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powerlaw
Non-Newtonian liquids having relaxation properties and also pseudoplastic and dilatant liquids with powerlaw equation of state are studied.
      
An analysis of the λ4244 ? continuum light curve of the eclipsing variable V444 Cyg is used to reconstruct the velocity law v(r) of the stellar wind of the WR star in terms of Lamers parametric and powerlaw models.
      
A powerlaw dependence H-3/4 on the external magnetic field H is obtained according to the law of magnetization approach to saturation.
      
Specifically there is a powerlaw-like decay of the order parameter with exponent β=0.20±0.05, and a rounded transition region which may be described by a Gaussian distribution of transition temperatures.
      
We find a powerlaw regime (R(t)~txwithx depending on temperature and larger than the Allen-Cahn value 0.5.
      
Alternatively, the data can be fitted by a simple powerlaw preexponential.
      
Generation of exact analytic bound state solutions from solvable non-powerlaw potentials by a transformation method
      
The generated quantum systems are, in general, energy-dependent with a single normalized eigenfunction, as the Hulthen potential is a non-powerlaw potential.
      
The equation for the thermal boundary layer of a non-Fourier powerlaw fluid on a flat plate with an exponential distribution of surface temperature is reduced to an ordinary equation and solved by the method of finite differences.
      
A method is proposed for solving some planar problems of nonlinear filtration with powerlaw resistance in the case of straight-line boundaries of the filtration region.
      
Solution of the Rayleigh problem for a powerlaw non-Newtonian conducting fluid via group method
      
We shall extend these results to the nonlinear model classified as powerlaw clasticity.
      
An approximate closed form analytical solution has been obtained for the motion of a solid sphere in powerlaw fluids and this solution has been verified experimentally.
      
It is found that for certain powerlaw distribution of surface heat flux or temperature and magnetic field with time, the governing boundary layer equations admit a self-similar solution locally.
      
The hatching time (days after fertilization for 10, 50% and 90% of the eggs to hatch) decreased with increasing temperature and the relationship between the two variables was well described by a powerlaw within the range 2.8°-18.1° C for E.
      
The 2-100 keV spectrum of η Car is instead well fitted with an absorbed powerlaw spectrum with photon index 2.53, suggesting non-thermal emission as an alternative model for the core source.
      
Separate analysis of the low and hard states show the presence of a hard powerlaw tail in both the states.
      
As a result, the exponents of the infra-red powerlaw behavior of the pseudoparticle spectral functions are modified w.r.t NCA and depend on the impurity occupation number.
      
Below a critical temperature, χ(O, q) exhibits a powerlaw divergence at the Fermi surface (q=2kF).
      
The size distributions of the florid and diffuse plaques were fitted successfully by a powerlaw function in 100% and 42% of brain areas investigated respectively.
      
 

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