147 research outputs found
Abelian deterministic self organized criticality model: Complex dynamics of avalanche waves
The aim of this study is to investigate a wave dynamics and size scaling of
avalanches which were created by the mathematical model {[}J. \v{C}ern\'ak
Phys. Rev. E \textbf{65}, 046141 (2002)]. Numerical simulations were carried
out on a two dimensional lattice in which two constant thresholds
and were randomly distributed. A density
of sites with the threshold and threshold are
parameters of the model. I have determined autocorrelations of avalanche size
waves, Hurst exponents, avalanche structures and avalanche size moments for
several densities and thresholds . I found correlated avalanche
size waves and multifractal scaling of avalanche sizes not only for specific
conditions, densities , 1.0 and thresholds , in
which relaxation rules were precisely balanced, but also for more general
conditions, densities and thresholds $8\leq E_{c}^{II}\leq3 in
which relaxation rules were unbalanced. The results suggest that the hypothesis
of a precise relaxation balance could be a specific case of a more general
rule
spectra in elementary cellular automata and fractal signals
We systematically compute the power spectra of the one-dimensional elementary
cellular automata introduced by Wolfram. On the one hand our analysis reveals
that one automaton displays spectra though considered as trivial, and on
the other hand that various automata classified as chaotic/complex display no
spectra. We model the results generalizing the recently investigated
Sierpinski signal to a class of fractal signals that are tailored to produce
spectra. From the widespread occurrence of (elementary) cellular
automata patterns in chemistry, physics and computer sciences, there are
various candidates to show spectra similar to our results.Comment: 4 pages (3 figs included
Stable fractal sums of pulses: the cylindrical case
A class of α-stable, 0\textlessα\textless2, processes is obtained as a sum of ’up-and-down’ pulses determined by an appropriate Poisson random measure. Processes are H-self-affine (also frequently called ’self-similar’) with H\textless1/α and have stationary increments. Their two-dimensional dependence structure resembles that of the fractional Brownian motion (for H\textless1/2), but their sample paths are highly irregular (nowhere bounded with probability 1). Generalizations using different shapes of pulses are also discussed
Selection mechanisms affect volatility in evolving markets
Financial asset markets are sociotechnical systems whose constituent agents
are subject to evolutionary pressure as unprofitable agents exit the
marketplace and more profitable agents continue to trade assets. Using a
population of evolving zero-intelligence agents and a frequent batch auction
price-discovery mechanism as substrate, we analyze the role played by
evolutionary selection mechanisms in determining macro-observable market
statistics. In particular, we show that selection mechanisms incorporating a
local fitness-proportionate component are associated with high correlation
between a micro, risk-aversion parameter and a commonly-used macro-volatility
statistic, while a purely quantile-based selection mechanism shows
significantly less correlation.Comment: 9 pages, 7 figures, to appear in proceedings of GECCO 2019 as a full
pape
Shortcomings of a Parametric VaR Approach and Nonparametric Improvements Based on a Non-Stationary Return Series Model
A non-stationary regression model for financial returns is examined theoretically in this paper. Volatility dynamics are modelled both exogenously and deterministic, captured by a nonparametric curve estimation on equidistant centered returns. We prove consistency and asymptotic normality of a symmetric variance estimator and of a one-sided variance estimator analytically, and derive remarks on the bandwidth decision. Further attention is paid to asymmetry and heavy tails of the return distribution, implemented by an asymmetric version of the Pearson type VII distribution for random innovations. By providing a method of moments for its parameter estimation and a connection to the Student-t distribution we offer the framework for a factor-based VaR approach. The approximation quality of the non-stationary model is supported by simulation studies
Markov Chain Monte Carlo and the Application to Geodetic Time Series Analysis
The time evolution of geophysical phenomena can be characterised by stochastic time series. The stochastic nature of the signal stems from the geophysical phenomena involved and any noise, which may be due to, e.g., un-modelled effects or measurement errors. Until the 1990's, it was usually assumed that white noise could fully characterise this noise. However, this was demonstrated to be not the case and it was proven that this assumption leads to underestimated uncertainties of the geophysical parameters inferred from the geodetic time series. Therefore, in order to fully quantify all the uncertainties as robustly as possible, it is imperative to estimate not only the deterministic but also the stochastic parameters of the time series. In this regard, the Markov Chain Monte Carlo (MCMC) method can provide a sample of the distribution function of all parameters, including those regarding the noise, e.g., spectral index and amplitudes. After presenting the MCMC method and its implementation in our MCMC software we apply it to synthetic and real time series and perform a cross-evaluation using Maximum Likelihood Estimation (MLE) as implemented in the CATS software. Several examples as to how the MCMC method performs as a parameter estimation method for geodetic time series are given in this chapter. These include the applications to GPS position time series, superconducting gravity time series and monthly mean sea level (MSL) records, which all show very different stochastic properties. The impact of the estimated parameter uncertainties on sub-sequentially derived products is briefly demonstrated for the case of plate motion models. Finally, the MCMC results for weekly downsampled versions of the benchmark synthetic GNSS time series as provided in Chapter 2 are presented separately in an appendix
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