Magnetic Coupling of Ni, Cu and Co Bi- and Trilayers Probed by Magnetic Circular X-Ray Dichroism

1997 ◽  
Vol 7 (C2) ◽  
pp. C2-389-C2-395 ◽  
Author(s):  
F. May ◽  
M. Tischer ◽  
D. Arvanitis ◽  
J. Hunter Dunn ◽  
H. Henneken ◽  
...  
Keyword(s):  
2013 ◽  
Vol 773 (2) ◽  
pp. 142 ◽  
Author(s):  
Yang Luo ◽  
Wei-Min Gu ◽  
Tong Liu ◽  
Ju-Fu Lu

1987 ◽  
Vol 125 ◽  
pp. 67-78
Author(s):  
Ramesh Narayan

The radio pulsars in the Galaxy are found predominantly in the disk, with a scale height of several hundred parsecs. After allowing for pulsar velocities, the data are consistent with the hypothesis that single pulsars form from massive stellar progenitors. The number of active single pulsars in the Galaxy is ∼ 1.5 × 105, and their birthrate is 1 per ∼ 60 yrs. There is some evidence that many single pulsars, particularly those with high magnetic fields, are born spinning slowly, with initial periods ∼ 0.5–1s. This could imply an origin through binary “recycling” followed by orbit disruption, or might suggest that the pre-supernova stellar core efficiently loses angular momentum to the envelope through magnetic coupling. The birthrate of binary radio pulsars, particularly of the millisecond variety, seems to be much larger than previous estimates, and might suggest that these systems do not originate in low mass X-ray binary systems.


2010 ◽  
Vol 1256 ◽  
Author(s):  
Danilo G Barrionuevo ◽  
Surinder P Singh ◽  
Ram S Katiyar ◽  
Maharaj S. Tomar

AbstractMaterials which possess electrical and magnetic coupling are of great interest for novel devices. Bi(Fe1-xCox)O3 (BFCO) material system was synthesized by solution route for various compositions and thin films were prepared by spin coating on Pt (Pt/Ti/SiO2/Si) substrates. Structural properties of the films were investigated by x-ray diffraction and Raman spectroscopy. X-ray diffraction patterns confirms intense (110) in BiFeO3 and Bi(Fe1-xCox)O3 with rhombohedra distorted perovskite structure without impure phase. Bi(Fe1-xCox)O3 films show week ferroelectric polarization and ferromagnetism at room temperature. Ferroelectric and ferromagnetic coupling could be attributed to the elimination of oxygen vacancies and increased stress in the crystal structure by partial replacement of Fe2+ ion by Co2+ ion.


2013 ◽  
Vol 4 ◽  
pp. 320-324 ◽  
Author(s):  
David Klar ◽  
Svetlana Klyatskaya ◽  
Andrea Candini ◽  
Bernhard Krumme ◽  
Kurt Kummer ◽  
...  

The magnetic and electronic properties of single-molecule magnets are studied by X-ray absorption spectroscopy and X-ray magnetic circular dichroism. We study the magnetic coupling of ultrathin Co and Ni films that are epitaxially grown onto a Cu(100) substrate, to an in situ deposited submonolayer of TbPc2 molecules. Because of the element specificity of the X-ray absorption spectroscopy we are able to individually determine the field dependence of the magnetization of the Tb ions and the Ni or Co film. On both substrates the TbPc2 molecules couple antiferromagnetically to the ferromagnetic films, which is possibly due to a superexchange interaction via the phthalocyanine ligand that contacts the magnetic surface.


1989 ◽  
Vol 173 ◽  
Author(s):  
Kunio Awaga ◽  
Tamotsu Inabe ◽  
Yusei Maruyama

ABSTRACTThe temperature dependence of the magnetic susceptibilities for several ±-nitronyl nitroxides have been measured. It is found that the intermolecular magnetic coupling in these radical crystals changes from antiferromagnetic to ferromagnetic depending on the substituents at ±-position. X-Ray crystal analysis and MO calculation have been carried out on the ferromagnetic ±-nitronyl nitroxide, 2-(4-nitrophenyl)-4,4,5,5-tetramethyl-4,5-dihydro-1H-imidazolyl-1-oxy 3-oxide, revealing a two-dimensional ferromagnetic network linked by the Nδ+...0δ− Coulomb attraction.


2001 ◽  
Vol 37 (4) ◽  
pp. 1661-1663 ◽  
Author(s):  
K. Chesnel ◽  
M. Belakhovsky ◽  
S. Landis ◽  
B. Rodmacq ◽  
E. Dudzik ◽  
...  

2002 ◽  
Vol 66 (2) ◽  
Author(s):  
K. Chesnel ◽  
M. Belakhovsky ◽  
S. Landis ◽  
J. C. Toussaint ◽  
S. P. Collins ◽  
...  

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