Posterior/likelihood maximization (i.e. -log(post) and chi^2 minimization).
The default is BOBYQA, which tends to work better on Cosmological problems with default settings.
If you use BOBYQA, please cite it as:
C. Cartis, J. Fiala, B. Marteau, L. Roberts, “Improving the Flexibility and Robustness of Model-Based Derivative-Free Optimization Solvers” (arXiv:1804.00154)
C. Cartis, L. Roberts, O. Sheridan-Methven, “Escaping local minima with derivative-free methods: a numerical investigation” (arXiv:1812.11343)
M.J.D. Powell, “The BOBYQA Algorithm for Bound Constrained Optimization without Derivatives”, (Technical Report 2009/NA06, DAMTP, University of Cambridge)
If you use scipy, you can find the appropriate references here.
It works more effectively when run on top of a Monte Carlo sample: it will use the maximum a posteriori as a starting point (or the best fit, depending on whether the prior is ignored, see below), and the recovered covariance matrix of the posterior to rescale the variables.
To take advantage of a previous run with a Monte Carlo sampler, either:
minimizein the input file,
or, if running from the shell, repeat the
cobaya-runcommand used for the original run, adding the
When called from a Python script, Cobaya’s
run function returns the updated info
and the products described below in the method
samplers.minimize.Minimize.products() (see below).
If text output is requested, it produces two different files:
[output prefix].minimum.txt, in the same format as Cobaya samples, but containing a single line.
[output prefix].minimum, the equivalent GetDist-formatted file.
For historical reasons, in the first two lines of the GetDist-formatted output file
-log(Like) indicates the negative log-posterior, and similarly
\(-2\) times the log-posterior. The actual log-likelihood can be obtained as
\(-2\) times the sum of the individual \(\chi^2\) (
chi2__, with double
underscore) in the table that follows these first lines.
It is recommended to run a couple of parallel MPI processes: it will finally pick the best among the results.
Since Cobaya is often used on likelihoods featuring numerical noise (e.g. Cosmology),
we have reduced the default accuracy criterion for the minimizers, so that they
converge in a limited amount of time. If your posterior is fast to evaluate, you may
want to refine the convergence parameters (see
override options in the
Maximizing the likelihood instead of the posterior¶
To maximize the likelihood, add
ignore_prior: True in the
minimize input block.
When producing text output, the generated files are named
.bestfit[.txt] instead of
minimum, and contain the best-fit (maximum of the likelihood) instead of the MAP
(maximum of the posterior).
Options and defaults¶
Simply copy this block in your input
yaml file and modify whatever options you want (you can delete the rest).
# Default arguments for the -logposterior/chi^2 minimizer # Method: bobyqa|scipy method: bobyqa # Minimizes the full posterior (False) or just the likelihood (True) # Likelihood maximization is subject to prior bounds! ignore_prior: False # Maximum number of iterations (default: practically infinite) max_evals: 1e6d # Number of different starting positions to try minimizing from (may be rounded up if MPI) best_of: 2 # Treatment of unbounded parameters: confidence level to use # (Use with care if there are likelihood modes close to the edge of the prior) confidence_for_unbounded: 0.9999995 # 5 sigmas of the prior # Seeding runs seed: # an initial seed (entropy) for the numpy random generator # Override keyword arguments for `scipy.optimize.minimize()` or `pybobyqa.solve()` # scipy: # - https://docs.scipy.org/doc/scipy/reference/generated/scipy.optimize.minimize.html # - options for individual methods override_scipy: # option: value # bobyqa: # - https://numericalalgorithmsgroup.github.io/pybobyqa/build/html/userguide.html # - https://numericalalgorithmsgroup.github.io/pybobyqa/build/html/advanced.html override_bobyqa: # option: value # Relaxed convergence criterion for numerically-noisy likelihoods rhoend: 0.05 # File (including path) or matrix defining a covariance matrix for the proposal: # - null (default): will be generated from params info (prior and proposal) # - matrix: remember to set `covmat_params` to the parameters in the matrix # - "auto" (cosmology runs only): will be looked up in a library # In any case, if an old chain its present, its covmat will be loaded instead. covmat: covmat_params:
- class samplers.minimize.Minimize(info_sampler, model, output=typing.Union[cobaya.output.Output, NoneType], packages_path=None, name=None)¶
Initializes the sampler: prepares the samples’ collection, prepares the output, deals with MPI scheduling, imports an external sampler, etc.
Options defined in the
defaults.yamlfile in the sampler’s folder are automatically recognized as attributes, with the value given in the input file, if redefined there.
The prior and likelihood are also accessible through the attributes with the same names.
- process_results(results, successes, affine_transform_baselines, transform_matrices)¶
Determines success (or not), chooses best (if MPI or multiple starts) and produces output (if requested).
Returns a dictionary containing:
OnePointthat maximizes the posterior or likelihood (depending on
M: inverse of the affine transform matrix (see below).
Noneif no transformation applied.
X0: offset of the affine transform matrix (see below)
Noneif no transformation applied.
X0are returned, this means that the minimizer has been working on an affine-transformed parameter space \(x^\prime\), from which the real space points can be obtained as \(x = M x^\prime + X_0\). This inverse transformation needs to be applied to the coordinates appearing inside the
- classmethod output_files_regexps(output, info=None, minimal=False)¶
Returns a list of tuples (regexp, root) of output files potentially produced. If root in the tuple is None, output.folder is used.
If minimal=True, returns regexp’s for the files that should really not be there when we are not resuming.
- classmethod check_force_resume(output, info=None)¶
Performs the necessary checks on existing files if resuming or forcing (including deleting some output files when forcing).