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We investigate the evolution of angular momentum in SPH simulations of galaxy formation, paying particular attention to artificial numerical effects. We find that a cold gas disc forming in an ambient hot gas halo receives a strong…

Astrophysics · Physics 2009-11-10 T. Okamoto , A. Jenkins , V. R. Eke , V. Quilis , C. S. Frenk

We calculate the torsional moduli of single-walled transition metal dichalcogenide (TMD) nanotubes using ab initio density functional theory (DFT). Specifically, considering forty-five select TMD nanotubes, we perform symmetry-adapted DFT…

Materials Science · Physics 2021-05-26 Arpit Bhardwaj , Abhiraj Sharma , Phanish Suryanarayana

We study the collective electronic excitations in metallic single- and bilayer transition metal dichalcogenides (TMDCs) using time dependent density functional theory in the random phase approximation. For very small momentum transfers…

Mesoscale and Nanoscale Physics · Physics 2015-06-17 Kirsten Andersen , Kristian S. Thygesen

We study the magneto-hydrodynamic tearing instability occurring in a double current sheet configuration when a guide field is present. This is investigated by means of resistive relativistic magneto-hydrodynamic (RRMHD) simulations.…

High Energy Astrophysical Phenomena · Physics 2015-10-28 Makoto Takamoto , J. Pétri , H. Baty

The magnetohydrodynamic linear stability with the localized bulk flow oriented parallel to the neutral sheet is investigated, by including the Hall effect and the guide magnetic field. We observe three different unstable modes: a "streaming…

Space Physics · Physics 2015-05-19 Masahiro Hoshino

In this paper, we provide a more accurate description of the evolution of the magnetic flux redistribution during prestellar core collapse by including resistive terms in the magnetohydrodynamics (MHD) equations. We focus more particularly…

Solar and Stellar Astrophysics · Physics 2016-02-17 Jacques Masson , Gilles Chabrier , Patrick Hennebelle , Neil Vaytet , Benoit Commerçon

We investigate the dynamic behaviour of a two-dimensional (2D) droplet adhering to a wall in Poiseuille flow at low Reynolds numbers, in a system where either the droplet is viscoelastic (V/N) or the surrounding medium (N/V). The results…

Fluid Dynamics · Physics 2024-05-24 Kazem Bazesefidpar , Outi Tammisola

Two-dimensional (2D) layered transition metal dichalcogenides (TMDs) have recently attracted tremendous interest as potential valleytronic and nano-electronic materials, in addition to being well-known as excellent lubricants in the bulk.…

Plasmons are elementary quantum excitations of conducting materials with Fermi surfaces. In two dimensions they may carry a static dipole moment that is transverse to their momentum which is quantum geometric in nature, the quantum…

Mesoscale and Nanoscale Physics · Physics 2025-07-02 Jinlyu Cao , Herb Fertig , Luis Brey

The linear drift-tearing mode is analyzed for different regimes of the plasma-$\beta$, ion-skin-depth parameter space with an unreduced, extended-MHD model. New dispersion relations are found at moderate plasma $\beta$ and previous…

Plasma Physics · Physics 2014-07-16 Jacob R King , Scott E Kruger

Hyper-accreting discs occur in compact-object mergers and collapsars, and may power gamma-ray bursts (GRBs). We calculate the microscopic viscosity and resistivity of plasma in these discs, and discuss the implications for their global…

Astrophysics · Physics 2009-11-13 Elena M. Rossi , Philip J. Armitage , Kristen Menou

Two-dimensional transition-metal dichalcogenides (TMDs) are gaining increasing attention as alternative to graphene for their very high potential in optoelectronics applications. Here we consider two prototypical metallic 2D TMDs, NbSe$_2$…

Materials Science · Physics 2015-06-18 Pierluigi Cudazzo , Matteo Gatti , Angel Rubio

The transport of angular momentum is capital during the formation of low-mass stars; too little removal and rotation ensures stellar densities are never reached, too much and the absence of rotation means no protoplanetary disks can form.…

Solar and Stellar Astrophysics · Physics 2018-07-04 Neil Vaytet , Benoît Commerçon , Jacques Masson , Matthias González , Gilles Chabrier

Layered accretion is one of the inevitable ingredients in protoplanetary disks when disk turbulence is excited by magnetorotational instabilities (MRIs). In the accretion, disk surfaces where MRIs fully operate have a high value of disk…

Earth and Planetary Astrophysics · Physics 2015-12-23 Yasuhiro Hasegawa , Taku Takeuchi

A conclusive model for the formation of dwarf spheroidal (dSph) galaxies still remains elusive. Owing to their proximity to the massive spirals Milky Way (MW) and M31, various environmental processes have been invoked to explain their…

Astrophysics of Galaxies · Physics 2017-03-29 Stelios Kazantzidis , Lucio Mayer , Simone Callegari , Massimo Dotti , Leonidas A. Moustakas

Magnetic reconnection is a ubiquitous phenomenon for magnetized plasmas and leads to the rapid reconfiguration of magnetic field lines. During reconnection events, plasma is heated and accelerated until the magnetic field lines enclose and…

High Energy Astrophysical Phenomena · Physics 2023-11-15 Jesse Vos , Hector Olivares , Benoit Cerutti , Monika Moscibrodzka

Understanding how polymer topology influences melt extrudability is critical for advancing material design in extrusion-based additive manufacturing. In this work, we develop a bottom-up, cross-scale modeling framework that integrates…

We investigate the effect of shear viscosity and Ohmic resistivity on the magnetorotational instability (MRI) in vertically stratified accretion disks through a series of local simulations with the Athena code. First, we use a series of…

High Energy Astrophysical Phenomena · Physics 2015-05-20 Jacob B. Simon , John F. Hawley , Kris Beckwith

The role of polymers additives on the turbulent convective flow of a Rayleigh--Taylor system is investigated by means of direct numerical simulations (DNS) of Oldroyd-B viscoelastic model. The dynamics of polymers elongation follow…

Chaotic Dynamics · Physics 2015-05-27 G. Boffetta , A. Mazzino , S. Musacchio

Within the improved quantum molecular dynamic (ImQMD) model we follow the evolution of nuclear matter for planar Couette flow in a periodic box. We focus on the region of liquid-gas phase transition and extract the shear viscosity…

Nuclear Theory · Physics 2022-06-29 X. G. Den , P. Danielewicz , Y. G. Ma , H. Lin , Y. X. Zhang
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