most citedWeak ferromagnetism and spiral spin structures in honeycomb Hubbard planes

10 citations

6 papers

astro-ph20051 cited

Global MHD Modelling of the ISM - From large towards small scale turbulence

Miguel A. de Avillez, Dieter Breitschwerdt

Dealing numerically with the turbulent nature and non-linearity of the physical processes involved in the ISM requires the use of sophisticated numerical schemes coupled to HD and…

astro-ph20051 cited

Disk-Halo-Disk Circulation and the Evolution of the ISM - 3D HD and MHD Adaptive Mesh Refinement Simulations

M. A. de Avillez, Dieter Breitschwerdt

State of the art models of the ISM use adaptive mesh refinement to capture small scale structures, by refining on the fly those regions of the grid where density and pressure gradi…

cond-mat.str-el200510 cited

Weak ferromagnetism and spiral spin structures in honeycomb Hubbard planes

M A N Araujo, N M R Peres

Within the Hartree Fock- RPA analysis, we derive the spin wave spectrum for the weak ferromagnetic phase of the Hubbard model on the honeycomb lattice. Assuming a uniform magnetiza…

astro-ph2005

Ovi Column Density Distribution in the Local Bubble - Results from 3D Adaptive Mesh Refinement Simulations

Miguel A. de Avillez, Dieter Breitschwerdt

The Local Bubble (LB) is an X-ray emitting region extending 100 pc in radius in the Galactic plane and 300 pc perpendicular to it, and it is embedded in a somewhat larger H{\sc i}…

astro-ph20052 cited

Keynote Lecture: Galactic and Extragalactic Bubbles

D. Breitschwerdt, M. A. de Avillez, M. J. Freyberg

The observational and theoretical state of Galactic and extragalactic bubbles are reviewed. Observations of superbubbles are discussed, with some emphasis on nearby bubbles such as…

astro-ph2004

3D Simulations of the Local Bubble

Dieter Breitschwerdt, Miguel A. de Avillez

We have performed high resolution 3D simulations of the Local Bubble (with 1.25 pc finest resolution) in a realistic background ISM, jointly with the dynamical evolution of the nei…