Code should execute sequentially if run in a Jupyter notebook

- See the set up page to install Jupyter, Julia (0.6+) and all necessary libraries
- Please direct feedback to contact@quantecon.org or the discourse forum

# A Stochastic Optimal Growth Model¶

## Overview¶

In this lecture we’re going to study a simple optimal growth model with one agent

The model is a version of the standard one sector infinite horizon growth model studied in

The technique we use to solve the model is dynamic programming

Our treatment of dynamic programming follows on from earlier treatments in our lectures on shortest paths and job search

We’ll discuss some of the technical details of dynamic programming as we go along

## The Model¶

Consider an agent who owns an amount \(y_t \in \mathbb R_+ := [0, \infty)\) of a consumption good at time \(t\)

This output can either be consumed or invested

When the good is invested it is transformed one-for-one into capital

The resulting capital stock, denoted here by \(k_{t+1}\), will then be used for production

Production is stochastic, in that it also depends on a shock \(\xi_{t+1}\) realized at the end of the current period

Next period output is

where \(f \colon \RR_+ \to \RR_+\) is called the production function

The resource constraint is

and all variables are required to be nonnegative

### Assumptions and Comments¶

In what follows,

- The sequence \(\{\xi_t\}\) is assumed to be IID
- The common distribution of each \(\xi_t\) will be denoted \(\phi\)
- The production function \(f\) is assumed to be increasing and continuous
- Depreciation of capital is not made explicit but can be incorporated into the production function

While many other treatments of the stochastic growth model use \(k_t\) as the state variable, we will use \(y_t\)

This will allow us to treat a stochastic model while maintaining only one state variable

We consider alternative states and timing specifications in some of our other lectures

### Optimization¶

Taking \(y_0\) as given, the agent wishes to maximize

subject to

where

- \(u\) is a bounded, continuous and strictly increasing utility function and
- \(\beta \in (0, 1)\) is a discount factor

In (3) we are assuming that the resource constraint (1) holds with equality — which is reasonable because \(u\) is strictly increasing and no output will be wasted at the optimum

In summary, the agent’s aim is to select a path \(c_0, c_1, c_2, \ldots\) for consumption that is

- nonnegative,
- feasible in the sense of (1),
- optimal, in the sense that it maximizes (2) relative to all other feasible consumption sequences, and
*adapted*, in the sense that the action \(c_t\) depends only on observable outcomes, not future outcomes such as \(\xi_{t+1}\)

In the present context

- \(y_t\) is called the
*state*variable — it summarizes the “state of the world” at the start of each period - \(c_t\) is called the
*control*variable — a value chosen by the agent each period after observing the state

### The Policy Function Approach¶

One way to think about solving this problem is to look for the best **policy function**

A policy function is a map from past and present observables into current action

We’ll be particularly interested in **Markov policies**, which are maps from the current state \(y_t\) into a current action \(c_t\)

For dynamic programming problems such as this one (in fact for any Markov decision process), the optimal policy is always a Markov policy

In other words, the current state \(y_t\) provides a sufficient statistic for the history in terms of making an optimal decision today

This is quite intuitive but if you wish you can find proofs in texts such as [SLP89] (section 4.1)

Hereafter we focus on finding the best Markov policy

In our context, a Markov policy is a function \(\sigma \colon \mathbb R_+ \to \mathbb R_+\), with the understanding that states are mapped to actions via

In what follows, we will call \(\sigma\) a *feasible consumption policy* if it satisfies

In other words, a feasible consumption policy is a Markov policy that respects the resource constraint

The set of all feasible consumption policies will be denoted by \(\Sigma\)

Each \(\sigma \in \Sigma\) determines a continuous state Markov process \(\{y_t\}\) for output via

This is the time path for output when we choose and stick with the policy \(\sigma\)

We insert this process into the objective function to get

This is the total expected present value of following policy \(\sigma\) forever, given initial income \(y_0\)

The aim is to select a policy that makes this number as large as possible

The next section covers these ideas more formally

### Optimality¶

The **policy value function** \(v_{\sigma}\) associated with a given policy \(\sigma\) is the mapping defined by

when \(\{y_t\}\) is given by (5) with \(y_0 = y\)

In other words, it is the lifetime value of following policy \(\sigma\) starting at initial condition \(y\)

The **value function** is then defined as

The value function gives the maximal value that can be obtained from state \(y\), after considering all feasible policies

A policy \(\sigma \in \Sigma\) is called **optimal** if it attains the supremum in (8) for all \(y \in \mathbb R_+\)

### The Bellman Equation¶

With our assumptions on utility and production function, the value function as defined in (8) also satisfies a **Bellman equation**

For this problem, the Bellman equation takes the form

This is a *functional equation in* \(w\)

The term \(\int w(f(y - c) z) \phi(dz)\) can be understood as the expected next period value when

- \(w\) is used to measure value
- the state is \(y\)
- consumption is set to \(c\)

As shown in EDTC, theorem 10.1.11 and a range of other texts

The value function\(v^*\)satisfies the Bellman equation

In other words, (9) holds when \(w=v^*\)

The intuition is that maximal value from a given state can be obtained by optimally trading off

- current reward from a given action, vs
- expected discounted future value of the state resulting from that action

The Bellman equation is important because it gives us more information about the value function

It also suggests a way of computing the value function, which we discuss below

### Greedy policies¶

The primary importance of the value function is that we can use it to compute optimal policies

The details are as follows

Given a continuous function \(w\) on \(\mathbb R_+\), we say that \(\sigma \in \Sigma\) is \(w\)-**greedy** if \(\sigma(y)\) is a solution to

for every \(y \in \mathbb R_+\)

In other words, \(\sigma \in \Sigma\) is \(w\)-greedy if it optimally trades off current and future rewards when \(w\) is taken to be the value function

In our setting, we have the following key result

A feasible consumption policy is optimal if and only if it is\(v^*\)-greedy

The intuition is similar to the intuition for the Bellman equation, which was provided after (9)

See, for example, theorem 10.1.11 of EDTC

Hence, once we have a good approximation to \(v^*\), we can compute the (approximately) optimal policy by computing the corresponding greedy policy

The advantage is that we are now solving a much lower dimensional optimization problem

### The Bellman Operator¶

How, then, should we compute the value function?

One way is to use the so-called **Bellman operator**

(An operator is a map that sends functions into functions)

The Bellman operator is denoted by \(T\) and defined by

In other words, \(T\) sends the function \(w\) into the new function \(Tw\) defined (11)

By construction, the set of solutions to the Bellman equation (9) *exactly coincides with* the set of fixed points of \(T\)

For example, if \(Tw = w\), then, for any \(y \geq 0\),

which says precisely that \(w\) is a solution to the Bellman equation

It follows that \(v^*\) is a fixed point of \(T\)

### Review of Theoretical Results¶

One can also show that \(T\) is a contraction mapping on the set of continuous bounded functions on \(\mathbb R_+\) under the supremum distance

See EDTC, lemma 10.1.18

Hence it has exactly one fixed point in this set, which we know is equal to the value function

It follows that

- The value function \(v^*\) is bounded and continuous
- Starting from any bounded and continuous \(w\), the sequence \(w, Tw, T^2 w, \ldots\) generated by iteratively applying \(T\) converges uniformly to \(v^*\)

This iterative method is called **value function iteration**

We also know that a feasible policy is optimal if and only if it is \(v^*\)-greedy

It’s not too hard to show that a \(v^*\)-greedy policy exists (see EDTC, theorem 10.1.11 if you get stuck)

Hence at least one optimal policy exists

Our problem now is how to compute it

### Unbounded Utility¶

The results stated above assume that the utility function is bounded

In practice economists often work with unbounded utility functions — and so will we

In the unbounded setting, various optimality theories exist

Unfortunately, they tend to be case specific, as opposed to valid for a large range of applications

Nevertheless, their main conclusions are usually in line with those stated for the bounded case just above (as long as we drop the word “bounded”)

Consult, for example, section 12.2 of EDTC, [Kam12] or [MdRV10]

## Computation¶

Let’s now look at computing the value function and the optimal policy

### Fitted Value Iteration¶

The first step is to compute the value function by value function iteration

In theory, the algorithm is as follows

- Begin with a function \(w\) — an initial condition
- Solving (11), obtain the function \(T w\)
- Unless some stopping condition is satisfied, set \(w = Tw\) and go to step 2

This generates the sequence \(w, Tw, T^2 w, \ldots\)

However, there is a problem we must confront before we implement this procedure: The iterates can neither be calculated exactly nor stored on a computer

To see the issue, consider (11)

Even if \(w\) is a known function, unless \(Tw\) can be shown to have some special structure, the only way to store it is to record the value \(Tw(y)\) for every \(y \in \mathbb R_+\)

Clearly this is impossible

What we will do instead is use **fitted value function iteration**

The procedure is to record the value of the function \(Tw\) at only finitely many “grid” points \(y_1 < y_2 < \cdots < y_I\) and reconstruct it from this information when required

More precisely, the algorithm will be

- Begin with an array of values \(\{ w_1, \ldots, w_I \}\) representing the values of some initial function \(w\) on the grid points \(\{ y_1, \ldots, y_I \}\)
- Build a function \(\hat w\) on the state space \(\mathbb R_+\) by interpolation or approximation, based on these data points
- Obtain and record the value \(T \hat w(y_i)\) on each grid point \(y_i\) by repeatedly solving (11)
- Unless some stopping condition is satisfied, set \(\{ w_1, \ldots, w_I \} = \{ T \hat w(y_1), \ldots, T \hat w(y_I) \}\) and go to step 2

How should we go about step 2?

This is a problem of function approximation, and there are many ways to approach it

What’s important here is that the function approximation scheme must not only produce a good approximation to \(Tw\), but also combine well with the broader iteration algorithm described above

One good choice from both respects is continuous piecewise linear interpolation (see `this paper`

for further discussion)

The next figure illustrates piecewise linear interpolation of an arbitrary function on grid points \(0, 0.2, 0.4, 0.6, 0.8, 1\)

Another advantage of piecewise linear interpolation is that it preserves useful shape properties such as monotonicity and concavity / convexity

### The Bellman Operator¶

Here’s a function that implements the Bellman operator using linear interpolation

```
#=
@authors : Spencer Lyon, John Stachurski
=#
using QuantEcon
using Optim
"""
The approximate Bellman operator, which computes and returns the
updated value function Tw on the grid points. An array to store
the new set of values Tw is optionally supplied (to avoid having to
allocate new arrays at each iteration). If supplied, any existing data in
Tw will be overwritten.
#### Arguments
`w` : Vector
The value of the input function on different grid points
`grid` : Vector
The set of grid points
`β` : AbstractFloat
The discount factor
`u` : Function
The utility function
`f` : Function
The production function
`shocks` : Vector
An array of draws from the shock, for Monte Carlo integration (to
compute expectations).
`Tw` : Vector, optional (default=similar(w))
Array to write output values to
`compute_policy` : Bool, optional (default=false)
Whether or not to compute policy function
"""
function bellman_operator(w::Vector,
grid::Vector,
β::AbstractFloat,
u::Function,
f::Function,
shocks::Vector,
Tw::Vector = similar(w);
compute_policy::Bool = false)
# === Apply linear interpolation to w === #
w_func = LinInterp(grid, w)
if compute_policy
σ = similar(w)
end
# == set Tw[i] = max_c { u(c) + β E w(f(y - c) z)} == #
for (i, y) in enumerate(grid)
objective(c) = - u(c) - β * mean(w_func.(f(y - c) .* shocks))
res = optimize(objective, 1e-10, y)
if compute_policy
σ[i] = res.minimizer
end
Tw[i] = - res.minimum
end
if compute_policy
return Tw, σ
else
return Tw
end
end
```

The arguments to bellman_operator are described in the docstring to the function

Notice that the expectation in (11) is computed via Monte Carlo, using the approximation

where \(\{\xi_i\}_{i=1}^n\) are IID draws from \(\phi\)

Monte Carlo is not always the most efficient way to compute integrals numerically but it does have some theoretical advantages in the present setting

(For example, it preserves the contraction mapping property of the Bellman operator — see, e.g., [PalS13])

### An Example¶

Let’s test out our operator when

- \(f(k) = k^{\alpha}\)
- \(u(c) = \ln c\)
- \(\phi\) is the distribution of \(\exp(\mu + \sigma \zeta)\) when \(\zeta\) is standard normal

As is well-known (see [LS12], section 3.1.2), for this particular problem an exact analytical solution is available, with

The optimal consumption policy is

Let’s code this up now so we can test against it below

```
α = 0.4
β = 0.96
μ = 0
s = 0.1
c1 = log(1 - α * β) / (1 - β)
c2 = (μ + α * log(α * β)) / (1 - α)
c3 = 1 / (1 - β)
c4 = 1 / (1 - α * β)
# Utility
u(c) = log(c)
u_prime(c) = 1 / c
# Deterministic part of production function
f(k) = k^α
f_prime(k) = α * k^(α - 1)
# True optimal policy
c_star(y) = (1 - α * β) * y
# True value function
v_star(y) = c1 + c2 * (c3 - c4) + c4 * log(y)
```

### A First Test¶

To test our code, we want to see if we can replicate the analytical solution numerically, using fitted value function iteration

We need a grid and some shock draws for Monte Carlo integration

```
grid_max = 4 # Largest grid point
grid_size = 200 # Number of grid points
shock_size = 250 # Number of shock draws in Monte Carlo integral
grid_y = collect(linspace(1e-5, grid_max, grid_size))
shocks = exp.(μ + s * randn(shock_size))
```

Now let’s do some tests

In the code shown below and all other code, we assume that you’ve already run the code above, as well as

```
using PyPlot
```

As one preliminary test, let’s see what happens when we apply our Bellman operator to the exact solution \(v^*\)

In theory, the resulting function should again be \(v^*\)

In practice we expect some small numerical error

```
w = bellman_operator(v_star.(grid_y),
grid_y,
β,
log,
k -> k^α,
shocks)
fig, ax = subplots(figsize=(9, 5))
ax[:set_ylim](-35, -24)
ax[:plot](grid_y, w, lw=2, alpha=0.6, label=L"$Tv^*$")
ax[:plot](grid_y, v_star.(grid_y), lw=2, alpha=0.6, label=L"$v^*$")
ax[:legend](loc="lower right")
show()
```

Here’s the output:

The two functions are essentially indistinguishable, so we are off to a good start

Now let’s have a look at iterating with the Bellman operator, starting off from an arbitrary initial condition

The initial condition we’ll start with is \(w(y) = 5 \ln (y)\)

```
w = 5 * log.(grid_y) # An initial condition -- fairly arbitrary
n = 35
fig, ax = subplots(figsize=(9, 6))
ax[:set_ylim](-50, 10)
ax[:set_xlim](minimum(grid_y), maximum(grid_y))
lb = "initial condition"
jet = ColorMap("jet")
ax[:plot](grid_y, w, color=jet(0), lw=2, alpha=0.6, label=lb)
for i in 1:n
w = bellman_operator(w,
grid_y,
β,
log,
k -> k^α,
shocks)
ax[:plot](grid_y, w, color=jet(i / n), lw=2, alpha=0.6)
end
lb = "true value function"
ax[:plot](grid_y, v_star.(grid_y), "k-", lw=2, alpha=0.8, label=lb)
ax[:legend](loc="lower right")
show()
```

The figure shows

- the first 36 functions generated by the fitted value function iteration algorithm, with hotter colors given to higher iterates
- the true value function \(v^*\) drawn in black

The sequence of iterates converges towards \(v^*\)

We are clearly getting closer

We can write a function that iterates until the difference is below a particular tolerance level

```
function solve_optgrowth(initial_w;
tol::AbstractFloat=1e-6,
max_iter::Integer=500)
w = initial_w # Set initial condition
error = tol + 1
i = 0
# == Create storage array for bellman_operator. Reduces memory
# allocation and speeds code up == #
Tw = similar(grid_y)
# Iterate to find solution
while (error > tol) && (i < max_iter)
w_new = bellman_operator(w,
grid_y,
β,
log,
k -> k^α,
shocks)
error = maximum(abs, w_new - w)
w = w_new
i += 1
end
return w
end
```

We can check our result by plotting it against the true value

```
initial_w = 5 * log.(grid_y)
v_star_approx = solve_optgrowth(initial_w)
fig, ax = subplots(figsize=(9, 5))
ax[:set_ylim](-35, -24)
ax[:plot](grid_y, v_star_approx, lw=2, alpha=0.6, label="approximate value function")
ax[:plot](grid_y, v_star.(grid_y), lw=2, alpha=0.6, label="true value function")
ax[:legend](loc="lower right")
show()
```

Alternatively, we can use QuantEcon‘s compute_fixed_point function to converge to \(v^*\)

```
import QuantEcon: compute_fixed_point
Tw = similar(grid_y)
initial_w = 5 * log.(grid_y)
bellman_operator(w) = bellman_operator(w,
grid_y,
β,
log,
k -> k^α,
shocks)
v_star_approx = compute_fixed_point(bellman_operator,
initial_w,
max_iter=500,
verbose=2,
print_skip=10,
err_tol=1e-5)
```

Here’s the output

```
Compute iterate 10 with error 0.709153897728406
Compute iterate 20 with error 0.47095844432889145
Compute iterate 30 with error 0.3131085083453158
Compute iterate 40 with error 0.20816475495214704
Compute iterate 50 with error 0.13839472275577336
Compute iterate 60 with error 0.09200932833702069
Compute iterate 70 with error 0.061170804294146564
Compute iterate 80 with error 0.04066834706496181
Compute iterate 90 with error 0.027037644380378367
Compute iterate 100 with error 0.01797550838462314
Compute iterate 110 with error 0.011950704623018282
Compute iterate 120 with error 0.00794521845620011
Compute iterate 130 with error 0.005282240529794535
Compute iterate 140 with error 0.003511805895449527
Compute iterate 150 with error 0.0023347631704915273
Compute iterate 160 with error 0.001552226753144481
Compute iterate 170 with error 0.0010319710041208907
Compute iterate 180 with error 0.0006860880028760619
Compute iterate 190 with error 0.0004561336956570017
Compute iterate 200 with error 0.00030325256715002524
Compute iterate 210 with error 0.00020161220411551994
Compute iterate 220 with error 0.0001340383727708172
Compute iterate 230 with error 8.911308481529545e-5
Compute iterate 240 with error 5.924528747414115e-5
Compute iterate 250 with error 3.9388200878676116e-5
Compute iterate 260 with error 2.6186561168373146e-5
Compute iterate 270 with error 1.7409680953761608e-5
Compute iterate 280 with error 1.1574523867352582e-5
Converged in 284 steps
```

Let’s have a look at the result

```
fig, ax = subplots(figsize=(9, 5))
ax[:set_ylim](-35, -24)
ax[:plot](grid_y, v_star_approx, lw=2, alpha=0.6, label="approximate value function")
ax[:plot](grid_y, v_star.(grid_y), lw=2, alpha=0.6, label="true value function")
ax[:legend](loc="lower right")
show()
```

The figure shows that we are pretty much on the money

### The Policy Function¶

To compute an approximate optimal policy, we take the approximate value function we just calculated and then compute the corresponding greedy policy

The next figure compares the result to the exact solution, which, as mentioned above, is \(\sigma(y) = (1 - \alpha \beta) y\)

```
Tw, σ = bellman_operator(v_star_approx,
grid_y,
β,
log,
k -> k^α,
shocks;
compute_policy=true)
cstar = (1 - α * β) * grid_y
fig, ax = subplots(figsize=(9, 5))
ax[:plot](grid_y, σ, lw=2, alpha=0.6, label="approximate policy function")
ax[:plot](grid_y, cstar, lw=2, alpha=0.6, label="true policy function")
ax[:legend](loc="lower right")
show()
```

The figure shows that we’ve done a good job in this instance of approximating the true policy

## Exercises¶

### Exercise 1¶

Once an optimal consumption policy \(\sigma\) is given, the dynamics for the capital stock follows (5)

The next figure shows a simulation of 100 elements of this sequence for three different discount factors (and hence three different policies)

In each sequence, the initial condition is \(y_0 = 0.1\)

The discount factors are `discount_factors = (0.8, 0.9, 0.98)`

We have also dialed down the shocks a bit

```
s = 0.05
shocks = exp.(μ + s * randn(shock_size))
```

Otherwise, the parameters and primitives are the same as the log linear model discussed earlier in the lecture

Notice that more patient agents typically have higher wealth

Replicate the figure modulo randomness

## Solutions¶

### Solution to Exercise 1¶

Here’s our solution, which assumes you’ve executed the code in the lecture

```
"""
Compute a time series given consumption policy σ.
"""
function simulate_og(σ, y0 = 0.1, ts_length=100)
y = Array{Float64}(ts_length)
ξ = randn(ts_length-1)
y[1] = y0
for t in 1:(ts_length-1)
y[t+1] = (y[t] - σ(y[t]))^α * exp(μ + s * ξ[t])
end
return y
end
fig, ax = subplots(figsize=(9, 6))
for β in (0.9, 0.94, 0.98)
Tw = similar(grid_y)
initial_w = 5 * log.(grid_y)
v_star_approx = compute_fixed_point(bellman_operator,
initial_w,
max_iter=50,
verbose=0,
print_skip=10,
err_tol=1e-5)
Tw, σ = bellman_operator(v_star_approx,
grid_y,
β,
log,
k -> k^α,
shocks,
compute_policy=true)
σ_func = LinInterp(grid_y, σ)
y = simulate_og(σ_func)
ax[:plot](y, lw=2, alpha=0.6, label="β = $β" )
end
ax[:legend](loc="lower right")
show()
```