2021
DOI: 10.1038/s41566-020-00744-0
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Organic phosphors with bright triplet excitons for efficient X-ray-excited luminescence

Abstract: Materials that exhibit X-ray excited luminescence have great potential in radiation detection, security inspection, biomedical applications, and X-ray astronomy [1][2][3][4] . However, such materials are almost exclusively limited to inorganic crystals, which are typically prepared under high temperatures 5 . Herein, we report a design principle of purely organic phosphors to boost X-ray excited luminescence with sufficient utilization of triplet excitons. Our experimental data reveal that proportion of emissi… Show more

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Cited by 300 publications
(243 citation statements)
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“…Namely, the ultralong RTP in aromatic hydrocarbon materials is extremely rare, ( Clapp, 1939 ; Bilen et al, 1978 ), because of the forbidden intersystem crossing (ISC) process between singlet and triplet excited states. To overcome this issue, the heavy atoms (eg., Br and I) ( Cai et al, 2018 ; Wang et al, 2021b ) and carbonyl groups ( Zhao et al, 2016 ; Jia et al, 2020 ) were incorporated into organic molecules to promote ISC process for achieving ultralong RTP, in combination with the suppression of the nonradiative quenching through rigid environment, ( Wu et al, 2020 ; Zheng et al, 2020 ; Zhou et al, 2020 ; Chen et al, 2021 ; Xie et al, 2021 ), such as crystal engineering and host-guest system. Very recently, Bechtold et al reported that the nonplanar aromatic hydrocarbon, named as 5,6,11,12,17,18-hexahydrobenzo [2,1-p]chrysene (HD), ( Salla et al, 2019 ), can show an ultralong RTP, which was attributed to the pronounced SOC induced by non-planar configuration.…”
Section: Introductionmentioning
confidence: 99%
“…Namely, the ultralong RTP in aromatic hydrocarbon materials is extremely rare, ( Clapp, 1939 ; Bilen et al, 1978 ), because of the forbidden intersystem crossing (ISC) process between singlet and triplet excited states. To overcome this issue, the heavy atoms (eg., Br and I) ( Cai et al, 2018 ; Wang et al, 2021b ) and carbonyl groups ( Zhao et al, 2016 ; Jia et al, 2020 ) were incorporated into organic molecules to promote ISC process for achieving ultralong RTP, in combination with the suppression of the nonradiative quenching through rigid environment, ( Wu et al, 2020 ; Zheng et al, 2020 ; Zhou et al, 2020 ; Chen et al, 2021 ; Xie et al, 2021 ), such as crystal engineering and host-guest system. Very recently, Bechtold et al reported that the nonplanar aromatic hydrocarbon, named as 5,6,11,12,17,18-hexahydrobenzo [2,1-p]chrysene (HD), ( Salla et al, 2019 ), can show an ultralong RTP, which was attributed to the pronounced SOC induced by non-planar configuration.…”
Section: Introductionmentioning
confidence: 99%
“…Moreover, organic matter often has advantages of low toxicity and good biocompatibility. [1][2][3][4][5][6][7][8][9][10] Therefore, constructing organic RTP materials would bene t tissue imaging, tumor diagnosis, and drug tracking. [10][11][12][13][14][15] To date, most phosphorescent materials have poor biological tissue permeability because the wavelengths of their emission spectra are short (less than 580 nm).…”
Section: Introductionmentioning
confidence: 99%
“…Recent years have witnessed intensive studies and rapid development of alarge variety of organic afterglow materials with luminescent lifetimes over 0.1 sf or various fascinating applications,r anging from light-emitting diodes,b iological imaging,i nformation storage,s ensing,a nd security protection. [1][2][3][4][5][6][7][8][9] Principally,t og enerate observable afterglow emission, the incorporation of heteroatoms to promote the spinorbital coupling (SOC) between excited singlet and triplet states for the enhanced intersystem crossing (ISC) and stabilization of the lowest triplet excited state (T 1 *) in pursuit of long-lived excitons for ultralong room-temperature phos-phorescence (OURTP) are essential [10][11][12][13][14][15] (Figure 1a). However,l ow-lying T 1 *w ill lead to bathochromic shift of the emission spectrum, so that most organic afterglow bands are in ar ange of 500-600 nm for yellow emission.…”
Section: Introductionmentioning
confidence: 99%