scholarly journals Dynamics of Domain Boundary with the Complex Internal Structure of the Cylindrical Magnetic Domain in External Magnetic Fields

2012 ◽  
Vol 13 (3) ◽  
pp. 225-240 ◽  
Author(s):  
A. B. Shevchenko
2019 ◽  
Vol 10 (1) ◽  
Author(s):  
Dafei Jin ◽  
Yang Xia ◽  
Thomas Christensen ◽  
Matthew Freeman ◽  
Siqi Wang ◽  
...  

Abstract Two-dimensional topological materials bearing time reversal-breaking magnetic fields support protected one-way edge modes. Normally, these edge modes adhere to physical edges where material properties change abruptly. However, even in homogeneous materials, topology still permits a unique form of edge modes – kink modes – residing at the domain boundaries of magnetic fields within the materials. This scenario, despite being predicted in theory, has rarely been demonstrated experimentally. Here, we report our observation of topologically-protected high-frequency kink modes – kink magnetoplasmons (KMPs) – in a GaAs/AlGaAs two-dimensional electron gas (2DEG) system. These KMPs arise at a domain boundary projected from an externally-patterned magnetic field onto a uniform 2DEG. They propagate unidirectionally along the boundary, protected by a difference of gap Chern numbers ($$\pm1$$ ± 1 ) in the two domains. They exhibit large tunability under an applied magnetic field or gate voltage, and clear signatures of nonreciprocity even under weak-coupling to evanescent photons.


Symmetry ◽  
2018 ◽  
Vol 10 (10) ◽  
pp. 513 ◽  
Author(s):  
Arbab Arbab ◽  
Mudhahir Al Ajmi

A quaternionic commutator bracket for position and momentum shows that the quaternionic wave function, viz. ψ ˜ = ( i c ψ 0 , ψ → ) , represents a state of a particle with orbital angular momentum, L = 3 ℏ , resulting from the internal structure of the particle. This angular momentum can be attributed to spin of the particle. The vector ψ → , points in an opposite direction of L → . When a charged particle is placed in an electromagnetic field, the interaction energy reveals that the magnetic moments interact with the electric and magnetic fields giving rise to terms similar to Aharonov–Bohm and Aharonov–Casher effects.


2015 ◽  
Vol 106 (7) ◽  
pp. 072408 ◽  
Author(s):  
S. Zohar ◽  
Y. Choi ◽  
D. M. Love ◽  
R. Mansell ◽  
C. H. W. Barnes ◽  
...  

2008 ◽  
Vol 103 (7) ◽  
pp. 073906 ◽  
Author(s):  
Matthew T. Bryan ◽  
Thomas Schrefl ◽  
Del Atkinson ◽  
Dan A. Allwood

2021 ◽  
Vol 12 (1) ◽  
Author(s):  
Zhuolin Li ◽  
Jian Su ◽  
Shi-Zeng Lin ◽  
Dan Liu ◽  
Yang Gao ◽  
...  

AbstractExploring and controlling topological textures such as merons and skyrmions has attracted enormous interests from the perspective of fundamental research and spintronic applications. It has been predicted theoretically and proved experimentally that the lattice form of topological meron-skyrmion transformation can be realized with the requirement of external magnetic fields in chiral ferromagnets. However, such topological transition behavior has yet to be verified in other materials. Here, we report real-space observation of magnetic topology transformation between meron pairs and skyrmions in the localized domain wall of ferrimagnetic GdFeCo films without the need of magnetic fields. The topological transformation in the domain wall of ferrimagnet is introduced by temperature-induced spin reorientation transition (SRT) and the underlying mechanism is revealed by micromagnetic simulations. The convenient electric-controlling topology transformation and driving motion along the confined domain wall is further anticipated, which will enable advanced application in magnetic devices.


1986 ◽  
Vol 90 ◽  
pp. 1-10
Author(s):  
David Moss

AbstractRival theories for the origin of the magnetic fields present in the CP stars are discussed, particular attention being paid to the claims of the ‘contemporary dynamo’ and ‘fossil’ theories. The internal structure of the field as predicted by calculations consistent with the fossil theory is discussed at length. It seems that current time dependent models can now give a coherent picture of the fields of the CP stars according to the fossil theory. Dynamo theory modelling has not been developed in such detail. As yet neither the theoretical predictions nor the observational material seem to be detailed enough to allow a decisive comparison between the theories.


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