Saturation Deficit in Various Air Masses

Formation of giant planets around stars with various masses

We examine the predictions of the core accretion gas capture model concerning the efficiency of planet formation around stars with various masses. First, we follow the evolution of gas and solids from the moment when all solids are in the form of small grains to the stage when most of them are in the form of planetesimals. We show that the surface density of the planetesimal swarm tends to be h...

Planet Formation around Stars of Various Masses: Hot Super-earths

We consider trends resulting from two formation mechanisms for short-period super-Earths: planetplanet scattering and migration. We model scenarios where these planets originate near the snow line in “cold finger” circumstellar disks. Low-mass planet-planet scattering excites planets to low periastron orbits only for lower mass stars. With long circularisation times, these planets reside on lon...

Pulmonary functions during saturation-excursion dives breathing air.

Air Shower Properties with the Gluon Saturation Model BBL

The hadronic interaction model BBL implements the ideas of gluon saturation due to large densities. When approaching the black body limit at high energies, leading partons acquire large transverse momenta which breaks up their coherence. This leads to a suppression of forward scattering, and is therefore important for air showers. We discuss some general aspects of this new approach and their i...

Arctic ice clouds and polluted air masses over

Introduction Conclusions References