Lens Models with Density Cusps
Lens models appropriate for representing cusped galaxies and clusters are developed. The analogue of the odd number theorem for cusped
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Cosmological Simulations with Scale-Free Initial Conditions II: Radiative Cooling
The growth of structure from scale-free initial conditions is one of the most important tests of cosmological simulation methods, providing
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Mapping spatial persistent large deviations of nonequilibrium surface growth processes onto the temporal persistent large deviations of stochastic random walk processes
Spatial persistent large deviations probability of surface growth processes governed by the Edwards-Wilkinson dynamics, $P_x(x,s)$, with $-1 \leq s \leq
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Comment on "Anomalous Spreading of Power-Law Quantum Wave Packets"
A family of wave packets with power law tails are employed to analyze the long time dependence of the corresponding
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Symmetry Under $α\rightarrow α+ 1$ is Forbidden by Helicity Conservation
The question as to whether helicity conservation in spin one-half Aharonov Bohm scattering is sufficient in itself to determine uniquely
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Competition-Induced Preferential Attachment
Models based on preferential attachment have had much success in reproducing the power law degree distributions which seem ubiquitous in
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Degeneracies and scaling relations in general power-law models for gravitational lenses
The time delay in gravitational lenses can be used to derive the Hubble constant in a relatively simple way. The
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Degree Distribution of Competition-Induced Preferential Attachment Graphs
We introduce a family of one-dimensional geometric growth models, constructed iteratively by locally optimizing the tradeoffs between two competing metrics,
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Non-asymptotically flat black holes/branes
In the framework of string-inspired dilatonic gravity theories (from 4 to $D$ space-time dimensions), we construct new non-asymptotically flat black
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Power law distribution in High School Education: Effect of Economical, Teaching and study conditions
We studied the statistical distribution of student's performance, which is measured through their marks, in university entrance examination (Vestibular) of
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Richardson's Laws for Relative Dispersion in Colored-Noise Flows with Kolmogorov-type Spectra
We prove limit theorems for small-scale pair dispersion in velocity fields with power-law spatial spectra and wave-number dependent correlation times.
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New Families of Scaling Multiparticle Distributions
Recently equations for the generating functional in the perturbative quantum chromodynamics (QCD) have been extended by including the non-perturbative dissipation
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Power spectra of extinction in the fossil record
Recent Fourier analyses of fossil extinction data have indicated that the power spectrum of extinction during the Phanerozoic may take
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A Renormalisation Group Analysis of 2d Freely Decaying Magnetohydrodynamic Turbulence
We study two dimensional freely decaying magnetohydrodynamic turbulence. We investigate the time evolution of the probability law of the gauge
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Analysis of scale-free networks based on a threshold graph with intrinsic vertex weights
Many real networks are complex and have power-law vertex degree distribution, short diameter, and high clustering. We analyze the network
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A Generalization of Tsallis' Non-Extensive Entropy and Energy Landscape Transformation Functions
This article extends the non-extensive entropy of Tsallis and uses this entropy to model an energy producing system in an
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Analysis of the self-similar spreading of power law fluids
We consider the equation that models the spreading of thin liquid films of power-law rheology. In particular, we analyze the
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Radiative Corrections in Nonrelativistic Chern-Simons Theory
We present the one-loop scalar field effective potential for the $N=2$ supersymmetric nonrelativistic self-interacting matter fields coupled to an Abelian
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On the deprojection of triaxial galaxies with Stäckel potentials
A family of triaxial Stäckel potential-density pairs is introduced. With the help of a Quadratic Programming method, a linear combination
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Fast and simple Complex and Slow
The decay of a general time dependent structure factors is considered. The dynamics is that of stochastic field equations of
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