On Perturbed Two-Dimensional Dirac Operators

2016 ◽  
Vol 41 (3) ◽  
pp. 1249-1263
Author(s):  
Suo Zhao
2017 ◽  
Vol 50 (1) ◽  
pp. 66-71
Author(s):  
Andrzej Sitarz

Abstract We investigate examples of Gauss-Bonnet theorem and the scalar curvature for the two-dimensional commutative sphere with quasi-spectral triples obtained by modifying the order-one condition.


2020 ◽  
Vol 279 (8) ◽  
pp. 108700
Author(s):  
Jussi Behrndt ◽  
Markus Holzmann ◽  
Thomas Ourmières-Bonafos ◽  
Konstantin Pankrashkin

2017 ◽  
Vol 18 (4) ◽  
pp. 1371-1383 ◽  
Author(s):  
Rafael D. Benguria ◽  
Søren Fournais ◽  
Edgardo Stockmeyer ◽  
Hanne Van Den Bosch

1966 ◽  
Vol 24 ◽  
pp. 118-119
Author(s):  
Th. Schmidt-Kaler

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.


1966 ◽  
Vol 24 ◽  
pp. 3-5
Author(s):  
W. W. Morgan

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.


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