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[Abridged] Observations of protoplanetary disks suggest that they are depleted in gas-phase CO. It has been posed that gas-phase CO is chemically consumed and converted into less volatile species through gas-grain processes. Observations of…

天体物理仪器与方法 · 物理学 2022-10-05 J. Terwisscha van Scheltinga , N. F. W. Ligterink , A. D. Bosman , M. R. Hogerheijde , H. Linnartz

Energy dissipation in water is very fast and more efficient than in many other liquids. This behavior is commonly attributed to the intermolecular interactions associated with hydrogen bonding. Here, we investigate the dynamic energy flow…

We present a molecular-dynamics study of the solvent reorganization energy of electron transfer in supercooled water. We observe a sharp decrease of the reorganization energy at a temperature identified as the temperature of structural…

软凝聚态物质 · 物理学 2007-05-23 Pradip K. Ghorai , Dmitry V. Matyushov

Nonthermal desorption of molecules from icy grain surfaces is required to explain molecular line observations in the cold gas of star-forming regions. Chemical desorption is one of the nonthermal desorption processes and is driven by the…

星系天体物理 · 物理学 2022-03-02 Kenji Furuya , Yasuhiro Oba , Takashi Shimonishi

The surface processes on interstellar dust grains have an important role in the chemical evolution in molecular clouds. Hydrogenation reactions on ice surfaces have been extensively investigated and are known to proceed at low temperatures…

星系天体物理 · 物理学 2021-01-11 Masashi Tsuge , Hiroshi Hidaka , Akira Kouchi , Naoki Watanabe

Dynamics of adsorption and desorption of (4S)-N on amorphous solid water are analyzed using molecular dynamics simulations. The underlying potential energy surface was provided by machine-learned interatomic potentials. Binding energies…

星系天体物理 · 物理学 2020-09-22 Germán Molpeceres , Viktor Zaverkin , Johannes Kästner

The relative desorption energies of CO and N$_2$ are key to interpretations of observed interstellar CO and N$_2$ abundance patterns, including the well-documented CO and N$_2$H$^+$ anti-correlations in disks, protostars and molecular cloud…

Context. Comets are small celestial bodies made of ice, dust, and rock that orbit the Sun. Understanding their behavior as they warm up at perihelion unveils many pieces of information about the interior and general morphology of the ices…

地球与行星天体物理 · 物理学 2023-07-19 Carla Tamai , Belen Mate , Stephanie Cazaux , Miguel Angel Satorre

Using ab initio molecular dynamics (AIMD) simulations, based on density functional theory that also accounts for van der Waals interactions, we study the oxidation of gas phase CO on MoSe$_2$ with a Se vacancy and oxygen coverage of…

化学物理 · 物理学 2024-11-25 Raúl Bombín , Ricardo Díez Muiño , J. Iñaki Juaristi , Maite Alducin

A study of a reacting boundary layer flow with heat transfer at conditions typical for configurations at elevated pressures has been performed using a set of direct numerical simulations. Effects of wall temperatures are investigated,…

流体动力学 · 物理学 2021-02-16 Nikolaos Perakis , Oskar Haidn , Matthias Ihme

A large number of water models exists for molecular simulations. They differ in the ability to reproduce specific features of real water instead of others, like the correct temperature for the density maximum or the diffusion coefficient.…

软凝聚态物质 · 物理学 2012-06-04 Roman Shevchuk , Diego Prada-Gracia , Francesco Rao

Chemical processes taking place on ice-grain mantles are pivotal to the complex chemistry of interstellar environments. In this study, we conducted a comprehensive analysis of the catalytic effects of an amorphous solid water (ASW) surface…

Water and silicon are chemically dissimilar substances with common physical properties. Their liquids display a temperature of maximum density, increased diffusivity on compression, they form tetrahedral crystals and tetrahedral amorphous…

软凝聚态物质 · 物理学 2008-09-18 Valeria Molinero , Emily B. Moore

We present SWAS detections of the ground-state 1(10)-1(01) transition of o-H2O at 557 GHz in 18 molecular outflows. These results are combined with ground-based observations of the J=1-0 transitions of 12CO and 13CO obtained at the FCRAO…

天体物理学 · 物理学 2009-11-13 J. Franklin , R. L. Snell , M. J. Kaufman , G. J. Melnick , D. A. Neufeld , D. J. Hollenbach , E. A. Bergin

In this work we investigate the dissociation of CO$_2$ on Cu(110) by performing density functional theory calculations using the vdW-DF2 exchange-correlation functional, with a potential energy surface parameterized using artificial neural…

材料科学 · 物理学 2025-12-29 Federico J. Gonzalez , Carmen A. Tachino , H. Fabio Busnengo

Water is abundantly present in the Universe. It is the main component of interstellar ice mantles and a key ingredient for life. Water in space is mainly formed through surface reactions. Three formation routes have been proposed in the…

太阳与恒星天体物理 · 物理学 2017-08-23 H. M. Cuppen , S. Ioppolo , C. Romanzin , H. Linnartz

This paper extends our earlier studies of free energy functions of density and crystalline order parameters for models of supercooled water, which allows us to examine the possibility of two distinct metastable liquid phases [J. Chem. Phys.…

统计力学 · 物理学 2015-06-15 David T. Limmer , David Chandler

Molecular beam experiments that use low-temperature bolometers as (energy-) detectors are well suited to the study of physisorption and recombination of hydrogen on low-temperature surfaces. Experiments where this technique is combined with…

化学物理 · 物理学 2007-05-23 Thomas Govers

The long-timescale behavior of adsorbed carbon monoxide on the surface of amorphous water ice is studied under dense cloud conditions by means of off-lattice, on-the-fly, kinetic Monte Carlo simula- tions. It is found that the CO mobility…

Diffusion of atoms and molecules is a key process for the chemical evolution in the star forming regions of the interstellar medium. Accurate data on the mobility of many important interstellar species is however often not available and…

星系天体物理 · 物理学 2014-10-01 L. J. Karssemeijer , H. M. Cuppen