output
20022009
most citedMott Insulators in the Strong Spin-Orbit Coupling Limit: From Heisenberg to a Quantum Compass and Kitaev Models

2.3k citations

Showing 2006 · astro-phShow all

68 papers · 2 filters

astro-ph2006

Forced oscillations in relativistic accretion disks and QPOs

J. Petri

In this work we explore the idea that the high frequency QPOs observed in LMXBs may be explained as a resonant coupling between the neutron star spin and epicyclic modes of accreti…

astro-ph200613 cited

A low density of the Extragalactic Background Light revealed by the H.E.S.S. spectra of the BLLac objects 1ES 1101-232 and H 2356-309

L. Costamante

The unexpectedly hard spectra measured by HESS for the BLLacs 1ES 1101-232 and H 2356-309 has allowed an upper limit on the Extragalactic Background Light (EBL) to be derived in th…

astro-ph2006

Neutrino-driven wind and wind termination shock in supernova cores

A. Arcones, L. Scheck, H. -Th. Janka

The neutrino-driven wind from a nascent neutron star at the center of a supernova expands into the earlier ejecta of the explosion. Upon collision with this slower matter the wind…

astro-ph200627 cited

Testing non-linear force-free coronal magnetic field extrapolations with the Titov-Demoulin equilibrium

Thomas Wiegelmann, Bernd Inhester, Bernhard Kliem +2

CONTEXT: As the coronal magnetic field can usually not be measured directly, it has to be extrapolated from photospheric measurements into the corona. AIMS: We test the quality of…

astro-ph200645 cited

Stereoscopy basics for the STEREO mission

Bernd Inhester

We discuss some basic principles of stereoscopy and their relevance to the reconstruction of coronal loops. The aim of the paper is to make the solar physicist familiar with basic…

astro-ph2006432 cited

Preprocessing of vector magnetograph data for a non-linear force-free magnetic field reconstruction

Thomas Wiegelmann, Bernd Inhester, Takashi Sakurai

Knowledge regarding the coronal magnetic field is important for the understanding of many phenomena, like flares and coronal mass ejections. Because of the low plasma beta in the s…