Tweaking the red emission, magneto, and dielectrical properties of perovskite type-LaFeO3 in the presence of Co substitution

2020 ◽  
Vol 31 (10) ◽  
pp. 7998-8014
Author(s):  
Ramesh Kumar Raji ◽  
Vishista Kurapati ◽  
Tholkappiyan Ramachandran ◽  
M. Muralidharan ◽  
R. Suriakarthick ◽  
...  
2021 ◽  
Author(s):  
Jiao Wu ◽  
Bo Wang ◽  
Zhiyuan Liu ◽  
Kang Zhang ◽  
Xiaoshuang Li ◽  
...  

Mn4+-activated oxidefluoride phosphors are attractive for application in wide solid-state lighting devices because of its distinct red emission at about 630 nm and the abundant storage of Mn4+ ion. However,...


RSC Advances ◽  
2020 ◽  
Vol 10 (32) ◽  
pp. 19020-19026 ◽  
Author(s):  
Mirosław Mączka ◽  
Anna Gągor ◽  
Adam Pikul ◽  
Dagmara Stefańska

The first perovskite-type hypophosphite-linked dense metal–organic framework exhibiting red emission and antiferromagnetic order at 6.5 K.


2001 ◽  
Vol 16 (9) ◽  
pp. 2568-2571 ◽  
Author(s):  
J. K. Park ◽  
C. H. Kim ◽  
K. J. Choi ◽  
H. D. Park ◽  
S. Y. Choi

The purpose of this study is to develop an understanding of the photoluminescence properties of Al3+, Pr3+ doped perovskite-type La2/3TiO3 and pyrochlore-type La2Ti2O7 phosphor, which is characterized by the red emission (1D2 →3H4 transition) of the Pr3+ ion. The explanation for the energy transfer and the corresponding critical distance is proposed on the basis of the role of Al3+ ions in the perovskite-type La2/3TiO3:Pr phosphor. To clarify the distinction of photoluminescence properties between the perovskite-type La2/3TiO3 and the pyrochlore-type La2Ti2O7, the trap-involved process and the charge transfer band have been investigated, respectively.


ChemInform ◽  
2010 ◽  
Vol 25 (50) ◽  
pp. no-no
Author(s):  
N. M. OLEKHNOVICH ◽  
T. E. ZHABKO ◽  
A. N. SALAK ◽  
O. I. PASHKOVSKII ◽  
A. D. SHILIN ◽  
...  

1994 ◽  
Vol 144 ◽  
pp. 597-599 ◽  
Author(s):  
I. V. Alexeyeva ◽  
N. L. Kroussanova ◽  
M. V. Streltsova

AbstractThe results of photometry of colour positives of the solar corona of July 11, 1991 are presented. Observations of the white corona were made without radial niters in Jojutla (Mexico). Dependences of coronal brightness on distance in the red (640 nm) and blue (420 nm) wavelength intervals are deduced for different coronal structures up to 3.0-3.5R⊙. The effect of ”reddening“ is noted. The excess of the red emission to the blue one (I640nm/I420nm) is found to be 1.20 and 1.17 at distance of 2.2R⊙for the N-E helmet streamer (P ≃ 37°) and the N-W region of low brightness (P ≃ 339°), respectively.


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