279 research outputs found
Discrete events: Perspectives from system theory
Systems Theory;differentiaal/ integraal-vergelijkingen
Parameter estimation and the statistics of nonlinear cosmic fields
The large scale distribution of matter in the universe contains valuable information
about fundamental cosmological parameters, the properties of dark matter
and the formation processes of galaxies. The best hope of retrieving this information
lies in providing a statistical description of the matter distribution that
may be used for comparing models with observation. Unfortunately much of the
important information lies on scales below which nonlinear gravitational effects
have taken hold, complicating both models and statistics considerably. This thesis
deals with the distribution of matter - mass and galaxies - on such scales. The
aim is to develop new statistical tools that make use of the nonlinear evolution
for the purposes of constraining cosmological models.A new derivation for the 1 -point probability distribution function (PDF) for density
inhomogeneities is presented first. The calculation is based upon an exact
statistical treatment, using the Chapman -Kolmogorov equation and second order
Eulerian perturbation theory to propagate the initial density field into the nonlinear
regime. The analysis yields the generating function for moments, allowing
for a straightforward derivation of the skewness. A new dependance upon the
perturbation spectrum is found for the skewness at second order. The results of
the analysis are compared against other methods for deriving the 1 -point PDF
and against data from numerical N -body simulations. Good agreement is found
in both cases.The 1 -point PDF for galaxies is derived next, taking into account nonlinear biasing
of the density field and the distorting effects associated with working in
redshift space. Once again perturbation theory is used to evolve the density field
into the nonlinear regime and the Chapman -Kolmogorov equation to propagate
the initial probabilities. Transformation of the dark matter density to a biased
galaxy distribution is done through an Eulerian biasing prescription, expanding
the nonlinear bias function to second order. An advantage of the Chapman-
Kolmogorov approach is the natural way that different initial conditions and biasing
models may be incorporated. It is shown that the method is general enough
to allow a non -deterministic (hidden variable) bias. The dependance on cosmological
parameters of the evolution of the galaxy 1 -point PDF is demonstrated
and a method for differentiating between degenerate models in linear theory is
presented. A new derivation of the skewness for a biased density field in red - shift space is also given and shown to depend significantly on the density and
bias parameters. The results are compared favourably with those of numerical
simulations.Finally a new, general formalism for analysing parameter information from non - Gaussian cosmic fields is developed. The method is general enough for application
to a range of problems including the measurement of parameters from galaxy
redshift surveys, weak lensing surveys and velocity field surveys. It may also be
used to test for non -Gaussianity in the Cosmic Microwave Background. Generalising
maximum likelihood analysis to second order, the non -Gaussian Fisher
information matrix is derived and the detailed shapes of likelihood surfaces in parameter
space are explored via a parameter entropy function. Concentrating on
non -Gaussianity due to nonlinear evolution under gravity, the generalised Fisher
analysis is applied to a model of a Galaxy redshift survey, including the effects
of biasing, redshift space distortions and shot noise. Incorporating second order
moments into the parameter estimation is found to have a large effect, breaking
all of the degeneracies between parameters. The results indicate that using
nonlinear likelihood analysis may yield parameter uncertainties around the few
percent level from forthcoming large galaxy redshift surveys
Stability Problems for Stochastic Models: Theory and Applications II
Most papers published in this Special Issue of Mathematics are written by the participants of the XXXVI International Seminar on Stability Problems for Stochastic Models, 2125 June, 2021, Petrozavodsk, Russia. The scope of the seminar embraces the following topics: Limit theorems and stability problems; Asymptotic theory of stochastic processes; Stable distributions and processes; Asymptotic statistics; Discrete probability models; Characterization of probability distributions; Insurance and financial mathematics; Applied statistics; Queueing theory; and other fields. This Special Issue contains 12 papers by specialists who represent 6 countries: Belarus, France, Hungary, India, Italy, and Russia
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