scholarly journals Large spectral gap and impurity-induced states in a two-dimensional Abrikosov vortex

2021 ◽  
Vol 103 (2) ◽  
Author(s):  
A. A. Bespalov ◽  
V. D. Plastovets
Keyword(s):  
Spectral Gap ◽  
Abrikosov Vortex ◽  
Two Dimensional

Accelerating diffusion on compact Riemannian surfaces by incompressible drift

2016 ◽  
Vol 15 (05) ◽  
pp. 653-666
Author(s):  
Brice Franke ◽  
Nejib Yaakoubi
Keyword(s):  
Incompressible Fluid ◽  
Uniform Distribution ◽  
Vector Fields ◽  
Spectral Gap ◽  
Brownian Particle ◽  
Fluid Motion ◽  
Convergence To Equilibrium ◽  
Two Dimensional ◽  
Riemannian Surfaces ◽  
Divergence Free Vector

We construct divergence free vector-fields on compact Riemannian surfaces which push the spectral gap of some diffusion generator above some prescribed value. The resulting diffusion describes some Brownian particle in a stationary incompressible fluid. The spectral gap is an indicator for the speed at which this diffusion converges toward its equilibrium, which corresponds to the uniform distribution. In other terms, we describe efficient fluid motion, to accelerate the convergence to equilibrium of some Brownian particle in a two-dimensional liquid.

Two-dimensional Abrikosov-vortex microclusters: Shell structure and melting

1997 ◽  
Vol 39 (6) ◽  
pp. 901-906
Author(s):  
Yu. E. Lozovik ◽  
E. A. Rakoch
Keyword(s):  
Shell Structure ◽  
Abrikosov Vortex ◽  
Two Dimensional

scholarly journals Continuous thermal melting of a two-dimensional Abrikosov vortex solid

2010 ◽  
Vol 82 (18) ◽  
Author(s):  
J. Iaconis ◽  
R. G. Melko ◽  
A. A. Burkov
Keyword(s):  
Abrikosov Vortex ◽  
Two Dimensional ◽  
Thermal Melting

Spectrophotometric measurements of objective-prism spectra

1966 ◽  
Vol 24 ◽  
pp. 118-119
Author(s):  
Th. Schmidt-Kaler
Keyword(s):  
Progress Report ◽  
Two Dimensional ◽  
Objective Prism ◽  
Made In

I should like to give you a very condensed progress report on some spectrophotometric measurements of objective-prism spectra made in collaboration with H. Leicher at Bonn. The procedure used is almost completely automatic. The measurements are made with the help of a semi-automatic fully digitized registering microphotometer constructed by Hög-Hamburg. The reductions are carried out with the aid of a number of interconnected programmes written for the computer IBM 7090, beginning with the output of the photometer in the form of punched cards and ending with the printing-out of the final two-dimensional classifications.

Introductory paper

1966 ◽  
Vol 24 ◽  
pp. 3-5
Author(s):  
W. W. Morgan
Keyword(s):  
Line Intensity ◽  
Classification Scheme ◽  
Two Dimensional ◽  
Spectral Classification ◽  
Dimensional Array ◽  
Rr Lyrae ◽  
Metallic Line ◽  
Introductory Paper ◽  
Parameter Varying ◽  
Definition Of

1. The definition of “normal” stars in spectral classification changes with time; at the time of the publication of theYerkes Spectral Atlasthe term “normal” was applied to stars whose spectra could be fitted smoothly into a two-dimensional array. Thus, at that time, weak-lined spectra (RR Lyrae and HD 140283) would have been considered peculiar. At the present time we would tend to classify such spectra as “normal”—in a more complicated classification scheme which would have a parameter varying with metallic-line intensity within a specific spectral subdivision.

Sign in / Sign up

Export Citation Format

Share Document