Abstract
Thermal transpiration is a rarefied gas flow driven by a wall temperature gradient and is a promising mechanism for gas pumping without moving parts, known as the Knudsen pump. Obtaining temperature measurements along capillary walls in a Knudsen pump is difficult due to extremely small length scales. Meanwhile, simplified analytical models are not applicable under the practical operating conditions of a thermal transpiration device, where the gas flow is in the transitional rarefied regime. Here, we present a coupled gas-phonon heat transfer and flow model to study a closed thermal transpiration system. Discretized Boltzmann equations are solved for molecular transport in the gas phase and phonon transport in the solid. The wall temperature distribution is the direct result of the interfacial coupling based on mass conservation and energy balance at gas-solid interfaces and is not specified a priori unlike in the previous modeling efforts. Capillary length scales of the order of phonon mean free path result in a smaller temperature gradient along the transpiration channel as compared to that predicted by the continuum solid-phase heat transfer. The effects of governing parameters such as thermal gradients, capillary geometry, gas and phonon Knudsen numbers and, gas-surface interaction parameters on the efficiency of thermal transpiration are investigated in light of the coupled model.
Date of this Version
2009
DOI
10.1103/PhysRevE.80.046310
Recommended Citation
Guo, Xiaohui; Singh, Dhruv; Murthy, Jayathi; and Alexeenko, Alina A., "Numerical simulation of gas-phonon coupling in thermal transpiration flows" (2009). School of Aeronautics and Astronautics Faculty Publications. Paper 40.
http://dx.doi.org/10.1103/PhysRevE.80.046310
Comments
This is the published version of X. Guo*, D. Singh, J. Y. Murthy, and A. A. Alexeenko, “Numerical Simulation of Gas-Phonon Coupling in Thermal Transpiration Flows,” Physical Review E, Vol. 80, No. March 2015 Page 4 of 224, 046310, 10 pages, 2009. First published in the Physical Review E and is available online at: http://dx.doi.org/10.1103/PhysRevE.80.046310.