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      Photolysis of 3‐Azido‐3‐phenyl‐3H‐isobenzofuran‐1‐one at Ambient and Cryogenic Temperatures†

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      https://www.riss.kr/link?id=O111806072

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      다국어 초록 (Multilingual Abstract)

      Although alkyl azides are known to typically form imines under direct irradiation, the product formation mechanism remains ambiguous as some alkyl azides also yield the corresponding triplet alkylnitrenes at cryogenic temperatures. The photoreactivity of 3‐azido‐3‐phenyl‐3H‐isobenzofuran‐1‐one (1) was investigated in solution and in cryogenic matrices. Irradiation (λ = 254 nm) of azide 1 in acetonitrile yielded a mixture of imines 2 and 3. Monitoring of the reaction progress using UV‐Vis absorption spectroscopy revealed an isosbestic point at 210 nm, indicating that the reaction proceeded cleanly. Similar results were observed for the photoreactivity of azide 1 in a frozen 2‐methyltetrahydrofuran (mTHF) matrix. Irradiation of azide 1 in an argon matrix at 6 K resulted in the disappearance of its IR bands with the concurrent appearance of IR bands corresponding to imines 2 and 3. Thus, it was theorized that azide 1 forms imines 2 and 3 via a concerted mechanism from its singlet excited state or through singlet alkylnitrene 11N, which does not intersystem cross to its triplet configuration. This proposal was supported by CASPT2 calculations on a model system, which suggested that the energy gap between the singlet and triplet configurations of alkylnitrene 1N is 33 kcal/mol, thus making intersystem crossing inefficient.
      Irradiation of alkyl azide 1 in acetonitrile at ambient temperature, in 2‐methyltetrahydrofuran at 80 K, or in an argon matrix at 6 K, yielded imines 2 and 3. It was postulated that 1 forms 2 and 3 via a concerted mechanism from its singlet excited state or through the corresponding singlet alkylnitrene 11N, which does not intersystem cross to its triplet configuration. This notion was supported by CASPT2 calculations, which suggested that the energy gap between the singlet and triplet configurations of 1N is 33 kcal/mol, thus making intersystem crossing inefficient.
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      Although alkyl azides are known to typically form imines under direct irradiation, the product formation mechanism remains ambiguous as some alkyl azides also yield the corresponding triplet alkylnitrenes at cryogenic temperatures. The photoreactivit...

      Although alkyl azides are known to typically form imines under direct irradiation, the product formation mechanism remains ambiguous as some alkyl azides also yield the corresponding triplet alkylnitrenes at cryogenic temperatures. The photoreactivity of 3‐azido‐3‐phenyl‐3H‐isobenzofuran‐1‐one (1) was investigated in solution and in cryogenic matrices. Irradiation (λ = 254 nm) of azide 1 in acetonitrile yielded a mixture of imines 2 and 3. Monitoring of the reaction progress using UV‐Vis absorption spectroscopy revealed an isosbestic point at 210 nm, indicating that the reaction proceeded cleanly. Similar results were observed for the photoreactivity of azide 1 in a frozen 2‐methyltetrahydrofuran (mTHF) matrix. Irradiation of azide 1 in an argon matrix at 6 K resulted in the disappearance of its IR bands with the concurrent appearance of IR bands corresponding to imines 2 and 3. Thus, it was theorized that azide 1 forms imines 2 and 3 via a concerted mechanism from its singlet excited state or through singlet alkylnitrene 11N, which does not intersystem cross to its triplet configuration. This proposal was supported by CASPT2 calculations on a model system, which suggested that the energy gap between the singlet and triplet configurations of alkylnitrene 1N is 33 kcal/mol, thus making intersystem crossing inefficient.
      Irradiation of alkyl azide 1 in acetonitrile at ambient temperature, in 2‐methyltetrahydrofuran at 80 K, or in an argon matrix at 6 K, yielded imines 2 and 3. It was postulated that 1 forms 2 and 3 via a concerted mechanism from its singlet excited state or through the corresponding singlet alkylnitrene 11N, which does not intersystem cross to its triplet configuration. This notion was supported by CASPT2 calculations, which suggested that the energy gap between the singlet and triplet configurations of 1N is 33 kcal/mol, thus making intersystem crossing inefficient.

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