3 Experiment I: Evaluation of classifiers using COSMIC v.50 5 3.1 Cost-Sensitive Classifier . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 6 3.2 Comparison of COSMIC All and COSMIC FG1 . . . . . . . . . . . . . . . . . . . . . 6 3.3 Ranking of 177 Putative EGFR Mutations COSMIC v.50 . . . . . . . . . . . . . . 7 3.3.1 Majority voting approach . . . . . . . . . . . . . . . ....

Distributional sources of cosmic walls crossed by cosmic strings from Riemann-Cartan (RC) Geometry. The matter density of the planar wall is maximum at the point where the cosmic string crosses the cosmic wall. Cartan torsion is has a support on the cosmic string given by the Dirac δ-function. Off the sources are left with a torsionless vacuum. PACS number(s) : 0420,0450,1127 Departamento de F́ı...

In this paper we study the footprint of cosmic string as the topological defects in the very early universe on the cosmic microwave background radiation. We develop the method of level crossing analysis in the context of the well-known Kaiser-Stebbins phenomenon for exploring the signature of cosmic strings. We simulate a Gaussian map by using the best fit parameter given by WMAP-7 and then sup...

We basis our initial analysis of the arrow time on a relationship between evolution operator quantum system and time-independent density which describes equilibrium state many-particle at temperature $T$. highlight through this identification imaginary temporal component branch-cut complex cosmic form factor with direction in time-parameter flows globally, or time. As novelty, work we calculate...

We develop methods for comparing the quasi-equilibrium theory of gravitational galaxy clustering with other theories in the non-linear regime. The volume integrals, N , of the gravitational N -point correlation functions are expressed as functions of the quasi-equilibrium parameter b in a closed form which is exact to all orders of b. This shows that the N scale as [N=2]N 1[ 2]N 1 for small b...

From the axiom of the unrestricted repeatability of all experiments, Bondi and Gold (also Hoyle) argued that the universe is in a stable, selfperpetuating equilibrium state. Their reasoning extends the usual cosmological principle to the perfect cosmological principle in which the universe looks the same from any location at any time. By itself, the perfect cosmological principle predicts the u...