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Efficient Solution-Processed Blue Electrophosphorescent Devices Based on a Novel Small-Molecule Host

Efficient Solution-Processed Blue Electrophosphorescent Devices Based on a Novel Small-Molecule Host
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摘要 Efficient blue small molecular phosphorescent fight-emitting diodes with a blue phosphorescent dye bis(3,5- difluoro-2-(2-pyridyl)-phenyl-(2-carboxypride) iridium (Ⅲ) (Flrpic) doped into a novel small-molecule host 9,9- bis[4-(3,6-di-tert-butylcarbazol-9-yl)phenyl] fluorene (TBCPF) as the light-emitting layer have been fabricated by spin-coating. The host TBCPF can form homogeneous amorphous films by spin-coating and has triplet energy higher than that of the blue phosphorescent dye Flrpic. All the devices with different Flrpic concentration in the emitting layer give emission from Flrpic indicating complete energy transfer from TBCPF to Flrpic. The device shows the best performance with a peak brightness of 8050 cd/m^2 at 10.2 V and the maximum current efficiency up to 3.52 cd/A, when the Flrpic doped concentration is as high as 16%. Efficient blue small molecular phosphorescent fight-emitting diodes with a blue phosphorescent dye bis(3,5- difluoro-2-(2-pyridyl)-phenyl-(2-carboxypride) iridium (Ⅲ) (Flrpic) doped into a novel small-molecule host 9,9- bis[4-(3,6-di-tert-butylcarbazol-9-yl)phenyl] fluorene (TBCPF) as the light-emitting layer have been fabricated by spin-coating. The host TBCPF can form homogeneous amorphous films by spin-coating and has triplet energy higher than that of the blue phosphorescent dye Flrpic. All the devices with different Flrpic concentration in the emitting layer give emission from Flrpic indicating complete energy transfer from TBCPF to Flrpic. The device shows the best performance with a peak brightness of 8050 cd/m^2 at 10.2 V and the maximum current efficiency up to 3.52 cd/A, when the Flrpic doped concentration is as high as 16%.
出处 《Chinese Physics Letters》 SCIE CAS CSCD 2008年第4期1457-1460,共4页 中国物理快报(英文版)
关键词 supernova explosion proto-neutron star shock wave supernova explosion, proto-neutron star, shock wave
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