English
Related papers

Related papers: Noble gases in carbonate melts: constraints on the…

200 papers

There has been notable uncertainty regarding the degree of solvation of alkaline-earth atoms, especially Mg, in free He-4 nanodroplets. We have measured the electron energy dependence of the ionization yield of picked-up atoms. There is a…

Other Condensed Matter · Physics 2011-11-10 Yanfei Ren , Vitaly V. Kresin

A high fraction of carbon bound in solid carbonaceous material is observed to exist in bodies formed in the cold outskirts of the solar nebula, while bodies in the terrestrial planets region contain nearly none. We study the fate of the…

Earth and Planetary Astrophysics · Physics 2017-10-04 Hans-Peter Gail , Mario Trieloff

Theory predicts that the temperature of the X-ray-emitting gas ($\sim$10$^{6}$ K) detected from planetary nebulae (PNe) is a consequence of mixing or thermal conduction when in contact with the ionized outer rim ($\sim$10$^{4}$ K). Gas at…

Solar and Stellar Astrophysics · Physics 2022-10-26 G. Rubio , J. Toalá , H. Todt , L. Sabin , E. Santamaría , G. Ramos-Larios , M. A. Guerrero

Experiments at 6-12 GPa showed that San Carlos olivine surrounded by carbon melts incongruently at 1400 C and higher temperatures, producing olivine with lower Fe contents, pyroxene, carbide, and carbonate melt. The relatively low melting…

Geophysics · Physics 2007-05-23 Jozsef Garai , Tibor Gasparik

We examine several different simplified approaches for modelling the chemistry of CO in three-dimensional numerical simulations of turbulent molecular clouds. We compare the different models both by looking at the behaviour of integrated…

Astrophysics of Galaxies · Physics 2015-05-27 S. C. O. Glover , P. C. Clark

The synthesis of hyper-heavy elements is investigated under conditions simulating neutron star environment. The Constrained Molecular Dynamics (CoMD) approach is used to simulate low energy collisions of extremely n-rich nuclei. A new type…

Nuclear Theory · Physics 2022-07-27 M. Veselsky , V. Petousis , Ch. C. Moustakidis , G. A. Souliotis , A. Bonasera

We use a one-dimensional line-by-line radiative-convective model to simulate hot, dense terrestrial-planet atmospheres. We find that strong shortwave absorption by H2O and CO2 inhibits near-surface convection, reducing surface temperatures…

Earth and Planetary Astrophysics · Physics 2025-05-05 Jessica Cmiel , Robin Wordsworth , Jacob T. Seeley

The first non-empirical computation of lattice thermal conductivity has been performed for MgO using molecular dynamics (MD), a non-empirical ionic model (the Variationally Induced Breathing (VIB) model), and Green-Kubo theory. The…

Materials Science · Physics 2008-02-03 Ronald E. Cohen

Adsorption properties of several gases (Ne, CH4, Ar, Xe) on the external surface of a carbon nanotube bundle are investigated. Calculations are performed at low coverage and variable temperature, and for some temperatures as a function of…

Soft Condensed Matter · Physics 2007-05-23 M. Mercedes Calbi , Milton W. Cole

Compositional convection is atmospheric mixing driven by density variations caused by compositional gradients. Previous studies have suggested that compositional gradients of atmospheric trace species within planetary atmospheres can impact…

Earth and Planetary Astrophysics · Physics 2025-11-18 Namrah Habib , Raymond T. Pierrehumbert

The standard approach to obtaining knowledge about the properties of the surface layer of a comet from observations of gas production consists of two stages. First, various thermophysical models are used to calculate gas production for a…

Earth and Planetary Astrophysics · Physics 2023-10-20 Yu. Skorov , J. Markkanen , V. Reshetnyk , S. Mottola , M. Küppers , S. Besse , M. R. El-Maarry , P. Hartogh

An elegant formula for coordinates of carbon atoms in a unit cell of a single-walled nanotube (SWNT) is presented and the potential of neon (Ne) inside an infinitely long SWNT is analytically derived out under the condition of the…

Statistical Mechanics · Physics 2016-08-31 Z. C. Tu , Z. C. Ou-Yang

Atmospheres are products of time-integrated mass exchange between the surface of a planet and its interior. On Earth and other planetary bodies, magma oceans likely marked significant atmosphere-forming events, during which both steam- and…

Earth and Planetary Astrophysics · Physics 2022-11-28 Paolo A. Sossi , Peter M. E. Tollan , James Badro , Dan J. Bower

As the number of detected rocky extrasolar planets increases, the question of whether their surfaces could be habitable is becoming more pertinent. On Earth, the long-term carbonate silicate cycle is able to regulate surface temperatures…

Earth and Planetary Astrophysics · Physics 2021-10-08 Amanda Kruijver , Dennis Höning , Wim van Westrenen

In an atmosphere, a cloud condensation region is characterized by a strong vertical gradient in the abundance of the related condensing species. On Earth, the ensuing gradient of mean molecular weight has relatively few dynamical…

Earth and Planetary Astrophysics · Physics 2017-02-08 Jérémy Leconte , Franck Selsis , Franck Hersant , Tristan Guillot

Uranus and Neptune have atmospheres dominated by molecular hydrogen and helium. In the upper troposphere, methane is the third main molecule and condenses, yielding a vertical gradient in CH4. This condensable species being heavier than H2…

We report the results of molecular dynamics simulations of the release of five species of noble gas atoms trapped inside a small cluster of fullerenes in the temperature range 4000K < T < 5000K. We find that larger noble gas atoms are…

Materials Science · Physics 2007-05-23 M. K. Balasubramanya , M. W. Roth , P. D. Tilton , B. A. Suchy

The electrolysis of CO$_2$ in molten carbonate has been introduced as an alternative mechanism to synthesize carbon nanomaterials inexpensively at high yield. Until recently, CO$_2$ was thought to be unreactive, making its removal a…

Materials Science · Physics 2022-01-21 Xinye Liu , Gad Licht , Xirui Wang , Stuart Licht

[abridged] We determine the relationship between turbulence energy and gas density variance for 15 molecular clouds in the Solar neighbourhood. We use the linewidths of the CO molecule as the probe of the turbulence energy (sonic Mach…

Astrophysics of Galaxies · Physics 2017-12-06 Jouni Kainulainen , Christoph Federrath

We present a theoretical study of solid carbon dioxide up to 50GPa and 1500K using first-principles calculations. In this pressure-temperature range, interpretations of recent experiments have suggested the existence of CO2 phases which are…

Materials Science · Physics 2009-11-10 S. A. Bonev , F. Gygi , T. Ogitsu , G. Galli
‹ Prev 1 4 5 6 7 8 10 Next ›