Thermal Steady States of Gases in a Gravitational Field Kunihiko Kigoshi

As the direction of current squeezing is determined by the sign of the field gradient, we find that for positive magnetic field values, the current is concentrated exponentially

• This is the first quantitative assessment of the textbook statement on gravitational -> thermal energy conversion in the large-scale structure formation (using the

In the present paper, we again start from the interacting many-body Hamiltonian and prove the matching lower bound, thus completely validating the random-phase approximation for

in die Kammer an gegenubcrlic- genden Siellen MeB- und Vcrglcichsgas einstromen, die Gase sich vermischen und das Gcmisch durch eine Mittelbohrung in cinem dcr Weicheiscnpol- schuhe

Thermal gradients are responsible for a wide range of non equilibrium effects, heat transport, electron transport (thermoelectricity) [1], mass transport in suspensions

In this study, the fluid flow and heat transfer characteristics of a two-dimensional, steady MHD flow of a non-Newtonian fluid in a channel with the presence of thermal radiation

Here, λ g is the ordinary thermal conductivity of the gas, (dT g / dz) is the vertical thermal gradient in the gaseous system, z is the vertical coordinate increasing upward, and Γ g

Influence of Heat Transfer and Magnetic Field on a Peristaltic Transport of a Jeffrey Fluid in an Asymmetric Channel with Partial Slip.. Sohail Nadeem and