Proceedings of the Particle Physics and Early Universe Conference (PPEUC).
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# 3 Parameter information and the solution to our problems

Suppose we have found the maximum likelihood solutions for each parameter, , then the likelihood function can be approximated by another multivariate Gaussian about this point;

where is the distance to the maximum in parameter space and the parameter covariance matrix is given by the inverse of , the Fisher Information matrix;

(if the means of the data are dependent on the parameters, this is modified -- see Tegmark, Taylor & Heavens (1997)). The far right hand side expression can be calculated for Gaussian distributed data sets (ie equation 1), where is the slope of the log of the data covariance matrix in parameter space.

By considering the Fisher matrix as the information content contained in the data set about each parameter, we see that the solution to our problem is to reduce the data set without changing the parameter information content. Hence to solve the problem of efficiency, we need to make a linear transformation of the data set

where is a matrix where , and so may be a smaller data set than . If the transformation is not invertible and some information about the data has been lost. To ensure that the lost information does not affect the parameter estimation (requirement (a)), we also require

where is the transformed Fisher matrix. In order to avoid learning the unhelpful fact that no data is an optimal solution, we add in the constraint that data exists. Since we have the freedom to transform the data covariance matrix, we add the constraint , where is the unit matrix and is a Lagrangian multiplier.

It can be shown (Tegmark, Taylor & Heavens (1997)) that this is equivalent to a generalised Karhunen-Loève eigenvalue problem, which has a unique solution for each parameter. These solutions have the property that

where are the eigenvalues of the transformed data set and the inverse errors associated with each eigenmode of the new data set.

The new, compressed data set, , can now be ordered by decreasing eigenvalue, so that the first eigenmode contains the most information about the desired parameter, the second slightly less information, and so on. The total error on the parameter is then simply given by the inverse of the Fisher matrix

We are now free to choose how many eigenmodes to include in the likelihood analysis. A compression of 10 will lead to a time saving of . However this is only exact if we know the true value of the parameters used to calculate . But if we are near the maximum likelihood solution then we can iterate towards the exact solution.

This procedure is optimal for all parameters -- linear and nonlinear -- in the model. In the special case of linear parameters that are just proportional to the signal part of the data covariance matrix (for example the amplitude of , if the data are the ), the eigenmodes reduce to signal-to-noise eigenmodes (Bond (1994)). Hence our eigenmodes are more general than signal-to-noise eigenmodes. Furthermore, as our eigenmodes satisfy the condition that the Fisher matrix is a maximum, they are the optimal ones for data compression. Any other choice, including signal-to-noise eigenmodes, would give a higher variance.

In Figure 1 we plot the uncertainty on 3 parameters for COBE-type data, the quadrupole, , the spectral index of scalar perturbations, and the re-ionization optical depth, .

Figure 1:  The 3 heavy lines show the error bars on 3 CMB parameters as a function of the number of modes used. Each set of modes has been optimised for the parameter in question. Note that approximately 400 modes are all that is required to get virtually all the information from the entire 4016 cut COBE dataset. The thin lines show the conditional errors from the SVD procedure outlined in section 5: virtually all the (conditional) information on all 3 parameters is obtained from the best 500 SVD modes.

PPEUC Proceedings
Fri Jun 20 15:22:24 BST 1997