scholarly journals Inter-grain Phase Transitions in Superconducting Ceramic YBa2Cu3O7−δ under Low Magnetic Fields

Author(s):  
Hiroyuki Deguchi ◽  
Takanori Fujii ◽  
Yuki Kato ◽  
Masaki Mito ◽  
Akihiko Hisada ◽  
...  
2020 ◽  
Vol 34 (13) ◽  
pp. 2050129
Author(s):  
Erhan Albayrak

The A, B and C atoms with spin-1/2, spin-3/2 and spin-5/2 are joined together sequentially on the Bethe lattice in the form of ABCABC[Formula: see text] to simulate a molecule as a triple mixed-spin system. The spins are assumed to be interacting with only their nearest-neighbors via bilinear exchange interaction parameter in addition to crystal and external magnetic fields. The order-parameters are obtained in terms of exact recursion relations, then from the study of their thermal variations, the phase diagrams are calculated on the possible planes of our system. It is found that the model gives only second-order phase transitions in addition to the compensation temperatures.


1981 ◽  
Vol 2 (1) ◽  
pp. 67-73 ◽  
Author(s):  
S. Juszczyk ◽  
J. Krok ◽  
I. Okońska-Kozłowska ◽  
H. Broda ◽  
J. Warczewski ◽  
...  

1997 ◽  
Vol 55 (8) ◽  
pp. 4582-4590 ◽  
Author(s):  
Günter Sigl ◽  
Angela V. Olinto ◽  
Karsten Jedamzik

2008 ◽  
Vol 4 (S259) ◽  
pp. 529-538 ◽  
Author(s):  
Eduardo Battaner ◽  
Estrella Florido

AbstractThere is increasing evidence that intense magnetic fields exist at large redshifts. They could arise after galaxy formation or in very early processes, such as inflation or cosmological phase transitions, or both. Early co-moving magnetic strengths in the range 1-10 nG could be present at recombination. The possibilities to detect them in future CMB experiments are discussed, mainly considering their impact in the anisotropy spectra as a result of Faraday rotation and Alfven waves. Magnetic fields this magnitude could also have a non-negligible influence in determining the filamentary large scale structure of the Universe.


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