Crystal-field spectrum of R 1-y Ca y Ba 2 Cu 3 O x high-T c superconductors in the overdoped regime

2002 ◽  
Vol 74 (0) ◽  
pp. s1019-s1021 ◽  
Author(s):  
A. Mirmelstein ◽  
A. Podlesnyak ◽  
V. Bobrovskii ◽  
N. Golosova
Keyword(s):  
Crystal Field ◽  
Field Spectrum

Crystal-field spectrum of γ-Ni2SiO4

1996 ◽  
Vol 8 (3) ◽  
pp. 471-476 ◽  
Author(s):  
Stéphanie Rossano ◽  
Laurence Galoisy ◽  
Gabriel Gwamnesia
Keyword(s):  
Crystal Field ◽  
Field Spectrum

The influence of Th substitution on the crystal structure and the crystal field spectrum of the high-Tc superconductor HoBa2Cu3O6.95

2004 ◽  
Vol 350 (1-3) ◽  
pp. E335-E337
Author(s):  
N Golosova ◽  
A Mirmelstein ◽  
V Bobrovskii ◽  
E Mitberg ◽  
A Podlesnyak ◽  
...  
Keyword(s):  
Crystal Structure ◽  
Crystal Field ◽  
High Tc ◽  
High Tc Superconductor ◽  
Field Spectrum

Crystal-field spectrum and linewidths in the heavy-fermion systemPrInAg2

2000 ◽  
Vol 61 (3) ◽  
pp. 1831-1835 ◽  
Author(s):  
T. M. Kelley ◽  
W. P. Beyermann ◽  
R. A. Robinson ◽  
F. Trouw ◽  
P. C. Canfield ◽  
...  
Keyword(s):  
Crystal Field ◽  
Heavy Fermion ◽  
Field Spectrum

Crystal-field spectrum in RBa2Cu3Ox(R = Er, Ho) high-Tcsuperconductors: evidence for charge order in CuO2planes

1999 ◽  
Vol 11 (37) ◽  
pp. 7155-7173 ◽  
Author(s):  
A Mirmelstein ◽  
A Podlesnyak ◽  
V Bobrovskii ◽  
I Zhdakhin
Keyword(s):  
Crystal Field ◽  
Charge Order ◽  
Field Spectrum

The effect of Ca and Th substitution on the crystal-field spectrum of the high-Tcsuperconductor HoBa2Cu3Ox

2002 ◽  
Vol 14 (8) ◽  
pp. 1923-1936 ◽  
Author(s):  
N Golosova ◽  
A Podlesnyak ◽  
E Mitberg ◽  
V Bobrovskii ◽  
A Mirmelstein ◽  
...  
Keyword(s):  
Crystal Field ◽  
Field Spectrum

Peculiarity Parameters

1976 ◽  
Vol 32 ◽  
pp. 233-254
Author(s):  
H. M. Maitzen
Keyword(s):  
Magnetic Field ◽  
Magnetic Fields ◽  
Theoretical Work ◽  
Observational Evidence ◽  
Rotator Model ◽  
Peculiar Behaviour ◽  
Field Spectrum ◽  
Oblique Rotator ◽  
Ap Stars ◽  
The Way

Ap stars are peculiar in many aspects. During this century astronomers have been trying to collect data about these and have found a confusing variety of peculiar behaviour even from star to star that Struve stated in 1942 that at least we know that these phenomena are not supernatural. A real push to start deeper theoretical work on Ap stars was given by an additional observational evidence, namely the discovery of magnetic fields on these stars by Babcock (1947). This originated the concept that magnetic fields are the cause for spectroscopic and photometric peculiarities. Great leaps for the astronomical mankind were the Oblique Rotator model by Stibbs (1950) and Deutsch (1954), which by the way provided mathematical tools for the later handling pulsar geometries, anti the discovery of phase coincidence of the extrema of magnetic field, spectrum and photometric variations (e.g. Jarzebowski, 1960).

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