We perform a comparative study of the quantum and classical transport probabilities of low-energy quasiparticles ballistically traversing normal and Andreev two-dimensional open cavities with a Sinai-billiard shape. We focus on the dependence of the transport on the strength of an applied magnetic field B. With increasing field strength the classical dynamics changes from mixed to regular phase space. Averaging out the quantum fluctuations, we find an excellent agreement between the quantum and classical transport coefficients in the complete range of field strengths. This allows an overall description of the non-monotonic behavior of the average magnetoconductance in terms of the corresponding classical trajectories, thus, establishing a b...
Umhlatuzana is an important archaeological site for the study of the Middle and Pleistocene Later St...
In-medium production of leading hadrons in hard reactions, carrying the main fraction of the jet mom...
Observations of the sun are almost always impaired by the turbulent motion of air in Earth's atmosph...
We perform a comparative study of the quantum and classical transport probabilities of low-energy qu...
We investigate, by means of numerical simulations, the lowest magnetic field level that can be detec...
The most prominent features on the surface of the solar disc are the sunspots, which have been studi...
Oriented precursors of MFCs consisting of HDPE and PA6 or PA12 are studied during strain-controlled ...
We consider the problem of compressing a Gaussian source for two decoders, one of which has access t...
The NuMI (Neutrinos at the Main Injector) facility produces an intense neutrino beam for experiments...
In this paper, we analyze the mean velocity profile and the Reynolds shear stress in a turbulent, in...
International audienceWhile engineers have been quantifying rainfall-runoff processes since the mid-...
We map out the detuning-magnetization phase diagram for a magnetized (unequal number of atoms in two...
Observed properties of Wolf-Rayet stars at high metallicity are reviewed. Wolf-Rayet stars are more ...
This documents presents the first version of the Bouclettes automatic parallelizer developed at LIP....
The BaBar electromagnetic calorimeter energy calibration method was compared with the local and glob...
Umhlatuzana is an important archaeological site for the study of the Middle and Pleistocene Later St...
In-medium production of leading hadrons in hard reactions, carrying the main fraction of the jet mom...
Observations of the sun are almost always impaired by the turbulent motion of air in Earth's atmosph...
We perform a comparative study of the quantum and classical transport probabilities of low-energy qu...
We investigate, by means of numerical simulations, the lowest magnetic field level that can be detec...
The most prominent features on the surface of the solar disc are the sunspots, which have been studi...
Oriented precursors of MFCs consisting of HDPE and PA6 or PA12 are studied during strain-controlled ...
We consider the problem of compressing a Gaussian source for two decoders, one of which has access t...
The NuMI (Neutrinos at the Main Injector) facility produces an intense neutrino beam for experiments...
In this paper, we analyze the mean velocity profile and the Reynolds shear stress in a turbulent, in...
International audienceWhile engineers have been quantifying rainfall-runoff processes since the mid-...
We map out the detuning-magnetization phase diagram for a magnetized (unequal number of atoms in two...
Observed properties of Wolf-Rayet stars at high metallicity are reviewed. Wolf-Rayet stars are more ...
This documents presents the first version of the Bouclettes automatic parallelizer developed at LIP....
The BaBar electromagnetic calorimeter energy calibration method was compared with the local and glob...
Umhlatuzana is an important archaeological site for the study of the Middle and Pleistocene Later St...
In-medium production of leading hadrons in hard reactions, carrying the main fraction of the jet mom...
Observations of the sun are almost always impaired by the turbulent motion of air in Earth's atmosph...