For finite quantum many-particle systems modeled with say $m$ fermions in $N$ single particle states and interacting $k$-body interactions ($k \leq m$), the wavefunction structure is studied using random matrix theory. Hamiltonian for system chosen to be $H=H_0(t) + \lambda V(k)$ unperturbed $H_0(t)$ being a $t$-body operator $V(k)$ interaction strength $\lambda$. Representing by independent Ga...

A non-relativistic Fokker-Planck equation for the electron distribution function is formulated incorporating the effects of stochastic acceleration by whistlermode waves and Coulomb collisions. The stationary solution f to the equation, subject to a zero-flux boundary condition, is found to be a generalized Lorentzian (or kappa) distribution, which satisfies f ∝ v for large velocity v, where κ ...

To determine the extent of kappa chain diversity in the preimmune repertoire early in development, kappa cDNA libraries were analyzed from 15-d old fetal omentum, 18-d-old fetal liver, and 3-wk old bone marrow. An anchored polymerase chain reaction approach was used to avoid bias for particular V kappa families. From the sequence analysis of 27 bone marrow clones, 10 different families and 20 u...

The nuclear factor kappa B is widely expressed in the distinct subpopulations of chorionic villi and deciduas of first-trimester pregnancies. We examined the cellular distribution and expression of nuclear factor kappa B in the human first-trimester chorionic villi and deciduas of women with early spontaneous miscarriage and viable pregnancy by confocal laser scanning microscope and immunohisto...

In Ref. [Physica A 296, 405 (2001)], starting from the one parameter deformation of the exponential function exp(kappa)(x)=(sqrt[1+kappa(2)x(2)]+kappax)(1/kappa), a statistical mechanics has been constructed which reduces to the ordinary Boltzmann-Gibbs statistical mechanics as the deformation parameter kappa approaches to zero. The distribution f=exp(kappa)(-beta E+betamu) obtained within this...

The probability distributions (PDFs) of the differences of any physical variable in the intermittent, turbulent interplanetary medium are scale dependent. Strong non-Gaussianity of solar wind fluctuations applies for short time-lag spacecraft observations, corresponding to small-scale spatial separations, whereas for large scales the differences turn into a Gaussian normal distribution. These c...

The quantum version of Olbert's kappa distribution applicable to fermions is obtained. Its construction straightforward but requires recognition the differences in nature states separated by Fermi momenta. complement, bosonic also given, as procedure how construct a hypothetical kappa-anyon distribution. At very low temperature degenerate yields kappa-modified ordinary energy and momentum. We p...

We study the question of what di€erence it makes for the derived ®eld-aligned conductance (K) values if one uses Maxwellian or kappa distributions for the ®tting of low-orbiting satellite electron ̄ux spectra in the auroral region. This question has arisen because sometimes a high-energy tail is seen in the spectra. In principle, the kappa ®ts should always be better, because the kappa distribu...