arXiv subjects

C. Steiner

Publications and source records attributed to C. Steiner.

3 recordsLinked to original sources

arXiv2022

Transport spectroscopy of ultraclean tunable band gaps in bilayer graphene

The importance of controlling both the charge carrier density and the band gap of a semiconductor cannot be overstated, as it opens the doors to a wide range of applications, including, e.g., highly-tunable transistors, photodetectors, and lasers. Bernal-stacked bilayer graphene is a unique van-der-Waals material that allows tuning the band gap by an out-of-plane electric field. Although the first evidence of the tunable gap was already found ten years ago, it took until recent to fabricate sufficiently clean heterostructures where the electrically induced gap could be used to fully suppress transport or confine charge carriers. Here, we present a detailed study of the tunable band gap in gated bilayer graphene characterized by temperature-activated transport and finite-bias spectroscopy measurements. The latter method allows comparing different gate materials and device technologies, which directly affects the disorder potential in bilayer graphene. We show that graphite-gated bilayer graphene exhibits extremely low disorder and as good as no subgap states resulting in ultraclean tunable band gaps up to 120 meV. The size of the band gaps are in good agreement with theory and allow complete current suppression making a wide range of semiconductor applications possible.

cond-mat.mes-hall↗

arXiv2013

Vlasov on GPU (VOG Project)

This work concerns the numerical simulation of the Vlasov-Poisson set of equations using semi- Lagrangian methods on Graphical Processing Units (GPU). To accomplish this goal, modifications to traditional methods had to be implemented. First and foremost, a reformulation of semi-Lagrangian methods is performed, which enables us to rewrite the governing equations as a circulant matrix operating on the vector of unknowns. This product calculation can be performed efficiently using FFT routines. Second, to overcome the limitation of single precision inherent in GPU, a δf type method is adopted which only needs refinement in specialized areas of phase space but not throughout. Thus, a GPU Vlasov-Poisson solver can indeed perform high precision simulations (since it uses very high order reconstruction methods and a large number of grid points in phase space). We show results for rather academic test cases on Landau damping and also for physically relevant phenomena such as the bump on tail instability and the simulation of Kinetic Electrostatic Electron Nonlinear (KEEN) waves.

physics.plasm-ph↗

arXiv2008

A deep INTEGRAL hard X-ray survey of the 3C 273/Coma region

(abridged) We present an analysis of the deepest hard X-ray survey to date of about 2500 deg^2 performed by the IBIS instrument on board INTEGRAL in the 20-60 keV band, with a total exposure time of 4 Ms. We find 34 candidate sources. The ratio of Seyfert 1 to Seyfert 2 is significantly more than the ratio found in the optical, which may be evidence for a receding torus, but could also be due to absorption columns > 10^{25} cm^{-2}. None of the predicted Compton-thick objects is detected unambiguously; when taking lower limits on Nh into account, the fraction of these objects is found to be lower than 24%. We do not see, but cannot exclude, a relationship between absorption and luminosity similar to what is seen in the 2-10 keV band. Our data suggests the possibility of a lack of objects with 10^{21} < Nh < 10^{22} cm^{-2}, as expected if absorption originates either in a torus-like structure or in the host galaxy. We find that the Log N-Log S diagram of our sources is compatible with those obtained in other surveys in hard X-rays. Compared to models of the AGN population selected in the 2-10 keV band, the Log N-Log S diagram is generally in good agreement, but the Nh distribution is significantly different, with significantly less unabsorbed sources (Nh<10^{22} cm^{-2}) at a given flux limit compared to the models. We resolve here about 2.5% of the cosmic X-ray background. We also study the local hard X-ray luminosity function, which is compatible with what is found in other recent hard X-ray surveys. The characteristic luminosity Log L*_{20-60 keV}=43.66 is found to be a factor about 5 lower than the value observed in the 2-10 keV band. We find a space density of 10^{-3} AGN with L>10^{41} per Mpc^3 and a corresponding luminosity density of 0.9 10^{39} erg s^{-1} Mpc^{-3}.

astro-ph↗