, checkpointFile="output/primates_cytb_JC.state")
The
checkpointInterval
andcheckpointFile
inputs specify respectively how often, and to which file, the chain should be saved. Three different files will be used for storing the state, with no extension and with extensions_mcmc
and_moves
. When multiple independent runs are specified, they will automatically be saved in separate files (with extensions_run_1
,_run_2
, etc.).Restarting the chain from a previous run is done by adding this line:
mymcmc.initializeFromCheckpoint("output/primates_cytb_JC.state")
before calling the function
mcmc.run()
. The file name should match what was given ascheckpointFile
when running the previous analysis. NB: Note that this line will create an error if the state file does not exist yet, and so should be commented out in the first run.The full MCMC block thus becomes:
mymcmc = mcmc(mymodel, monitors, moves, nruns=2, combine="mixed") mymcmc.initializeFromCheckpoint("output/primates_cytb_JC.state") #comment this out for the first run mymcmc.run(generations=100000000, checkpointInterval=100, checkpointFile="output/primates_cytb_JC.state")
Methods for visualizing the marginal densities of parameter values are not currently available in RevBayes itself. Thus, it is important to use programs like Tracer (Rambaut and Drummond 2011) to evaluate mixing and non-convergence.
Look at the file called output/primates_cytb_JC.log
in Tracer.
There you see the posterior distribution of the continuous parameters, e.g., the tree length variable TL
.
It is always important to carefully assess the MCMC samples for the various parameters in your analysis. You can read more about MCMC tuning and evaluating and improving mixing in the tutorials Introduction to Markov chain Monte Carlo (MCMC) Sampling.
We are interested in the phylogenetic relationship of the Tarsiers. Therefore, we need to summarize the trees sampled from the posterior distribution. RevBayes can summarize the sampled trees by reading in the tree-trace file:
treetrace = readTreeTrace("output/primates_cytb_JC.trees", treetype="non-clock")
The mapTree()
function will summarize the tree samples and write the
maximum a posteriori tree to file:
map_tree = mapTree(treetrace,"output/primates_cytb_JC_MAP.tree")
Look at the file called output/primates_cytb_JC_MAP.tree
in
FigTree
. We show it in .
Fill in the following table as you go through the tutorial.
Model | Lemuroidea | Lorisoidea | Platyrrhini | Catarrhini |
---|---|---|---|---|
Jukes-Cantor | ||||
HKY85 | ||||
F81 | ||||
GTR | ||||
GTR+Gamma | ||||
GTR+Gamma+I |
Note, you can query the posterior probability of a clade being monophyletic using the following command:
Lemuroidea <- clade("Cheirogaleus_major",
"Daubentonia_madagascariensis",
"Lemur_catta",
"Lepilemur_hubbardorum",
"Microcebus_murinus",
"Propithecus_coquereli",
"Varecia_variegata_variegata")
treetrace.cladeProbability( Lemuroidea )
Species | Family | Parvorder | Suborder |
---|---|---|---|
Aotus trivirgatus | Aotidae | Platyrrhini (NWM) | Haplorrhini |
Callicebus donacophilus | Pitheciidae | Platyrrhini (NWM) | Haplorrhini |
Cebus albifrons | Cebidae | Platyrrhini (NWM) | Haplorrhini |
Cheirogaleus major | Cheirogaleidae | Lemuroidea | Strepsirrhini |
Chlorocebus aethiops | Cercopithecoidea | Catarrhini | Haplorrhini |
Colobus guereza | Cercopithecoidea | Catarrhini | Haplorrhini |
Daubentonia madagascariensis | Daubentoniidae | Lemuroidea | Strepsirrhini |
Galago senegalensis | Galagidae | Lorisidae | Strepsirrhini |
Hylobates lar | Hylobatidea | Catarrhini | Haplorrhini |
Lemur catta | Lemuridae | Lemuroidea | Strepsirrhini |
Lepilemur hubbardorum | Lepilemuridae | Lemuroidea | Strepsirrhini |
Loris tardigradus | Lorisidae | Lorisidae | Strepsirrhini |
Macaca mulatta | Cercopithecoidea | Catarrhini | Haplorrhini |
Microcebus murinus | Cheirogaleidae | Lemuroidea | Strepsirrhini |
Nycticebus coucang | Lorisidae | Lorisidae | Strepsirrhini |
Otolemur crassicaudatus | Galagidae | Lorisidae | Strepsirrhini |
Pan paniscus | Hominoidea | Catarrhini | Haplorrhini |
Perodicticus potto | Lorisidae | Lorisidae | Strepsirrhini |
Propithecus coquereli | Indriidae | Lemuroidea | Strepsirrhini |
Saimiri sciureus | Cebidae | Platyrrhini (NWM) | Haplorrhini |
Tarsius syrichta | Tarsiidae | Tarsiiformes | Haplorrhini |
Varecia variegata variegata | Lemuridae | Lemuroidea | Strepsirrhini |
Setting up the Kimura 1980 (K80 or K2P) substitution model
The K80 model (AKA the K2P model) allows the rates of transition and transversion substitutions to be unequal (Kimura 1980). The parameter $\kappa$ describes the relative rate of transition to transversion substitutions (if $\kappa > 1$, transitions occur at a higher rate than transversions). The instantaneous-rate matrix for the K80 model is defined as:
Now, add the parameter $\kappa$ to the substitution model, and create a K80 rate matrix:
kappa ~ dnExp(1) moves.append( mvScale(kappa, weight=1.0) ) Q := fnK80(kappa)
The Jukes-Cantor model assumes that all substitution rates are equal, which also implies that the stationary frequencies of the four nucleotide bases are equal. These assumptions are not very biologically reasonable, so we might wish to consider a more realistic substitution model that relaxes some of these assumptions. For example, we might allow stationary frequencies, $\pi$, to be unequal, and allow rates of transition and transversion substitutions to differ, $\kappa$. This corresponds to the substitution model proposed by Hasegawa et al. (1985), which is specified with the following instantaneous-rate matrix:
where the diagonal ${\cdot}$ entries are equal to the negative sum of the elements in the corresponding row.
Use the file mcmc_JC.Rev
as a starting point for the HKY analysis.
Note that we are adding two new variables to our model. We can define a
variable pi
for the stationary frequencies that are drawn from a flat
Dirichlet distribution by
pi_prior <- v(1,1,1,1)
pi ~ dnDirichlet(pi_prior)
Since pi
is a stochastic variable, we need to specify a move to
propose updates to it. A good move on variables drawn from a Dirichlet
distribution is the mvBetaSimplex
. This move randomly takes an element
from the simplex, proposes a new value for it drawn from a Beta
distribution, and then rescales all values of the simplex to sum to 1
again.
moves.append( mvBetaSimplex(pi, weight=2) )
moves.append( mvDirichletSimplex(pi, weight=1) )
The second new variable is $\kappa$, which specifies the ratio of transition-transversion rates. The $\kappa$ parameter must be a positive-real number and a natural choice as the prior distribution is the lognormal distribution:
kappa ~ dnLognormal(0.0, 1.0)
Again, we need to specify a move for this new stochastic variable. A simple scaling move should do the job.
moves.append( mvScale(kappa) )
Finally, we need to create the HKY instantaneous-rate matrix using the
fnHKY
function:
Q := fnHKY(kappa,pi)
This should be all for the HKY model. Don’t forget to change the output file names, otherwise your old analyses files will be overwritten.
With as your guide, draw the probabilistic graphical model of the HKY model.
Download the file called mcmc_JC.Rev
and rename it
mcmc_HKY.Rev
. Save this file in a directory called scripts
located in the same
directory as your data
folder.
Modify mcmc_HKY.Rev
by including the
necessary parameters to specify the HKY substitution model. Be sure to change the output file names given to the monitors.
Run a MCMC analysis to estimate the posterior distribution under the HKY substitution model.
Are the resulting estimates of the base frequencies equal? If not,
how much do they differ? Are the estimated base frequencies similar
to the empirical base frequencies? The empirical base frequencies
are the frequencies of the characters in the alignment, which can be
computed with RevBayes by data.getEmpiricalBaseFrequencies()
.
Is the inferred rate of transition substitutions higher than the rate of transversion substitutions? If so, by how much?
Like the HKY model, the Felsenstein 1981 (F81) substitution model has unequal stationary frequencies, but it assumes equal transition-transversion rates (Felsenstein 1981). Can you set up the F81 model and run an analysis?
Complete the by reporting the posterior probabilities of phylogenetic relationships.
The HKY substitution model can accommodate unequal base frequencies and different rates of transition and transversion substitutions. Despite these extensions, the HKY model may still be too simplistic for many real datasets. Here, we extend the HKY model to specify the general time reversible (GTR) substitution model (Tavaré 1986), which allows all six exchangeability rates to differ ().
The instantaneous-rate matrix for the GTR substitution model is:
where the six exchangeability parameters, $r_{ij}$, specify the relative rates of change between states $i$ and $j$.
The GTR model requires that we define and specify a prior on the six
exchangeability rates, which we will describe using a flat Dirichlet
distribution. As we did previously for the Dirichlet prior on base
frequencies, we first define a constant node specifying the vector of
concentration-parameter values using the v()
function:
er_prior <- v(1,1,1,1,1,1)
This node defines the concentration-parameter values of the Dirichlet
prior distribution on the exchangeability rates. Now, we can create a
stochastic node for the exchangeability rates using the dnDirichlet()
function, which takes the vector of concentration-parameter values as an
argument and the ~
operator. Together, these create a stochastic node
named er
($\theta$ in ):
er ~ dnDirichlet(er_prior)
The Dirichlet distribution assigns probability densities to a group of parameters: e.g., those that measure proportions and must sum to 1. Here, we have specified a six-parameter Dirichlet prior, where each value describes one of the six relative rates of the GTR model: (1) $A\leftrightarrows C$; (2) $A\leftrightarrows G$; (3) $A\leftrightarrows T$; (4) $C\leftrightarrows G$; (5) $C\leftrightarrows T$; (6) $G\leftrightarrows T$. The input parameters of a Dirichlet distribution are called shape (or concentration) parameters. The expectation and variance for each variable are related to the sum of the shape parameters. The prior we specified above is a ‘flat’ or symmetric Dirichlet distribution; all of the shape parameters are equal (1,1,1,1,1,1). This describes a model that allows for equal rates of change between nucleotides, such that the expected rate for each is equal to $\frac{1}{6}$ (a).
We might also parameterize the Dirichlet distribution such that all of the shape parameters were equal to 100, which would also specify a prior with an expectation of equal exchangeability rates (b). However, by increasing the values of the shape parameters, er_prior <- v(100,100,100,100,100,100)
, the Dirichlet distribution will more strongly favor equal exchangeability rates; (i.e., a relatively informative prior).
Alternatively, we might consider an asymmetric Dirichlet parameterization that could reflect a strong prior belief that transition and transversion substitutions occur at different rates. For example, we might specify the prior density er_prior <- v(4,8,4,4,8,4)
. Under this model, the expected rate for transversions would be $\frac{4}{32}$ and that for transitions would be $\frac{8}{32}$, and there would be greater prior probability on sets of GTR rates that matched this configuration (c).
Yet another asymmetric prior could specify that each of the six GTR rates had a different value conforming to a Dirichlet(2,4,6,8,10,12). This would lead to a different prior probability density for each rate parameter (d). Without strong prior knowledge about the pattern of relative rates, however, we can better reflect our uncertainty by using a vague prior on the GTR rates. Notably, all patterns of relative rates have the same probability density under er_prior <- v(1,1,1,1,1,1)
.
For each stochastic node in our model, we must also specify a proposal mechanism if we wish to estimate that parameter. The Dirichlet prior on our parameter er
creates a simplex of values that sum to 1.
moves.append( mvBetaSimplex(er, weight=3) )
moves.append( mvDirichletSimplex(er, weight=1) )
We can use the same type of distribution as a prior on the 4 stationary frequencies ($\pi_A, \pi_C, \pi_G, \pi_T$) since these parameters also represent proportions. Specify a flat Dirichlet prior density on the base frequencies:
pi_prior <- v(1,1,1,1)
pi ~ dnDirichlet(pi_prior)
The node pi
represents the $\pi$ node in . Now add the simplex scale move on the stationary frequencies to the moves vector:
moves.append( mvBetaSimplex(pi, weight=2) )
moves.append( mvDirichletSimplex(pi, weight=1) )
We can finish setting up this part of the model by creating a deterministic node for the GTR instantaneous-rate matrix Q
. The fnGTR()
function takes a set of exchangeability rates and a set of base frequencies to compute the instantaneous-rate matrix used when calculating the likelihood of our model.
Q := fnGTR(er,pi)
Use one of your previous analysis files—either the mcmc_JC.Rev
or
mcmc_HKY.Rev
—to specify a GTR analysis in a new file called
mcmc_GTR.Rev
. Adapt the old analysis to be performed under the
GTR substitution model.
Run an MCMC analysis to estimate the posterior distribution.
Complete the table of the phylogenetic relationship of primates.
Members of the GTR family of substitution models assume that rates are homogeneous across sites, an assumption that is often violated by real data. We can accommodate variation in substitution rate among sites (ASRV) by adopting the discrete-gamma model (Yang 1994). This model assumes that the substitution rate at each site is a random variable that is described by a discretized gamma distribution, which has two parameters: the shape parameter, $\alpha$, and the rate parameter, $\beta$. In order that we can interpret the branch lengths as the expected number of substitutions per site, this model assumes that the mean site rate is equal to 1. The mean of the gamma is equal to $\alpha/\beta$, so a mean-one gamma is specified by setting the two parameters to be equal, $\alpha=\beta$. This means that we can fully describe the gamma distribution with the single shape parameter, $\alpha$. The degree of among-site substitution rate variation is inversely proportional to the value of the $\alpha$-shape parameter. As the value of the $\alpha$-shape increases, the gamma distribution increasingly resembles a normal distribution with decreasing variance, which therefore corresponds to decreasing levels of ASRV (). By contrast, when the value of the $\alpha$-shape parameter is $< 1$, the gamma distribution assumes a concave distribution that concentrates most of the prior density on low rates, but retains some prior mass on sites with very high rates, which therefore corresponds to high levels of ASRV (). Note that, when $\alpha = 1$, the gamma distribution collapses to an exponential distribution with a rate parameter equal to $\beta$.
We typically lack prior knowledge regarding the degree of ASRV for a given alignment. Accordingly, rather than specifying a precise value of $\alpha$, we can instead estimate the value of the $\alpha$-shape parameter from the data. This requires that we specify a diffuse (relatively ‘uninformative’) prior on the $\alpha$-shape parameter. For this analysis, we will use a uniform distribution between 0 and 10.
This approach for accommodating ASRV is another example of a hierarchical model (). That is, variation in substitution rates across sites is addressed by applying a site-specific rate multiplier to each of the $j$ sites, $r_j$. These rate-multipliers are drawn from a discrete, mean-one gamma distribution; the shape of this prior distribution (and the corresponding degree of ASRV) is governed by the $\alpha$-shape parameter. The $\alpha$-shape parameter, in turn, is treated as a lognormal distributed random variable. Finally, the shape of the lognormal prior is governed by the mean and standard deviation parameters, which are set to fixed values.
Then create a stochastic node called alpha
with a uniform prior distribution between 0.0 and $10$
(this represents the stochastic node for the $\alpha$-shape parameter in
):
alpha ~ dnUniform( 0.0, 10 )
The way the ASRV model is implemented involves discretizing the mean-one gamma distribution into a set number of rate categories, $k$. Thus, we can analytically marginalize over the uncertainty in the rate at each site. The likelihood of each site is averaged over the $k$ rate categories, where the rate multiplier is the mean (or median) of each of the discrete $k$ categories. To specify this, we need a deterministic node that is a vector that will hold the set of $k$ rates drawn from the gamma distribution with $k$ rate categories. The fnDiscretizeGamma()
function returns this deterministic node and takes three arguments: the shape and rate of the gamma distribution and the number of categories. Since we want to discretize a mean-one gamma distribution, we can pass in alpha
for both the shape and rate.
Initialize the sr
deterministic node vector using the fnDiscretizeGamma()
function with 4
bins:
sr := fnDiscretizeGamma( alpha, alpha, 4 )
Note that here, by convention, we set $k = 4$. The random variable that controls the rate variation is the stochastic node alpha
. We will apply a simple scale move to this parameter.
moves.append( mvScale(alpha, weight=2.0) )
Remember that you need to call the PhyloCTMC
constructor to include the new site-rate parameter:
seq ~ dnPhyloCTMC(tree=psi, Q=Q, siteRates=sr, type="DNA")
Modify the previous GTR analysis to specify the GTR+Gamma model. Run an MCMC simulation to estimate the posterior distribution.
Is there an impact on the estimated phylogeny compared with the previous analyses? Look at the MAP tree and the posterior probabilities of the clades.
Complete the table of the phylogenetic relationship of primates.
All of the substitution models described so far assume that the sequence data are potentially variable. That is, we assume that the sequence data are random variables; specifically, we assume that they are realizations of the specified PhyloCTMC
distribution. However, some sites may not be free to vary—when the substitution rate of a site is zero, it is said to be invariable. Invariable sites are often confused with invariant sites—when each species exhibits the same state, it is said to be invariant. The concepts are related but distinct. If a site is truly invariable, it will necessarily give rise to an invariant site pattern, as such sites will always have a zero substitution rate. However, an invariant site pattern may be achieved via multiple substitutions that happen to end in the same state for every species.
Here we describe an extension to our phylogenetic model to accommodate invariable sites. Under the invariable-sites model (Hasegawa et al. 1985), each site is invariable with probability p_inv
, and variable with probability $1-$p_inv
.
First, let’s have a look at the data and see how many invariant sites we have:
data.getNumInvariantSites()
There seem to be a substantial number of invariant sites.
Now let’s specify the invariable-sites model in RevBayes. We need to specify the prior probability that a site is invariable. A Beta distribution is a common choice for parameters representing probabilities.
p_inv ~ dnBeta(1,1)
The Beta(1,1)
distribution is a flat prior distribution that specifies equal probability for all values between 0 and 1.
Then, as usual, we add a move to change this stochastic variable; we’ll use a simple sliding window move.
moves.append( mvSlide(p_inv) )
Finally, you need to call the PhyloCTMC
constructor to include the
new p_inv
parameter:
seq ~ dnPhyloCTMC(tree=psi, Q=Q, siteRates=sr, pInv=p_inv, type="DNA")
Extend the GTR model to account for invariable sites and run an analysis.
What is the estimated probability of invariable sites and how does it relate to the ratio of invariant sites to the total number of sites?
Extend the GTR+$\Gamma$ model to account for invariable sites and run an analysis.
What is the estimated probability of invariable sites now?
Complete the table of the phylogenetic relationship of primates.