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A two-mode linear-Gaussian Rao–Blackwellized filter

Example

Let Z0 be uniform on {0,1} and let Z1=Z0. Conditional on Z0=z, take U0∼N(0,1) and U1=azU0+ξ1,Y1=U1+ε1, where a0=0, a1=1, and ξ1,ε1 are independent N(0,1) variables, independent of U0. Observe Y1=0. The exact conditional posterior is the two-component mixture L(U1,Z1∣Y1=0)=33+2N(0,1/2)⊗δ0+23+2N(0,2/3)⊗δ1. These are the component moments and mode weights that the Rao–Blackwellized filter represents analytically; a finite particle cloud still approximates the mode mixture.

Facts & Assumptions

Given: The finite model and observation in the Example.

[F1]

A conditionally linear-Gaussian state-space model has a Markov nonlinear component and a linear-Gaussian component conditional on its nonlinear path. Conditionally linear-Gaussian state-space model

[A1]

AC is inherited from the Gaussian-law and finite-horizon conditional-kernel conventions. The Axiom of Choice

[F2]

Conditional on a nonlinear path, the Kalman filter gives the exact Gaussian state filter and the marginal observation density. The Kalman filter is exact conditional on a nonlinear path

[F3]

The Rao–Blackwellized particle filter retains those conditional Gaussian components and weights nonlinear paths by their conditional observation densities. Rao–Blackwellized particle filter

[F4]

A positive-definite one-dimensional Gaussian covariance gives density (2πS)−1/2exp⁡(−v2/(2S)). A positive-definite multivariate normal law has its Gaussian density

Verification

Given: Z0∼Bernoulli⁡(1/2), Z1=Z0, the conditional Gaussian model stated in the Example, and Y1=0.

1.1A1F1F2given

The state and observation noises are independent centered Gaussians, the conditional initial covariance is 1, the process covariance is 1, and the observation covariance is 1>0. Thus the model satisfies [F1] and the exact conditional Kalman interface [F2].

1.2F2givenalgebra

Conditional on Z1=z, prediction gives m1∣0=0 and P1∣0=az2+1. Hence P1∣0=1 for z=0 and P1∣0=2 for z=1. The innovation is zero and the innovation variances are S0=2 and S1=3.

2.1A1F1F2F4step 1.2algebra

By [F4], the two conditional observation densities at zero are ℓ0=(4π)−1/2 and ℓ1=(6π)−1/2. Multiplying by the equal prior masses and normalizing gives P(Z1=0∣Y1=0)=3/(3+2) and P(Z1=1∣Y1=0)=2/(3+2).

3.1A1F2F3step 2.1algebra∎

The Kalman covariance update is P1∣1=P1∣0R/(P1∣0+R) here, so the two conditional posterior variances are 1/2 and 2/3; both conditional means remain zero. Mixing these exact conditional Gaussians with the mode probabilities from step 2.1 gives the displayed posterior. The filter in [F3] uses these same per-mode likelihoods and Gaussian components; only its finite particle approximation to the mode weights is random.

Depends on

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