Chaotic dynamics and basin erosion in nanomagnets subject to time-harmonic magnetic fields

2016 ◽  
Vol 486 ◽  
pp. 121-125 ◽  
Author(s):  
M. d'Aquino ◽  
A. Quercia ◽  
C. Serpico ◽  
G. Bertotti ◽  
I.D. Mayergoyz ◽  
...  

2015 ◽  
Vol 29 (35n36) ◽  
pp. 1550248
Author(s):  
Hai-Feng Yang ◽  
Yong-Gang Tan ◽  
Zhong-Li Liu ◽  
Hong-Zhi Fu

In this paper, the statistical properties of energy levels are studied numerically for atom in parallel electric and magnetic fields, which is an ideal system to examine the contributions of external fields and ionic core to quantum chaos. The Stark maps of diamagnetic spectra and nearest neighbor spacing (NNS) distributions are obtained by diagonalization method incorporating core effect. We identify obvious level anti-crossing and large value of [Formula: see text] for barium, indicating that core effect has predominant contribution to chaotic dynamics in barium. To study the core effect in detail, we sweep the quantum defect artificially and find that larger core effect will undoubtedly induce stronger chaotic dynamics.



2010 ◽  
Vol 172 (2) ◽  
pp. 55-63
Author(s):  
Kenji Miyata ◽  
Kazumasa Ide ◽  
Kazuo Shima






1990 ◽  
Vol 64 (13) ◽  
pp. 1581-1584 ◽  
Author(s):  
T. Geisel ◽  
J. Wagenhuber ◽  
P. Niebauer ◽  
G. Obermair


2017 ◽  
Vol 63 (3) ◽  
pp. 455-474
Author(s):  
V Z Grines ◽  
E V Zhuzhoma ◽  
O V Pochinka

We discuss application of contemporary methods of the theory of dynamical systems with regular and chaotic hyperbolic dynamics to investigation of topological structure of magnetic fields in conducting media. For substantial classes of magnetic fields, we consider well-known physical models allowing us to reduce investigation of such fields to study of vector fields and Morse-Smale diffeomorphisms as well as diffeomorphisms with nontrivial basic sets satisfying the A axiom introduced by Smale. For the point-charge magnetic field model, we consider the problem of separator playing an important role in the reconnection processes and investigate relations between its singularities. We consider the class of magnetic fields in the solar corona and solve the problem of topological equivalency of fields in this class. We develop a topological modification of the Zeldovich funicular model of the nondissipative cinematic dynamo, constructing a hyperbolic diffeomorphism with chaotic dynamics that is conservative in the neighborhood of its transitive invariant set.



1994 ◽  
Vol 144 ◽  
pp. 559-564
Author(s):  
P. Ambrož ◽  
J. Sýkora

AbstractWe were successful in observing the solar corona during five solar eclipses (1973-1991). For the eclipse days the coronal magnetic field was calculated by extrapolation from the photosphere. Comparison of the observed and calculated coronal structures is carried out and some peculiarities of this comparison, related to the different phases of the solar cycle, are presented.



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