97 resultados para DY-3
Resumo:
Dy^3+Ge-GaSe-<r>26713m440-530s273
Resumo:
Ce~(3+), Dy~(3+), Eu~(3+), CuCaS:Ce~(3)Cas: Dy~(3+)CaS:Dy~(3+)Dy~(3+)Dy~(3+)CaS:Ce~(3+)Dy~(3+)Ce~(3+)Dy~(3+)Dy~(3+) Ce~(3+)CaS:CuCu~+CuCaS:CuUV3bb nm)Cu~+Cu~(2+)EPRCu'_(Ca)Cu_i~+CaS:Ce~(3+),CuCuCe~(3+)CaS:Eu~(2+)Eu~(2+)CaS:Ce~(3+), CaS:Dy~(3+), CaS:CuCaS:Ce~(3+), CuCaS:Ce~(3+)V_S~(2+)CaS:Dy~(3+)V_S~(2+)-V_(Ca)~(2-)CaS:CuCaS:Ce~(3+), CuV_S~(2+)Cu'_(Ca)
Resumo:
SrAl2 B2 O7:Dy3+BaAl2 B2 O7:Dy3+SrAl3BO7:Dy3+La2 CaB10 O19:Dy3+- (UVVUV)UVDy3+ (Y/B)VUVDy3+f-d(CTS)
Resumo:
:Eu2 + ,Dy3 + , , , 5 16nm ,Eu2 + 5d 8S7/ 2 12 0 0 0lx 2 0 , 10 , 3 5 3cd/m2 , :x =0 2 84 2 ,y =0 5 772 ; 5 5 5 , 0 0 1cd/m2 ; 30 , ,
Resumo:
R3GeVO9(R =Y ,La) ,Eu3+Dy3+ ,Eu3+Eu3+R3GeVO9(R =Y ,La) ,R3+Z/rEu3+Dy3+Bi3+
Resumo:
R_2O_3(R=Y,Gd,La),V_2O_6,Nb_2O_5RVMb_2O_3,Eu~(3+)Dy~(3+).,Eu~(3+),Eu~(3+)/(R/O)Dy~(3+)/(Y/B)R~(3+).Bi~(3+)Dy~(3+).
Resumo:
Various borates, vanadates, niobates, antimonates, titanates, zirconates and CaS doped with Dy3+ were prepared. Factors which have an effect on the yellow-to-blue intensity ratio (Y/B) of Dy3+ emission are reported. Y/B increases with decreasing Z/r or electronegativity of the next-neighbour element M in the complex oxides Dy-O-M. The greater the degree of covalency between Dy3+ and O2-, the greater Y/B is. When Dy3+ is located at a site with an inverse centre and high symmetry, Dy3+ displays no luminescence. It seems that Y/B of Dy3+ located at a site deviated from an inverse centre is greater than that of Dy3+ located at a site without an inverse centre. Y/B does not vary much with the variation in concentration of Dy3+ when Dy3+ is substituted for an element with the same valency, but it does depend on the concentration of Dy3+ when Dy3+ is substituted for an element with a different valency in the matrix, because defects are formed in this case.
Resumo:
YP_xV_(1-x)O_4(0x1):Dy~(3+)YP_xV_(1-x)O_4(0x1),xStokesx,YP_xV_(1-x)O_4:0.006Dy~(3+),x>0.4P0_4~(3-)Dy~(3+)Dy~(3+)xBi~(3+)Dy~(3+)
Resumo:
Eu~(3+)D~(3+)YV_(1-x)B_xO_(4-x):B~(3+)V~(5+),Dy~(3+),B~(3+)Y~(3+),Dy~(3+)Bi~(3+)YV_(0.69)B_(0.31)O_(3.69):Dy~(3+)Dy~(3+)
Resumo:
Y_(0.5-x)Li_(1.5)VO_4:(Dy~(3+),Eu~(3+))_x,. (Y_2O_3Dy_2O_3Eu_2O_3)99.99V_2O_5Li_2CO_3,
Resumo:
60ABO_380 SrivastavaGdBO_3pr~(3+)Gd~(3+)Pr~(3+),
Resumo:
Eu~(3+),Dy~(3+)Ba_2RV_3O_(11)(R=Y,Gd,La)Bi~(3+)Dy~(3+)Dy~(3+).R~(3+)(R=Y,Gd,La)Eu~(3+)Dy~(3+),Dy~(3+).
Resumo:
In this paper, the yellow-to-blue intensity ratio of Dy3+ (Y/B) and the red-to-orange intensity ratio of Eu3+ (R/O) were studied in relation to the compositions and structures of alkaline-earth borates. The dependence of the energy of the Eu3+ charge-transfer band (CTB) and of the emission intensity of Dy3+ on the alkaline-earth ions and the boron content of the hosts is discussed.
Resumo:
(Tb~(3+)Tb~(3+)+Gd~(3+)Tb~(3+)+Dy~(3+)Tb~(3+)+Bi~(3+)Tb~(3+)Gd~(3+)Dy~(3+)Bj~(3+)Tb~(3+)B_2O_2-BaO-M_mO_n(M_mO_n=Li_2ONa_2OK_2OMgOCaOSrOAl_2O_3La_2O_3Bi_2O_3),M_mO_nMgOAl_2O_3,Tb~(3+);M_mO-nBi_2O_3,Tb~(3+)Tb~(3+)Gd~(3+)Dy~(3+)Bi~(3+)Tb~(3+)Gd~(3+),Tb~(3+)13.8,,
