We perform a renormalisation group analysis of the next-to-minimal su-persymmetric standard model (NMSSM) based on the following constraints: two-loop gauge coupling unification at a variable scale M X , running the gauge couplings through the low energy thresholds; universal soft supersym-metry breaking parameters; correct electroweak symmetry breaking. The phenomenological implications of our...

Most current methods for calculating radiative transfer treat radiance errors to the point where no one has seriously light as a scalar quantity, even though it is well known that a worried about the adequacy of the scalar approximation in proper description of light requires explicit recognition of its radiative transfer modeling. Moreover, the nature of radiative electromagnetic nature. Accor...

3GHr. The stirnuhis duration was 300ns and the profile duration, which corresponds to the time for which the scattering parameters measurements are performed during the stimulus duration, was 25011s. The maximum stable gain MSG was determined under different pulsed conditions at I' ds = 10V (Fig. 4). At room temperature in class B for the quiescent hias point, the MSG was -4dB. If the device wa...

Calculations of sensitivities of future experiments are a necessary ingredient in experimental high energy physics. Especially in the context of measurements of the neutrino oscillation parameters extensive studies are performed to arrive at the optimal configuration. In this note we clarify the definition of sensitivity as often applied in these studies. In addition we examine two of the most ...

The problem of clustering with constraints has received a lot of attention lately. Many existing algorithms assume the specified constraints are correct and consistent. We take a new approach and model a constraint as a random variable. This enables us to model the uncertainty of constraints in a principled manner. The effect of constraints can be readily propagated to the neighborhood by biasi...

We have examined the statistics of the polarization position angles determined for point sources in the NRAO-VLA sky survey (NVSS) and find that there is a statistically significant bias toward angles which are multiples of 45 degrees. The formal probability that the polarization angles are drawn from a uniform distribution is exponentially small. When the sample of those NVSS sources with pola...