Football Table RL

Reinforcement Learning Basics

The football table employs on-line value iteration, namely Greedy-GQ[math]\displaystyle{ (\lambda) }[/math] and Approximate-Q[math]\displaystyle{ (\lambda) }[/math]. This page does not explain Reinforcement learning theory, it just touches on the usage and implementation of the provided library, which can be applied to any learning problem (libvfa located on the SVN). Too get a basic understanding of Reinforcement Learning i suggest reading the book by Sutton & Barto . For a slightly more in-depth, hands-on, book on using RL with function approximation, i suggest the book by Lucian Busoniu (TU Delft) et al. , which is freely available as e-book from within the TU/e network. Unfortunately both books very different notations, here we use the notation from the former.

From here on out this section assumes familiarity with reinforcement learning and discusses how the provided libvfa library works and is used. Note, this can be used on any project provided the user provides transition samples correctly.

Value function approximation

For this project it was chosen to use a Gaussian Radial Basis Function Network(RBFs) to approximate the Q-function, a short explanation on the method can be found here in . Currently, this is the only method of function approximation available in the library, however other forms of linear parametric function approximation should be easy to incorporate (this requires to only change the membership function).

RBFs are a linear parametric function approximation, where the Q-function is estimated using:

[math]\displaystyle{ Q = \theta\cdot\phi(s,a)^{T} }[/math]

here [math]\displaystyle{ \phi(s,a)~(1 \times n) }[/math] denotes the so called feature vector, [math]\displaystyle{ \theta~(1 \times n) }[/math] denotes the parameter (or weight) vector and [math]\displaystyle{ n }[/math] denotes the number of nodes. The value of Q hence becomes a scalar, depended on the action and the state. During Reinforcement learning we are trying to estimate the vector [math]\displaystyle{ \theta }[/math]. A single member of a radial basis function is described like this (where the state is described by the vector [math]\displaystyle{ x }[/math]):

[math]\displaystyle{ \phi_i(x) = e^{\frac{||c_i-x||^2}{2\sigma_i^2}} }[/math]

The total feature vector has [math]\displaystyle{ n }[/math]-elements, each has a center [math]\displaystyle{ c_i\in S }[/math] and a width [math]\displaystyle{ \sigma_i }[/math]. A complete feature vector looks like this:

[math]\displaystyle{ \phi_i(x) = \left [\begin{array}{c}e^{\frac{||c_1-x||^2}{2\sigma_1^2}} \\ e{\frac{||c_2-x||^2}{2\sigma_2^2}} \\ ... \\ e{\frac{||c_n-x||^2}{2\sigma_n^2}}\end{array}\right ] }[/math]

Below, and example of a RBF network is shown. This particular example contains only three nodes and is 1-dimensional, with centers: [math]\displaystyle{ c = \left [\begin{array}{ccc} -x_{sat} & 0 & x_{sat}\end{array} \right ]^T }[/math]

Simple RBF network example

Note from the above picture the difference between normalized and `regular` RBFs. Normalization can achieve slightly higher accuracy, however it does add to the computational demands. Normalization will make sure [math]\displaystyle{ \sum \phi(x)_i = 1 }[/math], where ([math]\displaystyle{ x = \left [ \begin{array}{cccc} x_1 & x_2 & ... & x_m \end{array}\right ] }[/math] for an [math]\displaystyle{ m }[/math]-dimensional problem). Naturally this leads to increasingly lower valued elements of [math]\displaystyle{ \phi(x) }[/math] for a higher [math]\displaystyle{ m }[/math].

To counter this problem, yet still achieving the effect of normalization, we can normalize per dimension. This can be achieved with the knowledge that [math]\displaystyle{ e^{\frac{||c_1-x||^2}{2\sigma_1^2}} = e^{\frac{||c_1^1-x_1||}{2(\sigma_1^1)^2}} }[/math]

Formally, feature vector [math]\displaystyle{ \phi(s,a) }[/math], is depended on both the state and the action, creating one long vector that represents Q is its entirety (all combinations of actions and states). Basically allowing the feature vector have a different set of nodes, with different characteristics per action, changing the representation of the statespace per action. However, to make things more simple and comprehensible libvfa is implemented slighty different(still correctly).
Instead of creating one long vector, we store [math]\displaystyle{ \theta }[/math] matrix of [math]\displaystyle{ (n_a \times n) }[/math] ([math]\displaystyle{ n_a }[/math] denotes the number of actions). This still holds the same information, however they are now stored in seperate rows, making indexation easier. On top of that, we use the same feature vector for each action (same node distribution and width across the states-space) yielding [math]\displaystyle{ \phi(s) }[/math] instead of [math]\displaystyle{ \phi(s,a) }[/math].

The latter is a simplification, and keeps compact. In some cases could be better however to tailor the feature-vector to the subset of the state-space in which the action can occur (which could also allow higher precision with a lower amount of nodes). I.e. in some parts of the state space some actions will never be available at all, whilst others are available. Hence the elements in the feature vector representing this area of the state space are useless for the non-available actions. Furthermore, it could be so that a differnt level of detail is required per action. This could be easily added to libvfa, investigating it's use would be quite interesting.

Sparse Calculations

One of the nice things of designing/defining a RBF network yourself, is that it allows you to use the knowledge of the network itself to speed things up. The main advantage can be obtained from addressing only nodes in the network that have a significant impact on the value we obtained; we are using the fact that it is a local function approximation.

In libvfa, sparse calculations are executed whenever you call a function that ends with fast Fast. Also the traces are only implemented for the sparse calculations.

(to do - some renaming in library).

Library functions

In this section we explain how to use some of the important functions of libvfa. The best way too familiarize yourself is to read primitives_select.cpp. But here i present some basic explanation.

Initialize

Initialization is done using either the constructor or vfa::init.

int numberOfActions = 2;
int numberOfStates = 2;
double numberOfNodesPerState[2] = {3, 3};
double saturationPerState[2] = {1, 1};
double nodeWidthPerState[2] = {1, 1};
bool normalize = false;
bool varRate = false; //this does not work well

vfa EXAMPLE(numberOfActions, numberOfStates, numberOfNodesPerState, saturationPerState, nodeWidthPerState, normalize, varRate);


Or you can do this:

vfa EXAMPLE;


EXAMPLE.init(numberOfActions, numberOfStates, numberOfNodesPerState, saturationPerState, nodeWidthPerState, normalize, varRate);

The variables used for initialization in the previous example are explained below:

(int) numberOfActions

Total number of actions available to the decision maker (size only limited by memory).

(int) numberOfStates

Total number of state available to the decision maker (maximum currently is 8, expansion should be relatively simple (instructions in the code).

(double *)numberOfNodesPerState

Total number of nodes per state (above example code would yield ([math]\displaystyle{ 3 \times 3 }[/math]) nodes), equidistantly devided over the statespace.

(double *)saturationPerState

The (absolute) saturation per state, i.e. using 1 would yield nodescenters to be distributed between [math]\displaystyle{ -x_{sat}\leq c_i\leq x_{sat} }[/math]. (Nodes are always placed on the 'edge'([math]\displaystyle{ x_{sat} }[/math]) of the defined space

(double *)nodeWidthPerState

Width of the nodes, per state ([math]\displaystyle{ \sigma }[/math]). It is recommended to use (for state [math]\displaystyle{ i }[/math]):
[math]\displaystyle{ \sigma_i = \frac{x_{i,sat}}{n_{i,nodes}-1} }[/math].
This yields a width of half the distance in between the nodes.

(bool) normalize

Indicate whether you want to normalize the RBFs, this can be useful when using a small amount of nodes over a large interval (see figure)

(bool) varRate

Indicate if you want to use a variable learning rate, based previous on activation of nodes in the past. Does not work very well and is overly complicated.

Getting Values

If we want a single Q-value, we can use this:

int action = 0;
double state[2] = {0,0};
int width = 2; //Here we determine the number of neighbours we use


double value = EXAMPLE.getValueFast(action, state, width)


int width here describes how many surounding neigbouring nodes are use for approximation (per side, symmetrically). If we want the values of a couple of particalur actions

int nActions = 3; int actions[3] = {0,2,3};
double state[2] = {0,0};
int width = 2; //Here we determine the number of neighbours we use


fvec values = EXAMPLE.getValuesFast(state, actions, nActions, width)


If we want all, we can use getAllValuesFast. Using the last two we get a vector, which allows us to easily find the maximum:

uword maxQIndex  ; //uword is simular to int
double maxQ = values.max( maxQIndex); //Gives the maximum value and writes the index(in fvec values) to maxQIndex

Performing updates

To perform an in Q-learning update we need the [math]\displaystyle{ s,~a,~s_{t+1},~r_{t+1} }[/math]. Also currently we provide all the learning parameters as well ([math]\displaystyle{ \alpha, \beta, \gamma, \lambda, \epsilon }[/math]). You can choose either approximate-Q or Greedy-GQ to perform the update. For Greedy-GQ we use:

VFA.updateGQReallyFast(double * currentState, double * nextState, int action, double reward, double alpha, double beta, double gamma, double lambda , int width);

For approximate Q we use:

VFA.updateGQReallyFast(double * currentState, double * nextState, int action, double reward, double alpha, double gamma , int width);

Doing eligibility traces

Eligibility traces are done separately after a normal update, to perform such an update use:

VFA.updateGQLambda(double * traceState, int traceAction, double alpha,double beta,double gamma,double lambda , int width, int depth);

Here the int depth states how many steps back we are from the current state ([math]\displaystyle{ s_{t-depth} }[/math]). Similarly for approximate-Q we can use:

VFA.updateTDLambda(double * traceState, int traceAction, double alpha,double gamma,double lambda , int width, int depth);

So to perform an update on all previous states within the episode you need to loop back using a buffer. Here we have some example code, where we use phiBuf to break off the trace once an sub-optimal action was taken (if useWatkins is true).

for(int i = 1; i<traceDepth_; i++){


traceIndex = bufIndex - i;

/*Same episode && either (no Watkins || Watkins and we took an 'optimal' action)*/

if(eBuf(traceIndex) == eBuf(bufIndex) && (!useWatkins || useWatkins && phiBuf(traceIndex+1)!=0)){ //Do not break

}else{ break;}

for(int j = 0; j<nStates; j++){stateTrace[j] = csBuf(traceIndex, i);}

if(useGQ_){

VFA.updateGQLambda(stateTrace, aBuf(traceIndex), alpha_, beta_, gamma_, lambda_, epsilon_, 2, i);

}else if(useApproxQ_){

VFA.updateTDLambda(stateTrace, aBuf(traceIndex), alpha_,gamma_, lambda_, epsilon_, 2, i);

}

}