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Welcome to DYNAMAX!

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Dynamax is a library for probabilistic state space models (SSMs) written in JAX. It has code for inference (state estimation) and learning (parameter estimation) in a variety of SSMs, including:

  • Hidden Markov Models (HMMs)
  • Linear Gaussian State Space Models (aka Linear Dynamical Systems)
  • Nonlinear Gaussian State Space Models
  • Generalized Gaussian State Space Models (with non-Gaussian emission models)

The library consists of a set of core, functionally pure, low-level inference algorithms, as well as a set of model classes which provide a more user-friendly, object-oriented interface. It is compatible with other libraries in the JAX ecosystem, such as optax (used for estimating parameters using stochastic gradient descent), and Blackjax (used for computing the parameter posterior using Hamiltonian Monte Carlo (HMC) or sequential Monte Carlo (SMC)).

Documentation

For tutorials and API documentation, see: https://probml.github.io/dynamax/.

For an extension of dynamax that supports structural time series models, see https://github.com/probml/sts-jax.

For an illustration of how to use dynamax inside of bayeux to perform Bayesian inference for the parameters of an SSM, see https://jax-ml.github.io/bayeux/examples/dynamax_and_bayeux/.

Installation and Testing

To install the latest releast of dynamax from PyPi:

pip install dynamax                 # Install dynamax and core dependencies, or
pip install dynamax[notebooks]      # Install with demo notebook dependencies

To install the latest development branch:

pip install git+https://github.com/probml/dynamax.git

Finally, if you're a developer, you can install dynamax along with the test and documentation dependencies with:

git clone [email protected]:probml/dynamax.git
cd dynamax
pip install -e '.[dev]'

To run the tests:

pytest dynamax                         # Run all tests
pytest dynamax/hmm/inference_test.py   # Run a specific test
pytest -k lgssm                        # Run tests with lgssm in the name

What are state space models?

A state space model or SSM is a partially observed Markov model, in which the hidden state, $z_t$, evolves over time according to a Markov process, possibly conditional on external inputs / controls / covariates, $u_t$, and generates an observation, $y_t$. This is illustrated in the graphical model below.

The corresponding joint distribution has the following form (in dynamax, we restrict attention to discrete time systems):

$$p(y_{1:T}, z_{1:T} | u_{1:T}) = p(z_1 | u_1) p(y_1 | z_1, u_1) \prod_{t=1}^T p(z_t | z_{t-1}, u_t) p(y_t | z_t, u_t)$$

Here $p(z_t | z_{t-1}, u_t)$ is called the transition or dynamics model, and $p(y_t | z_{t}, u_t)$ is called the observation or emission model. In both cases, the inputs $u_t$ are optional; furthermore, the observation model may have auto-regressive dependencies, in which case we write $p(y_t | z_{t}, u_t, y_{1:t-1})$.

We assume that we see the observations $y_{1:T}$, and want to infer the hidden states, either using online filtering (i.e., computing $p(z_t|y_{1:t})$ ) or offline smoothing (i.e., computing $p(z_t|y_{1:T})$ ). We may also be interested in predicting future states, $p(z_{t+h}|y_{1:t})$, or future observations, $p(y_{t+h}|y_{1:t})$, where h is the forecast horizon. (Note that by using a hidden state to represent the past observations, the model can have "infinite" memory, unlike a standard auto-regressive model.) All of these computations can be done efficiently using our library, as we discuss below. In addition, we can estimate the parameters of the transition and emission models, as we discuss below.

More information can be found in these books:

Example usage

Dynamax includes classes for many kinds of SSM. You can use these models to simulate data, and you can fit the models using standard learning algorithms like expectation-maximization (EM) and stochastic gradient descent (SGD). Below we illustrate the high level (object-oriented) API for the case of an HMM with Gaussian emissions. (See this notebook for a runnable version of this code.)

import jax.numpy as jnp
import jax.random as jr
import matplotlib.pyplot as plt
from dynamax.hidden_markov_model import GaussianHMM

key1, key2, key3 = jr.split(jr.PRNGKey(0), 3)
num_states = 3
emission_dim = 2
num_timesteps = 1000

# Make a Gaussian HMM and sample data from it
hmm = GaussianHMM(num_states, emission_dim)
true_params, _ = hmm.initialize(key1)
true_states, emissions = hmm.sample(true_params, key2, num_timesteps)

# Make a new Gaussian HMM and fit it with EM
params, props = hmm.initialize(key3, method="kmeans", emissions=emissions)
params, lls = hmm.fit_em(params, props, emissions, num_iters=20)

# Plot the marginal log probs across EM iterations
plt.plot(lls)
plt.xlabel("EM iterations")
plt.ylabel("marginal log prob.")

# Use fitted model for posterior inference
post = hmm.smoother(params, emissions)
print(post.smoothed_probs.shape) # (1000, 3)

JAX allows you to easily vectorize these operations with vmap. For example, you can sample and fit to a batch of emissions as shown below.

from functools import partial
from jax import vmap

num_seq = 200
batch_true_states, batch_emissions = \
    vmap(partial(hmm.sample, true_params, num_timesteps=num_timesteps))(
        jr.split(key2, num_seq))
print(batch_true_states.shape, batch_emissions.shape) # (200,1000) and (200,1000,2)

# Make a new Gaussian HMM and fit it with EM
params, props = hmm.initialize(key3, method="kmeans", emissions=batch_emissions)
params, lls = hmm.fit_em(params, props, batch_emissions, num_iters=20)

These examples demonstrate the dynamax models, but we can also call the low-level inference code directly.

Contributing

Please see this page for details on how to contribute.

About

Core team: Peter Chang, Giles Harper-Donnelly, Aleyna Kara, Xinglong Li, Scott Linderman, Kevin Murphy.

Other contributors: Adrien Corenflos, Elizabeth DuPre, Gerardo Duran-Martin, Colin Schlager, Libby Zhang and other people listed here

MIT License. 2022