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Absorption and emission of light in red emissive carbon nanodots

The structure–function relationship, especially the origin of absorption and emission of light in carbon nanodots (CNDs), has baffled scientists. The multilevel complexity arises due to the large number of by-products synthesized during the bottom-up approach. By performing systematic purification a...

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Autores principales: Soni, Neeraj, Singh, Shivendra, Sharma, Shubham, Batra, Gayatri, Kaushik, Kush, Rao, Chethana, Verma, Navneet C., Mondal, Bhaskar, Yadav, Aditya, Nandi, Chayan K.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: The Royal Society of Chemistry 2021
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8179431/
https://www.ncbi.nlm.nih.gov/pubmed/34163635
http://dx.doi.org/10.1039/d0sc05879c
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author Soni, Neeraj
Singh, Shivendra
Sharma, Shubham
Batra, Gayatri
Kaushik, Kush
Rao, Chethana
Verma, Navneet C.
Mondal, Bhaskar
Yadav, Aditya
Nandi, Chayan K.
author_facet Soni, Neeraj
Singh, Shivendra
Sharma, Shubham
Batra, Gayatri
Kaushik, Kush
Rao, Chethana
Verma, Navneet C.
Mondal, Bhaskar
Yadav, Aditya
Nandi, Chayan K.
author_sort Soni, Neeraj
collection PubMed
description The structure–function relationship, especially the origin of absorption and emission of light in carbon nanodots (CNDs), has baffled scientists. The multilevel complexity arises due to the large number of by-products synthesized during the bottom-up approach. By performing systematic purification and characterization, we reveal the presence of a molecular fluorophore, quinoxalino[2,3-b]phenazine-2,3-diamine (QXPDA), in a large amount (∼80% of the total mass) in red emissive CNDs synthesized from o-phenylenediamine (OPDA), which is one of the well-known precursor molecules used for CND synthesis. The recorded NMR and mass spectra tentatively confirm the structure of QXPDA. The close resemblance of the experimental vibronic progression and the mirror symmetry of the absorption and emission spectra with the theoretically simulated spectra confirm an extended conjugated structure of QXPDA. Interestingly, QXPDA dictates the complete emission characteristics of the CNDs; in particular, it showed a striking similarity of its excitation independent emission spectra with that of the original synthesized red emissive CND solution. On the other hand, the CND like structure with a typical size of ∼4 nm was observed under a transmission electron microscope for a blue emissive species, which showed both excitation dependent and independent emission spectra. Interestingly, Raman spectroscopic data showed the similarity between QXPDA and the dot structure thus suggesting the formation of the QXPDA aggregated core structure in CNDs. We further demonstrated the parallelism in trends of absorption and emission of light from a few other red emissive CNDs, which were synthesized using different experimental conditions.
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spelling pubmed-81794312021-06-22 Absorption and emission of light in red emissive carbon nanodots Soni, Neeraj Singh, Shivendra Sharma, Shubham Batra, Gayatri Kaushik, Kush Rao, Chethana Verma, Navneet C. Mondal, Bhaskar Yadav, Aditya Nandi, Chayan K. Chem Sci Chemistry The structure–function relationship, especially the origin of absorption and emission of light in carbon nanodots (CNDs), has baffled scientists. The multilevel complexity arises due to the large number of by-products synthesized during the bottom-up approach. By performing systematic purification and characterization, we reveal the presence of a molecular fluorophore, quinoxalino[2,3-b]phenazine-2,3-diamine (QXPDA), in a large amount (∼80% of the total mass) in red emissive CNDs synthesized from o-phenylenediamine (OPDA), which is one of the well-known precursor molecules used for CND synthesis. The recorded NMR and mass spectra tentatively confirm the structure of QXPDA. The close resemblance of the experimental vibronic progression and the mirror symmetry of the absorption and emission spectra with the theoretically simulated spectra confirm an extended conjugated structure of QXPDA. Interestingly, QXPDA dictates the complete emission characteristics of the CNDs; in particular, it showed a striking similarity of its excitation independent emission spectra with that of the original synthesized red emissive CND solution. On the other hand, the CND like structure with a typical size of ∼4 nm was observed under a transmission electron microscope for a blue emissive species, which showed both excitation dependent and independent emission spectra. Interestingly, Raman spectroscopic data showed the similarity between QXPDA and the dot structure thus suggesting the formation of the QXPDA aggregated core structure in CNDs. We further demonstrated the parallelism in trends of absorption and emission of light from a few other red emissive CNDs, which were synthesized using different experimental conditions. The Royal Society of Chemistry 2021-01-14 /pmc/articles/PMC8179431/ /pubmed/34163635 http://dx.doi.org/10.1039/d0sc05879c Text en This journal is © The Royal Society of Chemistry https://creativecommons.org/licenses/by-nc/3.0/
spellingShingle Chemistry
Soni, Neeraj
Singh, Shivendra
Sharma, Shubham
Batra, Gayatri
Kaushik, Kush
Rao, Chethana
Verma, Navneet C.
Mondal, Bhaskar
Yadav, Aditya
Nandi, Chayan K.
Absorption and emission of light in red emissive carbon nanodots
title Absorption and emission of light in red emissive carbon nanodots
title_full Absorption and emission of light in red emissive carbon nanodots
title_fullStr Absorption and emission of light in red emissive carbon nanodots
title_full_unstemmed Absorption and emission of light in red emissive carbon nanodots
title_short Absorption and emission of light in red emissive carbon nanodots
title_sort absorption and emission of light in red emissive carbon nanodots
topic Chemistry
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8179431/
https://www.ncbi.nlm.nih.gov/pubmed/34163635
http://dx.doi.org/10.1039/d0sc05879c
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