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Analytical low-current and numerical high--current models for the impedance of a hydrogen--fed anode of an anode--supported button SOFC are developed. The models use the dusty gas transport model for the binary H$_2$--H$_2$O mixture. We…

化学物理 · 物理学 2025-01-15 Andrei Kulikovsky

Multicomponent gas transport is investigated with unprecedented precision by AC impedance analysis of porous YSZ anode-supported solid oxide fuel cells. A fuel gas mixture of H2-H2O-N2 is fed to the anode, and impedance data are measured…

化学物理 · 物理学 2014-09-11 Yeqing Fu , Yi Jiang , Abhijit Dutta , Aravind Mohanram , John D. Pietras , Martin Z. Bazant

We investigate the density large deviation function for a multidimensional conservation law in the vanishing viscosity limit, when the probability concentrates on weak solutions of a hyperbolic conservation law conservation law. When the…

统计力学 · 物理学 2018-03-14 Julien Barré , Cedric Bernardin , Raphaël Chetrite

There are two major theoretical issues for the star formation law (the relation between the surface densities of molecular gas and star formation rate on a galaxy scale): (i) At low metallicity, it is not obvious that star-forming regions…

星系天体物理 · 物理学 2018-01-24 Li-Hsin Chen , Hiroyuki Hirashita , Kuan-Chou Hou , Shohei Aoyama , Ikkoh Shimizu , Kentaro Nagamine

In order to interpret H2 (molecular hydrogen) quasar absorption line observations of damped Ly-alpha systems (DLAs) and sub-DLAs, we model their H2 abundance as a function of dust-to-gas ratio, including H2 self-shielding and dust…

天体物理学 · 物理学 2009-11-10 H. Hirashita , A. Ferrara

We apply novel survival analysis techniques to investigate the relationship between a number of the properties of galaxies and their atomic ($M_\mathrm{HI}$) and molecular ($M_{\mathrm{H_2}}$) gas mass, with the aim of devising efficient,…

星系天体物理 · 物理学 2019-11-06 Hassen M. Yesuf , Luis C. Ho

The molecular gas content of high-redshift galaxies is a highly sought-after property. However, H$_2$ is not directly observable in most environments, so its mass is probed through other emission lines (e.g., CO, [CI], [CII]), or through a…

星系天体物理 · 物理学 2020-10-07 Gareth C. Jones , Roberto Maiolino , Paola Caselli , Stefano Carniani

We combine modeling and measurements to investigate the dynamics of convective carbon dioxide (CO$_2$) dissolution in a pressure-volume-temperature cell, extending a recent study by Wen et al. (J. Fluid Mech., vol. 854, 2018, pp. 56--87) at…

流体动力学 · 物理学 2021-07-07 Baole Wen , Zhuofan Shi , Kristian Jessen , Marc A. Hesse , Theodore T. Tsotsis

We present a method to estimate the total gas column density, dust-to-gas and dust-to-metal ratios of distant galaxies from rest-frame optical spectra. The technique exploits the sensitivity of certain optical lines to changes in depletion…

宇宙学与河外天体物理 · 物理学 2015-06-15 Jarle Brinchmann , Stéphane Charlot , Guinevere Kauffmann , Tim Heckman , Simon D. M. White , Christy Tremonti

For the hyperbolic system of quasilinear first-order partial differential equations, linearizable by hodograph transformation, the conservation laws are used to solve the Cauchy problem. The equivalence of the initial problem for…

数学物理 · 物理学 2012-10-16 Sergey I. Senashov , Alexander Yakhno

We present exact results for steady-state density correlation functions in conserved-mass transport processes with {\it anisotropic}, reflection-symmetric hopping on a $d-$dimensional hypercubic lattice. In addition to mass conservation, we…

统计力学 · 物理学 2026-04-03 Aniket Samanta , Animesh Hazra , Punyabrata Pradhan

In this work, we combine Density Functional Theory data with a Thermodynamic and a kinetic model to determine the total concentration of hydrogen implanted in the sub-surface of tungsten exposed to a hydrogen flux. The sub-surface hydrogen…

材料科学 · 物理学 2019-04-30 E. Hodille , N Fernandez , Z. Piazza , M. Ajmalghan , Y. Ferro

Absorption-selected galaxies offer an effective way to study low-mass galaxies at high redshift. However, the physical properties of the underlying galaxy population remains uncertain. In particular, the multiphase circum-galactic medium is…

星系天体物理 · 物理学 2021-06-30 Anne Klitsch , Celine Peroux , Martin A. Zwaan , Annalisa De Cia , Cedric Ledoux , Sebastian Lopez

Robust knowledge of molecular gas mass is critical for understanding star formation in galaxies. The H$_{2}$ molecule does not emit efficiently in the cold interstellar medium, hence the molecular gas content of galaxies is typically…

星系天体物理 · 物理学 2016-10-12 Aditya Togi , J. D. T. Smith

The complete set of transport coefficients for two dimensional relativistic degenerate gases is derived within a relaxation approximation in kinetic theory, by considering both the particle and energy frames. A thorough comparison between…

量子气体 · 物理学 2021-10-08 A. R. Mendez , A. L. Garcia-Perciante , G. Chacon-Acosta

This paper deals with a mathematical model for oil filtration in a porous medium and its self-similar and traveling wave regimes. The model consists of the equation for conservation mass and dependencies for porosity, permeability, and oil…

数学物理 · 物理学 2025-04-23 Sergii Skurativskyi , Sergiy Mykulyak , Inna Skurativska

A two-dimensional generalized hydrodynamics (GH) model is developed to study the full spectrum of both longitudinal and transverse dust acoustic waves (DAW) in strongly coupled complex (dusty) plasmas, with memory-function-formalism being…

等离子体物理 · 物理学 2015-05-19 Nitin Upadhyaya , Z. L. Miskovic , L. -J. Hou

To explore the potential of molecular gas treatment of freshly cut lithium foils in non-electrolyte based passivation of high energy-density Li anodes, density functional theory (DFT) has been used to study the decomposition of molecular…

材料科学 · 物理学 2015-06-01 Stephan L. Koch , Benjamin J. Morgan , Stefano Passerini , Gilberto Teobaldi

We devise a physical model of formation and distribution of molecular gas clouds in galaxies. We use the model to predict the intensities of rotational transition lines of carbon monoxide (CO) and the molecular hydrogen (H$_{\rm 2}$)…

星系天体物理 · 物理学 2020-10-14 Shigeki Inoue , Naoki Yoshida , Hidenobu Yajima

According to traditional gas-phase chemical models, O2 should be abundant in molecular clouds, but until recently, attempts to detect interstellar O2 line emission with ground- and space-based observatories have failed. Following the…

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