Marginalize Next-State Distribution
Problem Statement
Given a policy pi over actions at a state, and a transition matrix P where P[a][s'] is the probability of reaching next state s' when taking action a, compute the marginal next-state distribution under the policy:
Pπ(s′∣s)=∑a​π(a∣s)P(s′∣s,a)
Implement marginal_next_state(pi, P) returning a distribution over next states.
Example:
marginal_next_state([0.5, 0.5], [[1.0, 0.0], [0.0, 1.0]])
[0.5, 0.5]
- Initialize the next-state distribution vector to zeros, representing that no probability mass has been accumulated yet for any state.
- Process the first action with policy probability π(0)=0.5: multiply this weight by the transition row [1.0,0.0] to get [0.5,0.0], and add this to the accumulator, resulting in [0.5,0.0].
- Process the second action with policy probability π(1)=0.5: multiply this weight by the transition row [0.0,1.0] to get [0.0,0.5], and add this to the current accumulator [0.5,0.0].
- Sum the contributions from both actions to obtain the final marginal probabilities: 0.5+0.0=0.5 for the first state and 0.0+0.5=0.5 for the second state.
- The final output is [0.5, 0.5]
Constraints:
len(pi) == len(P)(one row per action); all rows same lengthS.- Each
P[a]sums to 1;pisums to 1. - Output length
S, sums to 1.
1. Background Knowledge
In a Markov Decision Process (MDP), the environment is described by states, actions, and a transition function P(s′∣s,a) that gives the probability of transitioning to state s′ from state s when taking action a. A policy π(a∣s) is a probability distribution over actions at each state, representing the agent's strategy. When the agent follows a stochastic policy, the exact next state is not determined by a single action but by a mixture of all possible actions, weighted by their selection probabilities.
The marginal next-state distribution Pπ(s′∣s) answers the question: "If I am in state s and follow policy π, what is the probability of ending up in each next state s′?" This is computed by summing over all actions, weighting each action's transition probability by the probability of choosing that action. This operation is fundamental in Bellman equations, where the value of a state under a policy depends on the expected value of next states, which in turn depends on this marginal distribution.
Mathematically, this is a weighted sum (or expectation) over the action space. If π is a row vector of shape (A,) and P is a matrix of shape (A,S′), the result is a row vector of shape (S′,) obtained by multiplying π with P. This is a standard matrix-vector multiplication in linear algebra, which is the computational backbone of many RL algorithms.
2. Algorithm Approach
The core approach is to compute the expectation of the next-state distribution over the action distribution. For each possible next state s′, you sum the product of the policy probability for each action a and the transition probability from a to s′.
In code, this translates to:
- Iterate over each action a.
- For each action, scale the entire row P[a] (which is a distribution over next states) by π[a].
- Accumulate these scaled distributions into a single result vector.
This is equivalent to performing a dot product between the policy vector and the transition matrix. If you are using NumPy, this can be done in a single vectorized operation. If you are implementing it from scratch, you will use nested loops or a reduction operation.
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